MarketMay 1985 lunar eclipse
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May 1985 lunar eclipse

A total lunar eclipse occurred at the Moon's descending node of orbit on Saturday, May 4, 1985, with an umbral magnitude of 1.2369. A lunar eclipse occurs when the Moon moves into the Earth's shadow, causing the Moon to be darkened. A total lunar eclipse occurs when the Moon's near side entirely passes into the Earth's umbral shadow. 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. A total lunar eclipse can last up to nearly two hours, while a total solar eclipse lasts only a few minutes at any given place, because the Moon's shadow is smaller. Occurring only about 13.5 hours after perigee, the Moon's apparent diameter was larger.

Visibility
The eclipse was completely visible over central and east Africa, eastern Europe, the western half of Asia, western Australia, and Antarctica, seen rising over much of South America, west Africa, and western Europe and setting over east and northeast Asia and much of Australia. == 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 1985 A total lunar eclipse on May 4.A partial solar eclipse on May 19. • A total lunar eclipse on October 28. • A total solar eclipse on November 12. Metonic • Preceded by: Lunar eclipse of July 17, 1981 • Followed by: Lunar eclipse of February 20, 1989 Tzolkinex • Preceded by: Lunar eclipse of March 24, 1978 • Followed by: Lunar eclipse of June 15, 1992 Half-Saros • Preceded by: Solar eclipse of April 29, 1976 • Followed by: Solar eclipse of May 10, 1994 Tritos • Preceded by: Lunar eclipse of June 4, 1974 • Followed by: Lunar eclipse of April 4, 1996 Lunar Saros 121 • Preceded by: Lunar eclipse of April 24, 1967 • Followed by: Lunar eclipse of May 16, 2003 Inex • Preceded by: Lunar eclipse of May 24, 1956 • Followed by: Lunar eclipse of April 15, 2014 Triad • Preceded by: Lunar eclipse of July 3, 1898 • Followed by: Lunar eclipse of March 4, 2072 Lunar eclipses of 1984–1987 Metonic series Saros 121 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 annular solar eclipses of Solar Saros 128. == See also ==
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