Lunar Eclipses: 2071 - 2080

A concise summary of all lunar eclipses from 2071 through 2080 is presented in the following table. Diagrams and maps for each eclipse may be seen by clicking the eclipse's Date. This links to a figure showing the Moon's path through Earth's shadow(s) and a world map illustrating the region of visibility for that particular eclipse. These figures are described in greater detail in the Key to Lunar Eclipse Maps. Each figure is stored as a GIF file of about 60 kilobytes. The Eclipse Type (Penumbral, Partial or Total) is given followed by the number of the Saros series. Eclipses belonging to a given Saros series recur every 18 years 11 days. The Umbral Magnitude[1] (fourth column) gives the fraction of the Moon's diameter immersed in Earth's umbral shadow at the instant of greatest eclipse. The Eclipse Duration[2] gives the length of the partial eclipse. If the eclipse is total, then the duration of the total phase is also listed in bold. Finally, the Geographic Region of Eclipse Visibility[3] provides a brief description of the region where each eclipse will be seen.


Lunar Eclipses: 2071 - 2080
Date Eclipse Type Saros Umbral Magnitude Eclipse Duration Geographic Region of Eclipse Visibility
2071 Mar 16 Penumbral 114 -0.114 - Americas, Europe, Africa, w Asia
2071 Sep 09 Penumbral 119 -0.153 - e Europe, e Africa, Asia, Australia, w N.A.
2072 Mar 04 Total 124 1.250 03h20m
01h09m
e Europe, e Africa, Asia, Australia, w N.A.
2072 Aug 28 Total 129 1.171 03h41m
01h05m
Europe, Africa, Asia, Australia, w N America
2073 Feb 22 Total 134 1.256 03h20m
01h10m
e Asia, e Australia, Americas, Europe, w Africa
2073 Aug 17 Total 139 1.106 03h32m
00h51m
Europe, Africa, Asia, Australia
2074 Feb 11 Penumbral 144 -0.092 - e Americas, Europe, Africa, Asia, Australia
2074 Jul 08 Penumbral 111 -0.771 - e Africa, s Asia, Australia,
2074 Aug 07 Penumbral 149 -0.204 - Americas, Europe, Africa, Middle East
2075 Jan 02 Penumbral 116 -0.323 - e Asia, Australia, Americas
2075 Jun 28 Partial 121 0.628 02h38m e Asia, Australia, Americas
2075 Dec 22 Partial 126 0.906 03h23m e Asia, Australia, Americas, w Africa, Europe
2076 Jun 17 Total 131 1.800 03h36m
01h41m
Americas, Europe, Africa, Middle East
2076 Dec 10 Total 136 1.450 03h41m
01h31m
e Europe, Asia, Australia, Americas
2077 Jun 06 Partial 141 0.317 02h06m e Africa, s Asia, Australia
2077 Nov 29 Partial 146 0.241 01h46m e Americas, Europe, Africa, Asia, w Australia
2078 Apr 27 Penumbral 113 -0.420 - Americas, Europe, Africa
2078 Oct 21 Penumbral 118 -0.140 - Americas, Europe, Africa, w Asia
2078 Nov 19 Penumbral 156 -0.899 - ne Europe, Asia, Australia, N America
2079 Apr 16 Partial 123 0.950 03h24m e Australia, Americas, Europe, Africa
2079 Oct 10 Total 128 1.085 03h19m
00h44m
Europe, Africa, Asia, Australia, nw N America
2080 Apr 04 Total 133 1.351 03h34m
01h23m
e Asia, Australia, Americas
2080 Sep 29 Total 138 1.249 03h38m
01h15m
Americas, Europe, Africa, w Asia

Geographic abreviations (used above): n = north, s = south, e = east, w = west, c = central


[1] Umbral magnitude is the fraction of the Moon's diameter obscured by Earth's Umbra. For penumbral eclipses, the umbral magnitude is always less than 0. For partial eclipses, the umbral magnitude is always greater than 0 and less than 1. For total eclipses, the umbral magnitude is always greater than or equal to 1.

[2] Eclipse Duration is the duration of a partial eclipse. If the eclipse is total, the duration of totality is given in bold.

[3] Geographic Region of Eclipse Visibility is the portion of Earth's surface where a lunar eclipse can be seen.


Ten Year Tables of Lunar Eclipses

Every link in the following table displays a page containing 10 years of lunar eclipses. Each eclipse has links to diagrams, maps and saros tables.

Ten Year Tables of Lunar 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

Lunar Eclipse Resources
Lunar Eclipse Publications Online

Special thanks to National Space Club summer interns Christopher Barrow for his valuable assistance in preparing this web page (July 2004) and Sumit Dutta for meticulously updating the Eclipse Web Site to NASA/W3C standards (July 2005).

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 Lunar Eclipses: 1986 - 2035.

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

2008 Mar 24