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October 1939 lunar eclipse

A partial lunar eclipse occurred at the Moon’s descending node of orbit on Saturday, October 28, 1939, with an umbral magnitude of 0.9876. A lunar eclipse occurs when the Moon moves into the Earth's shadow, causing the Moon to be darkened. A partial lunar eclipse occurs when one part of the Moon is in the Earth's umbra, while the other part is in 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 about 5.3 days after apogee, the Moon's apparent diameter was smaller.

Visibility
The eclipse was completely visible over North America and western South America, seen rising over northeast Asia and eastern Australia and setting over eastern South America, west and central Africa, and Europe. == Eclipse details ==
Eclipse details
Shown below is a table describing 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 1939 An annular solar eclipse on April 19. • A total lunar eclipse on May 3. • A total solar eclipse on October 12. • A partial lunar eclipse on October 28. Metonic • Preceded by: Lunar eclipse of January 8, 1936 • Followed by: Lunar eclipse of August 15, 1943 Tzolkinex • Preceded by: Lunar eclipse of September 14, 1932 • Followed by: Lunar eclipse of December 8, 1946 Half-Saros • Preceded by: Solar eclipse of October 21, 1930 • Followed by: Solar eclipse of November 1, 1948 Tritos • Preceded by: Lunar eclipse of November 27, 1928 • Followed by: Lunar eclipse of September 26, 1950 Lunar Saros 135 • Preceded by: Lunar eclipse of October 16, 1921 • Followed by: Lunar eclipse of November 7, 1957 Inex • Preceded by: Lunar eclipse of November 17, 1910 • Followed by: Lunar eclipse of October 6, 1968 Triad • Preceded by: Lunar eclipse of December 26, 1852 • Followed by: Lunar eclipse of August 28, 2026 Lunar eclipses of 1937–1940 Saros 135 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 two total solar eclipses of Solar Saros 142. ==See also==
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