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April 1903 lunar eclipse

A partial lunar eclipse occurred at the Moon’s ascending node of orbit on Sunday, April 12, 1903, with an umbral magnitude of 0.9677. 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. The Moon's apparent diameter was near the average diameter because it occurred 6.2 days after perigee and 7.1 days before apogee.

Visibility
The eclipse was completely visible over eastern South America, Africa, Europe, and Antarctica, seen rising over western South America and much of North America and setting over much of Asia and western 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 1903 An annular solar eclipse on March 29. • A partial lunar eclipse on April 12.A total solar eclipse on September 21. • A partial lunar eclipse on October 6. Metonic • Preceded by: Lunar eclipse of June 23, 1899 • Followed by: Lunar eclipse of January 29, 1907 Tzolkinex • Preceded by: Lunar eclipse of February 28, 1896 • Followed by: Lunar eclipse of May 24, 1910 Half-Saros • Preceded by: Solar eclipse of April 6, 1894 • Followed by: Solar eclipse of April 17, 1912 Tritos • Preceded by: Lunar eclipse of May 11, 1892 • Followed by: Lunar eclipse of March 12, 1914 Lunar Saros 130 • Preceded by: Lunar eclipse of March 30, 1885 • Followed by: Lunar eclipse of April 22, 1921 Inex • Preceded by: Lunar eclipse of May 1, 1874 • Followed by: Lunar eclipse of March 22, 1932 Triad • Preceded by: Lunar eclipse of June 10, 1816 • Followed by: Lunar eclipse of February 9, 1990 Lunar eclipses of 1901–1904 This eclipse is a member of a semester series. An eclipse in a semester series of lunar eclipses repeats approximately every 177 days and 4 hours (a semester) at alternating nodes of the Moon's orbit. The penumbral lunar eclipse on March 2, 1904 occurs in the next lunar year eclipse set. Saros 130 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 hybrid solar eclipses of Solar Saros 137. ==See also==
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