NASA Solar Eclipse Paths: 2021 (original) (raw)

Google Maps and Solar Eclipse Paths: 2021 - 2040

Fred Espenak

The table below is a concise summary of all total, annular and hybridsolar eclipses from 2021 through 2040 (excluding partial eclipses). The links in the table provide additional information and graphics for each eclipse. In particular, the Eclipse Type (third column) links to dynamic maps showing the central path of eclipses across Earth's surface. These interactive maps utilize NASA eclipse path predictions and the plotting capabilities of Google Maps. The northern and southern limits of each eclipse path are plotted in blue while the central line is red. The yellow lines plotted across the path indicate the position of maximum eclipse at 10-minute intervals. You can zoom into the map and turn the satellite view on or off. When you click on a position, the eclipse times and circumstances at that location are calculated and displayed.

The first column in the table gives the Calendar Date of the instant of greatest eclipse[1]. This links to an orthographic projection map of Earth showing the region of visibility for an eclipse. The path of the Moon's penumbral shadow (cyan and magenta) covers the region of partial eclipse. The track of the umbral/antumbral shadow (blue/red) defines the path of total or annular eclipse. These figures are described in greater detail in the Key to Solar Eclipse Maps. Each figure is stored as a gif of approximately 60 kilobytes.

The second column TD of Greatest Eclipse is the Terrestrial Dynamical Time when the axis of the Moon's shadow passes closest to Earth's center. Animations of the Moon's penumbral and umbral shadows across Earth are accessed by clicking the this link. Each animated GIF file is from 40 KB to 175 KB in size.

The Eclipse Type (column 3) is either Total, Annular or Hybrid[2]. The link opens a window with the central eclipse path plotted on an interactive Google Map.

The Central Eclipse Class (column 4) indicates whether an eclipse is central or non-central. The parameters N and S identify paths that have no northern or southern limit, respectively. The link opens a table containing the central path coordinates.

Eclipses recur over the Saros cycle, a period of approximately 18 years 11 days. The Saros series that an eclipse belongs to is found in column 5. All eclipses in a particular Saros series can be viewed in a table via the Saros number link.

The parameter Gamma (column 6) is the perpendicular distance of the Moon's shadow axis and Earth's center at greatest eclipse. The link opens a table containing the Besselian elements for the eclipse.

The **Eclipse Magnitude**[3] (column 7) gives the fraction of the Sun's diameter obscured at the instant of greatest eclipse. The Path Width (column 8) gives the width of the central eclipse path (in kilometers) at the instant of greatest eclipse. The Central Duration[4] (column 9) gives the length of the eclipse as seen from the central line at greatest eclipse.

The Key to Solar Eclipse Path Tables contains a more detailed description of each item in the table.

For more data on solar eclipses during this period, see Catalog of Solar Eclipses: 1901 to 2000.

Solar Eclipse Paths: 2021 - 2040
Calendar Date TD of Greatest Eclipse Eclipse Type Central Eclipse Class Saros Series Gamma Eclipse Magnitude Path Width (km) Central Duration
(Link to Global Map) (Link to Animation) (Link to Google Map) (Link to Path Table) (Link to Saros) (Link to Besselian Elements)
2021 Jun 10 10:43:07 Annular central 147 0.9152 0.9435 526.8 03m51s
2021 Dec 04 07:34:38 Total central 152 -0.9526 1.0367 418.7 01m54s
2023 Apr 20 04:17:56 Hybrid central 129 -0.3952 1.0132 49.0 01m16s
2023 Oct 14 18:00:41 Annular central 134 0.3753 0.9520 187.4 05m17s
2024 Apr 08 18🔞29 Total central 139 0.3431 1.0566 197.5 04m28s
2024 Oct 02 18:46:13 Annular central 144 -0.3509 0.9326 266.5 07m25s
2026 Feb 17 12:13:06 Annular central 121 -0.9743 0.9630 616.3 02m20s
2026 Aug 12 17:47:06 Total central 126 0.8977 1.0386 293.9 02m18s
2027 Feb 06 16:00:48 Annular central 131 -0.2952 0.9281 281.6 07m51s
2027 Aug 02 10:07:50 Total central 136 0.1421 1.0790 257.7 06m23s
2028 Jan 26 15:08:59 Annular central 141 0.3901 0.9208 323.0 10m27s
2028 Jul 22 02:56:40 Total central 146 -0.6056 1.0560 230.2 05m10s
2030 Jun 01 06:29:13 Annular central 128 0.5626 0.9443 249.6 05m21s
2030 Nov 25 06:51:37 Total central 133 -0.3867 1.0468 169.3 03m44s
2031 May 21 07:16:04 Annular central 138 -0.1970 0.9589 152.2 05m26s
2031 Nov 14 21:07:31 Hybrid central 143 0.3078 1.0106 38.3 01m08s
2032 May 09 13:26:42 Annular central 148 -0.9375 0.9957 43.7 00m22s
2033 Mar 30 18:02:36 Total central 120 0.9778 1.0462 781.1 02m37s
2034 Mar 20 10🔞45 Total central 130 0.2894 1.0458 159.1 04m09s
2034 Sep 12 16:19:28 Annular central 135 -0.3936 0.9736 102.1 02m58s
2035 Mar 09 23:05:54 Annular central 140 -0.4368 0.9919 31.5 00m48s
2035 Sep 02 01:56:46 Total central 145 0.3727 1.0320 116.3 02m54s
2037 Jul 13 02:40:36 Total central 127 -0.7246 1.0413 200.6 03m58s
2038 Jan 05 13:47:11 Annular central 132 0.4169 0.9728 107.2 03m18s
2038 Jul 02 13:32:55 Annular central 137 0.0398 0.9911 31.2 01m00s
2038 Dec 26 01:00:10 Total central 142 -0.2881 1.0268 95.2 02m18s
2039 Jun 21 17:12:54 Annular central 147 0.8312 0.9454 365.3 04m05s
2039 Dec 15 16:23:46 Total central 152 -0.9458 1.0356 379.8 01m51s

Central Eclipse Class abbreviations (used above): N = no northern limit, S = no southern limit, AT = annular-total hybrid, TA = total-annular hybrid


[1] Greatest Eclipseis the instant when the distance between the Moon's shadow axis and Earth's center reaches a minimum.

[2] Hybrid eclipses are also known as annular/total eclipses. Such an eclipse is both total and annular along different sections of its umbral path.

[3] Eclipse magnitude is the fraction of the Sun's diameter obscured by the Moon. For annular eclipses, the eclipse magnitude is always less than 1. For total eclipses, the eclipse magnitude is always greater than or equal to 1. For both annular and total eclipses, the value listed is actually the ratio of diameters between the Moon and the Sun.

[4] Central Duration is the duration of a total or annular eclipse at greatest eclipse. This is the instant when the axis of the Moon's shadow passes closest to Earth's center.


Twenty Year Solar Eclipse Path Tables (w/Google Maps)

Each of the following links displays a table containing 20 years of total, annular and hybrid eclipses. Each eclipse offers links to a global map, shadow animation, interactive Google map, path coordinates table, and saros table.

Twenty Year Solar Eclipse Path Tables (w/Google Maps)
Years
1901-1920 1921-1940 1941-1960 1961-1980 1981-2000
2001-2020 2021-2040 2041-2060 2061-2080 2081-2100

Decade Tables of Solar Eclipses

Each link in the following table displays a page containing 10 years of eclipses. Every eclipse has links of global maps, interactive Google maps, animations, path coordinate tables, and saros tables.

Decade Tables of Solar Eclipses
Decades
1901-1910 1911-1920 1921-1930 1931-1940 1941-1950
1951-1960 1961-1970 1971-1980 1981-1990 1991-2000
2001-2010 2011-2020 2021-2030 2031-2040 2041-2050
2051-2060 2061-2070 2071-2080 2081-2090 2091-2100

Maps of Solar Eclipse Paths

Solar Eclipse Catalogs

Reproduction of Eclipse Data

All eclipse calculations are by Fred Espenak, and he assumes full responsibility for their accuracy. Some of the information presented on this web site is based on data originally published in:

Fifty Year Canon of Solar Eclipses: 1986 - 2035
and
Five Millennium Canon of Solar Eclipses: -1999 to +3000 (2000 BCE to 3000 CE)

Permission is freely granted to reproduce this data when accompanied by an acknowledgment:

"Eclipse Predictions by Fred Espenak, NASA's GSFC"

For more information, see: NASA Copyright Information