Christopher Scotese | University of Texas at Arlington (original) (raw)
Featured Publications by Christopher Scotese
Global Temperature Change in Deep Time Several recent studies have published estimates describing... more Global Temperature Change in Deep Time Several recent studies have published estimates describing how global temperature has changed during the last 540 million years (Figure 1; Scotese et al., 2021). These temperature curves identify times when the Earth's global average temperature was much warmer than the presentday (hothouse intervals) and time intervals when, like the present-day, the Earth has been locked in a frigid "icehouse" world. Figure 2 is a "heat map" which highlights these hothouse and icehouse intervals (Scotese et al., 2021). Figure 1. Estimates of Global Average Temperature during the Phanerozoic
Phanerozoic Paleotemperatures: The Earth Changing Climate during the last 540 million years, Earth-Science Reviews, 2021
This study provides a comprehensive and quantitative estimate of how global temperatures have cha... more This study provides a comprehensive and quantitative estimate of how global temperatures have changed during the last 540 million years. It combines paleotemperature measurements determined from oxygen isotopes with broader insights obtained from the changing distribution of lithologic indicators of climate, such as coals, evaporites, calcretes, reefs, and bauxite deposits. The waxing and waning of the Earth’s great polar icecaps have been mapped using the past distribution of tillites, dropstones, and glendonites. The global temperature model presented here includes estimates of global average temperate (GAT), changing tropical temperatures (∆T◦ tropical), deep ocean temperatures, and polar temperatures. Though similar, in many respects, to the temper- ature history deduced directly from the study of oxygen isotopes, our model does not predict the extreme high temperatures for the Early Paleozoic required by isotopic investigations. The history of global changes in tem- perature during the Phanerozoic has been summarized in a “paleotemperature timescale” that subdivides the many past climatic events into 8 major climate modes; each climate mode is made up of 3-4 pairs of warming and cooling episodes (chronotemps). A detailed narrative describes how these past temperature events have been affected by geological processes such as the eruption of Large Igneous Provinces (LIPS) (warming) and bolide impacts (cooling). The paleotemperature model presented here allows for a deeper understanding of the inter- connected geologic, tectonic, paleoclimatic, paleoceanographic, and evolutionary events that have shaped our planet, and we make explicit predictions about the Earth’s past temperature that can be tested and evaluated. By quantitatively describing the pattern of paleotemperature change through time, we may be able to gain important insights into the history of the Earth System and the fundamental causes of climate change on geological timescales. These insights can help us better understand the problems and challenges that we face as a result of Future Global Warming.
Scotese, C.R., 2017. Atlas of Ancient Oceans & Continents: Plate Tectonics 1.5 by - Today, PALEOMP Project, Evanston, IL, 75 p., 2017
Phylotectonics is the study of descendant/antecedent relationships between continents, paleoconti... more Phylotectonics is the study of descendant/antecedent relationships between continents, paleocontinents, and terranes based on their plate tectonic history. This "Tectonic Tree" diagram illustrates the phylotectonic relationships of the major continents, paleocontinents, and terranes during the last 1.5 billion years. For a description and discussion of how this diagram was created see Scotese (2017) , "Atlas of Oceans & Continents: Plate Tectonics 1.5 billion years - Today."
Scotese, C.R., 2016. Global Climate Change: Modern Times to 540 million years ago, https://www.youtube.com/watch?v=DGf5pZMkjA0, PALEOMAP Project, Evanston, IL.
Scotese, C.R., 2016. Figure 15 in Some Thoughts on Global Climate Change: The transition from Icehouse to Hothouse, in the Earth History: The evolution of the Earth System (in preparation), PALEOMAP Project, Evanston, IL., 2016
This diagram show the rise and fall of global temperatures during the last 540 million years. Sc... more This diagram show the rise and fall of global temperatures during the last 540 million years. Scotese (2016) describes how this curve was made. It replaces the curve published in Scotese et al., (1999).
PETM= Paleocene-Eocene Thermal Maximum (55.8 Ma), EEOC = Early Eocene Climatic Optimum (54 Ma – 46 Ma), MECO = Mid-Eocene Climatic Optimum(42 Ma), EOT = Eocene-Oligocene Transition (40 Ma – 33 Ma), MMCO=Mid-Miocene Climatic Optimum (15Ma – 13Ma), LGM = Last Glacial Maximum (21,000 years ago), 2016 = Modern MAT, PAW = Post-Anthropogenic Warming . White stars indicate rapid cooling episodes (Stoll-Schrag Events26) at 160Ma, 127Ma, 97Ma, 91Ma, 71Ma, and 65 Ma). Black stars represent rapid warming episodes (Kidder-Worsley Events16) at (Present-day, 15Ma, 43Ma, 56Ma, 65Ma, 93Ma, 120Ma, 183Ma, 200Ma, 251Ma, 300Ma, 359Ma, 374Ma, 444Ma, 499Ma, 520Ma, and 542 Ma).
Please cite as: Scotese, C.R., 2015. Phanerozoic Temperature Curve, PALEOMAP Project, Evanston, IL.
To learn more about how this curve was produced see:
Scotese, C.R., 2016. Some thoughts Global Climate Change: The Transition from Icehouse to Hothouse, in Scotese, C.R., Earth History: The Evolution of the Earth System as Revealed through Plate Tectonics, Paleogeography, Paleoclimate, and the Evolution of Life, PALEOMAP Project, (in preparation), Evanston, IL.
Scotese, C.R., 2016. Some Thoughts on Global Climate Change: The transition from Icehouse to Hothouse, in the Earth History: The evolution of the Earth System (in preparation), PALEOMAP Project, Evanston, IL., 2016
The Earth’s climate is changing. When humankind emerged from the last major Ice Age, about 21,00... more The Earth’s climate is changing. When humankind emerged from the last major Ice Age, about 21,000 years ago, both poles and much of the northern continents were covered with expanding ice sheets (Figure 1). In the past 10,000 years the Earth has naturally warmed and the ice sheet have retreated towards the poles. However, make no mistake about it, we are still locked in the depths of an Icehouse world.
According to a natural cycle, controlled in part, by changes in the shape of the Earth’s orbit, this warm period should continue for another 40,000 years or so. Then, if Nature has its way, the Earth will slip back again into the grips of another major Ice Age and frigid landscapes will once again expand outward from the poles.
But Nature may not have its way. Things have changed. We have changed things. The addition of CO2 to the atmosphere during the last 200 years of human industry has amplified this natural warming trend and the average global temperature has risen rapidly. The average global temperature was 12 ˚ C during the Last Glacial Maximum (21,000 years ago). During the following Interglacial period, the average global temperature slowly rose to 13.8˚C. Since 1880, it has increased another .6˚ degrees to 14.4˚C ( as of 2015). This rate of warming is 30 times faster1 than what occurred during the previous 20,000 years.
How much more will global temperatures rise? Will the increase in global temperature be enough to push the Earth from a frigid Icehouse world with thick polar icecaps to a sweltering Hothouse world with palm trees and alligators living at the North Pole? This is the question that I would like to address in this essay.
But before we discuss how much the Earth will warm, there are a few other questions we must tackle, such as:
-What exactly is an Icehouse World, and what causes the Earth to cool off so dramatically? ,
-Conversely, what is a Hothouse World?, and what causes the Earth to heat up so dramatically?
-And, what do we mean by “the average global temperature”? How is it calculated?
Abstract This report describes the contents of the PALEOMAP PaleoAtlas for GPlates, describes how... more Abstract
This report describes the contents of the PALEOMAP PaleoAtlas for GPlates, describes how the maps in the PaleoAtlas were made, documents the sources of information used to make the paleogeographic maps, and provides instructions how to plot user-defined paleodata on the paleogeographic maps using the program “PaleoDataPlotter”. The PALEOMAP PaleloAtlas and the program (Mac OSX) can be downloaded at http://www.earthbyte.org/paleomap-paleoatlas-for-gplates/ .
Please cite this work as: Scotese, C.R., 2016. PALEOMAP PaleoAtlas for GPlates and the PaleoData Plotter Program, PALEOMAP Project, http://www.earthbyte.org/paleomap-paleoatlas-for-gplates/
Part I. Introduction
The PALEOMAP PaleoAtlas for GPlates consists of 91 paleogeographic maps spanning the Phanerozoic and late Neoproterozoic. Table 1 lists all the time intervals that comprise the six volumes of the PALEOMAP PaleoAtlas for GPlates. The PaleoAtlas contains one map for nearly every stage in the Phanerozoic, as well as 3 maps for the late Precambrian. The PaleoAtlas can be directly loaded into GPLates as a “Time Dependant Raster” file (see Part III, “Loading the PALEOMAP PaleoAtlas into GPlates”). A paleogeographic map is defined as a map that shows the ancient configuration of the ocean basins and continents, as well as important topographic and bathymetric features such as mountains, lowlands, shallow sea, continental shelves, and deep oceans (Figure 1, Early Cretaceous, 121.8 Ma). Ideally, a paleogeographic map would be the kind of reference map that any time traveler would like to have before embarking on a journey back through time.
Colorful paleogeographic maps may be nice to look at, but the maps become much more useful for research and teaching purposes if users can plot their own data on the maps. In this regard, user-defined paleodata can be plotted on the paleogeographic maps in two ways: 1) using GPLates tools and procedures to import symbols and labels in a GIS-format (see GPlates Tutorial 1.1: Loading and Saving Data), and 2) by loading user-defined, latitude/longitude point data “text files” using the program “PaleoDataPlotter”. The latter method is described in the Section IV, “Plotting User-Defined Data on the Paleogeographic Reconstructions”.
PaleoDataPlotter, which is provided with this report, creates a variety of geometric symbols (circles, squares, triangles, stars, plus signs, crosses, small dots, and arrows) as well as short numeric labels (up to 5 digits), that can be plotted on the paleogeographic map at user-defined latitude/longitude coordinates (Figure 2). The PaleoDataPlotter program is ideal for plotting fossil localities, geological outcrops, as well as the locations of drill sites, wells, stratigraphic sections, or any point data set whose geographic location can be specified by modern, latitude and longitude coordinates. The arrow symbol, which can be oriented according to a user-supplied azimuth, is particularly useful for plotting “vector” information such as: ocean current directions, river flow, wind directions, paleomagnetic declinations, stress fields, and instantaneous plate motions. In a future version, the PaleoDataPlotter will also be able to plot text-labels at specific latitude/longitude coordinates.
Scotese, C.R., 2015. Plate Tectonics (flipbook), PALEOMAP Project, Evanston, IL, 41 pp., Aug 24, 2015
This "flipbook", which illustrates the plate tectonic development of the continents and ocean bas... more This "flipbook", which illustrates the plate tectonic development of the continents and ocean basins during the past 750 million years, was assembled to commemorate the scientific career of Professor Rob van der Voo. The flipbook consists of 34 plate tectonic reconstructions that map the past location of subduction zones (barbed lines), mid-ocean ridges, (dashed lines), and collision zones (marked x's). The tectonic reconstructions are based on the global plate tectonic model developed by the PALEOMAP Project.
The latitudinal orientation of the continents is derived largely from paleomagnetic data collected by Professor van der Voo (xref). Hot spots tracks and sea floor spreading isochrons (Seton et al., 2012) were used to constrain the longitudinal position of the continents back to ~200 million years. Plate tectonic reconstructions older than 200 million years are necessarily more speculative and have been derived by combining diverse lines of evidence from the tectonic histories of the continents (e.g., timing of continent-continent collisions or ages of rifting), the distribution of paleoclimatic indicators (i.e coals, tillites, salt deposits, and bauxites, see Boucot et al., 2013), and in some case, the biogeographic affinities of fossil faunas and floras.
Though a diverse data has been used to produce these reconstructions, this data, itself, is not enough. So much time has passed and so little direct evidence is preserved that guidance must also be sought from the "Rules of Plate Tectonics".
Plates do not move randomly but evolve in a manner that is consistent with the forces that drive them. The principal driving forces are: slab pull, ridge push and trench rollback. These forces shape the plates and provide important insights into how plate boundaries will evolve. Simply said, plates will only move if they are pulled by a subducting slab or pushed by the forces exerted by a mature ridge system. The evolving plate boundaries have been drawn to follow this maxim. It is also important to note that plate tectonics is a "catastrophic" system. Though "slow and steady" is the general rule, once every hundred million years or so, a major plate tectonic reorganization occurs. These "plate tectonic catastrophes" most often occur when mid-ocean ridges are subducted or when major continents collide. (For a more complete listing of the "Rules of Plate Tectonics", the reader is referred to XXXXXX.
The first "continental drift" flipbook was pushed as an undergraduate research project (Scotese, 1974; 1975abc). Subsequent editions have followed (1976ab; 1978; 1979; 1980; 1990, 1991, 1997, 2004). A more complete description of the data and information that is used to produce the flipbooks can be found in Scotese (2004). These maps could not have been produced without the GPlates plate modelling software and the tectonic data sets published by Dietmar Müller and his team at Earthbytes.
Special thanks to Maggie Geiger, and Robert and Jonathan Scotese for their help assembling this flipbook.
Time Scale
The age given next to each map represents age in millions of years. The corresponding geological ages (Ogg et al., 2008) are:
0 Modern World
20 Ma Early Miocene
40 Ma late Middle Eocene
60 Ma Paleocene
80 Ma Late Cretaceous - Campanian
100 Ma Early Cretaceous - late Albian
120 Ma Early Cretaceous - early Aptian
140 Ma Early Cretaceous - Berriasian
160 Ma Late Jurassic - Oxfordian
180 Ma Early Jurassic - Toarcian
200 Ma Triassic/Jurassic boundary
220 Ma Late Triassic - Carnian
240 Ma Middle Triassic - Anisian
260 Ma Middle Permian - Capitanian
280 Ma Early Permian - Artinskian
300 Ma Late Pennsylvanian
320 Ma Late Mississippian
340 Ma Middle Mississippian
360 Ma Devono-Carboniferous
380 Ma Late Devonian - Frasnian
400 Ma Early Devonian - Emsian
420 Ma Late Silurian - Ludlow
440 Ma Early Silurian - Llandovery
460 Ma Middle Ordovician
480 Ma Early Ordovician
500 Ma Late Cambrian
520 Ma Middle Cambrian
540 Ma Cambrian-Precambrian
560 Ma Neoproterozoic - lt. Ediacaran
600 Ma Neoporterozoic - m. Ediacaran
630 Ma Neoproterozoic - e. Ediacaran
660 Ma Neoproterozoic - e. Ediacaran
690 Ma Neoproterozoic - lt. Cryogenian
720 Ma m. Cryogenian
750 Ma m. Cryogenian
References Cited
Ogg, J., Ogg, G., and Gradstein, F.M., 2008. The Concise Geologic Time Scale, Cambridge University Press, 177 p.
Scotese, C.R. 1974. First Flip Book Images (from 35mm film from PLATO System), Unpublished.
Scotese, C.R., and Baker, D.W., 1975a. Continental drift reconstructions and animation, Journal of Geological Education, 23: 167-171.
Scotese, C.R., 1975b. Continental Drift Flip Book, 1stedition.Chicago, Illinois. (single page version
Scotese, C.R., 1975c. Continental Drift Flip Book, 1st edition. Chicago, Illinois. (double page version)
Scotese, C.R., 1976a. Continental
Drift “Flip Book”, edition 1.5, Department of Geological Sciences, University of Illinois. ResearchGate Academia
Scotese, C.R., 1976b. A continental drift “flip book", Computers & Geosciences, 2:113-116.
Scotese, C.R., and Ziegler, A.M., 1978. Paleozoic continental drift reconstructions and animation, American Geophysical Union, 1978 Spring Annual Meeting, Eos, v. 59. Issue 4, p. 263.
Scotese, C.R., 1979. Continental Drift (flip book), 2nd edition.
Scotese, C.R., Snelson, S.S., and Ross, W.C., 1980. A computer animation of continental drift, J. Geomag. Geoelectr., 32: suppl. III, 61-70.
Scotese, C.R., 1990. Atlas of Phanerozoic Plate Tectonic Reconstructions, PALEOMAP Progress 01-1090a, Department of Geology, University of Texas at Arlington, Texas, 57 pp.
Scotese, C.R., 1991. Continental Drift Flip Book, 4th edition, PALEOMAP Project, Arlington, TX, 49 pp.
Scotese, C.R., 1997. Continental Drift Flip Book, 7th edition, PALEOMAP Project, Department of Geology, University of Texas at Arlington, Texas, 80 pp.
Scotese, 2004.
Seton et al., 2012.
Van der Voo, R., 1993. Paleomagnetism of the Atlantic, Tethys, and Iapetus Oceans, Cambridge University Press, 411 p.
This "4 up" version of the Plate Tectonics flip book by C.R. Scotese, PALEOMAP Project, can be co... more This "4 up" version of the Plate Tectonics flip book by C.R. Scotese, PALEOMAP Project, can be copied and cut-up into 4 identical flip books. For the best results follow this procedure. 1) use 8 1/2" by 11" card stock (80 - 100 weight), 2) cut into quarters using a mechanical paper cutter, and 3) staple across the top of the booklet using 3/4" staples (upper left and upper right corners).
For high resolution, full-page sized maps see the link to: https://www.researchgate.net/publication/281393670_PlateTectonic_FlipBook_v.2.
This map of plate tectonics 50 million years in the future was created by projecting present-day ... more This map of plate tectonics 50 million years in the future was created by projecting present-day plate motions into the future. The northward movement of Australia and Africa will result in the collision of Australia with China and the closure of the Red Sea, Gulf of Aden, and Mediterranean. New subduction zones start in the Indian Ocean (Capricorn trench) and along the eastern coasts of North America and South America. The Atlantic subduction zone will consume the western half of the Atlantic Ocean and eventually will consume the Mid-Atlantic Ridge. The northern portions of the Central Indian Ridge will be subducted beneath the Capricorn Trench. When the Mid-Indian Ridge is eventually subducted, Antarctica will be pulled northward to join Australia and the new "Afroaustralasian" supercontinent.
There are three reasons why I do not show the East African rifts opening into a new ocean:
- Often, oceans open around a three-armed rift system called a “triple junction”. Only two arms of a triple junction open to form ocean basins. . In the case of East Africa, the Red Sea and Gulf of Aden are the two successful rifts. The East African rift system, starting at the Afar Triangle, in Ethiopia is an aulacogen or “failed arm” of a triple junction The East African rift system is a failed rift, much like the Benue Trough in the South Atlantic or the Labrador Sea in the North Atlantic.
- Let’s step back and ask the question, “What caused the rifting of the Red Sea , Gulf of Aden and East Africa in the first place? Though the Afar hotspot certainly helped to weaken the lithosphere, The driving force that caused the rifting was the subduction (beneath Eurasia , i.e., Iran) of oceanic crust attached to the northern margin of Arabia. (There was ocean an ocean between Arabian and Iran.) This subducting slab “pulled” Arabia northward tearing it away from Africa. This subduction zone has been completely destroyed by the collision of Arabia and Eurasia (Zagros Mountains). Consequently, there is no longer any “plate tectonic forces” acting on the African rifts and they will not continue to open.
- Also, if we look at the plate tectonic neighborhood of East Africa, we see that the dominant motion of plates in the western Indian Ocean is N-S, rather than E-W . In fact, a new subduction zone is just beginning in the central Indian Ocean (a zone of diffuse earthquakes ~ 5-10 S) that will continue to pull Australia and Antarctica northward towards Asia. In other words, there is no room for East Africa to expand towards the east. Rather the east coast of Madagascar will become a strike-slip margin accommodating the continued, northward movement of the Australian-Antarctic plate.
I hope this explanation is helpful. Of course all of this is scientific speculation, we will have to wait and see what happens, but this is my projection based on my understanding of the forces that drive plate motions and the history of past plate motions. Remember: “The past reveals patterns; Patterns inform process; Process permits prediction.”
Chris Scotese
Director, PALEOMAP Project
Atlases by Christopher Scotese
Scotese, C.R., 2017. Atlas of Ancient Oceans & Continents: Plate Tectonics during the Last 1.5 billion years, PALEOMAP Project, Evanston, IL, 21 pp., 2017
The maps in this atlas are the first draft of a new set of plate tectonic reconstructions that wi... more The maps in this atlas are the first draft of a new set of plate tectonic reconstructions that will provide the framework for the revised paleogeographic and paleoclimatic maps that I am preparing for my book, “Earth History: Evolution of the Earth Systems”. As the title of this work implies, the goal of this atlas is to identify the major continents and oceans back through time. Tables 1 and 2 list the names of the continents and oceans shown in this atlas. Names shown in bold are newly coined ocean and continent names. Figure X is a “tectonic phylogeny” that shows how these continents and oceans have deeloped through time.
Continents
Continents are defined to be regions of the Earth that are underlain by continental crust (~lithosphere). Continents may be “emergent” or “flooded” depending on sea level, which has varied from ~200 meters above modern sea level to ~200 meters below modern sea level. The continental regions on these maps are shown in two colors: gray and white. The gray areas represent extant regions of continental crust. The white regions represent areas of continental crust that have been removed by subduction (tectonic erosion), underthrusting beneath continents (like Greater India), or are simply squeezed and compressed into much narrower zones (e.g. the Rocky Mountains or the Central Asian collision zone).
Continents come in a variety of sizes and shapes. We reserve the name “continent” for regions of continental crust greater than 10 Mkm2 . The present-day continents are: Africa, Antarctica, Asia, Australia, Europe, North America, and South America. In the Early Ordovician the continents were: Baltica, Cathaysia, Gondwana, Laurentia, and Siberia. Regions with areas less than 10 Mkm2 are either “subcontinents”, like the Indian subcontinent (4.6 Mkm2), or “island continents” like Greenland or Madagascar. Subcontinents are continental regions that are contiguous with a larger continent, but are considered to be a distinct region. India is subcontinent because it is separated from Asia by the Himalaya mountains and Tibetan plateau. Island continents, on-the-other-hand, are simply very large islands. Zealandia is an example of a mostly submerged an island continent. Finally, Regions of continental crust less than 1 Mkm2 may be considered to be “microcontinents” (e.g., S. Orkney Islands, Seychelles, Rockall plateau, or Tasman Rise).
The naming conventions for continents . . .
Oceans
Ocean basins are defined to be regions of the Earth that are underlain by oceanic lithosphere. Ocean basins, together with the flooded portions of the continents, comprise the Earth’s oceans, seas, and seaways. It is interesting to note that following the definition of continent and ocean proposed here, there are regions of the Earth that can be considered to be both “continents” and “oceans”. These regions are the portions of the continents flooded by the sea. For example, the Grand Banks of eastern Canada is part of the continent of North America, but the water above the Grand Banks is part of the Atlantic Ocean. This duality is due to the fact that the landward boundary of the ocean is the shoreline, whereas the seaward boundary of the continent lies near the junction of the continental rise and continental slope. In the past, this duality has lead to a fair degree of confusion when it came to naming oceans and continents. Also, it should be noted that no attempt has been made to show past coastlines on the maps in this atlas.
The derivation of the names of the modern oceans generally falls into one of three categories: mythological names, location names, and descriptive names. For example, the Atlantic Ocean is named after the Greek god, Atlas; the Indian Ocean is named after the subcontinent of India; the Pacific Ocean was named by Francisco Pissarro, who thought that the Pacific Ocean looked “peaceful”. Some of Paleozoic and Mesozoic Oceans are named after Greek gods related to Atlas. Tethys was the XXX of Atlas. Iapetus was the XXX of XXX, a Rhea (Rheic Ocean) was the XXX of XXX. Because it is difficult to meaningfully continue these lineages, none of the new oceans are named after Greek gods. Instead we have adopted a dual naming convention. The names of the new oceans either reflect the local geography (e.g., the Mozambique Ocean once ran through most of East Africa, including Mozambique) or a related geologic/tectonic feature ( e.g., the Grenville Ocean is the ocean basin that closed during the Grenville Orogeny (~1050 Ma) in eastern North America.
Coining new names for every new ocean, however, can be confusing. To avoid confusion and promote clarity we have tried to make slight modification to existing names, especially if there is a relation of inheritance. For example, originally there was just one ocean called the “Tethys Ocean”. However, we now know that three distinct oceans: ProtoTethys, PaleoTethys, and NeoTethys once existed in the Tethyan realm. Using this format, we have coined the new terms “PaleoPanthalassa” and “ProtoPanthalassa” to described earlier versions of the Panthalassic Ocean.
The names of these bodies of water may change slightly depending on the maturity of an ocean basin. A newly formed ocean basin, one that is still relatively narrow, may be called a “sea”, like the Red Sea, or if it connects two larger bodies of water, it may be called a “seaway”. The term “sea” is also used for bodies of water surrounded or partially enclosed by continents, like the Mediterranean Sea or Weddell Sea. Oceans as they age, gradually narrow as the continents on either side of the ocean approach each other (through subduction of oceanic lithosphere). Thus, it is possible for a once mighty “ocean” to become a narrow “sea” or “seaway” prior to its demise.
Scotese, C.R., 2016. Plate Tectonic Evolution of the Arctic, https://www.youtube.com/watch?v=hPZEScNqU7U, PALEOMAP Project, Evanston, IL.
This is a pdf version of an animation that illustrates the plate tectonic evolution of the Arctic... more This is a pdf version of an animation that illustrates the plate tectonic evolution of the Arctic region during the last 200 million years. The animation can be viewed at: https://www.youtube.com/watch?v=hPZEScNqU7U.
Scotese, C.R., 2001. Atlas of Earth History, Volume 1, Paleogeography, PALEOMAP Project, Arlington, Texas, 52 pp, 2001
2001.06 This is an Atlas that is made up of maps from my website (www.scotese.com).
Scotese, C.R., 2014. Atlas of Neogene Paleogeographic Maps (Mollweide Projection), Maps 1-7, Volume 1, The Cenozoic, PALEOMAP Atlas for ArcGIS, PALEOMAP Project, Evanston, IL., 2014
2014.07 This Atlas of Neogene Paleogeographic Maps shows the changing paleogeography from the Ear... more 2014.07 This Atlas of Neogene Paleogeographic Maps shows the changing paleogeography from the Early Miocene (Auquitanian & Burdigalian, 19.5 Ma) to the Present-day. The maps are from volume 1 of the PALEOMAP PaleoAtlas for ArcGIS (Scotese, 2014). Absolute age assignments are from Ogg, Ogg & Gradstein (2008).
For Maps 3, 5 and 7, there are two versions of the paleogeography. One map shows the maximum highstand sea level (maximum flooding surface). The other map shows the minimum lowstand sea level (supersequence boundary). For each paleogeography there is an estimate of sea level change, in meters, relative to present-day sea level.
The following maps are included in the Atlas of Neogene Paleogeographic Maps:
Map 01 Modern World (Holocene, 0.0 Ma) Transgressive Systems Tract
Map 02 Last Glacial Maximum (Pleistocene, 21,000 years ago) Anthropocene Supersequence Boundary
Map 03 Plio-Pleistocene, (Gelasian & Piacenzian, 2.588 Ma Ma) Lowstand Systems Tract
Map 04 Latest Miocene (Messinian Event, 6.3 Ma) Maximum Flooding Surface
Map 05 Middle/Late Miocene, (Serravallian and Tortonian, 10.5 Ma) Messinian Supersequence Boundary & Tortonian Maximum Flooding Surface
Map 06 Middle Miocene (Langhian, 14.9 Ma) Maximum Flooding Surface
Map 07 Early Miocene (Aquitanian & Burdigalian, 19.5 Ma) Serravallian Supersequence Boundary, Aquitanian Maximum Flooding Surface
This Atlas should be cited as:
Scotese, C.R., 2014. Atlas of Neogene Paleogeographic Maps (Mollweide Projection), Maps 1-7, Volume 1, The Cenozoic, PALEOMAP Atlas for ArcGIS, PALEOMAP Project, Evanston, IL.
References Cited
Ogg, J.G., Ogg, G., Gradstein, F.M., 2008. The Concise Geologic Time Scale, Cambridge University Press, Cambridge, UK, 177 pp.
Scotese, C.R., 2014, The PALEOMAP Project PaleoAtlas for ArcGIS, version 2, Volume 1, Cenozoic Plate Tectonic, Paleogeographic, and Paleoclimatic Reconstructions, Maps 1-15, PALEOMAP Project, Evanston, IL.
Scotese, C.R., 2014. Atlas of Paleogene Paleogeographic Maps (Mollweide Projection), Maps 8-15, Volume 1, The Cenozoic, PALEOMAP Atlas for ArcGIS, PALEOMAP Project, Evanston, IL., 2014
2014.08 This Atlas of Paleogene Paleogeographic Maps shows the changing paleogeography from the P... more 2014.08 This Atlas of Paleogene Paleogeographic Maps shows the changing paleogeography from the Paleocene (60.6 Ma) to the Late Oligocene (25.7 Ma). The maps are from volume 1 of the PALEOMAP PaleoAtlas for ArcGIS (Scotese, 2014). Absolute age assignments are from Ogg, Ogg & Gradstein (2008).
For Maps 8, 10, 12, and 15, there are two versions of the paleogeography. One map shows the maximum highstand sea level (maximum flooding surface). The other map shows the minimum lowstand sea level (supersequence boundary). For each paleogeography there is an estimate of sea level change (m) relative to present-day sea level.
The following maps are included in the Atlas of Paleogene Paleogeographic Maps:
Map 08 Late Oligocene (Chattian, 25.7 Ma Ma) Aquitanian Superseqeunce Boundary & Late Oligocene Transgressive Systems Tract
Map 09 Early Oligocene (Rupelian, 31.1 Ma) Maximum Flooding Surface
Map 10 Late Eocene, (Priabonian, 35.6 Ma) Rupelian Supersequence Boundary & Priabonian Transgressive Systems Tract
Map 11 late Middle Eocene (Bartonian, 38.8 Ma) Bartonian Transgressive Systems Tract
Map 12 early Middle Eocene, (middle Lutetian, 44.6 Ma) Lutetian Maximum Flooding Surface & Lutetian Supersequence Boundary
Map 13 Early Eocene (Ypresian, 52.2 Ma) Ypresian Maximum Flooding Surface
Map 14 Paleocene/Eocene Boundary (PETM, Thanetian/Ypresian Boundary, 55.8 Ma) PETM Transgressive Systems Tract
Map 15 Paleocene (Danian & Thanetian, 60.6 Ma) Paleocene Maximum Flooding Surface & Danian Supersequence Boundary
This Atlas should be cited as:
Scotese, C.R., 2014. Atlas of Paleogene Paleogeographic Maps (Mollweide Projection), Maps 8-15, Volume 1, The Cenozoic, PALEOMAP Atlas for ArcGIS, PALEOMAP Project, Evanston, IL.
References Cited
Ogg, J.G., Ogg, G., Gradstein, F.M., 2008. The Concise Geologic Time Scale, Cambridge University Press, Cambridge, UK, 177 pp.
Scotese, C.R., 2014, The PALEOMAP Project PaleoAtlas for ArcGIS, version 2, Volume 1, Cenozoic Plate Tectonic, Paleogeographic, and Paleoclimatic Reconstructions, Maps 1-15, PALEOMAP Project, Evanston, IL.
Scotese, C.R., 2014. Atlas of Late Cretaceous Paleogeographic Maps, PALEOMAP Atlas for ArcGIS, volume 2, The Cretaceous, Maps 16 - 22, Mollweide Projection, PALEOMAP Project, Evanston, IL. , 2014
2014.09 This Atlas of Late Cretaceous Maps shows the changing paleogeography from the Cenomanian ... more 2014.09 This Atlas of Late Cretaceous Maps shows the changing paleogeography from the Cenomanian (96.6 Ma) to the K/T Boundary(65.5 Ma). The maps are from volume 2 of the PALEOMAP PaleoAtlas for ArcGIS (Scotese, 2014). For several time intervals there are versions of the map that show maximum sea level (maximum flooding surface) or minimum sea level (sequence boundary) during that stage.
The following maps are included in the Atlas of Late Cretaceous Paleogeographic Maps:
Map 16 K/T Boundary (latest Maastrichtian, 65.5 Ma)
Map 17 Late Cretaceous (Maastrichtian, 68 Ma)
Map 18 Late Cretaceous (Late Campanian, 73.8 Ma)
Map 19 Late Cretaceous (Early Campanian, 80.3 Ma)
Map 20 Late Cretaceous (Santonian & Coniacian, 86 Ma)
Map 21 Mid Cretaceous (Turonian, 91.1 Ma)
Map 22 Mid Cretaceous (Cenomanian, 96.6 Ma)
This work should be cited as
Scotese, C.R., 2014. Atlas of Late Cretaceous Paleogeographic Maps, PALEOMAP Atlas for ArcGIS, volume 2, The Cretaceous, Maps 16 ╨ 22, Mollweide Projection, PALEOMAP Project, Evanston, IL.
Scotese, C.R., 2014. Atlas of Early Cretaceous Paleogeographic Maps, PALEOMAP Atlas for ArcGIS, volume 2, The Cretaceous, Maps 23-31, Mollweide Projection, PALEOMAP Project, Evanston, IL. , 2014
2014.10 This Atlas of Early Cretaceous Paleogeographic Maps shows the changing paleogeography fro... more 2014.10 This Atlas of Early Cretaceous Paleogeographic Maps shows the changing paleogeography from the Berriasian (143 Ma) to the late Albian (101.8 Ma). The maps are from volume 2 of the PALEOMAP PaleoAtlas for ArcGIS (Scotese, 2014).
Also numeric time values are from Gradstein, Ogg & Smith (2008). For several stages there are versions of the map that show maximum sea level (maximum flooding surface) or minimum sea level (supersequence boundary) during that time interval.
The following maps are included in the Atlas of Early Cretaceous Paleogeographic Maps:
Map 23 Early Cretaceous (late Albian, 101.8 Ma)
Map 24 Early Cretaceous (middle Albian, 106 Ma)
Map 25 Early Cretaceous (early Albian, 110 Ma) Albian Supersequence Boundary and Transgressive System Tract
Map 26 Early Cretaceous (late Aptian, 115.2 Ma)
Map 27 Early Cretaceous (early Aptian, 121.8 Ma)
Map 28 Early Cretaceous (Barremian, 127.5 Ma)
Map 29 Early Cretaceous (Hauterivian, 132 Ma)
Map 30 Early Cretaceous (Valanginian, 137 Ma) Barremian-Hauterivian Supersequence boundary and Transgressive Systems Tract
Map 31 Early Cretaceous (Berriasian, 143 Ma) Berriasian Supersequence boundary and Maximum Flooding Surface
This work should be cited as
Scotese, C.R., 2014. Atlas of Early Cretaceous Paleogeographic Maps, PALEOMAP Atlas for ArcGIS, volume 2, The Cretaceous, Maps 23-31, Mollweide Projection, PALEOMAP Project, Evanston, IL.
Scotese, C.R., 2014. Atlas of Jurassic Paleogeographic Maps, PALEOMAP Atlas for ArcGIS, volume 3, The Jurassic and Triassic, Maps 32-42, Mollweide Projection, PALEOMAP Project, Evanston, IL. , 2014
2014.11 This Atlas of Jurassic Paleogeographic Maps shows the changing paleogeography from the He... more 2014.11 This Atlas of Jurassic Paleogeographic Maps shows the changing paleogeography from the Hettangian (198 Ma) to the Jurassic/Cretaceoous Boundary (145.5 Ma). The maps are from volume 3 of the PALEOMAP PaleoAtlas for ArcGIS (Scotese, 2014). Absolute age assignments are from Gradstein, Ogg & Smith (2008).
The following maps are included in the Atlas of Jurassic Paleogeographic Maps:
Map 32 Jurassic/Cretaceous Boundary (145.5 Ma) Berriasian Supersequence Boundary
Map 33 Late Jurassic (Tithonian, 148.2 Ma) Highstand Systems Track
Map 34 Late Jurassic (Kimmeridgian, 153.2) Maximum Flooding Surface
Map 35 Late Jurassic (Oxfordian, 158.4) Transgressive Systems Track
Map 36 Middle Jurassic (Callovian, 164.5 Ma) Transgressive Systems Tract
Map 37 Middle Jurassic (Bajocian & Bathonian, 169.7 Ma) Kimmeridgian-Oxfordian Supersequence Boundary & Maximum Flooding Surface
Map 38 Middle Jurassic (Aalenian, 173.2 Ma) Bathonian-Bajocian Supersequence Boundary
Map 39 Early Jurassic (Toarcian, 179.3 Ma) Toarcian Supersequence Boundary and Maximum Flooding Surface
Map 40 Early Jurassic (Pliensbachian, 186.3 Ma) Maximum Flooding Surface
Map 41 Early Jurassic (Sinemurian, 193 Ma) Transgressive Systems Track
Map 42 Early Jurassic (Hettangian, 198 Ma) Pliensbachian Supersequence Boundary
This work should be cited as
Scotese, C.R., 2014. Atlas of Jurassic Paleogeographic Maps, PALEOMAP Atlas for ArcGIS, volume 3, The Jurassic and Triassic, Maps 32-42, Mollweide Projection, PALEOMAP Project, Evanston, IL.
Scotese, C.R., 2014. Atlas of Middle & Late Permian and Triassic Paleogeographic Maps, Maps 43 – 52, Volumes 3 & 4, PALEOMAP PaleoAtlas for ArcGIS, PALEOMAP Project, Evanston, IL. , 2014
2014.12 This Atlas of Middle & Late Permian and Triassic Paleogeographic Maps shows the changing ... more 2014.12 This Atlas of Middle & Late Permian and Triassic Paleogeographic Maps shows the changing paleogeography from the Middle Permian (Roadian & Wordian, 268.2 Ma) to the end of the Triassic (Rhaetian, 201.6 Ma). The maps are from volumes 3 and 4 of the PALEOMAP PaleoAtlas for ArcGIS (Scotese, 2014). Absolute age assignments are from Gradstein, Ogg & Smith (2008).
The following maps are included in the Atlas of Jurassic Paleogeographic Maps:
Map 43 Late Triassic (Rhaetian, 201.6 Ma) Lowstand Systems Tract
Map 44 Late Triassic (Norian, 210 Ma) Maximum Flooding Surface
Map 45 Late Triassic (Carnian, 222.6 Ma) Transgressive Systems Tract
Map 46 Middle Triassic (Ladinian, 232.9 Ma) Transgressive Systems Tract
Map 47 Middle Triassic (Anisian, 241.5 Ma) Lowstand Systems Tract
Map 48 Early Triassic (Induan & Olenekian, 248.5 Ma) Lowstand Systems Track
Map 49 Permo-Triassic Boundary (251 Ma) Norian Supersequence Boundary
Map 50 Late Permian (Lopingian, 255.7 Ma) Transgressive Systems Tract
Map 51 late Middle Permian (Capitanian, 263.1 Ma) Lowstand Systems Tract
Map 52 Middle Permian (Roadian & Wordian, 268.2 Ma) Maximum Flooding Surface
This work should be cited as
Scotese, C.R., 2014. Atlas of Middle & Late Permian and Triassic Paleogeographic Maps, maps 43 - 48 from Volume 3 of the PALEOMAP Atlas for ArcGIS (Jurassic and Triassic) and maps 49 – 52 from Volume 4 of the PALEOMAP PaleoAtlas for ArcGIS (Late Paleozoic), Mollweide Projection, PALEOMAP Project, Evanston, IL.
Scotese, C.R., 2014. Atlas of Permo-Carboniferous Paleogeographic Maps (Mollweide Projection), Maps 53 – 64, Volumes 4, The Late Paleozoic, PALEOMAP Atlas for ArcGIS, PALEOMAP Project, Evanston, IL.
This Atlas of Permo-Carboniferous Paleogeographic Maps shows the changing paleogeography from the... more This Atlas of Permo-Carboniferous Paleogeographic Maps shows the changing paleogeography from the Early Mississippian (Tournasian, 352.3 Ma) to the Early Permian (Kungurian, 273.1 Ma). The maps are from volume 4 of the PALEOMAP PaleoAtlas for ArcGIS (Scotese, 2014). Absolute age assignments are from Gradstein, Ogg & Smith (2008).
The following maps are included in the Atlas of Permo-Carboniferous Paleogeographic Maps:
Map 53 Early Permian (Kungurian, 273.1 Ma) Highstand Systems Tract
Map 54 Early Permian (Artinskian, 280 Ma) Maximum Flooding Surface
Map 55 Early Permian (Sakmarian, 289.5 Ma) Maximum Flooding Surface
Map 56 Early Permian (Asselian, 296.8 Ma) Sakmarian Supersequence Boundary & Maximum Flooding Surface
Map 57 Late Pennsylvanian (Gzhelian, 301.2 Ma) Asselian Supersequence Boundary & Maximum Flooding Surface
Map 58 Late Pennsylvanian (Kasimovian, 305.3 Ma) Maximum Flooding Surface
Map 59 Middle Pennsylvanian (Moscovian, 309.5) Transgressive Systems Tract
Map 60 Early Pennsylvanian (Bashkirian, 314.9 Ma) Bashkirian Supersequence Boundary & Maximum Flooding Surface
Map 61 Late Mississippian (Serpukhovian, 323.2 Ma) Maximum Flooding Surface
Map 62 Middle Mississippian (late Visean, 332.5 Ma) Highstand Systems Tract
Map 63 Middle Mississippian (early Visean, 341.1 Ma) Maximum Flooding Surface
Map 64 Early Mississippian (Tournasian, 352.3 Ma) Maximum Flooding Surface
This work should be cited as
Scotese, C.R., 2014. Atlas of Permo-Carboniferous Paleogeographic Maps (Mollweide Projection), Maps 53 – 64, Volumes 4, The Late Paleozoic, PALEOMAP Atlas for ArcGIS, PALEOMAP Project, Evanston, IL.
Global Temperature Change in Deep Time Several recent studies have published estimates describing... more Global Temperature Change in Deep Time Several recent studies have published estimates describing how global temperature has changed during the last 540 million years (Figure 1; Scotese et al., 2021). These temperature curves identify times when the Earth's global average temperature was much warmer than the presentday (hothouse intervals) and time intervals when, like the present-day, the Earth has been locked in a frigid "icehouse" world. Figure 2 is a "heat map" which highlights these hothouse and icehouse intervals (Scotese et al., 2021). Figure 1. Estimates of Global Average Temperature during the Phanerozoic
Phanerozoic Paleotemperatures: The Earth Changing Climate during the last 540 million years, Earth-Science Reviews, 2021
This study provides a comprehensive and quantitative estimate of how global temperatures have cha... more This study provides a comprehensive and quantitative estimate of how global temperatures have changed during the last 540 million years. It combines paleotemperature measurements determined from oxygen isotopes with broader insights obtained from the changing distribution of lithologic indicators of climate, such as coals, evaporites, calcretes, reefs, and bauxite deposits. The waxing and waning of the Earth’s great polar icecaps have been mapped using the past distribution of tillites, dropstones, and glendonites. The global temperature model presented here includes estimates of global average temperate (GAT), changing tropical temperatures (∆T◦ tropical), deep ocean temperatures, and polar temperatures. Though similar, in many respects, to the temper- ature history deduced directly from the study of oxygen isotopes, our model does not predict the extreme high temperatures for the Early Paleozoic required by isotopic investigations. The history of global changes in tem- perature during the Phanerozoic has been summarized in a “paleotemperature timescale” that subdivides the many past climatic events into 8 major climate modes; each climate mode is made up of 3-4 pairs of warming and cooling episodes (chronotemps). A detailed narrative describes how these past temperature events have been affected by geological processes such as the eruption of Large Igneous Provinces (LIPS) (warming) and bolide impacts (cooling). The paleotemperature model presented here allows for a deeper understanding of the inter- connected geologic, tectonic, paleoclimatic, paleoceanographic, and evolutionary events that have shaped our planet, and we make explicit predictions about the Earth’s past temperature that can be tested and evaluated. By quantitatively describing the pattern of paleotemperature change through time, we may be able to gain important insights into the history of the Earth System and the fundamental causes of climate change on geological timescales. These insights can help us better understand the problems and challenges that we face as a result of Future Global Warming.
Scotese, C.R., 2017. Atlas of Ancient Oceans & Continents: Plate Tectonics 1.5 by - Today, PALEOMP Project, Evanston, IL, 75 p., 2017
Phylotectonics is the study of descendant/antecedent relationships between continents, paleoconti... more Phylotectonics is the study of descendant/antecedent relationships between continents, paleocontinents, and terranes based on their plate tectonic history. This "Tectonic Tree" diagram illustrates the phylotectonic relationships of the major continents, paleocontinents, and terranes during the last 1.5 billion years. For a description and discussion of how this diagram was created see Scotese (2017) , "Atlas of Oceans & Continents: Plate Tectonics 1.5 billion years - Today."
Scotese, C.R., 2016. Global Climate Change: Modern Times to 540 million years ago, https://www.youtube.com/watch?v=DGf5pZMkjA0, PALEOMAP Project, Evanston, IL.
Scotese, C.R., 2016. Figure 15 in Some Thoughts on Global Climate Change: The transition from Icehouse to Hothouse, in the Earth History: The evolution of the Earth System (in preparation), PALEOMAP Project, Evanston, IL., 2016
This diagram show the rise and fall of global temperatures during the last 540 million years. Sc... more This diagram show the rise and fall of global temperatures during the last 540 million years. Scotese (2016) describes how this curve was made. It replaces the curve published in Scotese et al., (1999).
PETM= Paleocene-Eocene Thermal Maximum (55.8 Ma), EEOC = Early Eocene Climatic Optimum (54 Ma – 46 Ma), MECO = Mid-Eocene Climatic Optimum(42 Ma), EOT = Eocene-Oligocene Transition (40 Ma – 33 Ma), MMCO=Mid-Miocene Climatic Optimum (15Ma – 13Ma), LGM = Last Glacial Maximum (21,000 years ago), 2016 = Modern MAT, PAW = Post-Anthropogenic Warming . White stars indicate rapid cooling episodes (Stoll-Schrag Events26) at 160Ma, 127Ma, 97Ma, 91Ma, 71Ma, and 65 Ma). Black stars represent rapid warming episodes (Kidder-Worsley Events16) at (Present-day, 15Ma, 43Ma, 56Ma, 65Ma, 93Ma, 120Ma, 183Ma, 200Ma, 251Ma, 300Ma, 359Ma, 374Ma, 444Ma, 499Ma, 520Ma, and 542 Ma).
Please cite as: Scotese, C.R., 2015. Phanerozoic Temperature Curve, PALEOMAP Project, Evanston, IL.
To learn more about how this curve was produced see:
Scotese, C.R., 2016. Some thoughts Global Climate Change: The Transition from Icehouse to Hothouse, in Scotese, C.R., Earth History: The Evolution of the Earth System as Revealed through Plate Tectonics, Paleogeography, Paleoclimate, and the Evolution of Life, PALEOMAP Project, (in preparation), Evanston, IL.
Scotese, C.R., 2016. Some Thoughts on Global Climate Change: The transition from Icehouse to Hothouse, in the Earth History: The evolution of the Earth System (in preparation), PALEOMAP Project, Evanston, IL., 2016
The Earth’s climate is changing. When humankind emerged from the last major Ice Age, about 21,00... more The Earth’s climate is changing. When humankind emerged from the last major Ice Age, about 21,000 years ago, both poles and much of the northern continents were covered with expanding ice sheets (Figure 1). In the past 10,000 years the Earth has naturally warmed and the ice sheet have retreated towards the poles. However, make no mistake about it, we are still locked in the depths of an Icehouse world.
According to a natural cycle, controlled in part, by changes in the shape of the Earth’s orbit, this warm period should continue for another 40,000 years or so. Then, if Nature has its way, the Earth will slip back again into the grips of another major Ice Age and frigid landscapes will once again expand outward from the poles.
But Nature may not have its way. Things have changed. We have changed things. The addition of CO2 to the atmosphere during the last 200 years of human industry has amplified this natural warming trend and the average global temperature has risen rapidly. The average global temperature was 12 ˚ C during the Last Glacial Maximum (21,000 years ago). During the following Interglacial period, the average global temperature slowly rose to 13.8˚C. Since 1880, it has increased another .6˚ degrees to 14.4˚C ( as of 2015). This rate of warming is 30 times faster1 than what occurred during the previous 20,000 years.
How much more will global temperatures rise? Will the increase in global temperature be enough to push the Earth from a frigid Icehouse world with thick polar icecaps to a sweltering Hothouse world with palm trees and alligators living at the North Pole? This is the question that I would like to address in this essay.
But before we discuss how much the Earth will warm, there are a few other questions we must tackle, such as:
-What exactly is an Icehouse World, and what causes the Earth to cool off so dramatically? ,
-Conversely, what is a Hothouse World?, and what causes the Earth to heat up so dramatically?
-And, what do we mean by “the average global temperature”? How is it calculated?
Abstract This report describes the contents of the PALEOMAP PaleoAtlas for GPlates, describes how... more Abstract
This report describes the contents of the PALEOMAP PaleoAtlas for GPlates, describes how the maps in the PaleoAtlas were made, documents the sources of information used to make the paleogeographic maps, and provides instructions how to plot user-defined paleodata on the paleogeographic maps using the program “PaleoDataPlotter”. The PALEOMAP PaleloAtlas and the program (Mac OSX) can be downloaded at http://www.earthbyte.org/paleomap-paleoatlas-for-gplates/ .
Please cite this work as: Scotese, C.R., 2016. PALEOMAP PaleoAtlas for GPlates and the PaleoData Plotter Program, PALEOMAP Project, http://www.earthbyte.org/paleomap-paleoatlas-for-gplates/
Part I. Introduction
The PALEOMAP PaleoAtlas for GPlates consists of 91 paleogeographic maps spanning the Phanerozoic and late Neoproterozoic. Table 1 lists all the time intervals that comprise the six volumes of the PALEOMAP PaleoAtlas for GPlates. The PaleoAtlas contains one map for nearly every stage in the Phanerozoic, as well as 3 maps for the late Precambrian. The PaleoAtlas can be directly loaded into GPLates as a “Time Dependant Raster” file (see Part III, “Loading the PALEOMAP PaleoAtlas into GPlates”). A paleogeographic map is defined as a map that shows the ancient configuration of the ocean basins and continents, as well as important topographic and bathymetric features such as mountains, lowlands, shallow sea, continental shelves, and deep oceans (Figure 1, Early Cretaceous, 121.8 Ma). Ideally, a paleogeographic map would be the kind of reference map that any time traveler would like to have before embarking on a journey back through time.
Colorful paleogeographic maps may be nice to look at, but the maps become much more useful for research and teaching purposes if users can plot their own data on the maps. In this regard, user-defined paleodata can be plotted on the paleogeographic maps in two ways: 1) using GPLates tools and procedures to import symbols and labels in a GIS-format (see GPlates Tutorial 1.1: Loading and Saving Data), and 2) by loading user-defined, latitude/longitude point data “text files” using the program “PaleoDataPlotter”. The latter method is described in the Section IV, “Plotting User-Defined Data on the Paleogeographic Reconstructions”.
PaleoDataPlotter, which is provided with this report, creates a variety of geometric symbols (circles, squares, triangles, stars, plus signs, crosses, small dots, and arrows) as well as short numeric labels (up to 5 digits), that can be plotted on the paleogeographic map at user-defined latitude/longitude coordinates (Figure 2). The PaleoDataPlotter program is ideal for plotting fossil localities, geological outcrops, as well as the locations of drill sites, wells, stratigraphic sections, or any point data set whose geographic location can be specified by modern, latitude and longitude coordinates. The arrow symbol, which can be oriented according to a user-supplied azimuth, is particularly useful for plotting “vector” information such as: ocean current directions, river flow, wind directions, paleomagnetic declinations, stress fields, and instantaneous plate motions. In a future version, the PaleoDataPlotter will also be able to plot text-labels at specific latitude/longitude coordinates.
Scotese, C.R., 2015. Plate Tectonics (flipbook), PALEOMAP Project, Evanston, IL, 41 pp., Aug 24, 2015
This "flipbook", which illustrates the plate tectonic development of the continents and ocean bas... more This "flipbook", which illustrates the plate tectonic development of the continents and ocean basins during the past 750 million years, was assembled to commemorate the scientific career of Professor Rob van der Voo. The flipbook consists of 34 plate tectonic reconstructions that map the past location of subduction zones (barbed lines), mid-ocean ridges, (dashed lines), and collision zones (marked x's). The tectonic reconstructions are based on the global plate tectonic model developed by the PALEOMAP Project.
The latitudinal orientation of the continents is derived largely from paleomagnetic data collected by Professor van der Voo (xref). Hot spots tracks and sea floor spreading isochrons (Seton et al., 2012) were used to constrain the longitudinal position of the continents back to ~200 million years. Plate tectonic reconstructions older than 200 million years are necessarily more speculative and have been derived by combining diverse lines of evidence from the tectonic histories of the continents (e.g., timing of continent-continent collisions or ages of rifting), the distribution of paleoclimatic indicators (i.e coals, tillites, salt deposits, and bauxites, see Boucot et al., 2013), and in some case, the biogeographic affinities of fossil faunas and floras.
Though a diverse data has been used to produce these reconstructions, this data, itself, is not enough. So much time has passed and so little direct evidence is preserved that guidance must also be sought from the "Rules of Plate Tectonics".
Plates do not move randomly but evolve in a manner that is consistent with the forces that drive them. The principal driving forces are: slab pull, ridge push and trench rollback. These forces shape the plates and provide important insights into how plate boundaries will evolve. Simply said, plates will only move if they are pulled by a subducting slab or pushed by the forces exerted by a mature ridge system. The evolving plate boundaries have been drawn to follow this maxim. It is also important to note that plate tectonics is a "catastrophic" system. Though "slow and steady" is the general rule, once every hundred million years or so, a major plate tectonic reorganization occurs. These "plate tectonic catastrophes" most often occur when mid-ocean ridges are subducted or when major continents collide. (For a more complete listing of the "Rules of Plate Tectonics", the reader is referred to XXXXXX.
The first "continental drift" flipbook was pushed as an undergraduate research project (Scotese, 1974; 1975abc). Subsequent editions have followed (1976ab; 1978; 1979; 1980; 1990, 1991, 1997, 2004). A more complete description of the data and information that is used to produce the flipbooks can be found in Scotese (2004). These maps could not have been produced without the GPlates plate modelling software and the tectonic data sets published by Dietmar Müller and his team at Earthbytes.
Special thanks to Maggie Geiger, and Robert and Jonathan Scotese for their help assembling this flipbook.
Time Scale
The age given next to each map represents age in millions of years. The corresponding geological ages (Ogg et al., 2008) are:
0 Modern World
20 Ma Early Miocene
40 Ma late Middle Eocene
60 Ma Paleocene
80 Ma Late Cretaceous - Campanian
100 Ma Early Cretaceous - late Albian
120 Ma Early Cretaceous - early Aptian
140 Ma Early Cretaceous - Berriasian
160 Ma Late Jurassic - Oxfordian
180 Ma Early Jurassic - Toarcian
200 Ma Triassic/Jurassic boundary
220 Ma Late Triassic - Carnian
240 Ma Middle Triassic - Anisian
260 Ma Middle Permian - Capitanian
280 Ma Early Permian - Artinskian
300 Ma Late Pennsylvanian
320 Ma Late Mississippian
340 Ma Middle Mississippian
360 Ma Devono-Carboniferous
380 Ma Late Devonian - Frasnian
400 Ma Early Devonian - Emsian
420 Ma Late Silurian - Ludlow
440 Ma Early Silurian - Llandovery
460 Ma Middle Ordovician
480 Ma Early Ordovician
500 Ma Late Cambrian
520 Ma Middle Cambrian
540 Ma Cambrian-Precambrian
560 Ma Neoproterozoic - lt. Ediacaran
600 Ma Neoporterozoic - m. Ediacaran
630 Ma Neoproterozoic - e. Ediacaran
660 Ma Neoproterozoic - e. Ediacaran
690 Ma Neoproterozoic - lt. Cryogenian
720 Ma m. Cryogenian
750 Ma m. Cryogenian
References Cited
Ogg, J., Ogg, G., and Gradstein, F.M., 2008. The Concise Geologic Time Scale, Cambridge University Press, 177 p.
Scotese, C.R. 1974. First Flip Book Images (from 35mm film from PLATO System), Unpublished.
Scotese, C.R., and Baker, D.W., 1975a. Continental drift reconstructions and animation, Journal of Geological Education, 23: 167-171.
Scotese, C.R., 1975b. Continental Drift Flip Book, 1stedition.Chicago, Illinois. (single page version
Scotese, C.R., 1975c. Continental Drift Flip Book, 1st edition. Chicago, Illinois. (double page version)
Scotese, C.R., 1976a. Continental
Drift “Flip Book”, edition 1.5, Department of Geological Sciences, University of Illinois. ResearchGate Academia
Scotese, C.R., 1976b. A continental drift “flip book", Computers & Geosciences, 2:113-116.
Scotese, C.R., and Ziegler, A.M., 1978. Paleozoic continental drift reconstructions and animation, American Geophysical Union, 1978 Spring Annual Meeting, Eos, v. 59. Issue 4, p. 263.
Scotese, C.R., 1979. Continental Drift (flip book), 2nd edition.
Scotese, C.R., Snelson, S.S., and Ross, W.C., 1980. A computer animation of continental drift, J. Geomag. Geoelectr., 32: suppl. III, 61-70.
Scotese, C.R., 1990. Atlas of Phanerozoic Plate Tectonic Reconstructions, PALEOMAP Progress 01-1090a, Department of Geology, University of Texas at Arlington, Texas, 57 pp.
Scotese, C.R., 1991. Continental Drift Flip Book, 4th edition, PALEOMAP Project, Arlington, TX, 49 pp.
Scotese, C.R., 1997. Continental Drift Flip Book, 7th edition, PALEOMAP Project, Department of Geology, University of Texas at Arlington, Texas, 80 pp.
Scotese, 2004.
Seton et al., 2012.
Van der Voo, R., 1993. Paleomagnetism of the Atlantic, Tethys, and Iapetus Oceans, Cambridge University Press, 411 p.
This "4 up" version of the Plate Tectonics flip book by C.R. Scotese, PALEOMAP Project, can be co... more This "4 up" version of the Plate Tectonics flip book by C.R. Scotese, PALEOMAP Project, can be copied and cut-up into 4 identical flip books. For the best results follow this procedure. 1) use 8 1/2" by 11" card stock (80 - 100 weight), 2) cut into quarters using a mechanical paper cutter, and 3) staple across the top of the booklet using 3/4" staples (upper left and upper right corners).
For high resolution, full-page sized maps see the link to: https://www.researchgate.net/publication/281393670_PlateTectonic_FlipBook_v.2.
This map of plate tectonics 50 million years in the future was created by projecting present-day ... more This map of plate tectonics 50 million years in the future was created by projecting present-day plate motions into the future. The northward movement of Australia and Africa will result in the collision of Australia with China and the closure of the Red Sea, Gulf of Aden, and Mediterranean. New subduction zones start in the Indian Ocean (Capricorn trench) and along the eastern coasts of North America and South America. The Atlantic subduction zone will consume the western half of the Atlantic Ocean and eventually will consume the Mid-Atlantic Ridge. The northern portions of the Central Indian Ridge will be subducted beneath the Capricorn Trench. When the Mid-Indian Ridge is eventually subducted, Antarctica will be pulled northward to join Australia and the new "Afroaustralasian" supercontinent.
There are three reasons why I do not show the East African rifts opening into a new ocean:
- Often, oceans open around a three-armed rift system called a “triple junction”. Only two arms of a triple junction open to form ocean basins. . In the case of East Africa, the Red Sea and Gulf of Aden are the two successful rifts. The East African rift system, starting at the Afar Triangle, in Ethiopia is an aulacogen or “failed arm” of a triple junction The East African rift system is a failed rift, much like the Benue Trough in the South Atlantic or the Labrador Sea in the North Atlantic.
- Let’s step back and ask the question, “What caused the rifting of the Red Sea , Gulf of Aden and East Africa in the first place? Though the Afar hotspot certainly helped to weaken the lithosphere, The driving force that caused the rifting was the subduction (beneath Eurasia , i.e., Iran) of oceanic crust attached to the northern margin of Arabia. (There was ocean an ocean between Arabian and Iran.) This subducting slab “pulled” Arabia northward tearing it away from Africa. This subduction zone has been completely destroyed by the collision of Arabia and Eurasia (Zagros Mountains). Consequently, there is no longer any “plate tectonic forces” acting on the African rifts and they will not continue to open.
- Also, if we look at the plate tectonic neighborhood of East Africa, we see that the dominant motion of plates in the western Indian Ocean is N-S, rather than E-W . In fact, a new subduction zone is just beginning in the central Indian Ocean (a zone of diffuse earthquakes ~ 5-10 S) that will continue to pull Australia and Antarctica northward towards Asia. In other words, there is no room for East Africa to expand towards the east. Rather the east coast of Madagascar will become a strike-slip margin accommodating the continued, northward movement of the Australian-Antarctic plate.
I hope this explanation is helpful. Of course all of this is scientific speculation, we will have to wait and see what happens, but this is my projection based on my understanding of the forces that drive plate motions and the history of past plate motions. Remember: “The past reveals patterns; Patterns inform process; Process permits prediction.”
Chris Scotese
Director, PALEOMAP Project
Scotese, C.R., 2017. Atlas of Ancient Oceans & Continents: Plate Tectonics during the Last 1.5 billion years, PALEOMAP Project, Evanston, IL, 21 pp., 2017
The maps in this atlas are the first draft of a new set of plate tectonic reconstructions that wi... more The maps in this atlas are the first draft of a new set of plate tectonic reconstructions that will provide the framework for the revised paleogeographic and paleoclimatic maps that I am preparing for my book, “Earth History: Evolution of the Earth Systems”. As the title of this work implies, the goal of this atlas is to identify the major continents and oceans back through time. Tables 1 and 2 list the names of the continents and oceans shown in this atlas. Names shown in bold are newly coined ocean and continent names. Figure X is a “tectonic phylogeny” that shows how these continents and oceans have deeloped through time.
Continents
Continents are defined to be regions of the Earth that are underlain by continental crust (~lithosphere). Continents may be “emergent” or “flooded” depending on sea level, which has varied from ~200 meters above modern sea level to ~200 meters below modern sea level. The continental regions on these maps are shown in two colors: gray and white. The gray areas represent extant regions of continental crust. The white regions represent areas of continental crust that have been removed by subduction (tectonic erosion), underthrusting beneath continents (like Greater India), or are simply squeezed and compressed into much narrower zones (e.g. the Rocky Mountains or the Central Asian collision zone).
Continents come in a variety of sizes and shapes. We reserve the name “continent” for regions of continental crust greater than 10 Mkm2 . The present-day continents are: Africa, Antarctica, Asia, Australia, Europe, North America, and South America. In the Early Ordovician the continents were: Baltica, Cathaysia, Gondwana, Laurentia, and Siberia. Regions with areas less than 10 Mkm2 are either “subcontinents”, like the Indian subcontinent (4.6 Mkm2), or “island continents” like Greenland or Madagascar. Subcontinents are continental regions that are contiguous with a larger continent, but are considered to be a distinct region. India is subcontinent because it is separated from Asia by the Himalaya mountains and Tibetan plateau. Island continents, on-the-other-hand, are simply very large islands. Zealandia is an example of a mostly submerged an island continent. Finally, Regions of continental crust less than 1 Mkm2 may be considered to be “microcontinents” (e.g., S. Orkney Islands, Seychelles, Rockall plateau, or Tasman Rise).
The naming conventions for continents . . .
Oceans
Ocean basins are defined to be regions of the Earth that are underlain by oceanic lithosphere. Ocean basins, together with the flooded portions of the continents, comprise the Earth’s oceans, seas, and seaways. It is interesting to note that following the definition of continent and ocean proposed here, there are regions of the Earth that can be considered to be both “continents” and “oceans”. These regions are the portions of the continents flooded by the sea. For example, the Grand Banks of eastern Canada is part of the continent of North America, but the water above the Grand Banks is part of the Atlantic Ocean. This duality is due to the fact that the landward boundary of the ocean is the shoreline, whereas the seaward boundary of the continent lies near the junction of the continental rise and continental slope. In the past, this duality has lead to a fair degree of confusion when it came to naming oceans and continents. Also, it should be noted that no attempt has been made to show past coastlines on the maps in this atlas.
The derivation of the names of the modern oceans generally falls into one of three categories: mythological names, location names, and descriptive names. For example, the Atlantic Ocean is named after the Greek god, Atlas; the Indian Ocean is named after the subcontinent of India; the Pacific Ocean was named by Francisco Pissarro, who thought that the Pacific Ocean looked “peaceful”. Some of Paleozoic and Mesozoic Oceans are named after Greek gods related to Atlas. Tethys was the XXX of Atlas. Iapetus was the XXX of XXX, a Rhea (Rheic Ocean) was the XXX of XXX. Because it is difficult to meaningfully continue these lineages, none of the new oceans are named after Greek gods. Instead we have adopted a dual naming convention. The names of the new oceans either reflect the local geography (e.g., the Mozambique Ocean once ran through most of East Africa, including Mozambique) or a related geologic/tectonic feature ( e.g., the Grenville Ocean is the ocean basin that closed during the Grenville Orogeny (~1050 Ma) in eastern North America.
Coining new names for every new ocean, however, can be confusing. To avoid confusion and promote clarity we have tried to make slight modification to existing names, especially if there is a relation of inheritance. For example, originally there was just one ocean called the “Tethys Ocean”. However, we now know that three distinct oceans: ProtoTethys, PaleoTethys, and NeoTethys once existed in the Tethyan realm. Using this format, we have coined the new terms “PaleoPanthalassa” and “ProtoPanthalassa” to described earlier versions of the Panthalassic Ocean.
The names of these bodies of water may change slightly depending on the maturity of an ocean basin. A newly formed ocean basin, one that is still relatively narrow, may be called a “sea”, like the Red Sea, or if it connects two larger bodies of water, it may be called a “seaway”. The term “sea” is also used for bodies of water surrounded or partially enclosed by continents, like the Mediterranean Sea or Weddell Sea. Oceans as they age, gradually narrow as the continents on either side of the ocean approach each other (through subduction of oceanic lithosphere). Thus, it is possible for a once mighty “ocean” to become a narrow “sea” or “seaway” prior to its demise.
Scotese, C.R., 2016. Plate Tectonic Evolution of the Arctic, https://www.youtube.com/watch?v=hPZEScNqU7U, PALEOMAP Project, Evanston, IL.
This is a pdf version of an animation that illustrates the plate tectonic evolution of the Arctic... more This is a pdf version of an animation that illustrates the plate tectonic evolution of the Arctic region during the last 200 million years. The animation can be viewed at: https://www.youtube.com/watch?v=hPZEScNqU7U.
Scotese, C.R., 2001. Atlas of Earth History, Volume 1, Paleogeography, PALEOMAP Project, Arlington, Texas, 52 pp, 2001
2001.06 This is an Atlas that is made up of maps from my website (www.scotese.com).
Scotese, C.R., 2014. Atlas of Neogene Paleogeographic Maps (Mollweide Projection), Maps 1-7, Volume 1, The Cenozoic, PALEOMAP Atlas for ArcGIS, PALEOMAP Project, Evanston, IL., 2014
2014.07 This Atlas of Neogene Paleogeographic Maps shows the changing paleogeography from the Ear... more 2014.07 This Atlas of Neogene Paleogeographic Maps shows the changing paleogeography from the Early Miocene (Auquitanian & Burdigalian, 19.5 Ma) to the Present-day. The maps are from volume 1 of the PALEOMAP PaleoAtlas for ArcGIS (Scotese, 2014). Absolute age assignments are from Ogg, Ogg & Gradstein (2008).
For Maps 3, 5 and 7, there are two versions of the paleogeography. One map shows the maximum highstand sea level (maximum flooding surface). The other map shows the minimum lowstand sea level (supersequence boundary). For each paleogeography there is an estimate of sea level change, in meters, relative to present-day sea level.
The following maps are included in the Atlas of Neogene Paleogeographic Maps:
Map 01 Modern World (Holocene, 0.0 Ma) Transgressive Systems Tract
Map 02 Last Glacial Maximum (Pleistocene, 21,000 years ago) Anthropocene Supersequence Boundary
Map 03 Plio-Pleistocene, (Gelasian & Piacenzian, 2.588 Ma Ma) Lowstand Systems Tract
Map 04 Latest Miocene (Messinian Event, 6.3 Ma) Maximum Flooding Surface
Map 05 Middle/Late Miocene, (Serravallian and Tortonian, 10.5 Ma) Messinian Supersequence Boundary & Tortonian Maximum Flooding Surface
Map 06 Middle Miocene (Langhian, 14.9 Ma) Maximum Flooding Surface
Map 07 Early Miocene (Aquitanian & Burdigalian, 19.5 Ma) Serravallian Supersequence Boundary, Aquitanian Maximum Flooding Surface
This Atlas should be cited as:
Scotese, C.R., 2014. Atlas of Neogene Paleogeographic Maps (Mollweide Projection), Maps 1-7, Volume 1, The Cenozoic, PALEOMAP Atlas for ArcGIS, PALEOMAP Project, Evanston, IL.
References Cited
Ogg, J.G., Ogg, G., Gradstein, F.M., 2008. The Concise Geologic Time Scale, Cambridge University Press, Cambridge, UK, 177 pp.
Scotese, C.R., 2014, The PALEOMAP Project PaleoAtlas for ArcGIS, version 2, Volume 1, Cenozoic Plate Tectonic, Paleogeographic, and Paleoclimatic Reconstructions, Maps 1-15, PALEOMAP Project, Evanston, IL.
Scotese, C.R., 2014. Atlas of Paleogene Paleogeographic Maps (Mollweide Projection), Maps 8-15, Volume 1, The Cenozoic, PALEOMAP Atlas for ArcGIS, PALEOMAP Project, Evanston, IL., 2014
2014.08 This Atlas of Paleogene Paleogeographic Maps shows the changing paleogeography from the P... more 2014.08 This Atlas of Paleogene Paleogeographic Maps shows the changing paleogeography from the Paleocene (60.6 Ma) to the Late Oligocene (25.7 Ma). The maps are from volume 1 of the PALEOMAP PaleoAtlas for ArcGIS (Scotese, 2014). Absolute age assignments are from Ogg, Ogg & Gradstein (2008).
For Maps 8, 10, 12, and 15, there are two versions of the paleogeography. One map shows the maximum highstand sea level (maximum flooding surface). The other map shows the minimum lowstand sea level (supersequence boundary). For each paleogeography there is an estimate of sea level change (m) relative to present-day sea level.
The following maps are included in the Atlas of Paleogene Paleogeographic Maps:
Map 08 Late Oligocene (Chattian, 25.7 Ma Ma) Aquitanian Superseqeunce Boundary & Late Oligocene Transgressive Systems Tract
Map 09 Early Oligocene (Rupelian, 31.1 Ma) Maximum Flooding Surface
Map 10 Late Eocene, (Priabonian, 35.6 Ma) Rupelian Supersequence Boundary & Priabonian Transgressive Systems Tract
Map 11 late Middle Eocene (Bartonian, 38.8 Ma) Bartonian Transgressive Systems Tract
Map 12 early Middle Eocene, (middle Lutetian, 44.6 Ma) Lutetian Maximum Flooding Surface & Lutetian Supersequence Boundary
Map 13 Early Eocene (Ypresian, 52.2 Ma) Ypresian Maximum Flooding Surface
Map 14 Paleocene/Eocene Boundary (PETM, Thanetian/Ypresian Boundary, 55.8 Ma) PETM Transgressive Systems Tract
Map 15 Paleocene (Danian & Thanetian, 60.6 Ma) Paleocene Maximum Flooding Surface & Danian Supersequence Boundary
This Atlas should be cited as:
Scotese, C.R., 2014. Atlas of Paleogene Paleogeographic Maps (Mollweide Projection), Maps 8-15, Volume 1, The Cenozoic, PALEOMAP Atlas for ArcGIS, PALEOMAP Project, Evanston, IL.
References Cited
Ogg, J.G., Ogg, G., Gradstein, F.M., 2008. The Concise Geologic Time Scale, Cambridge University Press, Cambridge, UK, 177 pp.
Scotese, C.R., 2014, The PALEOMAP Project PaleoAtlas for ArcGIS, version 2, Volume 1, Cenozoic Plate Tectonic, Paleogeographic, and Paleoclimatic Reconstructions, Maps 1-15, PALEOMAP Project, Evanston, IL.
Scotese, C.R., 2014. Atlas of Late Cretaceous Paleogeographic Maps, PALEOMAP Atlas for ArcGIS, volume 2, The Cretaceous, Maps 16 - 22, Mollweide Projection, PALEOMAP Project, Evanston, IL. , 2014
2014.09 This Atlas of Late Cretaceous Maps shows the changing paleogeography from the Cenomanian ... more 2014.09 This Atlas of Late Cretaceous Maps shows the changing paleogeography from the Cenomanian (96.6 Ma) to the K/T Boundary(65.5 Ma). The maps are from volume 2 of the PALEOMAP PaleoAtlas for ArcGIS (Scotese, 2014). For several time intervals there are versions of the map that show maximum sea level (maximum flooding surface) or minimum sea level (sequence boundary) during that stage.
The following maps are included in the Atlas of Late Cretaceous Paleogeographic Maps:
Map 16 K/T Boundary (latest Maastrichtian, 65.5 Ma)
Map 17 Late Cretaceous (Maastrichtian, 68 Ma)
Map 18 Late Cretaceous (Late Campanian, 73.8 Ma)
Map 19 Late Cretaceous (Early Campanian, 80.3 Ma)
Map 20 Late Cretaceous (Santonian & Coniacian, 86 Ma)
Map 21 Mid Cretaceous (Turonian, 91.1 Ma)
Map 22 Mid Cretaceous (Cenomanian, 96.6 Ma)
This work should be cited as
Scotese, C.R., 2014. Atlas of Late Cretaceous Paleogeographic Maps, PALEOMAP Atlas for ArcGIS, volume 2, The Cretaceous, Maps 16 ╨ 22, Mollweide Projection, PALEOMAP Project, Evanston, IL.
Scotese, C.R., 2014. Atlas of Early Cretaceous Paleogeographic Maps, PALEOMAP Atlas for ArcGIS, volume 2, The Cretaceous, Maps 23-31, Mollweide Projection, PALEOMAP Project, Evanston, IL. , 2014
2014.10 This Atlas of Early Cretaceous Paleogeographic Maps shows the changing paleogeography fro... more 2014.10 This Atlas of Early Cretaceous Paleogeographic Maps shows the changing paleogeography from the Berriasian (143 Ma) to the late Albian (101.8 Ma). The maps are from volume 2 of the PALEOMAP PaleoAtlas for ArcGIS (Scotese, 2014).
Also numeric time values are from Gradstein, Ogg & Smith (2008). For several stages there are versions of the map that show maximum sea level (maximum flooding surface) or minimum sea level (supersequence boundary) during that time interval.
The following maps are included in the Atlas of Early Cretaceous Paleogeographic Maps:
Map 23 Early Cretaceous (late Albian, 101.8 Ma)
Map 24 Early Cretaceous (middle Albian, 106 Ma)
Map 25 Early Cretaceous (early Albian, 110 Ma) Albian Supersequence Boundary and Transgressive System Tract
Map 26 Early Cretaceous (late Aptian, 115.2 Ma)
Map 27 Early Cretaceous (early Aptian, 121.8 Ma)
Map 28 Early Cretaceous (Barremian, 127.5 Ma)
Map 29 Early Cretaceous (Hauterivian, 132 Ma)
Map 30 Early Cretaceous (Valanginian, 137 Ma) Barremian-Hauterivian Supersequence boundary and Transgressive Systems Tract
Map 31 Early Cretaceous (Berriasian, 143 Ma) Berriasian Supersequence boundary and Maximum Flooding Surface
This work should be cited as
Scotese, C.R., 2014. Atlas of Early Cretaceous Paleogeographic Maps, PALEOMAP Atlas for ArcGIS, volume 2, The Cretaceous, Maps 23-31, Mollweide Projection, PALEOMAP Project, Evanston, IL.
Scotese, C.R., 2014. Atlas of Jurassic Paleogeographic Maps, PALEOMAP Atlas for ArcGIS, volume 3, The Jurassic and Triassic, Maps 32-42, Mollweide Projection, PALEOMAP Project, Evanston, IL. , 2014
2014.11 This Atlas of Jurassic Paleogeographic Maps shows the changing paleogeography from the He... more 2014.11 This Atlas of Jurassic Paleogeographic Maps shows the changing paleogeography from the Hettangian (198 Ma) to the Jurassic/Cretaceoous Boundary (145.5 Ma). The maps are from volume 3 of the PALEOMAP PaleoAtlas for ArcGIS (Scotese, 2014). Absolute age assignments are from Gradstein, Ogg & Smith (2008).
The following maps are included in the Atlas of Jurassic Paleogeographic Maps:
Map 32 Jurassic/Cretaceous Boundary (145.5 Ma) Berriasian Supersequence Boundary
Map 33 Late Jurassic (Tithonian, 148.2 Ma) Highstand Systems Track
Map 34 Late Jurassic (Kimmeridgian, 153.2) Maximum Flooding Surface
Map 35 Late Jurassic (Oxfordian, 158.4) Transgressive Systems Track
Map 36 Middle Jurassic (Callovian, 164.5 Ma) Transgressive Systems Tract
Map 37 Middle Jurassic (Bajocian & Bathonian, 169.7 Ma) Kimmeridgian-Oxfordian Supersequence Boundary & Maximum Flooding Surface
Map 38 Middle Jurassic (Aalenian, 173.2 Ma) Bathonian-Bajocian Supersequence Boundary
Map 39 Early Jurassic (Toarcian, 179.3 Ma) Toarcian Supersequence Boundary and Maximum Flooding Surface
Map 40 Early Jurassic (Pliensbachian, 186.3 Ma) Maximum Flooding Surface
Map 41 Early Jurassic (Sinemurian, 193 Ma) Transgressive Systems Track
Map 42 Early Jurassic (Hettangian, 198 Ma) Pliensbachian Supersequence Boundary
This work should be cited as
Scotese, C.R., 2014. Atlas of Jurassic Paleogeographic Maps, PALEOMAP Atlas for ArcGIS, volume 3, The Jurassic and Triassic, Maps 32-42, Mollweide Projection, PALEOMAP Project, Evanston, IL.
Scotese, C.R., 2014. Atlas of Middle & Late Permian and Triassic Paleogeographic Maps, Maps 43 – 52, Volumes 3 & 4, PALEOMAP PaleoAtlas for ArcGIS, PALEOMAP Project, Evanston, IL. , 2014
2014.12 This Atlas of Middle & Late Permian and Triassic Paleogeographic Maps shows the changing ... more 2014.12 This Atlas of Middle & Late Permian and Triassic Paleogeographic Maps shows the changing paleogeography from the Middle Permian (Roadian & Wordian, 268.2 Ma) to the end of the Triassic (Rhaetian, 201.6 Ma). The maps are from volumes 3 and 4 of the PALEOMAP PaleoAtlas for ArcGIS (Scotese, 2014). Absolute age assignments are from Gradstein, Ogg & Smith (2008).
The following maps are included in the Atlas of Jurassic Paleogeographic Maps:
Map 43 Late Triassic (Rhaetian, 201.6 Ma) Lowstand Systems Tract
Map 44 Late Triassic (Norian, 210 Ma) Maximum Flooding Surface
Map 45 Late Triassic (Carnian, 222.6 Ma) Transgressive Systems Tract
Map 46 Middle Triassic (Ladinian, 232.9 Ma) Transgressive Systems Tract
Map 47 Middle Triassic (Anisian, 241.5 Ma) Lowstand Systems Tract
Map 48 Early Triassic (Induan & Olenekian, 248.5 Ma) Lowstand Systems Track
Map 49 Permo-Triassic Boundary (251 Ma) Norian Supersequence Boundary
Map 50 Late Permian (Lopingian, 255.7 Ma) Transgressive Systems Tract
Map 51 late Middle Permian (Capitanian, 263.1 Ma) Lowstand Systems Tract
Map 52 Middle Permian (Roadian & Wordian, 268.2 Ma) Maximum Flooding Surface
This work should be cited as
Scotese, C.R., 2014. Atlas of Middle & Late Permian and Triassic Paleogeographic Maps, maps 43 - 48 from Volume 3 of the PALEOMAP Atlas for ArcGIS (Jurassic and Triassic) and maps 49 – 52 from Volume 4 of the PALEOMAP PaleoAtlas for ArcGIS (Late Paleozoic), Mollweide Projection, PALEOMAP Project, Evanston, IL.
Scotese, C.R., 2014. Atlas of Permo-Carboniferous Paleogeographic Maps (Mollweide Projection), Maps 53 – 64, Volumes 4, The Late Paleozoic, PALEOMAP Atlas for ArcGIS, PALEOMAP Project, Evanston, IL.
This Atlas of Permo-Carboniferous Paleogeographic Maps shows the changing paleogeography from the... more This Atlas of Permo-Carboniferous Paleogeographic Maps shows the changing paleogeography from the Early Mississippian (Tournasian, 352.3 Ma) to the Early Permian (Kungurian, 273.1 Ma). The maps are from volume 4 of the PALEOMAP PaleoAtlas for ArcGIS (Scotese, 2014). Absolute age assignments are from Gradstein, Ogg & Smith (2008).
The following maps are included in the Atlas of Permo-Carboniferous Paleogeographic Maps:
Map 53 Early Permian (Kungurian, 273.1 Ma) Highstand Systems Tract
Map 54 Early Permian (Artinskian, 280 Ma) Maximum Flooding Surface
Map 55 Early Permian (Sakmarian, 289.5 Ma) Maximum Flooding Surface
Map 56 Early Permian (Asselian, 296.8 Ma) Sakmarian Supersequence Boundary & Maximum Flooding Surface
Map 57 Late Pennsylvanian (Gzhelian, 301.2 Ma) Asselian Supersequence Boundary & Maximum Flooding Surface
Map 58 Late Pennsylvanian (Kasimovian, 305.3 Ma) Maximum Flooding Surface
Map 59 Middle Pennsylvanian (Moscovian, 309.5) Transgressive Systems Tract
Map 60 Early Pennsylvanian (Bashkirian, 314.9 Ma) Bashkirian Supersequence Boundary & Maximum Flooding Surface
Map 61 Late Mississippian (Serpukhovian, 323.2 Ma) Maximum Flooding Surface
Map 62 Middle Mississippian (late Visean, 332.5 Ma) Highstand Systems Tract
Map 63 Middle Mississippian (early Visean, 341.1 Ma) Maximum Flooding Surface
Map 64 Early Mississippian (Tournasian, 352.3 Ma) Maximum Flooding Surface
This work should be cited as
Scotese, C.R., 2014. Atlas of Permo-Carboniferous Paleogeographic Maps (Mollweide Projection), Maps 53 – 64, Volumes 4, The Late Paleozoic, PALEOMAP Atlas for ArcGIS, PALEOMAP Project, Evanston, IL.
Scotese, C.R., 2014. Atlas of Devonian Paleogeographic Maps, PALEOMAP Atlas for ArcGIS, volume 4, The Late Paleozoic, Maps 65-72, Mollweide Projection, PALEOMAP Project, Evanston, IL.
This Atlas of Devonian Paleogeographic Maps shows the changing paleogeography from the Lochkovian... more This Atlas of Devonian Paleogeographic Maps shows the changing paleogeography from the Lochkovian (413.6 Ma) to the Devono-Carboniferous Boundary (359.2 Ma). The maps are from volume 4 of the PALEOMAP PaleoAtlas for ArcGIS (Scotese, 2014). Absolute age assignments are from Gradstein, Ogg & Smith (2008). An additional map showing the disposition of the three major early Devonian faunal provinces (Malvinokaffric, Appalachian, and Rhenish-Bohemian; Cocks & Torsvik, 2002; Figure 9.) has also been included.
The following maps are included in the Atlas of Devonian Paleogeographic Maps:
Map 65 Devono-Carboniferous Boundary (359.2 Ma) Transgressive Systems Track
Map 66 Late Devonian (early Famennian, 370.3 Ma) Tournasian Supersequence Boundary
Map 67 Late Devonian (Frasnian, 379.9 Ma) Maximum Flooding Surface
Map 68 Middle Devonian (Givetian,388.2 Ma) Frasnian Supersequence Boundary
Map 69 Middle Devonian (Eifelian, 394.3 Ma) Transgressive Systems Tract
Map 70 Early Devonian (Emsian, 402.3 Ma) Maximum Flooding Surface
Map 71 Early Devonian (Pragian, 409.1 Ma) Emsian Supersequence Boundary
Map 72 Early Devonian (Lochkovian, 413.6 Ma) Lochkovian Supersequence Boundary
Extra Map – Early Devonian Biogeography
This atlas contains an “extra” map that shows the geographic distribution of three imp0ortant early Devonian biogeographic provinces: The Appalachian Province, the Rhenish-Bpohmeian Province, and the Malvino-Kaffric Province. The Appalachian and Rhenish-Bohemian provinces were populated by warm-water brachiopod faunas the occupied the subtropics. Though they inhabited the same latitudinal zones, they were separated by the Caledonian-Acadian mountain ranges. It is interesting to note that Appalachian faunas appear both in the Applachina Basin of the eastern U.S. and also in northern South America (Colombia and the Amazon Basin). Similarly, the Rhenish-Bohemian faunas are found in Northern Africa, Arabia, Central Europe, and eastern Avalonia (northern France, Belgium, and southern England). The less diverse Malvino-Kaffirc province occupied cooler latitudes closer to the South Pole.
The geographic distribution of these distinct, early Devonian faunal provices provides an important clue regarding the relative positions of Laurentia (North America), Baltic and Gondwana. Eastern North America was adjacent to northern South America (Venezuela & Colombia) and England and Central Europe were separated by a narrow ocean from northern Africa. The South Pole was located in the vicinity of southern Brazil.
This work should be cited as
Scotese, C.R., 2014. Atlas of Devonian Paleogeographic Maps, PALEOMAP Atlas for ArcGIS, volume 4, The Late Paleozoic, Maps 65-72, Mollweide Projection, PALEOMAP Project, Evanston, IL.
This Atlas of Silurian and Middle-Late Ordovician Paleogeographic Maps shows the changing paleoge... more This Atlas of Silurian and Middle-Late Ordovician Paleogeographic Maps shows the changing paleogeography from the Middle Ordovician (Darwillian, 464.5 Ma) to the Late Silurian (Ludlow & Prodoli, 419.5 Ma). The maps are from volume 5 of the PALEOMAP PaleoAtlas for ArcGIS (Scotese, 2014). Absolute age assignments are from Gradstein, Ogg & Smith (2008).
The following maps are included in the Atlas of Silurian and Middle-Late Ordovician Paleogeographic Maps:
Map 73 Late Silurian (Ludlow & Pridoli, 419.5 Ma) Lochkovian Supersequence Boundary
Map 74 Middle Silurian (Wenlock, 425.6 Ma) Highstand System Tract
Map 75 Early Silurian (late Llandovery, 432.1 Ma) Maximum Flooding Surface
Map 76 Early Silurian (early Llandovery, 439.8 Ma) Transgressive Systems Tract
Map 77 Late Ordovician (Hirnantian, 444.7 Ma) Llandoverian Supersequence Boundary
Map 78 Late Ordovician (Ashgill, 448.3 Ma) Lowstand Systems Tract & Maximum Flooding Surface
Map 79 Late Ordovician (Caradoc, 456 Ma) Maximum Flooding Surface
Map 80 Middle Ordovician (Darwillian, 464.5 Ma) Llandeilian Supersequence Boundary
This work should be cited as
Scotese, C.R., 2014. Atlas of Silurian and Middle-Late Ordovician Paleogeographic Maps (Mollweide Projection), Maps 73 – 80, Volumes 5, The Early Paleozoic, PALEOMAP Atlas for ArcGIS, PALEOMAP Project, Evanston, IL.
Scotese, C.R., 2014. Atlas of Cambrian and Early Ordovician Paleogeographic Maps (Mollweide Projection), Maps 81-88, Volumes 5, The Early Paleozoic, PALEOMAP Atlas for ArcGIS, PALEOMAP Project, Evanston, IL.
This Atlas of Cambrian and Early Ordovician Paleogeographic Maps shows the changing paleogeograph... more This Atlas of Cambrian and Early Ordovician Paleogeographic Maps shows the changing paleogeography from the base of the Cambrian (542 Ma) to the Early Ordovician (Arenig, 473.4 Ma). The maps are from volume 5 of the PALEOMAP PaleoAtlas for ArcGIS (Scotese, 2014). Absolute age assignments are from Gradstein, Ogg & Smith (2008).
The following maps are included in the Atlas of Cambrian and Early Ordovician Paleogeographic Maps:
Map 81 Early Ordovician (Arenig, 472.4 Ma) Arenigian Supersequence Boundary
Map 82 Early Ordovician (Tremadoc, 480 Ma) Maximum Flooding Surface
Map 83 Cambro-Ordovician Boundary (488.3 Ma) Tremadocian Supersequence Boundary
Map 84 Late Cambrian (Furongian, 494 Ma) Croixian Supersequence Boundary
Map 85 early Late Cambrian (510 Ma) Transgressive Systems Tract
Map 86 Middle Cambrian (520 Ma) Transgressive Systems Tract
Map 87 Early Cambrian (531.5 Ma) Albertan Supersequence Boundary
Map 88 Cambrian-Precambrian Boundary (542 Ma) Caerfaian Supersequence Boundary
This work should be cited as
Scotese, C.R., 2014. Atlas of Cambrian and Early Ordovician Paleogeographic Maps (Mollweide Projection), Maps 81-88, Volumes 5, The Early Paleozoic, PALEOMAP Atlas for ArcGIS, PALEOMAP Project, Evanston, IL.
2014.25 The Atlas of Plate Tectonic Reconstructions illustrates the plate tectonic development of... more 2014.25 The Atlas of Plate Tectonic Reconstructions illustrates the plate tectonic development of the Earth during the last 540 million years (Table 1). 28 plate tectonic reconstructions illustrate the location of active plate boundaries and the changing extent of both oceanic and continental plates (Scotese, 2014 a-f). Color-coded tectonic features include: mid ocean ridges (double red lines), continental rifts (dashed red lines), subduction zones (blue lines), continental volcanic arcs (light blue lines), collision zones (purple lines), ancient collision zones (dashed purple lines), and strike-slip faults (green lines). The Paleozoic plate tectonic reconstructions are modified from Scotese and McKerrow,1990; Scotese, 1990; Scotese,2001; and Scotese and Dammrose, 2008. The Mesozoic and Cenozoic plate tectonic reconstructions are modified from Scotese and Sager, 1988; Scotese, 1990; Scotese,2001; and Scotese and Dammrose, 2008.
Table 1. Maps for the following time intervals are included in this atlas:
Map 1 Modern World (0.0 Ma)
Map 7 Early Miocene (Aquitainian & Burdigalian, 19.5 Ma)
Map 11 late Middle Eocene (Bartonian, 38.3 Ma)
Map 15 Paleocene (Danian & Thanetian, 60.6 Ma)
Map 19 Late Cretaceous (early Campanian, 80.3 Ma)
Map 23 Early Cretaceous (late Albian, 101.8 Ma)
Map 27 Early Cretaceous (early Aptian, 121.8 Ma)
Map 31 Early Cretaceous (Berriasian, 143 Ma)
Map 35 Late Jurassic (Oxfordian, 158.4 Ma)
Map 39 Early Jurassic (Toarcian, 179.3 Ma)
Map 43 Triassic/Jurassic Boundary (199.6 Ma)
Map 45 Late Triassic (Carnian, 222.6 Ma)
Map 47 Middle Triassic (Anisian, 241.5 Ma)
Map 51 late Middle Permian (Capitanian, 263.1 Ma)
Map 54 Early Permian (Artinskian, 280 Ma)
Map 57 Late Pennsylvanian (Gzhelian, 301.2 Ma)
Map 61 Late Mississippian (Serpukhovian, 323.2 Ma)
Map 63 Middle Mississippian (early Visean, 341.1 Ma)
Map 65 Late Devonian (latest Famennian, 359.2 Ma)
Map 67 Late Devonian (Frasnian, 379.7 Ma)
Map 70 Early Devonian (Emsian, 394.3 Ma)
Map 73 Late Silurian (Ludlow & Pridoli, 419.5 Ma)
Map 77 Early Silurian (early Llandovery, 439.8 Ma)
Map 80 Middle Ordovician (Darwillian, 464.5 Ma)
Map 82 Early Ordovician (Tremadoc, 480 Ma)
Map 84 Late Cambrian (Furongian, 494 Ma)
Map 86 Middle Cambrian (520 Ma)
Map 88 Cambrian – Precambrian Boundary (542 Ma)
2014.19 The Atlas of Phanerozoic Climatic Zones plots the location of five principal climatic zon... more 2014.19 The Atlas of Phanerozoic Climatic Zones plots the location of five principal climatic zones on 28 paleogeographic maps ranging in age from early Cambrian to Miocene. The five principal climatic zones are: 1) Tropical Everwet (green shading), 2) Subtropical Arid (yellow shading), 3) Warm Temperate (yellow-green shading), 4) Cool Temperate (brown shading), and 5) Cold Polar (white shading). These five climatic zones correspond to the major Koeppen climatic zones A through E.
On several maps, an additional climatic zone, the “Boreal Tropical” zone is shown. In the Boreal Tropical climatic belt (olive green shading), tropical everwet conditions are present at anomalously high temperate latitudes (45˚ - 60˚ N and S latitudes. The Boreal Tropical Zone does not occur in today’s world. It occurs only during times when the global mean annual temperature is in excess of 18˚C (see Maps 9, 11, 13, 19, 23, 39, 43, and 45). These “Hot House” worlds are also characterized by the absence of polar ice caps.
In addition to plotting the paleoclimatic zones, the maps also show the distribution of rock types that from under specific climatic conditions. These lithologic indicators of climate, include: coals, bauxites, evaporites (salt & gypsum), calcretes, kaolinites, tillites, glendonites and dropstones (Figure 1). A complete description of each of these lithologic indicators of climate can be found in the compendium by Boucot et al., 2013. Reef localities (blue asterisks) have also been plotted on the maps (Kiessling et al., 2002).
Unlike the paleoclimatic zones in the other atlases (Scotese, 2014, a,b,c,d,e) which were based on the FOAM (Fast Ocean and Atmosphere) paleoclimatic simulations, the climatic zones plotted on these maps were drawn to conform with the distribution of these lithologic indicators of climate. The Tropical Everwet zone was mapped based on the distribution of coals and bauxites. The Subtropical Arid zone was mapped based on the distribution of evaporites and calcretes. The Warm Temperate Belt includes kaolinites, as well as coals. The Cool Temperate zone is based mostly on high latitude coals in association with tillites, glendonites, and dropstones. The Polar Cold zone is based entirely on the occurrence of tillites, glendonites, and dropstones. For a summary of the relationship between the lithologic indicators of climate and the climatic zones, see Figure 1.
The reef localities were not used to draw the climatic zones. The distribution of reefal facies, therefore, is an important, independent test of the inferred climatic zones. As expected, the reefs predominantly occur in tropics and subtropics (15˚ - 35˚, N&S). There are no reefs above 45˚ N&S latitude. Most of the reefs occur in the Subtropical Dry zone where it is both warm and sunny, and where there are fewer river deltas and other sources of clastics that might inhibit reef growth.
This work should be cited as
Scotese, C.R., Boucot, A.J, and Chen Xu, 2014. Atlas of Phanerozoic Climatic Zones (Mollweide Projection), Volumes 1-6, PALEOMAP Project PaleoAtlas for ArcGIS, PALEOMAP Project, Evanston, IL.
References Cited:
Boucot, A.J., Chen Xu, and Scotese, C.R, 2013. Phanerozoic Paleoclimate: An Atlas of LithologicIndicators of Climate, SEPM Concepts in Sedimentology and Paleontology, (Print-on-Demand Version), No. 11, 478 pp., ISBN 978-1-56576-289-3, October 2013, Society for Sedimentary Geology, Tulsa, OK.
Kiessling, W., Flügel, E., and Golonka, J., (editors) 2002. Phanerozoic Reef Patterns, SEPM (Society for Sedimentary Geology), Special Publications, 775 pp.
Scotese, C.R., 2014a, The PALEOMAP Project PaleoAtlas for ArcGIS, version 2, Volume 1, Cenozoic Plate Tectonic, Paleogeographic, and Paleoclimatic Reconstructions, Maps 1-15, PALEOMAP Project, Evanston, IL.
Scotese, C.R., 2014b, The PALEOMAP Project PaleoAtlas for ArcGIS, version 2, Volume 2, Cretaceous Plate Tectonic, Paleogeographic, and Paleoclimatic Reconstructions, Maps 16-32, PALEOMAP Project, Evanston, IL.
Scotese, C.R., 2014c, The PALEOMAP Project PaleoAtlas for ArcGIS, version 2, Volume 3, Triassic and Jurassic Plate Tectonic, Paleogeographic, and Paleoclimatic Reconstructions, Map 33-48, PALEOMAP Project, Evanston, IL.
Scotese, C.R., 2014d, The PALEOMAP Project PaleoAtlas for ArcGIS, version 2, Volume 4, Late Paleozoic Plate Tectonic, Paleogeographic, and Paleoclimatic Reconstructions, Map 49-74, PALEOMAP Project, Evanston, IL.
Scotese, C.R., 2014e, The PALEOMAP Project PaleoAtlas for ArcGIS, version 2, Volume 5, Early Paleozoic Plate Tectonic, Paleogeographic, and Paleoclimatic Reconstructions, Maps 75-88, PALEOMAP Project, Evanston, IL.
Scotese, C.R., 2014f, The PALEOMAP Project PaleoAtlas for ArcGIS, version 2, Volume 6, Precambrian Plate Tectonic, Paleogeographic, and Paleoclimatic Reconstructions, Maps 89-103, PALEOMAP Project, Evanston, IL.
2014.21 This Atlas of Phanerozoic Rainfall shows the pattern of mean annual rainfall for 22 time ... more 2014.21 This Atlas of Phanerozoic Rainfall shows the pattern of mean annual rainfall for 22 time periods from the base of the Cambrian (542 Ma) to the Middle/Late Miocene (Serravallian & Tortonian, 10.5 Ma), plus one additional map for the Neoproterozoic (Middle Ediacaran, 600 Ma). The light blue squares indicate the amount of rainfall. The areas shaded in green on the maps are regions where precipitation exceeds evaporation (P > E). The land areas in brown and tan on the map are regions where evaporation exceeds precipitation (E > P).
These plate tectonic and paleogeographic maps are the work of C. R. Scotese. The paleoclimate simulations were done by T.L. Moore using the FOAM (Fast Ocean and Atmosphere) Climate Simulation Program. The slight color differences between the symbolson the maps are due to the fact that the maps were made for four separate reports (Scotese et al., 2007; 2008; 2009; & 2011).
Some interesting patterns are apparent on all the maps. On the continents, Equatorial Everwet Belt generally spans latitudes, 15N – 15S. The Temperate wet belt is more variable, but generally spans the latitudes 45 – 75(N & S). In the oceans there are often noticeable gaps in precipitation apparent along the Equator and along the western sides of continents in the southern hemisphere. These gaps in precipitation are due to the chilling effect of oceanic upwelling, which reduces evaporation, and hence decreases precipitation.
The maps are from volumes 1-6 of the PALEOMAP PaleoAtlas for ArcGIS (Scotese, 2014a,b,c,d). Absolute age assignments are from Gradstein, Ogg & Smith (2008).
The following maps are included in the Atlas of Phanerozoic Rainfall:
Map 5 Middle/Late Miocene (Serravallian & Tortonian, 10.5 Ma)
Map 7 Early Miocene (Aquitainian & Burdigalian, 19.5 Ma)
Map 9 Early Oligocene (Rupelian, 31.1 Ma)
Map 12 early Middle Eocene (middle Lutetian, 44.6 Ma)
Map 17 Late Cretaceous (Maastrichtian, 68 Ma)
Map 21 Mid-Cretaceous (Turonian, 91.1 Ma)
Map 23 Early Cretaceous (late Albian, 101.8 Ma)
Map 27 Early Cretaceous (early Aptian, 121.8 Ma)
Map 31 Early Cretaceous (Berriasian, 143 Ma)
Map 35 Late Jurassic (Oxfordian, 158.4 Ma)
Map 39 Early Jurassic (Toarcian, 179.3 Ma)
Map 45 Late Triassic (Carnian, 222.6 Ma)
Map 49 Permo-Triassic Boundary (251 Ma)
Map 54 Early Permian (Artinskian, 280 Ma)
Map 57 Late Pennsylvanian (Gzhelian, 301.2 Ma)
Map 63 Middle Mississippian (early Visean, 341.1 Ma)
Map 65 Late Devonian (latest Famennian, 359.2 Ma)
Map 70 Early Devonian (Emsian, 394.3 Ma)
Map 75 Early Silurian (late Llandovery, 432.1 Ma)
Map 82 Tremadoc (480 Ma)
Map 88 Cambrian – Precambrian Boundary (542 Ma)
Map 90 Late Neoproterozoic (Middle Ediacaran, 600 Ma)
This work should be cited as
Scotese, C.R. and Moore, T.L., 2014. Atlas of Phanerozoic Rainfall(Mollweide Projection), Volumes 1-6, PALEOMAP Project PaleoAtlas for ArcGIS, PALEOMAP Project, Evanston, IL.
References Cited:
Scotese, C.R., Illich, H., Zumberge, J, and Brown, S., and Moore, T., 2007. The GANDOLPH Project: Year One Report: Paleogeographic and Paleoclimatic Controls on Hydrocarbon Source Rock Deposition, A Report on the Methods Employed, the Results of the Paleoclimate Simulations (FOAM), and Oils/Source Rock Compilation, Conclusions at the End of Year One: Cenomanian/Turonian (93.5 Ma), Kimmeridgian/Tithonian (151 Ma), Sakmarian/Artinskian (284 Ma), Frasnian/Famennian (375 Ma), February, 2007. GeoMark Research Ltd, Houston, Texas, 142 pp.
Scotese, C.R., Illich, H., Zumberge, J, and Brown, S., and Moore, T., 2008. The GANDOLPH Project: Year Two Report: Paleogeographic and Paleoclimatic Controls on Hydrocarbon Source Rock Deposition, A Report on the Methods Employed, the Results of the Paleoclimate Simulations (FOAM), and Oils/Source Rock Compilation, Conclusions at the End of Year Two: Miocene (10Ma), Aptian/Albian (120 Ma), Berriasian/Barremian (140 Ma), Late Triassic (220 Ma), and Early Silurian (430 Ma), July, 2008. GeoMark Research Ltd, Houston, Texas, 177 pp.
Scotese, C.R., Illich, H., Zumberge, J, and Brown, S., and Moore, T., 2009. The GANDOLPH Project: Year Three Report: Paleogeographic and Paleoclimatic Controls on Hydrocarbon Source Rock Deposition, A report on the Results of the Paleogeographic, Paleoclimatic Simulations (FOAM), and Oils/Source Rock Compilation, Conclusions at the End of Year Three: Eocene (45Ma), Early/Middle Jurassic (180 Ma), Mississippian (340 Ma), Neoproterozoic (600 Ma), August 2009. GeoMark Research Ltd, Houston, Texas, 154 pp.
Scotese, C.R., Illich, H., Zumberge, J, and Brown, S., and Moore, T., 2011. The GANDOLPH Project: Year Four Report: Paleogeographic and Paleoclimatic Controls on Hydrocarbon Source Rock Deposition, A report on the Results of the Paleogeographic, Paleoclimatic Simulations (FOAM), and Oils/Source Rock Compilation, Conclusions at the End of Year Four: Oligocene (30 Ma), Cretaceous/Tertiary (70 Ma), Permian/Triassic (250 Ma), Silurian/Devonian (400 Ma), Cambrian/Ordovician (480 Ma), April, 2011. GeoMark Research Ltd, Houston, Texas, 219 pp.
Scotese, C.R., 2014a, The PALEOMAP Project PaleoAtlas for ArcGIS, version 2, Volume 1, Cenozoic Plate Tectonic, Paleogeographic, and Paleoclimatic Reconstructions, Maps 1-15, PALEOMAP Project, Evanston, IL.
Scotese, C.R., 2014b, The PALEOMAP Project PaleoAtlas for ArcGIS, version 2, Volume 2, Cretaceous Plate Tectonic, Paleogeographic, and Paleoclimatic Reconstructions, Maps 16-32, PALEOMAP Project, Evanston, IL.
Scotese, C.R., 2014c, The PALEOMAP Project PaleoAtlas for ArcGIS, version 2, Volume 3, Triassic and Jurassic Plate Tectonic, Paleogeographic, and Paleoclimatic Reconstructions, Map 33-48, PALEOMAP Project, Evanston, IL.
Scotese, C.R., 2014d, The PALEOMAP Project PaleoAtlas for ArcGIS, version 2, Volume 4, Late Paleozoic Plate Tectonic, Paleogeographic, and Paleoclimatic Reconstructions, Map 49-74, PALEOMAP Project, Evanston, IL.
Scotese, C.R., 2014e, The PALEOMAP Project PaleoAtlas for ArcGIS, version 2, Volume 5, Early Paleozoic Plate Tectonic, Paleogeographic, and Paleoclimatic Reconstructions, Maps 75-88, PALEOMAP Project, Evanston, IL.
Scotese, C.R., 2014f, The PALEOMAP Project PaleoAtlas for ArcGIS, version 2, Volume 6, Precambrian Plate Tectonic, Paleogeographic, and Paleoclimatic Reconstructions, Maps 89-103, PALEOMAP Project, Evanston, IL.
2014.20 This Atlas of Phanerozoic Temperatures shows the pattern of global temperatures for the s... more 2014.20 This Atlas of Phanerozoic Temperatures shows the pattern of global temperatures for the summer months (northern hemisphere) for 22 time periods from the base of the Cambrian (542 Ma) to the Middle/Late Miocene (Serravallian & Tortonian, 10.5 Ma), plus one additional map for the Neoproterozoic (Middle Ediacaran, 600 Ma). Warmer temepratures are shown in shades of red; cooler temperatures are shown in shades of blue. The dashed lines represent isotherms of equal temperature and are often labeled with the temperature in degrees Centigrade.
As expected isotherms are generally parallel to lines of latitude, except in a few regions where land areas are either warmer or cooler than the surrounding marine waters. On all of the maps the blue colors near the south pole represent winter conditions in the southern hemisphere. In the next version of this Atlas maps illustrating the temperature during the northern hemisphere summer, northern hemisphere winter, and mean annual temperature (MAT) will be provided.
These plate tectonic and paleogeographic maps are the work of C. R. Scotese. The paleoclimate simulations were done by T.L. Moore using the FOAM (Fast Ocean and Atmosphere) Climate Simulation Program. The differences in color and symbology from map to map are due to the fact that these figures were originally published in four separate reports (Scotese et al., 2007; 2008; 2009; & 2011).
Though there are minor differences in coloration due to the version of the maps, it is remarkable how similar, overall, the maps are. This is presumably because the basic physics that controls atmospheric temperature has not changed very much in the past 600 million years. The atmosphere receives it energy from the Sun. This energy is modulated by several factors: the shape of the Earth’s orbit and the tilt (obliquity) of the Earth’s axis, the reflectivity or albedo of the surface of the Earth, the presence or absence of polar ice caps, and the amount of greenhouse gases in the Earth’s atmosphere.
The FOAM simulation program has variables that represent these temperature-modifying factors. Though these variables were adjusted to represent prevailing conditions for each simulation, it is remarkable how little effect these adjustments made. Table 1 lists the global mean annual temperature (MAT) for 12 times intervals back to the early Ordovician. The global mean temperature during the last glacial maximum (12 C˚; 21,000 years ago), and the global mean temperature for the modern world (about 14 C˚) have also been included.
Though mean global temperature does vary from time to time, there is little difference between the MAT of the modern world and the MAT of the warmest time (Early Cretaceous, 18.4 C˚; 4.4 degrees difference), or the MAT of the modern world and the MAT of the coolest time (Early Ordovician, 10.6 C˚; 3.4 degrees difference). Most of the simulated mean annual temperaturres are within 2.5 degrees of the modern value. Why is this?
The most likely reason why simulated past temperatures are nearly identical to modern temperatures is that the FOAM climate simulation was written to reproduce the patterns of today’s climate. If the results of the FOAM model did not closely resemble the modern climate, then there would be little confidence in the climate simulation. Unfortunately, FOAM, as well as all other General Circulation Models, do too good a job! Even when past geographic configurations, changes in land surface cover, or radical changes the abundance of atmospheric greenhouse gases are taken into account, the results still look a lot like the present-day.
Table I. Global Mean Atmospheric Temperatures (MAT)
Geologic Age MAT (Mean Annual Temperature) C˚
Present-day 14.0 C˚
21,000 years ago 12.0 C˚
30 Ma Oligocene 12.8 C˚
45 Ma mid Eocene 13.9 C˚
70 Ma Late Cretaceous 16.2 C˚
90 Ma Mid Cretaceous 17.3 C˚
120 Ma Early Cretaceous 18.4 C˚
140 Ma earliest Cretaceous 13.6 C˚
160 Ma Late Jurassic 14.2 C˚
250 Ma Permo Triassic 11.5 C˚
430 Ma Early Silurian 16.7 C˚
480 Ma Early Ordovician 10.6 C˚
The maps are from volumes 1-6 of the PALEOMAP PaleoAtlas for ArcGIS (Scotese, 2014a,b,c,d). Absolute age assignments are from Gradstein, Ogg & Smith (2008).
The following maps are included in the Atlas of Phanerozoic Temperatures:
Map 5 Middle/Late Miocene (Serravallian & Tortonian, 10.5 Ma)
Map 7 Early Miocene (Aquitainian & Burdigalian, 19.5 Ma)
Map 9 Early Oligocene (Rupelian, 31.1 Ma)
Map 12 early Middle Eocene (middle Lutetian, 44.6 Ma)
Map 17 Late Cretaceous (Maastrichtian, 68 Ma)
Map 21 Mid-Cretaceous (Turonian, 91.1 Ma)
Map 23 Early Cretaceous (late Albian, 101.8 Ma)
Map 27 Early Cretaceous (early Aptian, 121.8 Ma)
Map 31 Early Cretaceous (Berriasian, 143 Ma)
Map 35 Late Jurassic (Oxfordian, 158.4 Ma)
Map 39 Early Jurassic (Toarcian, 179.3 Ma)
Map 45 Late Triassic (Carnian, 222.6 Ma)
Map 49 Permo-Triassic Boundary (251 Ma)
Map 54 Early Permian (Artinskian, 280 Ma)
Map 57 Late Pennsylvanian (Gzhelian, 301.2 Ma)
Map 63 Middle Mississippian (early Visean, 341.1 Ma)
Map 65 Late Devonian (latest Famennian, 359.2 Ma)
Map 70 Early Devonian (Emsian, 394.3 Ma)
Map 75 Early Silurian (late Llandovery, 432.1 Ma)
Map 82 Early Ordovician (Tremadoc, 480 Ma)
Map 88 Cambrian – Precambrian Boundary (542 Ma)
Map 90 Late Neoproterozoic (Middle Ediacaran, 600 Ma)
This work should be cited as
Scotese, C.R., and Moore, T.L., 2014. Atlas of Phanerozoic Temperatures (Mollweide Projection), Volumes 1-6, PALEOMAP Project PaleoAtlas for ArcGIS, PALEOMAP Project, Evanston, IL.
References Cited:
Scotese, C.R., Illich, H., Zumberge, J, and Brown, S., and Moore, T., 2007. The GANDOLPH Project: Year One Report: Paleogeographic and Paleoclimatic Controls on Hydrocarbon Source Rock Deposition, A Report on the Methods Employed, the Results of the Paleoclimate Simulations (FOAM), and Oils/Source Rock Compilation, Conclusions at the End of Year One: Cenomanian/Turonian (93.5 Ma), Kimmeridgian/Tithonian (151 Ma), Sakmarian/Artinskian (284 Ma), Frasnian/Famennian (375 Ma), February, 2007. GeoMark Research Ltd, Houston, Texas, 142 pp.
Scotese, C.R., Illich, H., Zumberge, J, and Brown, S., and Moore, T., 2008. The GANDOLPH Project: Year Two Report: Paleogeographic and Paleoclimatic Controls on Hydrocarbon Source Rock Deposition, A Report on the Methods Employed, the Results of the Paleoclimate Simulations (FOAM), and Oils/Source Rock Compilation, Conclusions at the End of Year Two: Miocene (10Ma), Aptian/Albian (120 Ma), Berriasian/Barremian (140 Ma), Late Triassic (220 Ma), and Early Silurian (430 Ma), July, 2008. GeoMark Research Ltd, Houston, Texas, 177 pp.
Scotese, C.R., Illich, H., Zumberge, J, and Brown, S., and Moore, T., 2009. The GANDOLPH Project: Year Three Report: Paleogeographic and Paleoclimatic Controls on Hydrocarbon Source Rock Deposition, A report on the Results of the Paleogeographic, Paleoclimatic Simulations (FOAM), and Oils/Source Rock Compilation, Conclusions at the End of Year Three: Eocene (45Ma), Early/Middle Jurassic (180 Ma), Mississippian (340 Ma), Neoproterozoic (600 Ma), August 2009. GeoMark Research Ltd, Houston, Texas, 154 pp.
Scotese, C.R., Illich, H., Zumberge, J, and Brown, S., and Moore, T., 2011. The GANDOLPH Project: Year Four Report: Paleogeographic and Paleoclimatic Controls on Hydrocarbon Source Rock Deposition, A report on the Results of the Paleogeographic, Paleoclimatic Simulations (FOAM), and Oils/Source Rock Compilation, Conclusions at the End of Year Four: Oligocene (30 Ma), Cretaceous/Tertiary (70 Ma), Permian/Triassic (250 Ma), Silurian/Devonian (400 Ma), Cambrian/Ordovician (480 Ma), April, 2011. GeoMark Research Ltd, Houston, Texas, 219 pp.
Scotese, C.R., 2014a, The PALEOMAP Project PaleoAtlas for ArcGIS, version 2, Volume 1, Cenozoic Plate Tectonic, Paleogeographic, and Paleoclimatic Reconstructions, Maps 1-15, PALEOMAP Project, Evanston, IL.
Scotese, C.R., 2014b, The PALEOMAP Project PaleoAtlas for ArcGIS, version 2, Volume 2, Cretaceous Plate Tectonic, Paleogeographic, and Paleoclimatic Reconstructions, Maps 16-32, PALEOMAP Project, Evanston, IL.
Scotese, C.R., 2014c, The PALEOMAP Project PaleoAtlas for ArcGIS, version 2, Volume 3, Triassic and Jurassic Plate Tectonic, Paleogeographic, and Paleoclimatic Reconstructions, Map 33-48, PALEOMAP Project, Evanston, IL.
Scotese, C.R., 2014d, The PALEOMAP Project PaleoAtlas for ArcGIS, version 2, Volume 4, Late Paleozoic Plate Tectonic, Paleogeographic, and Paleoclimatic Reconstructions, Map 49-74, PALEOMAP Project, Evanston, IL.
Scotese, C.R., 2014e, The PALEOMAP Project PaleoAtlas for ArcGIS, version 2, Volume 5, Early Paleozoic Plate Tectonic, Paleogeographic, and Paleoclimatic Reconstructions, Maps 75-88, PALEOMAP Project, Evanston, IL.
Scotese, C.R., 2014f, The PALEOMAP Project PaleoAtlas for ArcGIS, version 2, Volume 6, Precambrian Plate Tectonic, Paleogeographic, and Paleoclimatic Reconstructions, Maps 89-103, PALEOMAP Project, Evanston, IL.
2014.22 This Atlas of Phanerozoic Ocean Currents and Salinity shows the patterns of surface ocean... more 2014.22 This Atlas of Phanerozoic Ocean Currents and Salinity shows the patterns of surface ocean currents and salinity for 22 time periods from the base of the Cambrian (542 Ma) to the Middle/Late Miocene (Serravallian & Tortonian, 10.5 Ma), plus one additional map for the Neoproterozoic (Middle Ediacaran, 600 Ma). Regions of high salinity are shown in red. Regions of low salinity and brackish conditions are shown in blue. Blue arrows indicate the direction of surface ocean currents during the winter months (December – January – February).
These plate tectonic and paleogeographic maps are the work of C. R. Scotese. The paleoclimate simulations were done by T.L. Moore using the FOAM (Fast Ocean and Atmosphere) Climate Simulation Program. The differences in color and symbology are due to the fact that the maps were originally published in four separate reports (Scotese et al., 2007; 2008; 2009; & 2011).
There are some patterns of salinity and ocean currents are illustrated by the maps. Areas of hypersalinity occur in both the north and south subtropical belts (15 – 35 degrees latitude). Hyposaline ocean waters, by contrast, tend to be located along the Equator and at temperate and polar latitudes. Salinity is also reduced along the many continental coastlines where freshwater from rivers enters the oceans. The broad shallow, epieric seas of the Paleozoic appear to have been susceptible to salinity extremes depending on the latitude of the continent and the proximity to runoff from adjacent land areas.
The pattern of surface ocean currents in the open ocean is largely zonal, following the prevailing winds. The currents move from east to west near the Equator, whereas at temperate latitudes the currents generally move eastwards. As in the modern world, these zonal surface currents are deflected N or S, depending on latitude, where they run into the continents. In the open ocean between these two zonal patterns of flow, large gyres are often present. These gyres rotate clockwise in the northern hemisphere and counter-clockwise in the southern hemisphere. It is interesting to note that in a few cases (Maps 35 & 63), the surface currents in large inland seas move in a unidirectional pattern. This is due to the fact that upwelling across long one shore of the inland sea and the currents move across the shallow and dive back down into the ocean in an “down-welling” zone adjacent to the opposite shore.
A complimentary set of surface ocean currents for the summer months (July-August-September) are plotted in the Atlas of Phanerozoic Oceanic Anoxia. Though similar to the results shown here, there are maps that show opposite flow directions due to monsoonal changes in wind directions.
The maps are from volumes 1-6 of the PALEOMAP PaleoAtlas for ArcGIS (Scotese, 2014a,b,c,d). Absolute age assignments are from Gradstein, Ogg & Smith (2008).
The following maps are included in the Atlas of Phanerozoic Ocean Currents and Salinity:
Map 5 Middle/Late Miocene (Serravallian & Tortonian, 10.5 Ma)
Map 7 Early Miocene (Aquitainian & Burdigalian, 19.5 Ma)
Map 9 Early Oligocene (Rupelian, 31.1 Ma)
Map 12 early Middle Eocene (middle Lutetian, 44.6 Ma)
Map 17 Late Cretaceous (Maastrichtian, 68 Ma)
Map 21 Mid-Cretaceous (Turonian, 91.1 Ma)
Map 23 Early Cretaceous (late Albian, 101.8 Ma)
Map 27 Early Cretaceous (early Aptian, 121.8 Ma)
Map 31 Early Cretaceous (Berriasian, 143 Ma)
Map 35 Late Jurassic (Oxfordian, 158.4 Ma)
Map 39 Early Jurassic (Toarcian, 179.3 Ma)
Map 45 Late Triassic (Carnian, 222.6 Ma)
Map 49 Permo-Triassic Boundary (251 Ma)
Map 54 Early Permian (Artinskian, 280 Ma)
Map 57 Late Pennsylvanian (Gzhelian, 301.2 Ma)
Map 63 Middle Mississippian (early Visean, 341.1 Ma)
Map 65 Late Devonian (latest Famennian, 359.2 Ma)
Map 70 Early Devonian (Emsian, 394.3 Ma)
Map 75 Early Silurian (late Llandovery, 432.1 Ma)
Map 82 Early Ordovician (Tremadoc, 480 Ma)
Map 88 Cambrian – Precambrian Boundary (542 Ma)
Map 90 Late Neoproterozoic (Middle Ediacaran, 600 Ma)
This work should be cited as
Scotese, C.R., and Moore, T.L., 2014. Atlas of Phanerozoic Ocean Currents and Salinity (Mollweide Projection), Volumes 1-6, PALEOMAP Project PaleoAtlas for ArcGIS, PALEOMAP Project, Evanston, IL.
References Cited:
Scotese, C.R., Illich, H., Zumberge, J, and Brown, S., and Moore, T., 2007. The GANDOLPH Project: Year One Report: Paleogeographic and Paleoclimatic Controls on Hydrocarbon Source Rock Deposition, A Report on the Methods Employed, the Results of the Paleoclimate Simulations (FOAM), and Oils/Source Rock Compilation, Conclusions at the End of Year One: Cenomanian/Turonian (93.5 Ma), Kimmeridgian/Tithonian (151 Ma), Sakmarian/Artinskian (284 Ma), Frasnian/Famennian (375 Ma), February, 2007. GeoMark Research Ltd, Houston, Texas, 142 pp.
Scotese, C.R., Illich, H., Zumberge, J, and Brown, S., and Moore, T., 2008. The GANDOLPH Project: Year Two Report: Paleogeographic and Paleoclimatic Controls on Hydrocarbon Source Rock Deposition, A Report on the Methods Employed, the Results of the Paleoclimate Simulations (FOAM), and Oils/Source Rock Compilation, Conclusions at the End of Year Two: Miocene (10Ma), Aptian/Albian (120 Ma), Berriasian/Barremian (140 Ma), Late Triassic (220 Ma), and Early Silurian (430 Ma), July, 2008. GeoMark Research Ltd, Houston, Texas, 177 pp.
Scotese, C.R., Illich, H., Zumberge, J, and Brown, S., and Moore, T., 2009. The GANDOLPH Project: Year Three Report: Paleogeographic and Paleoclimatic Controls on Hydrocarbon Source Rock Deposition, A report on the Results of the Paleogeographic, Paleoclimatic Simulations (FOAM), and Oils/Source Rock Compilation, Conclusions at the End of Year Three: Eocene (45Ma), Early/Middle Jurassic (180 Ma), Mississippian (340 Ma), Neoproterozoic (600 Ma), August 2009. GeoMark Research Ltd, Houston, Texas, 154 pp.
Scotese, C.R., Illich, H., Zumberge, J, and Brown, S., and Moore, T., 2011. The GANDOLPH Project: Year Four Report: Paleogeographic and Paleoclimatic Controls on Hydrocarbon Source Rock Deposition, A report on the Results of the Paleogeographic, Paleoclimatic Simulations (FOAM), and Oils/Source Rock Compilation, Conclusions at the End of Year Four: Oligocene (30 Ma), Cretaceous/Tertiary (70 Ma), Permian/Triassic (250 Ma), Silurian/Devonian (400 Ma), Cambrian/Ordovician (480 Ma), April, 2011. GeoMark Research Ltd, Houston, Texas, 219 pp.
Scotese, C.R., 2014a, The PALEOMAP Project PaleoAtlas for ArcGIS, version 2, Volume 1, Cenozoic Plate Tectonic, Paleogeographic, and Paleoclimatic Reconstructions, Maps 1-15, PALEOMAP Project, Evanston, IL.
Scotese, C.R., 2014b, The PALEOMAP Project PaleoAtlas for ArcGIS, version 2, Volume 2, Cretaceous Plate Tectonic, Paleogeographic, and Paleoclimatic Reconstructions, Maps 16-32, PALEOMAP Project, Evanston, IL.
Scotese, C.R., 2014c, The PALEOMAP Project PaleoAtlas for ArcGIS, version 2, Volume 3, Triassic and Jurassic Plate Tectonic, Paleogeographic, and Paleoclimatic Reconstructions, Map 33-48, PALEOMAP Project, Evanston, IL.
Scotese, C.R., 2014d, The PALEOMAP Project PaleoAtlas for ArcGIS, version 2, Volume 4, Late Paleozoic Plate Tectonic, Paleogeographic, and Paleoclimatic Reconstructions, Map 49-74, PALEOMAP Project, Evanston, IL.
Scotese, C.R., 2014e, The PALEOMAP Project PaleoAtlas for ArcGIS, version 2, Volume 5, Early Paleozoic Plate Tectonic, Paleogeographic, and Paleoclimatic Reconstructions, Maps 75-88, PALEOMAP Project, Evanston, IL.
Scotese, C.R., 2014f, The PALEOMAP Project PaleoAtlas for ArcGIS, version 2, Volume 6, Precambrian Plate Tectonic, Paleogeographic, and Paleoclimatic Reconstructions, Maps 89-103, PALEOMAP Project, Evanston, IL.
2014.24 This Atlas of Phanerozoic Upwelling Zones shows the pattern of marine upwelling for 22 ti... more 2014.24 This Atlas of Phanerozoic Upwelling Zones shows the pattern of marine upwelling for 22 time periods from the base of the Cambrian (542 Ma) to the Middle/Late Miocene (Serravallian & Tortonian, 10.5 Ma), plus one additional map for the Neoproterozoic (Middle Ediacaran, 600 Ma). The light blue shading represents areas of upwelling. The blue circles indicate the strength and persistence of the upwelling systems.
These plate tectonic and paleogeographic maps are the work of C. R. Scotese. The paleoclimate simulations were done by T.L. Moore using the FOAM (Fast Ocean and Atmosphere) Climate Simulation Program. The slight color differences between the symbolson the maps are due to the fact that the maps were made for four separate reports (Scotese et al., 2007; 2008; 2009; & 2011).
There are some notable patterns of upwelling illustrated by the maps. A strong upwelling system is always present along the Equator and along the west coasts of continents in the southern hemisphere and to a lesser extent along the east coasts of continents in the northern hemisphere. In addition, moderate zonal upwelling systems are present in temperate latitudes at 45 – 60 degrees (N&S). Broad regions of oceanic ‘downwelling’, are found in the northern and southern subtropics (23 – 40 degrees, N&S) and in the polar regions. The polar downwelling zones generate cold bottom-water that chills the oceans during times when the Earth has polar icecaps.
The location of ancient upwelling systems is also a good predictor of world-class source rock deposits. This is especially true for times when continents, covered by shallow seas, cross the Equator. Extremely rich source rock deposits occur along the eastern edge of the Arabian platform because this area was located beneath the Western Tethys Equatorial Upwelling System for nearly 100 million years (mid-Triassic to mid-Cretaceous). Rich source rock deposits were similarly deposited in Venezuela and Colombia when the vigorous westward moving Equatorial Current crossed the northernmost part of South America (Cretaceous, Maps 27-17).
The maps are from volumes 1-6 of the PALEOMAP PaleoAtlas for ArcGIS (Scotese, 2014a,b,c,d). Absolute age assignments are from Gradstein, Ogg & Smith (2008).
The following maps are included in the Atlas of Phanerozoic Upwelling Zones:
Map 5 Middle/Late Miocene (Serravallian & Tortonian, 10.5 Ma)
Map 7 Early Miocene (Aquitainian & Burdigalian, 19.5 Ma)
Map 9 Early Oligocene (Rupelian, 31.1 Ma)
Map 12 early Middle Eocene (middle Lutetian, 44.6 Ma)
Map 17 Late Cretaceous (Maastrichtian, 68 Ma)
Map 21 Mid-Cretaceous (Turonian, 91.1 Ma)
Map 23 Early Cretaceous (late Albian, 101.8 Ma)
Map 27 Early Cretaceous (early Aptian, 121.8 Ma)
Map 31 Early Cretaceous (Berriasian, 143 Ma)
Map 35 Late Jurassic (Oxfordian, 158.4 Ma)
Map 39 Early Jurassic (Toarcian, 179.3 Ma)
Map 45 Late Triassic (Carnian, 222.6 Ma)
Map 49 Permo-Triassic Boundary (251 Ma)
Map 54 Early Permian (Artinskian, 280 Ma)
Map 57 Late Pennsylvanian (Gzhelian, 301.2 Ma)
Map 63 Middle Mississippian (early Visean, 341.1 Ma)
Map 65 Late Devonian (latest Famennian, 359.2 Ma)
Map 70 Early Devonian (Emsian, 394.3 Ma)
Map 75 Early Silurian (late Llandovery, 432.1 Ma)
Map 82 Tremadoc (480 Ma)
Map 88 Cambrian – Precambrian Boundary (542 Ma)
Map 90 Late Neoproterozoic (Middle Ediacaran, 600 Ma)
This work should be cited as
Scotese, C.R., and Moore, T.L., 2014. Atlas of Phanerozoic Upwelling Zones (Mollweide Projection), Volumes 1-6, PALEOMAP Project PaleoAtlas for ArcGIS, PALEOMAP Project, Evanston, IL.
References Cited:
Scotese, C.R., Illich, H., Zumberge, J, and Brown, S., and Moore, T., 2007. The GANDOLPH Project: Year One Report: Paleogeographic and Paleoclimatic Controls on Hydrocarbon Source Rock Deposition, A Report on the Methods Employed, the Results of the Paleoclimate Simulations (FOAM), and Oils/Source Rock Compilation, Conclusions at the End of Year One: Cenomanian/Turonian (93.5 Ma), Kimmeridgian/Tithonian (151 Ma), Sakmarian/Artinskian (284 Ma), Frasnian/Famennian (375 Ma), February, 2007. GeoMark Research Ltd, Houston, Texas, 142 pp.
Scotese, C.R., Illich, H., Zumberge, J, and Brown, S., and Moore, T., 2008. The GANDOLPH Project: Year Two Report: Paleogeographic and Paleoclimatic Controls on Hydrocarbon Source Rock Deposition, A Report on the Methods Employed, the Results of the Paleoclimate Simulations (FOAM), and Oils/Source Rock Compilation, Conclusions at the End of Year Two: Miocene (10Ma), Aptian/Albian (120 Ma), Berriasian/Barremian (140 Ma), Late Triassic (220 Ma), and Early Silurian (430 Ma), July, 2008. GeoMark Research Ltd, Houston, Texas, 177 pp.
Scotese, C.R., Illich, H., Zumberge, J, and Brown, S., and Moore, T., 2009. The GANDOLPH Project: Year Three Report: Paleogeographic and Paleoclimatic Controls on Hydrocarbon Source Rock Deposition, A report on the Results of the Paleogeographic, Paleoclimatic Simulations (FOAM), and Oils/Source Rock Compilation, Conclusions at the End of Year Three: Eocene (45Ma), Early/Middle Jurassic (180 Ma), Mississippian (340 Ma), Neoproterozoic (600 Ma), August 2009. GeoMark Research Ltd, Houston, Texas, 154 pp.
Scotese, C.R., Illich, H., Zumberge, J, and Brown, S., and Moore, T., 2011. The GANDOLPH Project: Year Four Report: Paleogeographic and Paleoclimatic Controls on Hydrocarbon Source Rock Deposition, A report on the Results of the Paleogeographic, Paleoclimatic Simulations (FOAM), and Oils/Source Rock Compilation, Conclusions at the End of Year Four: Oligocene (30 Ma), Cretaceous/Tertiary (70 Ma), Permian/Triassic (250 Ma), Silurian/Devonian (400 Ma), Cambrian/Ordovician (480 Ma), April, 2011. GeoMark Research Ltd, Houston, Texas, 219 pp.
Scotese, C.R., 2014a, The PALEOMAP Project PaleoAtlas for ArcGIS, version 2, Volume 1, Cenozoic Plate Tectonic, Paleogeographic, and Paleoclimatic Reconstructions, Maps 1-15, PALEOMAP Project, Evanston, IL.
Scotese, C.R., 2014b, The PALEOMAP Project PaleoAtlas for ArcGIS, version 2, Volume 2, Cretaceous Plate Tectonic, Paleogeographic, and Paleoclimatic Reconstructions, Maps 16-32, PALEOMAP Project, Evanston, IL.
Scotese, C.R., 2014c, The PALEOMAP Project PaleoAtlas for ArcGIS, version 2, Volume 3, Triassic and Jurassic Plate Tectonic, Paleogeographic, and Paleoclimatic Reconstructions, Map 33-48, PALEOMAP Project, Evanston, IL.
Scotese, C.R., 2014d, The PALEOMAP Project PaleoAtlas for ArcGIS, version 2, Volume 4, Late Paleozoic Plate Tectonic, Paleogeographic, and Paleoclimatic Reconstructions, Map 49-74, PALEOMAP Project, Evanston, IL.
Scotese, C.R., 2014e, The PALEOMAP Project PaleoAtlas for ArcGIS, version 2, Volume 5, Early Paleozoic Plate Tectonic, Paleogeographic, and Paleoclimatic Reconstructions, Maps 75-88, PALEOMAP Project, Evanston, IL.
Scotese, C.R., 2014f, The PALEOMAP Project PaleoAtlas for ArcGIS, version 2, Volume 6, Precambrian Plate Tectonic, Paleogeographic, and Paleoclimatic Reconstructions, Maps 89-103, PALEOMAP Project, Evanston, IL.
2014.23 This Atlas of Phanerozoic Oceanic Anoxia shows the patterns of oceanic anoxia for 22 time... more 2014.23 This Atlas of Phanerozoic Oceanic Anoxia shows the patterns of oceanic anoxia for 22 time periods from the base of the Cambrian (542 Ma) to the Middle/Late Miocene (Serravallian & Tortonian, 10.5 Ma), plus one additional map for the Neoproterozoic (Middle Ediacaran, 600 Ma). Regions where anoxic conditions may have existed are shown in red. Regions where well-oxygenated waters occurred are shown in blue. Various shades of green, yellow and orange indicate somewhat dysoxic conditions. Red arrows indicate the direction of surface ocean currents during the summer months (June-July-August).
These plate tectonic and paleogeographic maps are the work of C. R. Scotese. The paleoclimate simulations were done by T.L. Moore using the FOAM (Fast Ocean and Atmosphere) Climate Simulation Program. The differences in color and symbology from map to map are due to the fact that these figures were originally published in four separate reports (Scotese et al., 2007; 2008; 2009; & 2011).
These estimates of anoxic oceanic conditions have been made by calculating the degree of “restriction” in each sedimentary basin. Restriction is a quantitative estimate of the degree of connection between any marine region and the open ocean. Restriction values ranged from 0 (not restricted) to 100 (very restricted). For example a marine region that is completely surrounded ocean would be classified as “nonrestricted” and would have a restriction value near zero. On the other hand, a marine embayment that is surrounded mostly by land grid cells would be considered very restricted and would have a high restriction value (>80).
The restriction value was determined by calculating the average distance of each marine grid cell to the nearest land grid cell. Distance measurements were made in 8 compass directions (N,NE,E,SE,S,SW,W,and NW). When the average distance to from each marine grid cell to the nearest land cells was small, it indicated that the marine cell was surrounded by land cells, and hence was “restricted” and likely to be prone to anoxic conditions. Conversely, if the average distance between a marine grid cell and the surrounding land grid cells was very large then it could be inferred that the grid cell was in the “open ocean”, and hence not prone to anoxic conditions. In our approach we use “restriction” as a proxy for oceanic anoxia.
It should be clear from the above description that this simple method of estimating oceanic anoxia does not take into account any geochemical measurements of anoxia, or bring into play any aspects of ocean dynamics (e.g. upwelling, surface currents or salinity). This approach is purely geographical, and consequently, has a few drawbacks. Firstly, high values of anoxia along ocean-facing coastlines are suspect. Also all of the estimates of oceanic anoxia have been made only for surface waters. In other words, the restriction calculation indicates how well connected the surface waters are to the open ocean but doesn’t say anything about the connectedness of the deeper portions of the basin. An exception is the map of oceanic anoxia for the Permo-Triassic Boundary (Map 49, 251 Ma). In this case, the degree of restriction was calculated for a water depth of 1000m. This was done in order to highlight the degree to which the Paleotethys ocean basin was restricted from the Panthalassic ocean basin. The restriction of deep waters in the Paleotethys may have contributed to the global anoxic oceanic conditions that are thought to have played an important role in the great Permo-Triassic extinction.
A third artifact is sometimes apparent in the maps. Because the restriction calculation were made in only the cardinal compass directions, diagonal streaks are sometimes apparent (e.g. Maps 39 and 45).
Despite the simple method employed to estimate oceanic anoxia, some obvious patterns emerge from these maps. Ocean basins are most likely to become restricted, and hence anoxic, at two times during their tectonic history: 1) shortly after their initial opening when they are narrow (Maps 21, 27, 31, and 35), and then again 2) when the ocean basin closes, prior to continent-continent collision (Maps 9, 17, 45, 65 and 75). It therefore comes as no surprise that times of widespread oceanic anoxia, such as the mid-Mesozoic oceanic anoxic events (OAEs), are often coincident with times during which numerous, narrow, poorly connected ocean basins are beginning to open or close.
A complimentary set of surface ocean currents for the winter months (December-January-February) are plotted in the Atlas of Phanerozoic Salinity and Ocean Currents. Though similar to the results shown here, there are maps that show opposite flow directions due to monsoonal changes in wind directions.
The maps are from volumes 1-6 of the PALEOMAP PaleoAtlas for ArcGIS (Scotese, 2014a,b,c,d). Absolute age assignments are from Gradstein, Ogg & Smith (2008).
The following maps are included in the Atlas of Phanerozoic Oceanic Anoxia:
Map 5 Middle/Late Miocene (Serravallian & Tortonian, 10.5 Ma)
Map 7 Early Miocene (Aquitainian & Burdigalian, 19.5 Ma)
Map 9 Early Oligocene (Rupelian, 31.1 Ma)
Map 12 early Middle Eocene (middle Lutetian, 44.6 Ma)
Map 17 Late Cretaceous (Maastrichtian, 68 Ma)
Map 21 Mid-Cretaceous (Turonian, 91.1 Ma)
Map 23 Early Cretaceous (late Albian, 101.8 Ma)
Map 27 Early Cretaceous (early Aptian, 121.8 Ma)
Map 31 Early Cretaceous (Berriasian, 143 Ma)
Map 35 Late Jurassic (Oxfordian, 158.4 Ma)
Map 39 Early Jurassic (Toarcian, 179.3 Ma)
Map 45 Late Triassic (Carnian, 222.6 Ma)
Map 49 Permo-Triassic Boundary (251 Ma)
Map 54 Early Permian (Artinskian, 280 Ma)
Map 57 Late Pennsylvanian (Gzhelian, 301.2 Ma)
Map 63 Middle Mississippian (early Visean, 341.1 Ma)
Map 65 Late Devonian (latest Famennian, 359.2 Ma)
Map 70 Early Devonian (Emsian, 394.3 Ma)
Map 75 Early Silurian (late Llandovery, 432.1 Ma)
Map 82 Early Ordovician (Tremadoc, 480 Ma)
Map 88 Cambrian – Precambrian Boundary (542 Ma)
Map 90 Late Neoproterozoic (Middle Ediacaran, 600 Ma)
This work should be cited as
Scotese, C.R., and Moore, T.L., 2014. Atlas of Phanerozoic Oceanic Anoxia (Mollweide Projection), Volumes 1-6, PALEOMAP Project PaleoAtlas for ArcGIS, PALEOMAP Project, Evanston, IL.
References Cited:
Scotese, C.R., Illich, H., Zumberge, J, and Brown, S., and Moore, T., 2007. The GANDOLPH Project: Year One Report: Paleogeographic and Paleoclimatic Controls on Hydrocarbon Source Rock Deposition, A Report on the Methods Employed, the Results of the Paleoclimate Simulations (FOAM), and Oils/Source Rock Compilation, Conclusions at the End of Year One: Cenomanian/Turonian (93.5 Ma), Kimmeridgian/Tithonian (151 Ma), Sakmarian/Artinskian (284 Ma), Frasnian/Famennian (375 Ma), February, 2007. GeoMark Research Ltd, Houston, Texas, 142 pp.
Scotese, C.R., Illich, H., Zumberge, J, and Brown, S., and Moore, T., 2008. The GANDOLPH Project: Year Two Report: Paleogeographic and Paleoclimatic Controls on Hydrocarbon Source Rock Deposition, A Report on the Methods Employed, the Results of the Paleoclimate Simulations (FOAM), and Oils/Source Rock Compilation, Conclusions at the End of Year Two: Miocene (10Ma), Aptian/Albian (120 Ma), Berriasian/Barremian (140 Ma), Late Triassic (220 Ma), and Early Silurian (430 Ma), July, 2008. GeoMark Research Ltd, Houston, Texas, 177 pp.
Scotese, C.R., Illich, H., Zumberge, J, and Brown, S., and Moore, T., 2009. The GANDOLPH Project: Year Three Report: Paleogeographic and Paleoclimatic Controls on Hydrocarbon Source Rock Deposition, A report on the Results of the Paleogeographic, Paleoclimatic Simulations (FOAM), and Oils/Source Rock Compilation, Conclusions at the End of Year Three: Eocene (45Ma), Early/Middle Jurassic (180 Ma), Mississippian (340 Ma), Neoproterozoic (600 Ma), August 2009. GeoMark Research Ltd, Houston, Texas, 154 pp.
Scotese, C.R., Illich, H., Zumberge, J, and Brown, S., and Moore, T., 2011. The GANDOLPH Project: Year Four Report: Paleogeographic and Paleoclimatic Controls on Hydrocarbon Source Rock Deposition, A report on the Results of the Paleogeographic, Paleoclimatic Simulations (FOAM), and Oils/Source Rock Compilation, Conclusions at the End of Year Four: Oligocene (30 Ma), Cretaceous/Tertiary (70 Ma), Permian/Triassic (250 Ma), Silurian/Devonian (400 Ma), Cambrian/Ordovician (480 Ma), April, 2011. GeoMark Research Ltd, Houston, Texas, 219 pp.
Scotese, C.R., 2014a, The PALEOMAP Project PaleoAtlas for ArcGIS, version 2, Volume 1, Cenozoic Plate Tectonic, Paleogeographic, and Paleoclimatic Reconstructions, Maps 1-15, PALEOMAP Project, Evanston, IL.
Scotese, C.R., 2014b, The PALEOMAP Project PaleoAtlas for ArcGIS, version 2, Volume 2, Cretaceous Plate Tectonic, Paleogeographic, and Paleoclimatic Reconstructions, Maps 16-32, PALEOMAP Project, Evanston, IL.
Scotese, C.R., 2014c, The PALEOMAP Project PaleoAtlas for ArcGIS, version 2, Volume 3, Triassic and Jurassic Plate Tectonic, Paleogeographic, and Paleoclimatic Reconstructions, Map 33-48, PALEOMAP Project, Evanston, IL.
Scotese, C.R., 2014d, The PALEOMAP Project PaleoAtlas for ArcGIS, version 2, Volume 4, Late Paleozoic Plate Tectonic, Paleogeographic, and Paleoclimatic Reconstructions, Map 49-74, PALEOMAP Project, Evanston, IL.
Scotese, C.R., 2014e, The PALEOMAP Project PaleoAtlas for ArcGIS, version 2, Volume 5, Early Paleozoic Plate Tectonic, Paleogeographic, and Paleoclimatic Reconstructions, Maps 75-88, PALEOMAP Project, Evanston, IL.
Scotese, C.R., 2014f, The PALEOMAP Project PaleoAtlas for ArcGIS, version 2, Volume 6, Precambrian Plate Tectonic, Paleogeographic, and Paleoclimatic Reconstructions, Maps 89-103, PALEOMAP Project, Evanston, IL.
2013.07 These maps (rectilinear projection) are from the PALEOMAP PaleoAtlas for ArcGIS (Scotese,... more 2013.07 These maps (rectilinear projection) are from the PALEOMAP PaleoAtlas for ArcGIS (Scotese, 2013a-f). This is a digital atlas of plate tectonic, paleogeographic, and paleoclimatic reconstructions designed for use with the GIS software, ArcMap (ESRI). Table 1 lists the various types of maps that comprise the PALEOMAP PaleoAtlas. The maps included in this folio are highlighted in bold text (Table 1).
The last map in each folio is a rectilinear graticule that can be overlain on the maps to provide a geographic reference frame. A rectilinear projection was used because it can be easily georeferenced in ArcMap and transformed into a variety of other map projections. The rectilinear, or plate caree map projection can also be directly “wrapped” onto a spherical projection, like the oneused by Google Earth. A set of Google Earth paleoglobes has made from the maps in this folio. These Google Earth paleoglobes can be downloaded at: www.globalgeology.com.
If the map you need is missing, or if there doesn’t seem to be a map folio for the exact time interval of interest, please contact me (cscotese@gmail.com). Table 2 lists all the time intervals that comprise the PALEOMAP PaleoAtlas for ArcGIS. The PaleoAtlas contains one map for every stage in the Phanerozoic, as well as 6 maps for the late Precambrian. Eventually, Map Folios, like this one, will be published for every time interval in the PALEOMAP PaleoAtlas. The following section is a brief description of the maps that makeup the Map Folio.
2013.08 These maps (rectilinear projection) are from the PALEOMAP PaleoAtlas for ArcGIS (Scotese,... more 2013.08 These maps (rectilinear projection) are from the PALEOMAP PaleoAtlas for ArcGIS (Scotese, 2013a-f). This is a digital atlas of plate tectonic, paleogeographic, and paleoclimatic reconstructions designed for use with the GIS software, ArcMap (ESRI). Table 1 lists the various types of maps that comprise the PALEOMAP PaleoAtlas. The maps included in this folio are highlighted in bold text (Table 1).
The last map in each folio is a rectilinear graticule that can be overlain on the maps to provide a geographic reference frame. A rectilinear projection was used because it can be easily georeferenced in ArcMap and transformed into a variety of other map projections. The rectilinear, or plate caree map projection can also be directly “wrapped” onto a spherical projection, like the oneused by Google Earth. A set of Google Earth paleoglobes has made from the maps in this folio. These Google Earth paleoglobes can be downloaded at: www.globalgeology.com.
If the map you need is missing, or if there doesn’t seem to be a map folio for the exact time interval of interest, please contact me (cscotese@gmail.com). Table 2 lists all the time intervals that comprise the PALEOMAP PaleoAtlas for ArcGIS. The PaleoAtlas contains one map for every stage in the Phanerozoic, as well as 6 maps for the late Precambrian. Eventually, Map Folios, like this one, will be published for every time interval in the PALEOMAP PaleoAtlas. The following section is a brief description of the maps that makeup the Map Folio.
2013.11 These maps (rectilinear projection) are from the PALEOMAP PaleoAtlas for ArcGIS (Scotese,... more 2013.11 These maps (rectilinear projection) are from the PALEOMAP PaleoAtlas for ArcGIS (Scotese, 2013a-f). This is a digital atlas of plate tectonic, paleogeographic, and paleoclimatic reconstructions designed for use with the GIS software, ArcMap (ESRI). Table 1 lists the various types of maps that comprise the PALEOMAP PaleoAtlas. The maps included in this folio are highlighted in bold text (Table 1).
The last map in each folio is a rectilinear graticule that can be overlain on the maps to provide a geographic reference frame. A rectilinear projection was used because it can be easily georeferenced in ArcMap and transformed into a variety of other map projections. The rectilinear, or plate caree map projection can also be directly “wrapped” onto a spherical projection, like the oneused by Google Earth. A set of Google Earth paleoglobes has made from the maps in this folio. These Google Earth paleoglobes can be downloaded at: www.globalgeology.com.
If the map you need is missing, or if there doesn’t seem to be a map folio for the exact time interval of interest, please contact me (cscotese@gmail.com). Table 2 lists all the time intervals that comprise the PALEOMAP PaleoAtlas for ArcGIS. The PaleoAtlas contains one map for every stage in the Phanerozoic, as well as 6 maps for the late Precambrian. Eventually, Map Folios, like this one, will be published for every time interval in the PALEOMAP PaleoAtlas. The following section is a brief description of the maps that makeup the Map Folio.
2013.13 These maps (rectilinear projection) are from the PALEOMAP PaleoAtlas for ArcGIS (Scotese,... more 2013.13 These maps (rectilinear projection) are from the PALEOMAP PaleoAtlas for ArcGIS (Scotese, 2013a-f). This is a digital atlas of plate tectonic, paleogeographic, and paleoclimatic reconstructions designed for use with the GIS software, ArcMap (ESRI). Table 1 lists the various types of maps that comprise the PALEOMAP PaleoAtlas. The maps included in this folio are highlighted in bold text (Table 1).
The last map in each folio is a rectilinear graticule that can be overlain on the maps to provide a geographic reference frame. A rectilinear projection was used because it can be easily georeferenced in ArcMap and transformed into a variety of other map projections. The rectilinear, or plate caree map projection can also be directly “wrapped” onto a spherical projection, like the oneused by Google Earth. A set of Google Earth paleoglobes has made from the maps in this folio. These Google Earth paleoglobes can be downloaded at: www.globalgeology.com.
If the map you need is missing, or if there doesn’t seem to be a map folio for the exact time interval of interest, please contact me (cscotese@gmail.com). Table 2 lists all the time intervals that comprise the PALEOMAP PaleoAtlas for ArcGIS. The PaleoAtlas contains one map for every stage in the Phanerozoic, as well as 6 maps for the late Precambrian. Eventually, Map Folios, like this one, will be published for every time interval in the PALEOMAP PaleoAtlas. The following section is a brief description of the maps that makeup the Map Folio.
2013.15 These maps (rectilinear projection) are from the PALEOMAP PaleoAtlas for ArcGIS (Scotese,... more 2013.15 These maps (rectilinear projection) are from the PALEOMAP PaleoAtlas for ArcGIS (Scotese, 2013a-f). This is a digital atlas of plate tectonic, paleogeographic, and paleoclimatic reconstructions designed for use with the GIS software, ArcMap (ESRI). Table 1 lists the various types of maps that comprise the PALEOMAP PaleoAtlas. The maps included in this folio are highlighted in bold text (Table 1).
The last map in each folio is a rectilinear graticule that can be overlain on the maps to provide a geographic reference frame. A rectilinear projection was used because it can be easily georeferenced in ArcMap and transformed into a variety of other map projections. The rectilinear, or plate caree map projection can also be directly “wrapped” onto a spherical projection, like the oneused by Google Earth. A set of Google Earth paleoglobes has made from the maps in this folio. These Google Earth paleoglobes can be downloaded at: www.globalgeology.com.
If the map you need is missing, or if there doesn’t seem to be a map folio for the exact time interval of interest, please contact me (cscotese@gmail.com). Table 2 lists all the time intervals that comprise the PALEOMAP PaleoAtlas for ArcGIS. The PaleoAtlas contains one map for every stage in the Phanerozoic, as well as 6 maps for the late Precambrian. Eventually, Map Folios, like this one, will be published for every time interval in the PALEOMAP PaleoAtlas. The following section is a brief description of the maps that makeup the Map Folio.
2013.17 These maps (rectilinear projection) are from the PALEOMAP PaleoAtlas for ArcGIS (Scotese,... more 2013.17 These maps (rectilinear projection) are from the PALEOMAP PaleoAtlas for ArcGIS (Scotese, 2013a-f). This is a digital atlas of plate tectonic, paleogeographic, and paleoclimatic reconstructions designed for use with the GIS software, ArcMap (ESRI). Table 1 lists the various types of maps that comprise the PALEOMAP PaleoAtlas. The maps included in this folio are highlighted in bold text (Table 1).
The last map in each folio is a rectilinear graticule that can be overlain on the maps to provide a geographic reference frame. A rectilinear projection was used because it can be easily georeferenced in ArcMap and transformed into a variety of other map projections. The rectilinear, or plate caree map projection can also be directly “wrapped” onto a spherical projection, like the oneused by Google Earth. A set of Google Earth paleoglobes has made from the maps in this folio. These Google Earth paleoglobes can be downloaded at: www.globalgeology.com.
If the map you need is missing, or if there doesn’t seem to be a map folio for the exact time interval of interest, please contact me (cscotese@gmail.com). Table 2 lists all the time intervals that comprise the PALEOMAP PaleoAtlas for ArcGIS. The PaleoAtlas contains one map for every stage in the Phanerozoic, as well as 6 maps for the late Precambrian. Eventually, Map Folios, like this one, will be published for every time interval in the PALEOMAP PaleoAtlas. The following section is a brief description of the maps that makeup the Map Folio.
2013.19 These maps (rectilinear projection) are from the PALEOMAP PaleoAtlas for ArcGIS (Scotese,... more 2013.19 These maps (rectilinear projection) are from the PALEOMAP PaleoAtlas for ArcGIS (Scotese, 2013a-f). This is a digital atlas of plate tectonic, paleogeographic, and paleoclimatic reconstructions designed for use with the GIS software, ArcMap (ESRI). Table 1 lists the various types of maps that comprise the PALEOMAP PaleoAtlas. The maps included in this folio are highlighted in bold text (Table 1).
The last map in each folio is a rectilinear graticule that can be overlain on the maps to provide a geographic reference frame. A rectilinear projection was used because it can be easily georeferenced in ArcMap and transformed into a variety of other map projections. The rectilinear, or plate caree map projection can also be directly “wrapped” onto a spherical projection, like the oneused by Google Earth. A set of Google Earth paleoglobes has made from the maps in this folio. These Google Earth paleoglobes can be downloaded at: www.globalgeology.com.
If the map you need is missing, or if there doesn’t seem to be a map folio for the exact time interval of interest, please contact me (cscotese@gmail.com). Table 2 lists all the time intervals that comprise the PALEOMAP PaleoAtlas for ArcGIS. The PaleoAtlas contains one map for every stage in the Phanerozoic, as well as 6 maps for the late Precambrian. Eventually, Map Folios, like this one, will be published for every time interval in the PALEOMAP PaleoAtlas. The following section is a brief description of the maps that makeup the Map Folio.
2013.21 These maps (rectilinear projection) are from the PALEOMAP PaleoAtlas for ArcGIS (Scotese,... more 2013.21 These maps (rectilinear projection) are from the PALEOMAP PaleoAtlas for ArcGIS (Scotese, 2013a-f). This is a digital atlas of plate tectonic, paleogeographic, and paleoclimatic reconstructions designed for use with the GIS software, ArcMap (ESRI). Table 1 lists the various types of maps that comprise the PALEOMAP PaleoAtlas. The maps included in this folio are highlighted in bold text (Table 1).
The last map in each folio is a rectilinear graticule that can be overlain on the maps to provide a geographic reference frame. A rectilinear projection was used because it can be easily georeferenced in ArcMap and transformed into a variety of other map projections. The rectilinear, or plate caree map projection can also be directly “wrapped” onto a spherical projection, like the oneused by Google Earth. A set of Google Earth paleoglobes has made from the maps in this folio. These Google Earth paleoglobes can be downloaded at: www.globalgeology.com.
If the map you need is missing, or if there doesn’t seem to be a map folio for the exact time interval of interest, please contact me (cscotese@gmail.com). Table 2 lists all the time intervals that comprise the PALEOMAP PaleoAtlas for ArcGIS. The PaleoAtlas contains one map for every stage in the Phanerozoic, as well as 6 maps for the late Precambrian. Eventually, Map Folios, like this one, will be published for every time interval in the PALEOMAP PaleoAtlas. The following section is a brief description of the maps that makeup the Map Folio.
2012.23 These maps (rectilinear projection) are from the PALEOMAP PaleoAtlas for ArcGIS (Scotese,... more 2012.23 These maps (rectilinear projection) are from the PALEOMAP PaleoAtlas for ArcGIS (Scotese, 2013a-f). This is a digital atlas of plate tectonic, paleogeographic, and paleoclimatic reconstructions designed for use with the GIS software, ArcMap (ESRI). Table 1 lists the various types of maps that comprise the PALEOMAP PaleoAtlas. The maps included in this folio are highlighted in bold text (Table 1).
The last map in each folio is a rectilinear graticule that can be overlain on the maps to provide a geographic reference frame. A rectilinear projection was used because it can be easily georeferenced in ArcMap and transformed into a variety of other map projections. The rectilinear, or plate caree map projection can also be directly “wrapped” onto a spherical projection, like the oneused by Google Earth. A set of Google Earth paleoglobes has made from the maps in this folio. These Google Earth paleoglobes can be downloaded at: www.globalgeology.com.
If the map you need is missing, or if there doesn’t seem to be a map folio for the exact time interval of interest, please contact me (cscotese@gmail.com). Table 2 lists all the time intervals that comprise the PALEOMAP PaleoAtlas for ArcGIS. The PaleoAtlas contains one map for every stage in the Phanerozoic, as well as 6 maps for the late Precambrian. Eventually, Map Folios, like this one, will be published for every time interval in the PALEOMAP PaleoAtlas. The following section is a brief description of the maps that makeup the Map Folio.
2013.25 These maps (rectilinear projection) are from the PALEOMAP PaleoAtlas for ArcGIS (Scotese,... more 2013.25 These maps (rectilinear projection) are from the PALEOMAP PaleoAtlas for ArcGIS (Scotese, 2013a-f). This is a digital atlas of plate tectonic, paleogeographic, and paleoclimatic reconstructions designed for use with the GIS software, ArcMap (ESRI). Table 1 lists the various types of maps that comprise the PALEOMAP PaleoAtlas. The maps included in this folio are highlighted in bold text (Table 1).
The last map in each folio is a rectilinear graticule that can be overlain on the maps to provide a geographic reference frame. A rectilinear projection was used because it can be easily georeferenced in ArcMap and transformed into a variety of other map projections. The rectilinear, or plate caree map projection can also be directly “wrapped” onto a spherical projection, like the oneused by Google Earth. A set of Google Earth paleoglobes has made from the maps in this folio. These Google Earth paleoglobes can be downloaded at: www.globalgeology.com.
If the map you need is missing, or if there doesn’t seem to be a map folio for the exact time interval of interest, please contact me (cscotese@gmail.com). Table 2 lists all the time intervals that comprise the PALEOMAP PaleoAtlas for ArcGIS. The PaleoAtlas contains one map for every stage in the Phanerozoic, as well as 6 maps for the late Precambrian. Eventually, Map Folios, like this one, will be published for every time interval in the PALEOMAP PaleoAtlas. The following section is a brief description of the maps that makeup the Map Folio.
2013.27 These maps (rectilinear projection) are from the PALEOMAP PaleoAtlas for ArcGIS (Scotese,... more 2013.27 These maps (rectilinear projection) are from the PALEOMAP PaleoAtlas for ArcGIS (Scotese, 2013a-f). This is a digital atlas of plate tectonic, paleogeographic, and paleoclimatic reconstructions designed for use with the GIS software, ArcMap (ESRI). Table 1 lists the various types of maps that comprise the PALEOMAP PaleoAtlas. The maps included in this folio are highlighted in bold text (Table 1).
The last map in each folio is a rectilinear graticule that can be overlain on the maps to provide a geographic reference frame. A rectilinear projection was used because it can be easily georeferenced in ArcMap and transformed into a variety of other map projections. The rectilinear, or plate caree map projection can also be directly “wrapped” onto a spherical projection, like the oneused by Google Earth. A set of Google Earth paleoglobes has made from the maps in this folio. These Google Earth paleoglobes can be downloaded at: www.globalgeology.com.
If the map you need is missing, or if there doesn’t seem to be a map folio for the exact time interval of interest, please contact me (cscotese@gmail.com). Table 2 lists all the time intervals that comprise the PALEOMAP PaleoAtlas for ArcGIS. The PaleoAtlas contains one map for every stage in the Phanerozoic, as well as 6 maps for the late Precambrian. Eventually, Map Folios, like this one, will be published for every time interval in the PALEOMAP PaleoAtlas. The following section is a brief description of the maps that makeup the Map Folio.
2013.29 These maps (rectilinear projection) are from the PALEOMAP PaleoAtlas for ArcGIS (Scotese,... more 2013.29 These maps (rectilinear projection) are from the PALEOMAP PaleoAtlas for ArcGIS (Scotese, 2013a-f). This is a digital atlas of plate tectonic, paleogeographic, and paleoclimatic reconstructions designed for use with the GIS software, ArcMap (ESRI). Table 1 lists the various types of maps that comprise the PALEOMAP PaleoAtlas. The maps included in this folio are highlighted in bold text (Table 1).
The last map in each folio is a rectilinear graticule that can be overlain on the maps to provide a geographic reference frame. A rectilinear projection was used because it can be easily georeferenced in ArcMap and transformed into a variety of other map projections. The rectilinear, or plate caree map projection can also be directly “wrapped” onto a spherical projection, like the oneused by Google Earth. A set of Google Earth paleoglobes has made from the maps in this folio. These Google Earth paleoglobes can be downloaded at: www.globalgeology.com.
If the map you need is missing, or if there doesn’t seem to be a map folio for the exact time interval of interest, please contact me (cscotese@gmail.com). Table 2 lists all the time intervals that comprise the PALEOMAP PaleoAtlas for ArcGIS. The PaleoAtlas contains one map for every stage in the Phanerozoic, as well as 6 maps for the late Precambrian. Eventually, Map Folios, like this one, will be published for every time interval in the PALEOMAP PaleoAtlas. The following section is a brief description of the maps that makeup the Map Folio.
2013.31 These maps (rectilinear projection) are from the PALEOMAP PaleoAtlas for ArcGIS (Scotese,... more 2013.31 These maps (rectilinear projection) are from the PALEOMAP PaleoAtlas for ArcGIS (Scotese, 2013a-f). This is a digital atlas of plate tectonic, paleogeographic, and paleoclimatic reconstructions designed for use with the GIS software, ArcMap (ESRI). Table 1 lists the various types of maps that comprise the PALEOMAP PaleoAtlas. The maps included in this folio are highlighted in bold text (Table 1).
The last map in each folio is a rectilinear graticule that can be overlain on the maps to provide a geographic reference frame. A rectilinear projection was used because it can be easily georeferenced in ArcMap and transformed into a variety of other map projections. The rectilinear, or plate caree map projection can also be directly “wrapped” onto a spherical projection, like the oneused by Google Earth. A set of Google Earth paleoglobes has made from the maps in this folio. These Google Earth paleoglobes can be downloaded at: www.globalgeology.com.
If the map you need is missing, or if there doesn’t seem to be a map folio for the exact time interval of interest, please contact me (cscotese@gmail.com). Table 2 lists all the time intervals that comprise the PALEOMAP PaleoAtlas for ArcGIS. The PaleoAtlas contains one map for every stage in the Phanerozoic, as well as 6 maps for the late Precambrian. Eventually, Map Folios, like this one, will be published for every time interval in the PALEOMAP PaleoAtlas. The following section is a brief description of the maps that makeup the Map Folio.
2013.33 These maps (rectilinear projection) are from the PALEOMAP PaleoAtlas for ArcGIS (Scotese,... more 2013.33 These maps (rectilinear projection) are from the PALEOMAP PaleoAtlas for ArcGIS (Scotese, 2013a-f). This is a digital atlas of plate tectonic, paleogeographic, and paleoclimatic reconstructions designed for use with the GIS software, ArcMap (ESRI). Table 1 lists the various types of maps that comprise the PALEOMAP PaleoAtlas. The maps included in this folio are highlighted in bold text (Table 1).
The last map in each folio is a rectilinear graticule that can be overlain on the maps to provide a geographic reference frame. A rectilinear projection was used because it can be easily georeferenced in ArcMap and transformed into a variety of other map projections. The rectilinear, or plate caree map projection can also be directly “wrapped” onto a spherical projection, like the oneused by Google Earth. A set of Google Earth paleoglobes has made from the maps in this folio. These Google Earth paleoglobes can be downloaded at: www.globalgeology.com.
If the map you need is missing, or if there doesn’t seem to be a map folio for the exact time interval of interest, please contact me (cscotese@gmail.com). Table 2 lists all the time intervals that comprise the PALEOMAP PaleoAtlas for ArcGIS. The PaleoAtlas contains one map for every stage in the Phanerozoic, as well as 6 maps for the late Precambrian. Eventually, Map Folios, like this one, will be published for every time interval in the PALEOMAP PaleoAtlas. The following section is a brief description of the maps that makeup the Map Folio.
2013.35 These maps (rectilinear projection) are from the PALEOMAP PaleoAtlas for ArcGIS (Scotese,... more 2013.35 These maps (rectilinear projection) are from the PALEOMAP PaleoAtlas for ArcGIS (Scotese, 2013a-f). This is a digital atlas of plate tectonic, paleogeographic, and paleoclimatic reconstructions designed for use with the GIS software, ArcMap (ESRI). Table 1 lists the various types of maps that comprise the PALEOMAP PaleoAtlas. The maps included in this folio are highlighted in bold text (Table 1).
The last map in each folio is a rectilinear graticule that can be overlain on the maps to provide a geographic reference frame. A rectilinear projection was used because it can be easily georeferenced in ArcMap and transformed into a variety of other map projections. The rectilinear, or plate caree map projection can also be directly “wrapped” onto a spherical projection, like the oneused by Google Earth. A set of Google Earth paleoglobes has made from the maps in this folio. These Google Earth paleoglobes can be downloaded at: www.globalgeology.com.
If the map you need is missing, or if there doesn’t seem to be a map folio for the exact time interval of interest, please contact me (cscotese@gmail.com). Table 2 lists all the time intervals that comprise the PALEOMAP PaleoAtlas for ArcGIS. The PaleoAtlas contains one map for every stage in the Phanerozoic, as well as 6 maps for the late Precambrian. Eventually, Map Folios, like this one, will be published for every time interval in the PALEOMAP PaleoAtlas. The following section is a brief description of the maps that makeup the Map Folio.
2013.37 These maps (rectilinear projection) are from the PALEOMAP PaleoAtlas for ArcGIS (Scotese,... more 2013.37 These maps (rectilinear projection) are from the PALEOMAP PaleoAtlas for ArcGIS (Scotese, 2013a-f). This is a digital atlas of plate tectonic, paleogeographic, and paleoclimatic reconstructions designed for use with the GIS software, ArcMap (ESRI). Table 1 lists the various types of maps that comprise the PALEOMAP PaleoAtlas. The maps included in this folio are highlighted in bold text (Table 1).
The last map in each folio is a rectilinear graticule that can be overlain on the maps to provide a geographic reference frame. A rectilinear projection was used because it can be easily georeferenced in ArcMap and transformed into a variety of other map projections. The rectilinear, or plate caree map projection can also be directly “wrapped” onto a spherical projection, like the oneused by Google Earth. A set of Google Earth paleoglobes has made from the maps in this folio. These Google Earth paleoglobes can be downloaded at: www.globalgeology.com.
If the map you need is missing, or if there doesn’t seem to be a map folio for the exact time interval of interest, please contact me (cscotese@gmail.com). Table 2 lists all the time intervals that comprise the PALEOMAP PaleoAtlas for ArcGIS. The PaleoAtlas contains one map for every stage in the Phanerozoic, as well as 6 maps for the late Precambrian. Eventually, Map Folios, like this one, will be published for every time interval in the PALEOMAP PaleoAtlas. The following section is a brief description of the maps that makeup the Map Folio.
Scotese, C.R., 2013. Map Folio 33, Late Jurassic (Tithonian, 148.2 Ma), PALEOMAP PaleoAtlas for ArcGIS, volume 3, Triassic and Jurassic Paleogeographic, Paleoclimatic and Plate Tectonic Reconstructions, PALEOMAP Project, Evanston, IL., 2013
2013.39 These maps (rectilinear projection) are from the PALEOMAP PaleoAtlas for ArcGIS (Scotese,... more 2013.39 These maps (rectilinear projection) are from the PALEOMAP PaleoAtlas for ArcGIS (Scotese, 2013a-f). This is a digital atlas of plate tectonic, paleogeographic, and paleoclimatic reconstructions designed for use with the GIS software, ArcMap (ESRI). Table 1 lists the various types of maps that comprise the PALEOMAP PaleoAtlas. The maps included in this folio are highlighted in bold text (Table 1).
The last map in each folio is a rectilinear graticule that can be overlain on the maps to provide a geographic reference frame. A rectilinear projection was used because it can be easily georeferenced in ArcMap and transformed into a variety of other map projections. The rectilinear, or plate caree map projection can also be directly “wrapped” onto a spherical projection, like the oneused by Google Earth. A set of Google Earth paleoglobes has made from the maps in this folio. These Google Earth paleoglobes can be downloaded at: www.globalgeology.com.
Scotese, C.R., 2013. Map Folio 35, Late Jurassic (Oxfordian, 158.4 Ma), PALEOMAP PaleoAtlas for ArcGIS, volume 3, Triassic and Jurassic Paleogeographic, Paleoclimatic and Plate Tectonic Reconstructions, PALEOMAP Project, Evanston, IL., 2013
2013.41 These maps (rectilinear projection) are from the PALEOMAP PaleoAtlas for ArcGIS (Scotese,... more 2013.41 These maps (rectilinear projection) are from the PALEOMAP PaleoAtlas for ArcGIS (Scotese, 2013a-f). This is a digital atlas of plate tectonic, paleogeographic, and paleoclimatic reconstructions designed for use with the GIS software, ArcMap (ESRI). Table 1 lists the various types of maps that comprise the PALEOMAP PaleoAtlas. The maps included in this folio are highlighted in bold text (Table 1).
The last map in each folio is a rectilinear graticule that can be overlain on the maps to provide a geographic reference frame. A rectilinear projection was used because it can be easily georeferenced in ArcMap and transformed into a variety of other map projections. The rectilinear, or plate caree map projection can also be directly “wrapped” onto a spherical projection, like the oneused by Google Earth. A set of Google Earth paleoglobes has made from the maps in this folio. These Google Earth paleoglobes can be downloaded at: www.globalgeology.com.
Scotese, C.R., 2013. Map Folio 37 Middle Jurassic (Bajocian & Bathonian, 169.7 Ma), PALEOMAP PaleoAtlas for ArcGIS, volume 3, Triassic and Jurassic Paleogeographic, Paleoclimatic and Plate Tectonic Reconstructions, PALEOMAP Project, Evanston, IL., 2013
2013.43 These maps (rectilinear projection) are from the PALEOMAP PaleoAtlas for ArcGIS (Scotese,... more 2013.43 These maps (rectilinear projection) are from the PALEOMAP PaleoAtlas for ArcGIS (Scotese, 2013a-f). This is a digital atlas of plate tectonic, paleogeographic, and paleoclimatic reconstructions designed for use with the GIS software, ArcMap (ESRI). Table 1 lists the various types of maps that comprise the PALEOMAP PaleoAtlas. The maps included in this folio are highlighted in bold text (Table 1).
The last map in each folio is a rectilinear graticule that can be overlain on the maps to provide a geographic reference frame. A rectilinear projection was used because it can be easily georeferenced in ArcMap and transformed into a variety of other map projections. The rectilinear, or plate caree map projection can also be directly “wrapped” onto a spherical projection, like the oneused by Google Earth. A set of Google Earth paleoglobes has made from the maps in this folio. These Google Earth paleoglobes can be downloaded at: www.globalgeology.com.
If the map you need is missing, or if there doesn’t seem to be a map folio for the exact time interval of interest, please contact me (cscotese@gmail.com). Table 2 lists all the time intervals that comprise the PALEOMAP PaleoAtlas for ArcGIS. The PaleoAtlas contains one map for every stage in the Phanerozoic, as well as 6 maps for the late Precambrian. Eventually, Map Folios, like this one, will be published for every time interval in the PALEOMAP PaleoAtlas. The following section is a brief description of the maps that makeup the Map Folio.
Scotese, C.R., 2013. Map Folio 39 Early Jurassic Toarcian, 179.3 Ma), PALEOMAP PaleoAtlas for ArcGIS, volume 3, Triassic and Jurassic Paleogeographic, Paleoclimatic and Plate Tectonic Reconstructions, PALEOMAP Project, Evanston, IL., 2013
2013.45 These maps (rectilinear projection) are from the PALEOMAP PaleoAtlas for ArcGIS (Scotese,... more 2013.45 These maps (rectilinear projection) are from the PALEOMAP PaleoAtlas for ArcGIS (Scotese, 2013a-f). This is a digital atlas of plate tectonic, paleogeographic, and paleoclimatic reconstructions designed for use with the GIS software, ArcMap (ESRI). Table 1 lists the various types of maps that comprise the PALEOMAP PaleoAtlas. The maps included in this folio are highlighted in bold text (Table 1).
The last map in each folio is a rectilinear graticule that can be overlain on the maps to provide a geographic reference frame. A rectilinear projection was used because it can be easily georeferenced in ArcMap and transformed into a variety of other map projections. The rectilinear, or plate caree map projection can also be directly “wrapped” onto a spherical projection, like the oneused by Google Earth. A set of Google Earth paleoglobes has made from the maps in this folio. These Google Earth paleoglobes can be downloaded at: www.globalgeology.com.
If the map you need is missing, or if there doesn’t seem to be a map folio for the exact time interval of interest, please contact me (cscotese@gmail.com). Table 2 lists all the time intervals that comprise the PALEOMAP PaleoAtlas for ArcGIS. The PaleoAtlas contains one map for every stage in the Phanerozoic, as well as 6 maps for the late Precambrian. Eventually, Map Folios, like this one, will be published for every time interval in the PALEOMAP PaleoAtlas. The following section is a brief description of the maps that makeup the Map Folio.
Plate Tectonics @ Night v01.052317, May 23, 2018
Ride back through the darkness of times past with the continents and their city lights. This anim... more Ride back through the darkness of times past with the continents and their city lights. This animation is based on the PALEOMAP Global Plate Tectonic Model using the the program "GPlates" developed by R.D. Müller (EarthByte). The map is the composite satellite image of the "Earth at Night" (NASA) combined with a 3D relief model of the ocean floor and the modern coastlines and political boundaries, for reference. www.nasa.gov/specials/blackmarble/2016/globalmaps/BlackMarble_2016_3km.jpg - C.R. Scotese, Evanston, IL May 23, 2017. version 01.052317
Upchurch, G.R., Jr., Kiehl, J., Shields, C., Scherer, J., and Scotese, C., 2015. Latitudinal temperature gradients and high-latitude temperatures during the latest Cretaceous: Congurence of geologic data and climate models, Geology, v. 43, no, 8., 683-686
2015-01 A major challenge in paleoclimatology is disagreement between data and models for periods... more 2015-01 A major challenge in paleoclimatology is disagreement between data and models for periods of warm climate. Data indicate equable conditions and reduced latitudinal temperature gradients, while models produce colder conditions and steeper latitudinal gradients when using realistic levels of CO2. Here we demonstrate congruence between temperature indicators and climate model output for the cool greenhouse interval of the latest Cretaceous (Maastrichtian) using a comprehensive database of terrestrial and marine indicators and fully coupled simulations with the Community Climate System Model, version 3 (CCSM3). In these simulations we explore the potential roles of greenhouse gases, vegetation, and properties of pre-anthropogenic liquid clouds in creating warm equable conditions. Our model simulations successfully reproduce warm polar temperatures and the latitudinal temperature gradient without overheating the tropics, using geologically realistic levels of atmospheric CO2. The best fit for Mean Annual Temperature is a simulation that prescribes 560 ppm CO2 (2x preindustrial), 2000 ppb CH4, realistic vegetation, and liquid cloud properties that may reflect pre-anthropogenic levels of cloud condensation nuclei. The most problematic region is the Siberian interior, which may relate in part to reconstructed elevation and the presence of a large lake not included in model simulations. Data and models together indicate an average equator to pole temperature difference of 25–30°C, and a mid-latitudinal gradient of mean annual temperature of ~0.4°C. This is consistent with suggestions that intervals of greenhouse climate were characterized by significant equator to pole temperature differences and moderate latitudinal temperature gradients.
Scotese, C.R., 2015. The Ultimate PLate Tectonic Flipbook (PowerPoint), Rob Vander Voo Retirement Symposium, August 25-27, 2015, Ann Arbor, MI., Aug 27, 2015
This "flipbook", which illustrates the plate tectonic development of the continents and ocean bas... more This "flipbook", which illustrates the plate tectonic development of the continents and ocean basins during the past 750 million years, was assembled to commemorate the scientific career of Professor Rob van der Voo. The flipbook consists of 34 plate tectonic reconstructions that map the past location of subduction zones (barbed lines), mid-ocean ridges, (dashed lines), and collision zones (marked x's). The tectonic reconstructions are based on the global plate tectonic model developed by the PALEOMAP Project.
The latitudinal orientation of the continents is derived largely from paleomagnetic data collected by Professor van der Voo (xref). Hot spots tracks and sea floor spreading isochrons (Seton et al., 2012) were used to constrain the longitudinal position of the continents back to ~200 million years. Plate tectonic reconstructions older than 200 million years are necessarily more speculative and have been derived by combining diverse lines of evidence from the tectonic histories of the continents (e.g., timing of continent-continent collisions or ages of rifting), the distribution of paleoclimatic indicators (i.e coals, tillites, salt deposits, and bauxites, see Boucot et al., 2013), and in some case, the biogeographic affinities of fossil faunas and floras.
Though a diverse data has been used to produce these reconstructions, this data, itself, is not enough. So much time has passed and so little direct evidence is preserved that guidance must also be sought from the "Rules of Plate Tectonics".
Plates do not move randomly but evolve in a manner that is consistent with the forces that drive them. The principal driving forces are: slab pull, ridge push and trench rollback. These forces shape the plates and provide important insights into how plate boundaries will evolve. Simply said, plates will only move if they are pulled by a subducting slab or pushed by the forces exerted by a mature ridge system. The evolving plate boundaries have been drawn to follow this maxim. It is also important to note that plate tectonics is a "catastrophic" system. Though "slow and steady" is the general rule, once every hundred million years or so, a major plate tectonic reorganization occurs. These "plate tectonic catastrophes" most often occur when mid-ocean ridges are subducted or when major continents collide. (For a more complete listing of the "Rules of Plate Tectonics", the reader is referred to XXXXXX.
The first "continental drift" flipbook was pushed as an undergraduate research project (Scotese, 1974; 1975abc). Subsequent editions have followed (1976ab; 1978; 1979; 1980; 1990, 1991, 1997, 2004). A more complete description of the data and information that is used to produce the flipbooks can be found in Scotese (2004). These maps could not have been produced without the GPlates plate modelling software and the tectonic data sets published by Dietmar Müller and his team at Earthbytes.
Special thanks to Maggie Geiger, and Robert and Jonathan Scotese for their help assembling this flipbook.
Time Scale
The age given next to each map represents age in millions of years. The corresponding geological ages (Ogg et al., 2008) are:
0 Modern World
20 Ma Early Miocene
40 Ma late Middle Eocene
60 Ma Paleocene
80 Ma Late Cretaceous - Campanian
100 Ma Early Cretaceous - late Albian
120 Ma Early Cretaceous - early Aptian
140 Ma Early Cretaceous - Berriasian
160 Ma Late Jurassic - Oxfordian
180 Ma Early Jurassic - Toarcian
200 Ma Triassic/Jurassic boundary
220 Ma Late Triassic - Carnian
240 Ma Middle Triassic - Anisian
260 Ma Middle Permian - Capitanian
280 Ma Early Permian - Artinskian
300 Ma Late Pennsylvanian
320 Ma Late Mississippian
340 Ma Middle Mississippian
360 Ma Devono-Carboniferous
380 Ma Late Devonian - Frasnian
400 Ma Early Devonian - Emsian
420 Ma Late Silurian - Ludlow
440 Ma Early Silurian - Llandovery
460 Ma Middle Ordovician
480 Ma Early Ordovician
500 Ma Late Cambrian
520 Ma Middle Cambrian
540 Ma Cambrian-Precambrian
560 Ma Neoproterozoic - lt. Ediacaran
600 Ma Neoporterozoic - m. Ediacaran
630 Ma Neoproterozoic - e. Ediacaran
660 Ma Neoproterozoic - e. Ediacaran
690 Ma Neoproterozoic - lt. Cryogenian
720 Ma m. Cryogenian
750 Ma m. Cryogenian
References Cited
Ogg, J., Ogg, G., and Gradstein, F.M., 2008. The Concise Geologic Time Scale, Cambridge University Press, 177 p.
Scotese, C.R. 1974. First Flip Book Images (from 35mm film from PLATO System), Unpublished.
Scotese, C.R., and Baker, D.W., 1975a. Continental drift reconstructions and animation, Journal of Geological Education, 23: 167-171.
Scotese, C.R., 1975b. Continental Drift Flip Book, 1stedition.Chicago, Illinois. (single page version
Scotese, C.R., 1975c. Continental Drift Flip Book, 1st edition. Chicago, Illinois. (double page version)
Scotese, C.R., 1976a. Continental
Drift “Flip Book”, edition 1.5, Department of Geological Sciences, University of Illinois. ResearchGate Academia
Scotese, C.R., 1976b. A continental drift “flip book", Computers & Geosciences, 2:113-116.
Scotese, C.R., and Ziegler, A.M., 1978. Paleozoic continental drift reconstructions and animation, American Geophysical Union, 1978 Spring Annual Meeting, Eos, v. 59. Issue 4, p. 263.
Scotese, C.R., 1979. Continental Drift (flip book), 2nd edition.
Scotese, C.R., Snelson, S.S., and Ross, W.C., 1980. A computer animation of continental drift, J. Geomag. Geoelectr., 32: suppl. III, 61-70.
Scotese, C.R., 1990. Atlas of Phanerozoic Plate Tectonic Reconstructions, PALEOMAP Progress 01-1090a, Department of Geology, University of Texas at Arlington, Texas, 57 pp.
Scotese, C.R., 1991. Continental Drift Flip Book, 4th edition, PALEOMAP Project, Arlington, TX, 49 pp.
Scotese, C.R., 1997. Continental Drift Flip Book, 7th edition, PALEOMAP Project, Department of Geology, University of Texas at Arlington, Texas, 80 pp.
Scotese, 2004.
Seton et al., 2012.
Van der Voo, R., 1993. Paleomagnetism of the Atlantic, Tethys, and Iapetus Oceans, Cambridge University Press, 411 p.
Scotese, C.R., 2015. Plate Tectonics (flipbook), v.082415, PALEOMAP Project, Evanston, IL. 41 pp., Aug 26, 2015
This "flipbook", which illustrates the plate tectonic development of the continents and ocean bas... more This "flipbook", which illustrates the plate tectonic development of the continents and ocean basins during the past 750 million years, was assembled to commemorate the scientific career of Professor Rob van der Voo. The flipbook consists of 34 plate tectonic reconstructions that map the past location of subduction zones (barbed lines), mid-ocean ridges, (dashed lines), and collision zones (marked x's). The tectonic reconstructions are based on the global plate tectonic model developed by the PALEOMAP Project.
The latitudinal orientation of the continents is derived largely from paleomagnetic data collected by Professor van der Voo (xref). Hot spots tracks and sea floor spreading isochrons (Seton et al., 2012) were used to constrain the longitudinal position of the continents back to ~200 million years. Plate tectonic reconstructions older than 200 million years are necessarily more speculative and have been derived by combining diverse lines of evidence from the tectonic histories of the continents (e.g., timing of continent-continent collisions or ages of rifting), the distribution of paleoclimatic indicators (i.e coals, tillites, salt deposits, and bauxites, see Boucot et al., 2013), and in some case, the biogeographic affinities of fossil faunas and floras.
Though a diverse data has been used to produce these reconstructions, this data, itself, is not enough. So much time has passed and so little direct evidence is preserved that guidance must also be sought from the "Rules of Plate Tectonics".
Plates do not move randomly but evolve in a manner that is consistent with the forces that drive them. The principal driving forces are: slab pull, ridge push and trench rollback. These forces shape the plates and provide important insights into how plate boundaries will evolve. Simply said, plates will only move if they are pulled by a subducting slab or pushed by the forces exerted by a mature ridge system. The evolving plate boundaries have been drawn to follow this maxim. It is also important to note that plate tectonics is a "catastrophic" system. Though "slow and steady" is the general rule, once every hundred million years or so, a major plate tectonic reorganization occurs. These "plate tectonic catastrophes" most often occur when mid-ocean ridges are subducted or when major continents collide. (For a more complete listing of the "Rules of Plate Tectonics", the reader is referred to XXXXXX.
The first "continental drift" flipbook was pushed as an undergraduate research project (Scotese, 1974; 1975abc). Subsequent editions have followed (1976ab; 1978; 1979; 1980; 1990, 1991, 1997, 2004). A more complete description of the data and information that is used to produce the flipbooks can be found in Scotese (2004). These maps could not have been produced without the GPlates plate modelling software and the tectonic data sets published by Dietmar Müller and his team at Earthbytes.
Special thanks to Maggie Geiger, and Robert and Jonathan Scotese for their help assembling this flipbook.
Time Scale
The age given next to each map represents age in millions of years. The corresponding geological ages (Ogg et al., 2008) are:
0 Modern World
20 Ma Early Miocene
40 Ma late Middle Eocene
60 Ma Paleocene
80 Ma Late Cretaceous - Campanian
100 Ma Early Cretaceous - late Albian
120 Ma Early Cretaceous - early Aptian
140 Ma Early Cretaceous - Berriasian
160 Ma Late Jurassic - Oxfordian
180 Ma Early Jurassic - Toarcian
200 Ma Triassic/Jurassic boundary
220 Ma Late Triassic - Carnian
240 Ma Middle Triassic - Anisian
260 Ma Middle Permian - Capitanian
280 Ma Early Permian - Artinskian
300 Ma Late Pennsylvanian
320 Ma Late Mississippian
340 Ma Middle Mississippian
360 Ma Devono-Carboniferous
380 Ma Late Devonian - Frasnian
400 Ma Early Devonian - Emsian
420 Ma Late Silurian - Ludlow
440 Ma Early Silurian - Llandovery
460 Ma Middle Ordovician
480 Ma Early Ordovician
500 Ma Late Cambrian
520 Ma Middle Cambrian
540 Ma Cambrian-Precambrian
560 Ma Neoproterozoic - lt. Ediacaran
600 Ma Neoporterozoic - m. Ediacaran
630 Ma Neoproterozoic - e. Ediacaran
660 Ma Neoproterozoic - e. Ediacaran
690 Ma Neoproterozoic - lt. Cryogenian
720 Ma m. Cryogenian
750 Ma m. Cryogenian
References Cited
Ogg, J., Ogg, G., and Gradstein, F.M., 2008. The Concise Geologic Time Scale, Cambridge University Press, 177 p.
Scotese, C.R. 1974. First Flip Book Images (from 35mm film from PLATO System), Unpublished.
Scotese, C.R., and Baker, D.W., 1975a. Continental drift reconstructions and animation, Journal of Geological Education, 23: 167-171.
Scotese, C.R., 1975b. Continental Drift Flip Book, 1stedition.Chicago, Illinois. (single page version
Scotese, C.R., 1975c. Continental Drift Flip Book, 1st edition. Chicago, Illinois. (double page version)
Scotese, C.R., 1976a. Continental
Drift “Flip Book”, edition 1.5, Department of Geological Sciences, University of Illinois. ResearchGate Academia
Scotese, C.R., 1976b. A continental drift “flip book", Computers & Geosciences, 2:113-116.
Scotese, C.R., and Ziegler, A.M., 1978. Paleozoic continental drift reconstructions and animation, American Geophysical Union, 1978 Spring Annual Meeting, Eos, v. 59. Issue 4, p. 263.
Scotese, C.R., 1979. Continental Drift (flip book), 2nd edition.
Scotese, C.R., Snelson, S.S., and Ross, W.C., 1980. A computer animation of continental drift, J. Geomag. Geoelectr., 32: suppl. III, 61-70.
Scotese, C.R., 1990. Atlas of Phanerozoic Plate Tectonic Reconstructions, PALEOMAP Progress 01-1090a, Department of Geology, University of Texas at Arlington, Texas, 57 pp.
Scotese, C.R., 1991. Continental Drift Flip Book, 4th edition, PALEOMAP Project, Arlington, TX, 49 pp.
Scotese, C.R., 1997. Continental Drift Flip Book, 7th edition, PALEOMAP Project, Department of Geology, University of Texas at Arlington, Texas, 80 pp.
Scotese, 2004.
Seton et al., 2012.
Van der Voo, R., 1993. Paleomagnetism of the Atlantic, Tethys, and Iapetus Oceans, Cambridge University Press, 411 p.
Jacobs, B.F., Pan, A.D., and C. R. Scotese, 2010. A review of the Cenozoic vegetation of Africa, in Cenozoic Mammals of Africa, Werdelin, L., and Sanders, W.J., (editors), University of California Press, Berkeley, CA, p. 57-72. , 2010
2010.02 The aim of this chapter is to review and interpret the Cenozoic paleobotanical record of ... more 2010.02 The aim of this chapter is to review and interpret the Cenozoic paleobotanical record of Africa. Ideally, we want to present a dynamic view of plant community and ecosystem change through time, so that the evolutionary and biogeographic history of Cenozoic African mammals can be considered in the context of the communities to which they belonged. To facilitate this goal, we discuss environmental change in the context of major physiographic change such as graben formation associated with rifting in East Africa, and show paleobotanical sites in their correct position on paleogeographic maps (citations provided in table 5.1). However, spatial and temporal coverage are uneven, allowing detailed paleoenvironmental reconstruction for some localities and only the most general inferences for most time intervals.
Chatterjee, S., Goswami, A., and C.R. Scotese, 2013. The longest voyage: Tectonic, magmatic, and paleoclimatic evolution of the Indian plate during its northward flight from Gondwana to Asia, Gondwana Research, 23: 238-267. , 2013
2013.01 The tectonic evolution of the Indian Plate, which started in Late Jurassic about 167 mill... more 2013.01 The tectonic evolution of the Indian Plate, which started in Late Jurassic about 167 million years ago (approximately 167Ma) with the breakup of Gondwana, presents an exceptional and intricate case history against which a variety of plate tectonic events such as: continental breakup, sea-floor spreading, birth of new oceans, flood basalt volcanism, hotspot tracks, transform faults, subduction, obduction, continental collision, accretion, and mountain building can be investigated. Plate tectonic maps are presented here illustrating the repeated rifting of the Indian plate from surrounding Gondwana continents, its northward migration, and its collision first with the Kohistan-Ladakh Arc at the Indus Suture Zone, and then with Tibet at the Shyok -
Tsangpo Suture. The associations between flood basalts and the recurrent separation of the Indian plate from Gondwana are assessed. The breakup of India from Gondwana and the
opening of the Indian Ocean is thought to have been caused by plate tectonic forces which were localized along zones of weakness caused by mantle plumes (Bouvet, Marion, Kerguelen, and Reunion Plumes). The sequential spreading of the Southwest Indian Ridge/Davie Ridge, Southeast Indian Ridge, Central Indian Ridge, Palitana Ridge, and Carlsberg Ridge in the Indian Ocean were responsible for the fragmentation of the Indian Plate during the Late Jurassic and Cretaceous times. The Reunion and the Kerguelen Plumes left two spectacular hotspot tracks on either side of the Indian Plate. With the breakup of Gondwana, India remained isolated as an island continent, but reestablished its biotic links with Africa during the Late Cretaceous during its collision with the Kohistan-Ladakh Arc ( approximately 85Ma) along the Indus Suture. Soon after
the Deccan eruption, India drifted northward as an island continent by rapid motion carrying Gondwana biota, about 20cm/year, between 67Ma to 50Ma; it slowed down dramatically to 5cm/year during its collision with Asia in early Eocene (approximately 50Ma). A northern corridor was established between India and Asia soon after the collision allowing faunal interchange. This is reflected by mixed Gondwana and Eurasian elements in the fossil record preserved in several continental Eocene formations of India. A revised India-Asia collision model suggests that the Indus Suture represents the obduction zone between India and the Kohistan-Ladakh Arc, whereas the Shyok Suture represents the collision between the Kohistan-Ladakh Arc and Tibet. Eventually, the Indus-Tsangpo Zone became the locus of the final India-Asia collision, which probably began in early Eocene ( approximately 50Ma) with the closure of Neotethys Ocean. The post-collisional tectonics for the last 50 million years is best expressed in the evolution of the
Himalaya-Tibetan Orogen. The great thickness of crust beneath Tibet and Himalaya and a series of north vergent thrust zones in the Himalaya and the south-vergent subduction zones in Tibetan Plateau suggest the progressive convergence between India and Asia of about 2500km since the time of collision. In the early Eohimalayan phase ( approximately 50 to 25Ma) of Himalayan Orogeny (middle Eocene-late Oligocene), thick sediments on the leading edge of the Indian Plate were squeezed, folded, and faulted to form the Tethyan Himalaya. With continuing convergence of India, the architecture of the Himalayan - Tibetan Orogen is dominated by deformational
structures developed in the Neogene Period during the Neohimalayan phase ( approximately 21Ma to present), creating a series of north-vergent thrust belt systems such as the Main Central Thrust, the Main Boundary Thrust, and the Main Frontal Thrust to accommodate crustal shortening. Neogene molassic sediment shed from the rise of the Himalaya was deposited in a
nearly continuous foreland trough in the Siwalik Group containing rich vertebrate assemblages. Tomographic imaging of the India-Asia Orogen reveals that Indian lithospheric slab has been subducted subhorizontally beneath the entire Tibetan Plateau that has played a key role in the uplift of the Tibetan Plateau. The low-viscosity channel flow in response to topographic loading of Tibet provides a mechanism to explain the Himalayan-Tibetan Orogen. From the start of its
voyage in Southern Hemisphere, to its final impact with the Asia, the Indian Plate has experienced changes in climatic conditions both short-term and long-term. We present a series of
paleoclimatic maps illustrating the temperature and precipitation conditions based on estimates of Fast Ocean Atmospheric Model, a coupled global climate model. The uplift of the Himalaya-Tibetan Plateau above the snow line created two most important global climate phenomena-the
birth of the Asian monsoon and the onset of Pleistocene glaciation. As the mountains rose, and the monsoon rains intensified, increasing erosional sediments from the Himalaya were carried down by the Ganga River in the east and the Indus River in the west, and were deposited in two great deep-sea fans, the Bengal and the Indus. Vertebrate fossils provide additional resolution for the timing of three crucial tectonic events: India-KL Arc collision during the Late Cretaceous,
India-Asia collision during the early Eocene, and the rise of the Himalaya during the early Miocene.
2010.03 Palaeobiogeographic analysis of Indian tetrapods during the Late Cretaceous-Early Tertiar... more 2010.03 Palaeobiogeographic analysis of Indian tetrapods during the Late Cretaceous-Early Tertiary time has recognized that both vicariance and geodispersal have played important roles in producing biogeographic congruence. The biogeographic patterns show oscillating cycles of geodispersal (Late Cretaceous), followed by congruent episodes of vicariance and geodispersal (Early Eocene), followed by another geodispersal event (Middle Eocene). New biogeographic synthesis suggests that the Late Cretaceous Indian tetrapod fauna is cosmopolitan with both Gondwanan and Laurasian elements. Throughout most of the Cretaceous, India was separated from the rest of Gondwana, but in the latest Cretaceous it reestablished contact with Africa through Kohistan-Dras (K-D) volcanic arc, and maintained biotic link with South America via Ninetyeast Ridge-Kerguelen-Antarctica corridor. These two geodispersal routes allowed exchanges of “pan-Gondwana” terrestrial tetrapods from Africa, South America, and Madagascar. During that time India also maintained biotic connections with Laurasia across the Neotethys via Kohistan-Dras Arc and Africa. During the Palaeocene, India, welded to the K-D Arc, rafted like a “Noah’s Ark” as an island continent and underwent rapid cladogenesis because of allopatric speciation. Although the Palaeocene fossil record is blank, Early Eocene tetrapods contain both endemic and cosmopolitan elements, but Middle Eocene faunas have strong Asian character. India collided with Asia in Early and Middle Eocene time and established a new northeast corridor for faunal migration to facilitate the bidirectional “Great Asian Interchange” dispersals.
Jacobs, L.L., Strganac, C., and C.R. Scotese, 2011. Plate motions, Gondwana dinosaurs, Noah’s arks, beached Viking funeral ships, ghost ships, and landspans, Anals da Academia Brasileira de Ciencias. v. 83:3-22., 2011
2011.01 Gondwana landmasses have served as large-scale biogeographic Noah's Arks and Beached Viki... more 2011.01 Gondwana landmasses have served as large-scale biogeographic Noah's Arks and Beached Viking Funeral Ships, as defined by McKenna. The latitudinal trajectories of selected Gondwana dinosaur localities were traced through time in order to evaluate their movement through climate zones relative to those in which they originally formed. The dispersal of fauna during the breakup of Gondwana may have been facilitated by the presence of offshelf islands forming landspans (sensu Iturralde-Vinent and MacPhee) in the Equatorial Atlantic Gateway and elsewhere.
Parfenov,L.,Berzin,N.,Badarch,G.,Gombosuren,V.,Bulgatov, A.,Dril, S.,Khanchuk,A.,Kirillova,G.,Kuz’min,Nokleberg,W.,Ogasawara,M.,Obolenskiy,A.,Prokopiev A.,Scotese,C.,et al.,2010. Tectonic and metallogenic model for Northeast Asia,Metallogenesis and tectonics of NEAsia:USG PP 1765,ch. 9,56 p. , 2010
2010.16
Osen, A., Winguth, A., Winguth, C., and C.R. Scotese, 2013. Sensitivity of Late Permian climate to bathymetric features and implications for the mass extinction, Global and Planetary Change, 105:171-179., 2013
2013.02 Evidence from stratigraphic sections of the Panthalassa, Paleo-Tethys and Neo-Tethys sugg... more 2013.02 Evidence from stratigraphic sections of the Panthalassa, Paleo-Tethys and Neo-Tethys suggests that the oceans experienced widespread anoxia during the Late Permian, which likely contributed to the extinction of approximately 90% of marine and approximately 70% of terrestrial species. The Late Permian and Early Triassic were also characterized by significant carbon isotope excursions implying that considerable perturbations in the carbon cycle occurred. Bathymetric features of the Panthalassa during this period are not well known since most of the ocean floor has been subducted; however, tectonic reconstructions suggest that active marine subduction zones surrounded Pangea. Thus, it is reasonable to assume that there was an active mid-ocean ridge system located in Panthalassa during the Late Permian. In this study, the impact of such a spreading center within Panthalassa on the climate and carbon cycle is investigated using a comprehensive climate system model for the end-Permian. This is a novel approach because a majority of previous simulations assumed a flat bottom for the Panthalassa deep-sea. The mid-ocean ridge (MOR) simulation enhanced vertical mixing and topographic steering of the currents near the ridge-axis but in comparison with the simulation using a flat bottom, changes in the global distribution of water masses and circulation in the Panthalassa were insignificant. Dissolved oxygen concentrations were not considerably affected by the implementation of the midocean ridge. Thus the approximation of using a flat-bottom topography in ocean models for the Late Permian remains valid. In a second sensitivity study, the effect of a sill between the deep Paleo-Tethys and Panthalassa on water mass distribution and oxygen content has been investigated. Model results suggest that the introduction of a sill led to enhanced stratification, as well as an increase in salinity and temperature in the Paleo-Tethys. An associated reduction of the dissolved oxygen concentration to dysoxic to near-anoxic conditions below 1800m suggests that the changes in sill height between the Paleo-Tethys and Panthalassa may have been a contributing factor of regional importance to the Permian-Triassic mass extinction
Chen, Xu, Boucot, A.J., Scotese, C.R., 2012. Pangaean aggregation and disaggregation with evidence from global climate belts, Journal of Paleogeography, vol. 1, pp. 5-13., 2012
2012.01 A study of using climate sensitive deposits as a compiled climatic data to locate global ... more 2012.01 A study of using climate sensitive deposits as a compiled climatic data to locate global
climatic belt boundaries through time is developed by the present authors since the 1990s. Global
latitudinal belts were presented from Cambrian to Permian as well as the in terval from the early
Late Cretaceous to the present. However, during the later Permian and into the Early Cretaceous
we noted that the failure of the tropical subtropical belt to penetrate into the interior of Pangaean
resulted in the merging of the two arid belts associated with the northern and southern Hadley
Cells into one vast, interior arid region. A Pangaeanic paleogeography dominates and obviously
affects the climatic distribution from the Late Permian to Early Cretaceous. We employ the
dismission and reoccurrence of the global latitudinal climate belts to determine the aggregation
and disaggregation of the Pangaean.
2009.04 The plate tectonic and palaeogeographic history of the late Proterozoic is a tale of two... more 2009.04 The plate tectonic and palaeogeographic history of the late Proterozoic is a tale of two supercontinents: Rodinia and Pannotia. Rodinia formed during the Grenville Event (c. 1100 Ma) and remained intact until its collision with the Congo continent (800-750 Ma). This collision closed the southern part of the Mozambique Seaway, and triggered the break-up of Rodinia. The Panthalassic Ocean opened as the supercontinent of Rodinia split into a northern half (East Gondwana, Cathaysia and Cimmeria) and a southern half (Laurentia, Amazonia-NW Africa, Baltica, and Siberia). Over the next 150 Ma, North Rodinia rotated counter-clockwise over the North Pole, while South Rodinia rotated clockwise across the South Pole. In the latest Precambrian (650-550 Ma), the three Neoproterozoic continents--North Rodinia, South Rodinia and the Congo continents--collided during the Pan-Africa Event forming the second Neoproterozoic supercontinent, Pannotia (Greater Gondwanaland). Pan-African mountain building and the fall in sea level associated with the assembly of Pannotia may have triggered the extreme Ice House conditions that characterize the middle and late Neoproterozoic. Although the palaeogeographic maps presented here do not prohibit a Snowball Earth, the mapped extent of Neoproterozoic ice sheets favour a bipolar Ice House World with a broad expanse of ocean at the equator. Soon after it was assembled (c. 560 Ma), Pannotia broke apart into the four principal Palaeozoic continents: Laurentia (North America), Baltica (northern Europe), Siberia and Gondwana. The amalgamation and subsequent break-up of Pannotia may have triggered the "Cambrian Explosion". The first economically important accumulations of hydrocarbons are from Neoproterozoic sources. The two major source rocks of this age (Nepa of Siberia and Huqf of Oman) occur in association with massive Neoproterozoic evaporite deposits and in the warm equatorial-subtropical belt, within 30 degrees of the equator.
White, J.M., Jessop, C.M., Scotese, C.R., Lai, G., and R.J. da Roza, 2009. Depicting biostratigraphical data from Palynodata: Experiments and questions in data presentation and manipulation, Palynology, v. 33:157-174. , 2009
2009.01 Experiments are presented here in analysis and depiction of Palynodata records. Palynodat... more 2009.01 Experiments are presented here in analysis and depiction of Palynodata records. Palynodata, a database of pre-Quaternary records of fossil palynomorphs compiled from global literature, is now available as Geological Survey of Canada (GSC) Open File 5793. Palynodata is a non-random sample of the distributions of palynomorphs. Hence, for any taxon, occurrence records in Palynodata serve as a proxy for its "real" distribution in geological time and paleogeographical space. These experiments may be useful starting points for students of palynology in their exploration of Palynodata records. Palynoplot software bins and plots. Palynodata taxa retrievals by time, and by the modern latitude of the study sites. It uses geographical coordinates for the study localities in Palynodata and the geological time scale. Such plots reveal temporal and latitudinal distribution patterns, and potential taxonomic and data problems such as outliers and inconsistent taxonomy. Taxonomic studies can be supported by considering time by latitude distributions, in addition to traditional morphology and priorities. The modern latitude of the sites studied gives increasing distortion with geological age. Palynodata output and the study locality file was input for PaleoGIS software to depict occurrence records on paleogeographical maps. PaleoGIS software showed changing occurrence patterns on rotated plates. An experimental trend surface model of the Jurassic-Cretaceous transition used binned records of common filicale genera which were evolutionarily sensitive between 180 and 100 Ma. The results demonstrate potential for the technique, and lessons for interpretation and future refinement. Common taxa may become useful for biostratigraphical problems and, by calibration against reference sections, this technique might be refined to provide a useful biostratigraphical standard for geological system boundaries. These manipulations of Palynodata records are a "proof-of-concept" demonstration of techniques that may help to reveal the biostratigraphical, paleoecological, and paleoclimatological significance of fossil palynomorphs. Such work also reveals desirable improvements in Palynodata. The precision of indexing species in Palynodata may limit the potential level of chronostratigraphical resolution.
Kominz, M. A., Browning, J. V., Miller, K. G., Sugarman, P. J., Mizintseva, S., and Scotese, C. R., 2008. Late Cretaceous to Miocene sea-level estimates from the New Jersey and Delaware coastal plain coreholes; an error analysis, Basin Research, v. 20, issue 2, p. 211-226, 2008
2008.09
2008.04 Abstract: The stratigraphic and regional distributions of paleosol morphology in latest P... more 2008.04 Abstract: The stratigraphic and regional distributions of paleosol morphology in latest Pennsylvanian through Early Permian strata in Colorado, Utah, Arizona, New Mexico, Texas, and Oklahoma are presented in this paper. This regional extent corresponds to a paleolatitudinal gradient spanning approximately 5 degrees S to 10 degrees N. Morphological trends from this region delineate significant and systematic temporal and spatial changes in Permian-Carboniferous paleoenvironment and paleoclimate. The inferred latest Pennsylvanian (Virgilian) through early Early Permian environmental pattern is complex, but it indicates persistently dry, semiarid to arid conditions in Colorado, Utah, and Arizona, at paleolatitudes north of approximately 2 degrees N, whereas lower paleolatitude (approximately 2 degrees S to 2 degrees N) tropical regions in New Mexico exhibit a stepwise shift from subhumid to semiarid and variably seasonal conditions throughout late Pennsylvanian and the first half of Early Permian (Virgilian through Wolfcampian) time, followed by a subsequent shift to more arid conditions during the latter part of the Early Permian (Leonardian). Notably, strata from the southernmost paleosites, in Texas and Oklahoma, exhibit the most significant and abrupt climate changes through this period; they show a rapid transition from nearly ever-wet latest Pennsylvanian climate (at approximately 5 degrees S) to drier and seasonal climate across the Permian-Carboniferous system boundary, and finally to arid and seasonal climate by Leonardian time (at approximately 2-4 degrees N). The inferred climate patterns show no robust long-term correlation with the high-latitude Gondwanan records of glaciation. Rather, the long-term record of Permian-Pennsylvanian climate indicators from the southwestern United States is most simply explained by an approximately 8 degrees northward tectonic drift through (essentially) static climate zones over western tropical Pangea during the interval of study. However, the relatively rapid perturbations to climate recorded by these pedogenic archives appear to be too rapid for tectonic forces and might correspond to changes in climate drivers, such as atmospheric pCO (sub 2) , atmospheric circulation, and glacial-interglacial cycles.
Geophysical Journal International, 2005
2005.03 Synthetic apparent polar wander (APW) paths for North America, South America, Eurasia, In... more 2005.03 Synthetic apparent polar wander (APW) paths for North America, South America, Eurasia, India, Central Africa, Australia and Antarctica for the last 200 Myr are proposed. Computation of these APW paths is based upon the latest version (4.5a) of the Global Paleomagnetic Database (GPMDB), a revised global plate tectonic model since the Early Jurassic, and a new technique for generating smoothed APW paths. The smoothing technique includes the following steps: (1) pre-selection of palaeopoles, including pre-filtering parameters (number of sites, number of samples per site, 95 per cent confidence circle about mean direction, cleaning procedure, and time uncertainty); (2) generation of palaeolatitude and declination plots for a reference site on each continent that combines palaeopoles via a global plate tectonic circuit; (3) independent spline regression analyses of the palaeolatitude and declination plots; (4) removal of palaeolatitude or declination data that deviate by more than 10° from the regression curves (post-filtering process); (5) generation of synthetic APW paths from the resulting palaeolatitude and declination plots. These synthetic APW paths are then rotated into African coordinates to determine the best-fit APW path and a global palaeomagnetic reference frame. Four representative plate tectonic reconstructions and global plate velocity fields are presented for the three time intervals that correspond to globally synchronous changes in plate motion.
Scotese, C., Nokleberg, W., Monger, J., Norton, I., Parfenov, L., Khanchuk, A., Bundtzen, T., Dawson, K., Eremin, R., Frolov, Y., Fujita, K., Goryachev, N., Pozdeev, A., et al., 2001. Dynamic computer model for the metallogenesis and tectonics of the Circum-North Pacific, USGS, OF 01-0261., 2001
2001.03
Nokleberg, W., Bundtzen, T., Eremin, R., Ratkin, V., Dawson, K., Shpikerman, V., Goryachev, N., Byalobzhesky, S., Frolov, Yu., Khanchuk, A., Koch, R., Monger, Scotese, C., et al. 2005. Metallogenesis and tectonics of the Russian Far East, Alaska, and the Canadian Cordillera, USGS PP 1697, 397 pp. , 2005
2005.04 The Proterozoic and Phanerozoic metallogenic and tectonic evolution of the Russian Far Ea... more 2005.04 The Proterozoic and Phanerozoic metallogenic and tectonic evolution of the Russian Far East, Alaska, and the Canadian Cordillera is recorded in the cratons, craton margins, and orogenic collages of the Circum- North Pacific mountain belts that separate the North Pacific from the eastern North Asian and western North American Cratons. The collages consist of tectonostratigraphic terranes and contained metallogenic belts, which are composed of fragments of igneous arcs, accretionary-wedge and subduction-zone complexes, passive continental margins, and cratons. The terranes are overlapped by continental-margin-arc and sedimentary-basin assemblages and contained metallogenic belts. The metallogenic and geologic history of terranes, overlap assemblages, cratons, and craton margins has been complicated by postaccretion dismemberment and translation during strike-slip faulting that occurred subparallel to continental margins.
Eos, Transactions American Geophysical Union, 2001
2001.02
2006.01 Reconstructions of Phanerozoic CO2 levels have generally relied on geochemical modeling o... more 2006.01 Reconstructions of Phanerozoic CO2 levels have generally relied on geochemical modeling or proxy data. Because the uncertainty inherent in such reconstructions is large enough to be climatically significant, inverse climate modeling may help to constrain paleo-CO2 estimates. In particular, we test the plausibility of this technique by focusing on the climate from 360 to 260 Ma, a time in which the Siberian landmass was in middle to high latitudes, yet had little or no permanent land ice. Our climate model simulations predict a lower limit for CO2—the value beneath which Siberia acquires “excess” ice. Simulations provide little new information for the period in which Siberia was at a relatively low paleoaltitude (360 340 Ma), but model results imply that paleo-CO2 levels had to be greater than 2 4× modern values to be consistent with an apparently ice-free Siberia in the late Permian. These results for the later period in general agree with soil CO2 proxies and the timing of Gondwanan deglaciation, thus providing support for a significant CO2 increase before the end-Permian boundary event. Our technique may be applicable to other time intervals of unipolar glaciation.
2007.06 General circulation models (GCMs) are useful tools for investigating the characteristics ... more 2007.06 General circulation models (GCMs) are useful tools for investigating the characteristics and dynamics of past climates. Understanding of past climates contributes significantly to our overall understanding of Earth's climate system. One of the most time consuming, and often daunting, tasks facing the paleoclimate modeler, particularly those without a geological background, is the production of surface boundary conditions for past time periods. These boundary conditions consist of, at a minimum, continental configurations derived from plate tectonic modeling, topography, bathymetry, and a vegetation distribution. Typically, each researcher develops a unique set of boundary conditions for use in their simulations. Thus, unlike simulations of modern climate, basic assumptions in paleo surface boundary conditions can vary from researcher to researcher. This makes comparisons between results from multiple researchers difficult and, thus, hinders the integration of studies across the broader community. Unless special changes to surface conditions are warranted, researcher dependent boundary conditions are not the most efficient way to proceed in paleoclimate investigations. Here we present surface boundary conditions (land-sea distribution, paleotopography, paleobathymetry, and paleovegetation distribution) for four Cretaceous time slices (120 Ma, 110 Ma, 90 Ma, and 70 Ma). These boundary conditions are modified from base datasets to be appropriate for incorporation into numerical studies of Earth's climate and are available in NetCDF format upon request from the lead author. The land-sea distribution, bathymetry, and topography are based on the 1°×1° (latitude × longitude) paleo Digital Elevation Models (paleoDEMs) of Christopher Scotese. Those paleoDEMs were adjusted using the paleogeographical reconstructions of Ronald Blakey (Northern Arizona University) and published literature and were then modified for use in GCMs. The paleovegetation distribution is based on published data and reconstructions and consultation with members of the paleobotanical community and is represented as generalized biomes that should be easily translatable to many vegetation-modeling schemes.
2004.07 Abstract: Compilation of climatically sensitive deposits (chiefly evaporites, calcretes, ... more 2004.07 Abstract: Compilation of climatically sensitive deposits (chiefly evaporites, calcretes, coals, bauxites, kaolin’s and kaolinites, tillites, dropstones, glendonites and cool-water marine sediments, palms, as well as crocodilians etc.) through twenty-seven Phanerozoic time intervals enables one to revise the contemporary paleogeography in a manner consistent with the climatic information. We also take account of some of the available biogeographic information. Comparison of the changing Phanerozoic global climatic gradients based on geological evidence with the previously published models of Phanerozoic atmospheric CO (sub 2) based on geochemical assumptions indicates that either the assumptions on which the geochemical models are based are erroneous or that atmospheric CO (sub 2) is not a greenhouse gas. We prefer the former possibility.
Palaeogeography Palaeoclimatology Palaeoecology, 2000
2000.01
Peters, K. E., Ramos, L. S., Zumberge, J. E., Zenon V., and, Scotese, C. R., 2008. Restoration of circum-Arctic Upper Jurassic source rock paleolatitude based on crude oil geochemistry, AAPG Annual Convention and Exhibition, San Antonio, Texas, Abstracts Volume, p. , 2008
2008.02 Tectonic geochemical paleolatitude (TGP) models were developed to predict the paleolatitu... more 2008.02 Tectonic geochemical paleolatitude (TGP) models were developed to predict the paleolatitude of petroleum source rock from the geochemical composition of crude oil. The results validate studies designed to reconstruct ancient source rock depositional environments using oil chemistry and tectonic reconstruction of paleogeography from coordinates of the present day collection site. TGP models can also be used to corroborate tectonic paleolatitude in cases where the predicted paleogeography conflicts with the depositional setting predicted by the oil chemistry, or to predict paleolatitude when the present day collection locality is far removed from the source rock, as might occur due to long distance subsurface migration or transport of tarballs by ocean currents. Biomarker and stable carbon isotope ratios were measured for 496 crude oil samples inferred to originate from Upper Jurassic source rock in West Siberia, the North Sea and offshore Labrador. First, a unique, multi-tiered chemometric (multivariate statistics) decision tree was used to classify these samples into seven oil families and infer the type of organic matter, lithology and depositional environment of each organofacies of source rock [Peters, K.E., Ramos, L.S., Zumberge, J.E., Valin, Z.C., Scotese, C.R., Gautier, D.L., 2007. Circum-Arctic petroleum systems identified using decision-tree chemometrics. American Association of Petroleum Geologists Bulletin 91, 877-913]. Second, present day geographic locations for each sample were used to restore the tectonic paleolatitude of the source rock during Late Jurassic time (approximately 150 Ma). Third, partial least squares regression (PLSR) was used to construct inear TGP models that relate tectonic and geochemical paleolatitude, where the latter is based on 19 source-related biomarker and isotope ratios for each oil family. The TGP models were calibrated using 70% of the samples in each family and the remaining 30% of samples were used for model validation. Positive relationships exist between tectonic and geochemical paleolatitude for each family. Standard error of prediction for geochemical paleolatitude ranges from 0.9 degrees to 2.6 degrees of tectonic paleolatitude, which translates to a relative standard error of prediction in the range 1.5-4.8%. The results suggest that the observed effect of source rock paleolatitude on crude oil composition is caused by (i) stable carbon isotope fractionation during photosynthetic fixation of carbon and (ii) species diversity at different latitudes during Late Jurassic time.
Aapg Bulletin, 2007
2007.03
Scotese, C.R. and McKerrow, W.S., 1990. Revised world maps and introduction, in Paleozoic Paleogeography and Biogeography, W.S. McKerrow and C.R. Scotese (editors), Geological Society of London, Memoir 12, pp. 1-21. , 1990
1990.04
These maps were produced by the combined efforts of the PALEOMAP Project (International Liuthosph... more These maps were produced by the combined efforts of the PALEOMAP Project (International Liuthosphere Program) and Mobile Exploration and Production Services. These 28 paleogeographic reconstrcutions illustrate the changing configuration of mountains, land, shallow seas, and deep ocean basins during the last 545 million years. The active plate boundaries, such as spreading centers and and subduction zones, are also shown. All age assignments are based on the Decade of North American Geology timescale.
Golonka, J., Ross, M.I., and Scotese, C.R., 1994. Phanerozoic Paleogeographic and Paleoclimatic Modeling Maps, in A. F. Embry, B. Beauchamp, and D.J. Glass (editors), Pangea, Global Environments and Resources, Canadian Society of Petroleum Geologists, Memoir 17, p. 1-47., 1994
McKerrow, W.S. and Scotese, C.R. (editors),1990. Paleozoic Paleogeography and Biogeography, Geological Society of London, Memoir 12, 435 p., 1990
1990.03
Jurdy, D. M., Stefanick, M., and Scotese, C.R., 1995. Paleozoic plate dynamics, Journal of Geophysical Research, v. 100, no. B9, pp. 17965-17975. , 1995
1995.01 Current plate motions can be accounted for by a balance of active forces, slab pull, ridg... more 1995.01 Current plate motions can be accounted for by a balance of active forces, slab pull, ridge push, and, for continental plates, trench suction, with drag beneath the plate as a resistive force. If we assume that the same forces have acted through time, we can reconstruct plate motions from the geometry of past plate boundaries. Paleozoic reconstructions are made with paleomagnetic, tectonic, climatic, and biogeographic data, as no ocean floor remains. PALEOMAP reconstructions are used to estimate past plate speeds and to test simple dynamical models in order to determine which ranges of forces best accounts for the observations. Over the last 600 m.y., plate speeds averaged over 40- to 100-m.y. intervals show considerable variation; Gondwana's speed oscillates from 20 to 60 km/m.y. over a long timescale (200-400 m.y.) with considerable noise superposed. Over the Paleozoic Era motions for large continental regions average 28 km/m.y.; force balance models based on present-day observations suggest that continental regions without a large attached slab would move 30 mm/yr. The opening and closing of the ocean between Laurentia and Gondwana 560-400 Ma is used to test dynamical models and the parameter values assumed. In the late Precambrian, Laurentia rifted away from Gondwana. In the earliest Cambrian it was near 40 degrees S; by Late Cambrian and Ordovician it had moved to the equator. During the Silurian and Devonian, Laurentia reversed direction and later collided with Gondwana at 40 degrees S. In a model of the forces acting on the plates, slab pull, ridge push, and trench suction are assumed to balance plate drag. Only certain ranges of ridge-push and trench parameters can model both the opening and subsequent closing of the ocean. The dynamic models, with parameter values inferred from present rates, bracket the rates required by the reconstructions.
Scotese, C.R., 1999. Teaching Earth System History: A Computer Assisted Approach, Geological Society of America Short Course Notes, Geological Society of America Annual Meeting, October 24, 1999, Denver, CO, 171 pp., 1999
1999.10
Worsley, T. R., Moore, T. L., Fraticelli, C. M., and Scotese, C.R., 1994. Phanerozoic CO2 levels and global temperatures inferred from changing paleogeography, GSA Special Paper 288, p. 57-73, Boulder, CO. , 1994
1994.02 A simple model that tracks global land area and its average latitude to specify CO2 level... more 1994.02 A simple model that tracks global land area and its average latitude to specify CO2 levels and consequent surface temperatures has been used to infer paleotem-peratures of 20 Phanerozoic global paleogeographic reconstructions. The model is based on the premise that global CO2 levels and temperature are directly proportional to the average latitude of the world landmass and inversely proportional to total land area. In all 20 cases, inferred CO2 and paleotemperature values are plausible and generally compatible with previous estimates. However, raw model output must be refined to take into account changes in rates of other climate modifiers such as orogeny, organic carbon burial, and precipitation that can be inferred from additional evidence. Results show a warm (19 degrees C) ice-free Cambrian world of small land area (75% emergent) at mid-latitudes (35 degrees ). Rapid equatorward migration of world landmass to 25 degrees latitude then led to a cool (13 degrees C) ice-capped late Ordovician world that was 70% emergent. Equally rapid migration back to higher latitudes (39 degrees ) by the Silurian coupled with decreased emergence (64%) produced the warmest temperatures of the Phanerozoic (22 degrees ). Return of the landmass to mid-latitudes (32 degrees ) coupled with reemergence (71%) by early Devonian reestablished cooler (18 degrees ) temperatures. As Pangea coalesced from early Devonian to late Carboniferous, percent emergence continually increased to virtually 100% as average latitude continually increased to 38 degrees , resulting in an ice-capped world of 16 degrees C. High organic carbon burial rates and orogeny at that time would suggest that our temperature estimates are slightly too high for this interval. By early Triassic, our results indicate continual iceenhanced emergence at virtually 100% and equatorward migration of land to 33 degrees latitude, yielding a global temperature of 16 degrees C. Other lines of evidence (absence of ice, low organic carbon burial, weak orogeny, aridity) suggest a slightly warmer world, or at least one with a lower pole-equator thermal gradient. From Triassic to mid Cretaceous, average latitude again increased to 38 degrees and emergence decreased to 75%, producing a warming of global temperature to 20 degrees C. Cretaceous to Recent results indicate that average latitude of the landmass decreases to 30 degrees as India and Australia move equatorward and that there is an increase to as much as 100% emergence during maximum late Cenozoic ice-sheet growth. Corresponding global temperatures decline to as low as 13 degrees C.
Scotese, C.R., Boucot, A.J., and McKerrow, W.S., 1999. Gondwanan paleogeography and paleoclimatology, in Gondwana 10: Event Stratigraphy, Journal of African Earth Sciences, v. 28, issue 1, pp. 99-114., 1999
1999.03
Scotese, C.R. and Barrett, S.F., 1990. Gondwana's movement over the South Pole during the Paleozoic: evidence from lithologic indicators of climate, in Paleozoic Paleogeography and Biogeography, W.S. McKerrow and C.R. Scotese (editors), Geological Society of London, Memoir 12, pp. 75-85., 1990
1990.06 A statistical technique is described that uses the geographical distribution of lithologi... more 1990.06 A statistical technique is described that uses the geographical distribution of lithological indicators of climate (carbonates, evaporites, coals and tillites) to estimate the past position of the geographic pole. This technique was used to estimate the movement of the South Pole across the supercontinent of Gondwana during the Palaeozoic. Results indicate that during the Cambrian and Early Ordovician the South Pole was located adjacent to northwestern Africa. The pole moved into the Amazon Basin during the Late Ordovician and into south-central Argentina during the Silurian. Throughout the Devonian and Early Carboniferous the pole moved slowly from a location in southern Argentina to a position near the south coast of Africa. From the Late Carboniferous and into the Permian the South Pole swung eastward across central Antarctica. The Early Palaeozoic and Late Palaeozoic portions of the palaeoclimatically determined APW (apparent polar wander) path are in good agreement with available palaeomagnetic data. The Middle Palaeozoic portion of the palaeoclimatically determined APW path agrees better with the palaeomagnetic data that places the South Pole in southern Argentina, than with the palaeomagnetic results that place the Devonian pole in central Africa.
hatterjee, S. and Scotese, C.R., 1999. The Breakup of Gondwana and the Evolution and Biogeography of the Indian Plate, Proceedings of the Indian National Sci. Acad., Part A: Phys. Sci., v. 65A, No. 3, pp. 397-425., 1999
1999.02 The palaeopositions of India after its breakup from Gondwana and its subsequent northward... more 1999.02 The palaeopositions of India after its breakup from Gondwana and its subsequent northward journey during the Mesozoic and Early Palaeogene pose many plate tectonic and palaeobiogeographic riddles. Most reconstructions show peninsular India separating from Gondwana, and remaining an island continent for more than 100 million years until it collided with Asia. However, the lack of endemism among Indian Cretaceous terrestrial vertebrates is clearly inconsistent with the island continent hypothesis. A new model for the tectonic evolution of the Indian plate from its Pangean origin to the present day is proposed that is well constrained by geological and geophysical evidence. In this model, a previously unrecognized land area, called Greater Somalia, occupied the position between eastern Arabia and northwestern India. During the Late Jurassic, India rifted away from Greater Somalia. Throughout most of the Cretaceous India was separated from the rest of Gondwana but in the latest Cretaceous it reestablished contact with Africa through Greater Somalia. India maintained contact until the Eocene Period when it collided with Asia. Based on this plate tectonic model, 14 new paleogeographic maps are presented showing the evolution of the Indian plate from its Pangean origin to its final union with Asia. An area cladogram identifies the 11 nodes of hierarchial tectonic evolution of the Indian plate during the last 250 million years. A major question of Indian palaeobiogeography is how the terrestrial vertebrates such as dinosaurs responded to fragmentation of India from Gondwana. The similarities and differences between Indian vertebrates with those of other continental fragments provide an independent check for a number of key events during its tectonic evolution. Using the plate tectonic reconstructions as a guide, the distributions of dinosaurs and other vertebrates during the Mesozoic and Early Cenozoic are discussed. A close correspondence between the continental position of India and the distribution of vertebrates is generally observed. However, the Indian vertebrate fauna seems more closely related to Europe at the familial level to that of Africa during the Mesozoic. This disjunct endemism of fossil distribution pattern may reflect poor sampling from the intervening Africa. Whenever Indian vertebrate records are missing from certain geologic periods, their compositions are inferred from the contemporary animals in adajacent landmasses. The Late Triassic and Jurassic vertebrates of India are cosmopolitan in the Pangean world indicating various transcontinental migration routes. Four such dispersal routes are identified, northern, central, southern and western. During the mid-Cretaceous, India became isolated and these dispersal routes were closed. During the Late Cretaceous (approximately 70 Ma), the northern route across the Greater Somalia was reopened allowing immigration of dinosaurs and other vertebrates from Africa and Europe. This northern dispersal route explains for the first time why the Indian Maastrichtian vertebrates do not show any evidence of endemism. About 65 million years ago, the Shiva impact event at the Indo-Seychelles boundary and the Chicxulub impact in Mexico triggered a biotic catastrophe and led to the demise of dinosaurs and other organisms. Mammals rebounded from this catastrophe and became the dominant land vertebrates during the early Tertiary. Fossil evidence suggests that India made the initial contact with Asia during the Eocene and opened a new northeastern corridor for faunal interchange.
Scotese, C.R., 1998. Gondwana’s climate changes, in J. Almond et al., (editors), Special Abstracts Issue, Gondwana 10: Event Stratigraphy of Gondwana, Journal of African Earth Sciences, v. 27, n. 1A, p. 172-173., 1998
1998.05 Climate can change on two scales: globally and regionally. Regional climatic change is si... more 1998.05 Climate can change on two scales: globally and regionally. Regional climatic change is simply the result of movement of a continent across Earth's climatic zones. During its long history Gondwana crossed numerous climatic belts. During the Late Precambrian and Early Palaeozoic this was especially true for the western part of Gondwana (northern South America and western Africa), which moved from south polar latitudes to equatorial latitudes. In contrast, Australia. Antarctica and the Cathaysian Terranes of northeastern Gondwana remained at relatively low latitudes throughout most of the Early and Middle Palaeozoic. The opposite was true for the Late Palaeozoic and Early Mesozoic. Eastern Gondwana (India and Australia) moved rapidly from subtropical to polar latitudes during the Carboniferous, Permian and Triassic, while the western half of Gondwana (northern South America and western Africa, remained at subtropical latitudes. During the Jurassic and Cretaceous the general tendency has been for all the Gondwana continents to move northward, either from subtropical to equatorial positions (Africa, Arabia, and India), or from temperate to tropical positions (Australia). Antarctica has remained near the South Pole for 300 Ma and South America, though it has shifted westwards, has not changed latitude by more than 20 degrees during the last 300 Ma.
Superimposed on regional climate change is a global climatic signal.. During the 400 Ma that Gondwana existed, the Earth's global climate system shifted from 'Ice House' conditions to ’Hot House' conditions four times (Fig. 1). The first Ice House episode was the great Vendian Ice Age, which was just ending as Gondwana became fully assembled. The collisions which formed Gondwana may have a had a role in creating Ice House conditions during the Late Precambrian. This Ice House world was followed by global warming during the Cambrian and Early-Middle Ordovician. The second Ice House episode was a brief, but extensive period of global cooling during the latest Ordovican ( earliest Silurian?). It was followed by global warming from the Silurian through to the Middle Devonian. The third episode of Ice House conditions began in the Late Devonian-Early Carboniferous, expanded during the Middle Carboniferous (Namurian B), and terminated during the Early Permian (Artinskian). This Ice House world was followed by global warming during the Late Permian, Triassic, and Early and Middle Jurassic. Geological indicators of climate and palaeontological evidence suggests that Earth may have experienced 'run away' greenhouse warming at the end of the Palaeozoic. This 'Super Hot House World' may have been responsible for the Late Permian mass extinction event. The final episode of global cooling, during the Late Jurassic and Early Cretaceous, was a 'mild' Ice House episode, by all accounts. It was followed by the Cretaceous and Early Tertiary Hot House World.
In this presentation, palaeoclimatic reconstructions will be presented for 8 time intervals, corresponding to the 4 major Ice House (I) and Hot House (H) couplets: (I1) Vendian (650 Ma), (H1) Late Cambrian Early Ordovician (500 Ma); (I2) Late Ordovician (450 Ma), (H2) Siluro- Devonian (400 Ma); (I3) Late Carboniferous-Early Permian (300 Ma), (H3) Early Triassic (240 Ma); and (i4) Late Jurassic-Early Cretaceous (140 Ma), (H4) Late Cretaceous (80 Ma). The changing distribution of climatically sensitive lithofacies, such as coals, evaporites. calcretes, bauxites, kaolinites. glendonites and tillites, will be plotted on maps, as well as the results of recent palaeoclimatic simulations.
Scotese, C.R., 1998. What we really don’t know about the plate tectonic, palaeogeographic, palaeoclimatic and biogeographic history of Gondwana in J. Almond et al., (editors), Special Abstracts Issue, Gondwana 10: Event Stratigraphy of Gondwana, Journal of Af. Earth Sci., v. 27, n. 1A, p. 173-174., 1998
1998.03 During the past 20 years, as a result of careful revisions and refinements, the broad pla... more 1998.03 During the past 20 years, as a result of careful revisions and refinements, the broad plate tectonic, palaeogeographic, palaeoclimatic, and biogeographic history of Gondwana has become well known. The supercontinent of Gondwana was wrought during the Pan-African collisional event (600 Ma ago) and remained intact for over 400 Ma. During that time interval it crossed the South Pole, joined the northern continents to form Pangaea, and split apart in 3 distinct phases beginning in the Early Jurassic and ending in the Late Cretaceous. So what else is new? What more is there to know? Lots.
Though the broad outline is well known, important questions remain unanswered. Regarding its formation, 'How many continents were involved?', 'What was the exact timing of collision between these pieces?', 'What was the polarity of subduction?', 'When, exactly, was the process finished?'. 'What, if anything, did the formation of Gondwana have to do with the Vendian Ice Age, or the diversification of metazoans?'.
Gondwana was largely intact, and traversed the South Pole during the Palaeozoic, however, the details of its Palaeozoic history are not well known. For instance, 'What initiated subduction along the Tasman-Transantarctic-Cape Trend?'. 'Does palaeomagnetic and palaeoclimatic eyidence from Gondwana support a period of rapid True Polar Wander during the Late Precambrian-Early Cambrian?', 'What path did Gondwana take as it crossed the South Pole? Was it slow, steady, or rapid with loops and twirls?'. 'How extensive was the Late Ordovician Ice sheet?, Did it really stretch from Cape Town to Yemen?', and 'Can we make sense out of the history of terrane accretion in southern South America and eastern Ausutralia?'.
During the Early Palaeozoic, the Cathaysian and Cimmerian Terranes seemed to be associated with the Indo-Australian region of Gondwana, 'Where exactly were they located?', and 'When did they rift away from Gondwana?'. Biogeographically speaking, 'What does the distribution of the earliest fossil fish tell us about Siluro-Devonian palaeogeography?', 'When did the first terrestrial vertebrates arrive in Australia?', and 'Where did they come from?'.
The Early Jurassic through Late Cretaceous break-up of Gondwana is well documented by geological, tectonic, and marine geophysical data, however a few nagging questions remain. 'Are the Karoo rifts a precursor to Gondwana break-up, or an earlier, unrelated event?', 'What was the fit of the continents that comprised eastern Gondwana?', 'Was it a loose fit or a tight fit?', 'How exactly does India fit against Madagascar?', 'What went in that gap between northwestern India and Arabia?', 'What rifted away from northwestern Australia?', 'Was there a large chunk of continental crust north of India (Greater India)?', 'Where did it go?'. Concerning the break-up of Gondwana: 'Were the Early Jurassic flood basalts of South America, South Africa, and East Antarctica produced by a hot spot, or do they signal the beginning of break-up?', 'Why did Gondwana break apart, in the first place?', 'Why did the break-up take place in 3 distinct stages {Middle Jurassic, Early Cretaceous. Late Cretaceous)?'.
During the Late Cretaceous. Gondwona was in its final phase of dispersal, yet important questions remain, 'Why can't we get the older M anomalies to fit togther properly?', 'What caused the Deccan flood basalts?', 'Is there a relationship between these flood basalts and the K/T extinction?', 'When was the ligation between Africa and South America terminated?', and 'How did those darn dinosaurs get from Africa to India in the Late Cretaceous?!'. I would like answers to these questions. Realizing, however, that it is often easier to ask questions rather than seek out solutions, I would like to review various solutions and relate my own answers to these questions, however fantastic and controversial they may be.
Scotese, C.R., 1998. A tale of two supercontinents: the assembly of Rodinia, its break-up, and the formation of Pannotia during the Pan-African event, in J. Almond et al. (editors), Special Abstracts Issue, Gondwana 10: Event Stratigraphy of Gondwana, J. Afr. Earth Sci., v. 27, n. 1A, pp. 171., 1998
1998.12 Recent tectonic syntheses by I. Dalziel. P. Hoffman, E- Moores, and J. Rodgers, as well a... more 1998.12 Recent tectonic syntheses by I. Dalziel. P. Hoffman, E- Moores, and J. Rodgers, as well as palaeomagnetic summaries by J. Meert, C. Powell, T. Torsvik, and R. van der Voo, have led to the proposal that there were two Late Precambrian supercontinents: Rodinia and Pannotia. Rodinia formed during the Grenville event 1-1100 Ma) and broke apart approximately 750 Ma ago. The rifted fragments of Rodinia sequentially collided during the Pan- African Orogeny (700-550 Ma) forming a new supercontinent, Pannotia.
Though the exact Size end configuration of Rodinia is not known, it appears that North America formed the core of this supercontinent. The cast coast of North America was adjacent to western South America and the west coast of North America lay next to Australia and Antarctica. About 750 Ma ago, Rodinia collided with a smaller continent, the Congo Craton. This collision is marked by the Mozambique Granulite Belt of East Africa. As shown in Fig. 1, this collision may have triggered the break-up of Rodinia. Rodinia split into two halves, opening the Panthalassic Ocean. North America, together with Baltica. Siberia, and the Saharan and Amazonian Cratons, rotated southward towards the South Pole. The other half of Rodinia. composed primarily of East Gondwana {Antarctica. Australia, India. Arabia) and the continental fragments that would one day become China and the Middle East, rotated counter-clockwise, northwards across the North Pole. Between the two halves of Rodinia lay a third continent, the Congo Craton, made up of much of north central Africa. From 750 to 600 Ma, the Mozambique Seaway between the northern half of Rodinia (East Gondwana) and the Congo Craton progressively closed. Oceanic crust was subducted beneath the Congo Craton. generating the Hijaz island-arc of Cgypt, Arabia and Sudan. On the south side of the Congo Craton, the Pan-African Ocean was consumed as the southern half of Rodinia {the Saharan and Amazonian Cratons, among others), swung northward, eventually colliding with the Congo Craton between 650 and 550 Ma (Fig. 1).
The sequence of continental collisions that started 750 Ma ago and continued to the end of the Precambnan {approximately 550 Ma) assembled the supercontinent of Pannotia, with Gondwana at its core. Pan-African mountain building produced a series of mountain ranges of Himalyan proportions. These mountain ranges occupied low palaeolatitudes and, like the modem Himalayas, may have triggered the episode of Vendlan glaciation. The supercontinent of Pannotia was short lived and began to rift apart in the latest Precambrian (-570 Ma).
Plate tectonic reconstructions for 1100, 850, 750, 700. 650, 600 and 550 Ma. together with a computer animation of plate motions during the same time interval will be shown. A palaeogeographic reconstruction showing the ancient distribution of mountains, land, shallow sea, and deep sea will be presented for 650 Ma (Vendian Ice Age). It is suggested that the Vendian Ice Age was mainly due to palaeogeographic effects, namely the location of land areas near the poles, and the presence of Himalyan-sized mountain ranges near the Equator.
Journal of The Geological Society, 1992
1992.01
Scotese, C.R., Totterdell, J.M., Holliday, S. and Langford, R.P, 1985. Paleogeographic Mapping Software for the Intergraph Work Station. BMR-AMIRA Paleogeographic Project, Special Report, Bureau of Mineral Resources, Canberra, Australia, 136 pp., 1985
1985.12 This report describes a set of programs that produces palaeocontinental reconstructions i... more 1985.12 This report describes a set of programs that produces palaeocontinental reconstructions illustrating the positions of the continents during the last 600 million years and plots on these base maps lithologic information portraying the llthofacies and environments of deposition. These programs are based on the PALEOMAP software package written by C.R. Scotese, and the lithologic data illustrated on these data maps have been compiled by A.M. Ziegler and associates, as part of the Palaeogeographic Atlas Project, University of Chicago. The PALEOMAP software package was installed on the Intergraph system in the Division of Continental Geology, Bureau of Mineral Resources by C.R. Scotese, with the help of J.M. Totterdell, S. Holliday, and R.P. Langford during November of 1985.This report 1) describes the programs that comprise the PALEOMAP software package, 2) provides illustrations of the output of these programs (Table 1; Figures 2-45), 3) provides examples of the user input required to run the programs (Appendices A-D), and 4) documents both the programs (Appendices E-H) and lithologic data that were used to produce the paleogeographic lithofacies maps of Australia (Appendices I-Y).
Scotese, C.R., Gahagan, L.M., and Larson, R.L., 1988. Plate tectonic reconstructions of the Cretaceous and Cenozoic ocean basins, in 8th Geodynamics Symposium, Mesozoic and Cenozoic Plate Reconstructions, C.R. Scotese & W.W. Sager (editors), Tectonophysics, 155:261-283., 1988
1988.02
Scotese, C.R. and Summerhayes, C.P., 1986. Computer model of paleoclimate to predict upwelling in the Mesozoic and Cenozoic. Geobyte, 1:28-42., 1986
1986.02 A computer program has been developed that models paleoclimate using a parametric approac... more 1986.02 A computer program has been developed that models paleoclimate using a parametric approach. The program generates atmospheric pressure values and contours them to produce atmospheric pressure for past times of known land and sea distribution. Wind directions inferred from the pressure distribution can be added to the maps to show where coastal upwelling may have taken place. Organic-rich muds form in such places today, thus upwelling predictions from paleoclimate models may provide clues about the distribution of potential petroleum source rocks. These predictions proved satisfactory for the Volgian and Cenomanian, the two times for which maps of organic-rich rocks were readily available. Similar test are recommended for other time slices. The paleoclimate maps derived by the computer modeling approach use here are preliminary. Nevertheless they offer a reasonable best-guess as to the earth's climate in the past. Eventually, more sophisticated modeling techniques may provide netter results.
Scotese, C.R., Gahagan, L.M., Ross, M.I., Royer, J.Y., Nuernberg, D., Mayes, C.L., Lawver, L., Tomlins, R.L., Newman, J.S., Heubeck, C.E., Winn, J.K., Beckley, L., and Sclater, J.G., 1987. Phanerozoic Plate Tectonic Reconstructions, Tech. Report 90, Instit. Geophys., U. Texas, Austin, 20 pp., 1987
1987.09
Scotese, C.R. and Sager, W.W., 1988. 8th Geodynamics Symposium, Mesozoic and Cenozoic Plate Reconstructions, Tectonophysics, v. 155, issues 1-4, pp. 1-399., 1988
1988.01
Bally, A.W., Scotese, C.R., and Ross, M.I., North America: Plate tectonic setting and tectonic elements, in A.W. Bally and A.R. Palmer, (editors), The Geology of North America; An Overview, Decade of North American Geology, The Geology of North America, Volume A., 1-15. , 1989
1989.01
Tectonophysics, 1988
1988.09
Royer, J.-Y., Patriat, P., Bergh, H., and Scotese, C.R., 1988. Evolution of the southwest Indian Ridge from the Late Cretaceous (anomaly 34) to the Middle Eocene (anomaly 20), Tectonophysics, 155:235-260, 1988
1988.03
Gahagan, L.M., Scotese, C.R., Royer, J.Y., Sandwell, D.T., Winn, K., Tomlins, R., Ross, M.I., Newman, J.S., Mueller, D., Mayes, C.L., Lawver, L.A. and Heubeck, C.E., Tectonic fabric map of the ocean basins from satellite altimetry data, Tectonophysics, 155:1-26. (39), 1988
1988.04
Van der Voo, R.,Scotese, C.R., and Bonhommet, N., (editors) 1984. Plate Reconstruction from Paleozoic Paleomagnetism, Geodynamics V. 12, Amer. Geophys. Union, Washington, D.C., 136 pp., 1984
1984.04
American Scientist, 1980
1980.03
Journal of Geology, 1979
1979.02
Annual Review of Earth and Planetary Sciences, 1979
1979.01
1975.01 This paper documents the software that I wrote to produce my first flip book and first co... more 1975.01 This paper documents the software that I wrote to produce my first flip book and first com-outer animation.
1974.01 First Published Paper
Geobios, 1997
... of the Emsian, which does not correlate withany notably widespread climatic changes.11) The e... more ... of the Emsian, which does not correlate withany notably widespread climatic changes.11) The eleventh event is the minor, although glo-bally widespread ... faunas may be a cause and effectgenerated by a global lowering of the climatic gra-dient that eliminated the cool waters for ...
Aapg Bulletin, 1987
1987.02
Oceanographic Literature Review, 1998
Plate reconstructions for the opening of the Central and North Atlantic were made by combining Ge... more Plate reconstructions for the opening of the Central and North Atlantic were made by combining Geosat altimetry and magnetic anomaly data. Geosat deflection of the vertical (horizontal gravity) data, which reflect the short wavelength basement topography of the ocean floor allowed us to construct a much improved map of fracture zones m the Central and North Atlantic. The fabric of prominent fracture zones, as interpreted from Geosat deflection of the vertical data, was utilized to constrain the fits of corresponding magnetic anomaly lineations by using an Evans and Sutherland 3-D graphics computer system. For example, we have used the trace of the Charlie-Gibbs Fracture Zone to better constrain the spreading history between the North American and Eurasian plate. Movements of smaller plates such as in the Canadian Arctic and the western Mediterranean were tied to the relative motion of the major plates by applying a hierarchical plate analysis technique. Our tectonic model served as a base to construct a self-consistent isochron chart of the Central and North Atlantic ocean floor.UT Institute for Geophysics Paleoceanographic Mapping Project (POMP)Institute for Geophysic
Climate of The Past, Jul 19, 2021
Earth-Science Reviews, Apr 1, 2021
2014.11 This Atlas of Jurassic Paleogeographic Maps shows the changing paleogeography from the He... more 2014.11 This Atlas of Jurassic Paleogeographic Maps shows the changing paleogeography from the Hettangian (198 Ma) to the Jurassic/Cretaceoous Boundary (145.5 Ma). The maps are from volume 3 of the PALEOMAP PaleoAtlas for ArcGIS (Scotese, 2014). Absolute age assignments are from Gradstein, Ogg & Smith (2008). The following maps are included in the Atlas of Jurassic Paleogeographic Maps: Map 32 Jurassic/Cretaceous Boundary (145.5 Ma) Berriasian Supersequence Boundary Map 33 Late Jurassic (Tithonian, 148.2 Ma) Highstand Systems Track Map 34 Late Jurassic (Kimmeridgian, 153.2) Maximum Flooding Surface Map 35 Late Jurassic (Oxfordian, 158.4) Transgressive Systems Track Map 36 Middle Jurassic (Callovian, 164.5 Ma) Transgressive Systems Tract Map 37 Middle Jurassic (Bajocian & Bathonian, 169.7 Ma) Kimmeridgian-Oxfordian Supersequence Boundary & Maximum Flooding Surface Map 38 Middle Jurassic (Aalenian, 173.2 Ma) Bathonian-Bajocian Supersequence Boundary Map 39 Early Jurassic (Toarcian, 179.3 Ma) Toarcian Supersequence Boundary and Maximum Flooding Surface Map 40 Early Jurassic (Pliensbachian, 186.3 Ma) Maximum Flooding Surface Map 41 Early Jurassic (Sinemurian, 193 Ma) Transgressive Systems Track Map 42 Early Jurassic (Hettangian, 198 Ma) Pliensbachian Supersequence Boundary This work should be cited as Scotese, C.R., 2014. Atlas of Jurassic Paleogeographic Maps, PALEOMAP Atlas for ArcGIS, volume 3, The Jurassic and Triassic, Maps 32-42, Mollweide Projection, PALEOMAP Project, Evanston, IL.
The Geological Society of London was founded in 1807 for the purpose of'... more The Geological Society of London was founded in 1807 for the purpose of'investigating the mineral structures of the earth'. It received its Royal Charter in 1825. The Society promotes all aspects of geological science by means of meetings, special lectures and courses, ...
U.S. Geological Survey professional paper, 2000
Journal of the Geological Society, Jul 1, 1992
Journal of African Earth Sciences, 1999
... la dérive des continents (Wegener, 1912; du Toit, 1937) ont reconnu ce fait et déduit que les... more ... la dérive des continents (Wegener, 1912; du Toit, 1937) ont reconnu ce fait et déduit que leschangements climatiques (par exemple, les tillites de l'Ordovicien tardif dans le Désert du Sahara) résultaient en fait du déplacement du Gondwana à travers ces ceintures climatiques. ...
Springer eBooks, 2005
ABSTRACT 2008.01 Nokleberg, W. J., Parfenov, L. M., Scotese, C. R., Badarch, G. Berzin, N. A., Kh... more ABSTRACT 2008.01 Nokleberg, W. J., Parfenov, L. M., Scotese, C. R., Badarch, G. Berzin, N. A., Khanchuk, A. I ., Kuzmin, M. I., Obolenskiy, A. A., Prokopiev, A. V., Rodionov, S. M., Yan Hongquan, Tectonic and metallogenic evolution of Northeast Asia, 2008. 33rd International Geological Congress, Norway, 2008, International Geological Congress, Abstracts, v. 33, Abstract 1342127. Abstract: The vast, mountainous terranes of Northeast Asia hold the key to the tectonic and metallogenic evolution of a major and geologically complicated region of the world. This region stretches from the Ural Mountains and the Arctic Islands of central Russia to the Kamchatka volcanic arc in the Russian Far East. The region also includes northern Kazakhstan, China, Mongolia, the Korean Peninsula, and Japan. The tectonic development of the region is recorded in a series of cratons, craton margins, oceanic plates, active rifts, and orogenic collages of the present-day Northeast Asia continent. The collages consist of tectonostratigraphic terranes that are com-posed of fragments of igneous arcs, accretionary-wedge and subduction-zone complexes, passive continental margins, and cratons. The tectonostratigraphic terranes are overlapped by continental-margin-arc and sedimentary-basin assemblages. The tectonic history of cratons, craton mar-gins, oceanic plates, terranes, and overlap assemblages is complex due to extensional dispersion and translation during strike-slip faulting that occurred subparallel to continental margins. This talk presents a series of regional tectonic time-slice maps and a computer animation that dynamically illustrate the tectonic assembly and major metallogenic events of Northeast Asia since the late Precambrian. The key events in the tectonic history of Northeast Asia are: (1) the formation of the North Asian Craton during the breakup of a late Precambrian supercontinent; (2) during the late Precambrian and early Paleozoic, establishment of an active subduction zone along the present-day, southern margin of the North Asian Craton (Mongolian subduction zone); (3) during the late Paleozoic, closure of oceans between Siberia, Baltica, Kazakhstan, and north China; (4) during the Triassic and Jurassic, progressive closure of the Mongol-Okhotsk Ocean between Sino-Korean and the North Asian Cratons to form the core of present-day North-east Asia; (5) during the Late Jurassic through early Cenozoic, accretion of allochthonous terranes along the northern margin of the North Asian Craton, and along the margin of Eastern Asia; (6) for the first time in the early Cretaceous, formation of a continuous continental complex between the Russian Northeast and northwestern North America; and finally (7) in the Cenozoic, formation of continental-margin arcs and back-arc basins along the entire Pacific-facing margin of Northeast Asia. These time-slice maps provide the basis of a preliminary dynamic tectonic and metallogenic model of Northeast Asia that as an animation provides new insights into the geologic, tectonic, and metallogenic evolution of this complex region.
Data in Brief, Aug 1, 2022
Nature Communications, Jun 23, 2021
U.S. Geological Survey professional paper, 2005
Geological Society of America, Abstracts with Programs; (United States), Feb 1, 1993
PALEOMAP-PC (PMAPPC) allows users to interactively view Phanerozoic plate reconstructions on IBM ... more PALEOMAP-PC (PMAPPC) allows users to interactively view Phanerozoic plate reconstructions on IBM compatible personal computers. This software compliments Macintosh and Unix software developed to conjunction with the PALEOMAP Project at the University of Texas at Arlington. The past positions of the continents can be viewed on the PC monitor in a variety of map projections including the spherical projection which gives a 3-D perspective of the Earth. Once a reconstruction time has been entered, the total finite rotations for over 150 independently moving plates are calculated and the plates are rotated back through time and drawn in reconstructed coordinates. The user can zoom in and out focusing on particular areas of interest. Hard copy output is available to a variety of output devices, both as a screen dump utility and as a selected option within the program. Although visualizing continental configurations through time is the core of the program, its primary strength is that user-defined data, such as stratigraphic or structural data, can be incorporated and plotted on reconstructed basemaps. This allows the time aspect of all geological data to be united with other user-supplied data within the plate tectonic framework.
Geobios, 1997
... of the Emsian, which does not correlate withany notably widespread climatic changes.11) The e... more ... of the Emsian, which does not correlate withany notably widespread climatic changes.11) The eleventh event is the minor, although glo-bally widespread ... faunas may be a cause and effectgenerated by a global lowering of the climatic gra-dient that eliminated the cool waters for ...
Nature Communications, Dec 4, 2020
2014.08 This Atlas of Paleogene Paleogeographic Maps shows the changing paleogeography from the P... more 2014.08 This Atlas of Paleogene Paleogeographic Maps shows the changing paleogeography from the Paleocene (60.6 Ma) to the Late Oligocene (25.7 Ma). The maps are from volume 1 of the PALEOMAP PaleoAtlas for ArcGIS (Scotese, 2014). Absolute age assignments are from Ogg, Ogg & Gradstein (2008). For Maps 8, 10, 12, and 15, there are two versions of the paleogeography. One map shows the maximum highstand sea level (maximum flooding surface). The other map shows the minimum lowstand sea level (supersequence boundary). For each paleogeography there is an estimate of sea level change (m) relative to present-day sea level. The following maps are included in the Atlas of Paleogene Paleogeographic Maps: Map 08 Late Oligocene (Chattian, 25.7 Ma Ma) Aquitanian Superseqeunce Boundary & Late Oligocene Transgressive Systems Tract Map 09 Early Oligocene (Rupelian, 31.1 Ma) Maximum Flooding Surface Map 10 Late Eocene, (Priabonian, 35.6 Ma) Rupelian Supersequence Boundary & Priabonian Transgressive Systems Tract Map 11 late Middle Eocene (Bartonian, 38.8 Ma) Bartonian Transgressive Systems Tract Map 12 early Middle Eocene, (middle Lutetian, 44.6 Ma) Lutetian Maximum Flooding Surface & Lutetian Supersequence Boundary Map 13 Early Eocene (Ypresian, 52.2 Ma) Ypresian Maximum Flooding Surface Map 14 Paleocene/Eocene Boundary (PETM, Thanetian/Ypresian Boundary, 55.8 Ma) PETM Transgressive Systems Tract Map 15 Paleocene (Danian & Thanetian, 60.6 Ma) Paleocene Maximum Flooding Surface & Danian Supersequence Boundary This Atlas should be cited as: Scotese, C.R., 2014. Atlas of Paleogene Paleogeographic Maps (Mollweide Projection), Maps 8-15, Volume 1, The Cenozoic, PALEOMAP Atlas for ArcGIS, PALEOMAP Project, Evanston, IL. References Cited Ogg, J.G., Ogg, G., Gradstein, F.M., 2008. The Concise Geologic Time Scale, Cambridge University Press, Cambridge, UK, 177 pp. Scotese, C.R., 2014, The PALEOMAP Project PaleoAtlas for ArcGIS, version 2, Volume 1, Cenozoic Plate Tectonic, Paleogeographic, and Paleoclimatic Reconstructions, Maps 1-15, PALEOMAP Project, Evanston, IL.