Google Maps and Solar Eclipse Paths: 2061 - 2080

Fred Espenak

The table below is a concise summary of all total, annular and hybrid solar eclipses from 2061 through 2080 (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: 2061 - 2080
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)
2061 Apr 20 02:56:49 Total central 149 0.9578 1.048 558.8 02m37s
2061 Oct 13 10:32:10 Annular central 154 -0.9639 0.947 742.7 03m41s
2063 Feb 28 07:43:30 Annular central 131 -0.3360 0.929 279.6 07m41s
2063 Aug 24 01:22:11 Total central 136 0.2771 1.075 252.2 05m49s
2064 Feb 17 07:00:23 Annular central 141 0.3597 0.926 294.6 08m56s
2064 Aug 12 17:46:06 Total central 146 -0.4652 1.049 183.7 04m28s
2066 Jun 22 19:25:48 Annular central 128 0.7330 0.943 308.6 04m40s
2066 Dec 17 00:23:40 Total central 133 -0.4043 1.042 152.2 03m14s
2067 Jun 11 20:42:26 Annular central 138 -0.0387 0.967 119.0 04m05s
2067 Dec 06 14:03:43 Hybrid central 143 0.2845 1.001 4.1 00m08s
2068 May 31 03:56:39 Total central 148 -0.7970 1.011 62.8 01m06s
2070 Apr 11 02:36:09 Total central 130 0.3652 1.047 168.2 04m04s
2070 Oct 04 07:08:57 Annular central 135 -0.4950 0.973 110.2 02m44s
2071 Mar 31 15:01:06 Annular central 140 -0.3739 0.992 30.7 00m52s
2071 Sep 23 17:20:28 Total central 145 0.2620 1.033 116.1 03m11s
2072 Sep 12 08:59:20 Total central 155 0.9655 1.056 732.5 03m13s
2073 Aug 03 17:15:23 Total central 127 -0.8763 1.029 206.4 02m29s
2074 Jan 27 06:44:15 Annular central 132 0.4251 0.980 79.3 02m21s
2074 Jul 24 03:10:32 Annular central 137 -0.1242 0.984 57.8 01m57s
2075 Jan 16 18:36:04 Total central 142 -0.2799 1.031 109.7 02m42s
2075 Jul 13 06:05:44 Annular central 147 0.6583 0.947 261.9 04m45s
2076 Jan 06 10:07:27 Total central 152 -0.9373 1.034 340.4 01m49s
2077 May 22 02:46:05 Total central 129 -0.5725 1.029 118.8 02m54s
2077 Nov 15 17:07:56 Annular central 134 0.4705 0.937 262.5 07m54s
2078 May 11 17:56:55 Total central 139 0.1838 1.070 232.1 05m40s
2078 Nov 04 16:55:44 Annular central 144 -0.2285 0.926 287.5 08m29s
2079 May 01 10:50:13 Total central 149 0.9081 1.051 405.7 02m55s
2079 Oct 24 18:11:21 Annular central 154 -0.9243 0.948 494.7 03m39s

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


[1] Greatest Eclipse is 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

2013 Dec 09