Lunar Eclipses: 1911 - 1920

A concise summary of all lunar eclipses from 1911 through 1920 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: 1911 - 1920
Date Eclipse Type Saros Umbral Magnitude Eclipse Duration Geographic Region of Eclipse Visibility
1911 May 13 Penumbral 139 -0.266 - e Australia, Americas, w Europe, w Africa
1911 Nov 06 Penumbral 144 -0.168 - Europe, e Africa, Asia, Australia, w N America
1912 Apr 01 Partial 111 0.187 01h37m The Americas, Europe, Africa, Asia, Australia
1912 Sep 26 Partial 116 0.123 01h23m e S America, Asia, Australia, Americas
1913 Mar 22 Total 121 1.574 03h30m
01h33m
Asia, Australia, Pacific, Americas
1913 Sep 15 Total 126 1.435 03h51m
01h34m
e Africa, Asia, Australia, Americas
1914 Mar 12 Partial 131 0.917 03h02m Americas, Europe, Africa, w Asia
1914 Sep 04 Partial 136 0.863 03h17m e Africa, Asia, Australia, w Americas
1915 Jan 31 Penumbral 103 -0.994 - Americas, Europe, w Africa
1915 Mar 01 Penumbral 141 -0.447 - Europe, Africa, Asia, Australia, w N America
1915 Jul 26 Penumbral 108 -0.607 - e Asia, Australia, w Americas
1915 Aug 24 Penumbral 146 -0.417 - S America, Europe, Africa, Asia, Australia
1916 Jan 20 Partial 113 0.137 01h29m e Asia, Australia, Americas, w Europe, w Africa
1916 Jul 15 Partial 118 0.800 02h53m Americas, w Europe, Africa
1917 Jan 08 Total 123 1.369 03h48m
01h28m
e Asia, e Australia, Americas, Europe, w Africa
1917 Jul 04 Total 128 1.624 03h33m
01h37m
S America, Europe, Africa, s Asia, Australia
1917 Dec 28 Total 133 1.010 03h23m
00h16m
e Asia, Australia, Americas, w Africa, w Europe
1918 Jun 24 Partial 138 0.135 01h24m e Asia, Australia, Americas
1918 Dec 17 Penumbral 143 -0.163 - Europe, Africa Asia, Australia, n N America
1919 May 15 Penumbral 110 -0.160 - e N America, S America, Europe, Africa, w Asia
1919 Nov 07 Partial 115 0.184 01h31m Americas, Europe, Africa, Asia,
1920 May 03 Total 120 1.224 03h40m
01h12m
Americas, Europe, Africa, w Asia
1920 Oct 27 Total 125 1.404 03h32m
01h26m
e Europe, e Africa, Asia, Australia, N America

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