MarketMay 1937 lunar eclipse
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May 1937 lunar eclipse

A penumbral lunar eclipse occurred at the Moon’s ascending node of orbit on Tuesday, May 25, 1937, with an umbral magnitude of −0.3033. A lunar eclipse occurs when the Moon moves into the Earth's shadow, causing the Moon to be darkened. A penumbral lunar eclipse occurs when part or all of the Moon's near side passes into the Earth's penumbra. Unlike a solar eclipse, which can only be viewed from a relatively small area of the world, a lunar eclipse may be viewed from anywhere on the night side of Earth. Occurring only about 18 hours after apogee, the Moon's apparent diameter was smaller.

Visibility
The eclipse was completely visible over much of North America, western and central South America, and Antarctica, seen rising over Australia and setting over northeastern North America, eastern South America, and west Africa. == Eclipse details ==
Eclipse details
Shown below is a table displaying details about this particular solar eclipse. It describes various parameters pertaining to this eclipse. == Eclipse season ==
Eclipse season
This eclipse is part of an eclipse season, a period, roughly every six months, when eclipses occur. Only two (or occasionally three) eclipse seasons occur each year, and each season lasts about 35 days and repeats just short of six months (173 days) later; thus two full eclipse seasons always occur each year. Either two or three eclipses happen each eclipse season. In the sequence below, each eclipse is separated by a fortnight. == Related eclipses ==
Related eclipses
Eclipses in 1937 A penumbral lunar eclipse on May 25.A total solar eclipse on June 8. • A partial lunar eclipse on November 18. • An annular solar eclipse on December 2. Metonic • Preceded by: Lunar eclipse of August 5, 1933 • Followed by: Lunar eclipse of March 13, 1941 Tzolkinex • Preceded by: Lunar eclipse of April 13, 1930 • Followed by: Lunar eclipse of July 6, 1944 Half-Saros • Preceded by: Solar eclipse of May 19, 1928 • Followed by: Solar eclipse of May 30, 1946 Tritos • Preceded by: Lunar eclipse of June 25, 1926 • Followed by: Lunar eclipse of April 23, 1948 Lunar Saros 110 • Preceded by: Lunar eclipse of May 15, 1919 • Followed by: Lunar eclipse of June 5, 1955 Inex • Preceded by: Lunar eclipse of June 14, 1908 • Followed by: Lunar eclipse of May 4, 1966 Triad • Preceded by: Lunar eclipse of July 24, 1850 • Followed by: Lunar eclipse of March 25, 2024 Lunar eclipses of 1937–1940 Saros 110 Tritos series Inex series Half-Saros cycle A lunar eclipse will be preceded and followed by solar eclipses by 9 years and 5.5 days (a half saros). This lunar eclipse is related to one total and one partial = two solar eclipses of Solar Saros 117. ==See also==
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