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Solar eclipse of May 6, 1883

A total solar eclipse occurred at the Moon's descending node of orbit between Sunday, May 6, and Monday, May 7, 1883, with a magnitude of 1.0634. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth. A total solar eclipse occurs when the Moon's apparent diameter is larger than the Sun's, blocking all direct sunlight, turning day into darkness. Totality occurs in a narrow path across Earth's surface, with the partial solar eclipse visible over a surrounding region thousands of kilometres wide. Occurring about 1.1 days after perigee, the Moon's apparent diameter was larger.

Observations
, Caroline Islands. An expedition of American astronomers traveled from Peru to Caroline Island aboard the to observe the total solar eclipse. A French expedition also observed the eclipse from Caroline, and the United States Navy mapped the atoll. Johann Palisa, a member of the expedition, discovered an asteroid later that year which he named Carolina "in remembrance of his visit to [the] island". == Eclipse details ==
Eclipse details
Shown below are two tables displaying details about this particular solar eclipse. The first table outlines times at which the Moon's penumbra or umbra attains the specific parameter, and the second table describes various other 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 1883 A partial lunar eclipse on April 22. • A total solar eclipse on May 6.A partial lunar eclipse on October 16. • An annular solar eclipse on October 30. Metonic • Preceded by: Solar eclipse of July 19, 1879 • Followed by: Solar eclipse of February 22, 1887 Tzolkinex • Preceded by: Solar eclipse of March 25, 1876 • Followed by: Solar eclipse of June 17, 1890 Half-Saros • Preceded by: Lunar eclipse of May 1, 1874 • Followed by: Lunar eclipse of May 11, 1892 Tritos • Preceded by: Solar eclipse of June 6, 1872 • Followed by: Solar eclipse of April 6, 1894 Solar Saros 136 • Preceded by: Solar eclipse of April 25, 1865 • Followed by: Solar eclipse of May 18, 1901 Inex • Preceded by: Solar eclipse of May 26, 1854 • Followed by: Solar eclipse of April 17, 1912 Triad • Preceded by: Solar eclipse of July 4, 1796 • Followed by: Solar eclipse of March 7, 1970 Solar eclipses of 1880–1884 The solar eclipses on January 11, 1880 (total), July 7, 1880 (annular), and December 31, 1880 (partial) occur in the previous lunar year eclipse set, and the partial solar eclipse on March 27, 1884 occurs in the next lunar year eclipse set. Saros 136 Metonic series Tritos series Inex series ==Notes==
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