A concise summary of all lunar eclipses from 2081 through 2090 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: 2081 - 2090 | |||||
| Date | Eclipse Type | Saros | Umbral Magnitude | Eclipse Duration | Geographic Region of Eclipse Visibility |
| 2081 Mar 25 | Partial | 143 | 0.100 | 01h09m | e Americas, Europe, Africa, w Asia |
| 2081 Sep 18 | Penumbral | 148 | -0.151 | - | Americas, Europe, Africa, w Asia |
| 2082 Feb 13 | Partial | 115 | 0.019 | 00h31m | ne Asia, Americas, Europe, w Africa |
| 2082 Aug 08 | Penumbral | 120 | -0.024 | - | e Africa, Asia, Australia, w N America |
| 2083 Feb 02 | Total | 125 | 1.211 | 03h29m 01h08m |
Europe, Africa, Asia, Australia, nw N America |
| 2083 Jul 29 | Total | 130 | 1.483 | 03h34m 01h31m |
Americas, Europe, Africa, w Asia, w Australia |
| 2084 Jan 22 | Total | 135 | 1.155 | 03h37m 01h01m |
Americas, Europe, Africa, Asia, w Australia |
| 2084 Jul 17 | Partial | 140 | 0.917 | 03h02m | e Europe, e Africa, Asia, Australia |
| 2085 Jan 10 | Penumbral | 145 | -0.108 | - | Americas, Europe, Africa, Asia, w Australia |
| 2085 Jun 08 | Penumbral | 112 | -0.462 | - | Americas, Europe, Africa, w Asia |
| 2085 Jul 07 | Penumbral | 150 | -0.442 | - | e Asia, Australia, Americas |
| 2085 Dec 01 | Penumbral | 117 | -0.390 | - | ne Asia, e Australia, Americas, w Africa, Europe |
| 2086 May 28 | Partial | 122 | 0.824 | 03h10m | e Africa, e Asia, Australia, w Americas |
| 2086 Nov 20 | Partial | 127 | 0.992 | 03h09m | e Americas, Europe, Africa, Asia, Australia |
| 2087 May 17 | Total | 132 | 1.460 | 03h51m 01h36m |
e Europe, e Africa, Asia, Australia |
| 2087 Nov 10 | Total | 137 | 1.506 | 03h27m 01h30m |
ne Europe, Asia, Australia, Americas |
| 2088 May 05 | Partial | 142 | 0.106 | 01h19m | e Europe, e Africa, Asia, Australia |
| 2088 Oct 30 | Partial | 147 | 0.188 | 01h35m | Americas, Europe, Africa, w Asia |
| 2089 Mar 26 | Penumbral | 114 | -0.162 | - | e Asia, Australia, Americas |
| 2089 Sep 19 | Penumbral | 119 | -0.269 | - | e Australia, e Americas, Europe, Africa, w Asia |
| 2090 Mar 15 | Total | 124 | 1.207 | 03h18m 01h04m |
Americas, Europe, Africa, w Asia, w Australia |
| 2090 Sep 08 | Total | 129 | 1.043 | 03h34m 00h34m |
Americas, Europe, Africa, w Asia, Australia |
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.
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 | |
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.
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 | |
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
