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Solar eclipse of September 9, 1904

A total solar eclipse occurred at the Moon's ascending node of orbit on Friday, September 9, 1904, with a magnitude of 1.0709. 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 1.5 hours after perigee, the Moon's apparent diameter was larger.

Observations
The National Astronomical Observatory of Chile established an observation station in Taltal, Antofagasta, but the eclipse was clouded out and could not be seen. In the capital city Santiago, a partial eclipse was seen just before sunset. == 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 1904 A penumbral lunar eclipse on March 2. • An annular solar eclipse on March 17. • A penumbral lunar eclipse on March 31. • A total solar eclipse on September 9.A penumbral lunar eclipse on September 24. Metonic • Preceded by: Solar eclipse of November 22, 1900 • Followed by: Solar eclipse of June 28, 1908 Tzolkinex • Preceded by: Solar eclipse of July 29, 1897 • Followed by: Solar eclipse of October 22, 1911 Half-Saros • Preceded by: Lunar eclipse of September 4, 1895 • Followed by: Lunar eclipse of September 15, 1913 Tritos • Preceded by: Solar eclipse of October 9, 1893 • Followed by: Solar eclipse of August 10, 1915 Solar Saros 133 • Preceded by: Solar eclipse of August 29, 1886 • Followed by: Solar eclipse of September 21, 1922 Inex • Preceded by: Solar eclipse of September 29, 1875 • Followed by: Solar eclipse of August 21, 1933 Triad • Preceded by: Solar eclipse of November 9, 1817 • Followed by: Solar eclipse of July 11, 1991 Solar eclipses of 1902–1906 Saros 133 Metonic series Tritos series Inex series == Notes ==
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