| low-titanium basalt deduced from the iron isotopic signature in Luna 16, 20, and 24 soils Satoki Okabayashi,...low-titanium basalt deduced from the iron isotopic signature in Luna 16, 20, and 24 soils, Geochimica et Cosmochimica...undergone enhancements after acceptance, such as the addition of a cover page and metadata, and formatting...formatting for readability, but it is not yet the definitive version of record. This version will undergo...version to give early visibility of the article. Please note that, during the production process, errors may |
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Demidova, S. I., Anosova, M. O., Kononkova, N. N., Brandstätter, F., Ntaflos, T. (2019) Phosphorus-bearing Olivines of Lunar Rocks: Sources and Localization in the Lunar Crust. Geochemistry International, 57 (8) 873-892 doi:10.1134/s0016702919080032 |
Journal (article/letter/editorial) |
| Pleiades Publishing, Ltd., 2019. Russian Text © The Author(s), 2019, published in Geokhimiya, 2019, No...Olivines of Lunar Rocks: Sources and Localization in the Lunar Crust S. I. Demidovaa, *, M. O. Anosovaa, *...highland, mare, and mingled meteorites and in “Apollo-14”, “_Luna_-16, -20, -_24_” lunar samples. The olivines...possible sources of P-bearing olivine were found in the lunar material: 1) highland anorthositic–noritic–troctolitic...to high-Mg suite rocks: 2) late-stage products of mare basalts crystallization; and 3) unusual olivine–orthopyroxene |
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ARAI, Tomoko, WARREN, Paul H., TAKEDA, Hiroshi (1996) Four lunar mare meteorites: Crystallization trends of pyroxenes and spinels. Meteoritics & Planetary Science, 31 (6) 877-892 doi:10.1111/j.1945-5100.1996.tb02121.x |
Journal (article/letter/editorial) |
| Meteoritical Society, 1996. Printed in USA. Four lunar mare meteorites: Crystallization trends of pyroxenes...Antarctic meteorites known to be derived from mare regions of the Moon: Y-793 169 and A-881757 (YA meteorites)...All have relatively low bulkrock Ti02 content, and the YA meteorites are uncommonly ancient. Our electron...microanalysis (EPMA) data indicate that the Y A meteorites and the dominant mare components of Y-793274 and EET...general trend for Ti-poor (low-Ti and very low-Ti) mare basalts. Their pyroxenes show a strong correlation |
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Zeng, Xiaojia, Joy, Katherine H., Li, Shijie, Pernet-Fisher, John F., Li, Xiongyao, Martin, Dayl J. P., Li, Yang, Wang, Shijie (2018) Multiple lithic clasts in lunar breccia Northwest Africa 7948 and implication for the lithologic components of lunar crust. Meteoritics & Planetary Science, 53 (5) 1030-1050 doi:10.1111/maps.13049 |
Journal (article/letter/editorial) |
| breccia Northwest Africa 7948 and implication for the lithologic components of lunar crust Xiaojia ZENG...14 December 2017) Abstract–This study presents the petrography, mineralogy, and bulk composition of...Apollo regolith breccias. Comparing the bulk composition of the meteorite with remotely sensed geochemical...suggests that the sample was derived from a region of the lunar surface distal from the nearside Th-rich...ejected from a nearside highlands-mare boundary (e.g., around Mare Crisium or Orientale) or a cryptomare |
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Warren, Paul H. (2005) “New” lunar meteorites: Implications for composition of the global lunar surface, lunar crust, and the bulk Moon. Meteoritics & Planetary Science, 40 (3) 477-506 doi:10.1111/j.1945-5100.2005.tb00395.x |
Journal (article/letter/editorial) |
| Implications for composition of the global lunar surface, lunar crust, and the bulk Moon Paul H. WARREN Institute...significant implications for the interpretation of global Th data and for the Moon’s bulk composition. As...(Prettyman et al. 2002), the Lunar Prospector gamma-ray data imply that the average global surface Th...calibration yields implausibly high concentrations for the three most Th-poor documented sampling sites, it...in a misfit toward too-high Th when compared with the global regolith Th spectrum as constrained using |
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Zeng, Xiaojia, Li, Shijie, Joy, Katherine H., Li, Xiongyao, Liu, Jianzhong, Li, Yang, Li, Rui, Wang, Shijie (2020) Occurrence and implications of secondary olivine veinlets in lunar highland breccia Northwest Africa 11273. Meteoritics & Planetary Science, 55 (1) 36-55 doi:10.1111/maps.13421 |
Journal (article/letter/editorial) |
| breccias preserve the records of geologic processes on the Moon. In this study, we report the occurrence, petrography...petrography, mineralogy, and geologic significance of the observed secondary olivine veinlets in lunar feldspathic...dominated by interconnecting olivine mineral grains. The host clasts are mainly composed of mafic minerals...lithology. The studied olivine veinlets (~5 to 30 lm in width) are distributed within the mafic mineral...mineral host, but do not extend into the adjacent plagioclase. Chemically, these olivine veinlets are Fe-richer |
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Barsukov, V. L., Nazarav, M. A., Tarasov, L. S. (1982) Moon rock mineralogy. International Geology Review, 24 (2) 238-248 doi:10.1080/00206818209452398 |
Journal (article/letter/editorial) |
| homepage: http://www.tandfonline.com/loi/tigr20 Moon rock mineralogy V. L. Barsukov , M. A. Nazarav &...& L. S. Tarasov (1982) Moon rock mineralogy, International Geology Review, 24:2, 238-248, DOI: 10.10...13:40 Moon rock mineralogy V.L. Borsukov, M.A. Nozorov, ond L.S. Torosov is restricted to the range...parts of the hloon (Vinogradov, 1975; Schmitt, 1975; Florenskiy et al., 1977). Nevertheless, the material...various laboratories throughout the world is reasonably representative, and the data can be combined with orbital |
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Jolliff, Bradley L., Wieczorek, Mark A., Shearer, Charles K., Neal, Clive R. - Eds. (2006) New Views of the Moon. Reviews in Mineralogy and Geochemistry Vol. 60. Mineralogical Society of America |
Report (volume) |
| MINERALOGY & GEOCHEMISTRY Volume 60 NEW VIEWS of the MOON EDITORS: Bradley L. Jolliff, Mark A. Wieczorek...This book is dedicated to the memory of the late Graham Ryder, who was one of the original four members of...of CAPTEM when the New Views of the Moon scientific initiative was first conceived. Graham, who was a...owing to his broad knowledge of the lunar samples and his residence at the Lunar and Planetary Institute...where CAPTEM met, was a logical choice to be one of the co-leaders of this lunarscience initiative. Not only |
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Williams, Jean-Pierre, van der Bogert, Carolyn H., Pathare, Asmin V., Michael, Gregory G., Kirchoff, Michelle R., Hiesinger, Harald (2018) Dating very young planetary surfaces from crater statistics: A review of issues and challenges. Meteoritics & Planetary Science, 53 (4) 554-582 doi:10.1111/maps.12924 |
Journal (article/letter/editorial) |
| revision accepted 25 May 2017) Abstract–Determining the ages of young planetary surfaces relies on using...small, often sub-km diameter impact craters due to the higher frequency at which they form. Smaller craters...used at all. With the current plethora of meter-scale resolution images acquired of the lunar and Martian...establish the temporal relation of recent geologic events. In this review paper, we discuss the many factors...ultimately requires an understanding of the geologic context of the surface being dated as reliability can |
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(1981) Proceedings of the Twelfth Lunar and Planetary Science Conference - Section 2: Planets, Asteroids and Satellites. Geochimica et Cosmochimica Acta Supplement 16. The Geochemical Society and the Meteoritical Society |
Report (issue) |
| GEOCHIMICA ETT COSMOCHIMICA ACTA + Journal ey The Geochemical ce and. The ercenitter] Society Albright College...miles). North is at the upper right edge of the disc. Seen above the planet are the satellites Dione (right)...spot at the south edge of a yellow band; in true color, the spot would appear brown and the band white...spot slightly above and to the left in this image moves eastward relative to the green spot at a rate that...it to pass the green feature in about 50 days. The convective clouds that appear between the two spots |
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