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Solar eclipse of May 9, 1929

A total solar eclipse occurred at the Moon's ascending node of orbit on Thursday, May 9, 1929, with a magnitude of 1.0562. 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 1.7 days before perigee, the Moon's apparent diameter was larger.

Observations
A team of British and German scientists observed the total eclipse in Pattani province in southern Siam. King Rama VII and Queen Rambai Barni also visited the observation camp set up by foreign scientists and observed the eclipse together in Pattani. This was the last time that Siam (Thailand) received a large-scale solar eclipse observation team so far. The other teams Thailand received later, including the American team for the total solar eclipse of June 20, 1955 were much smaller. == 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 1929 A total solar eclipse on May 9.A penumbral lunar eclipse on May 23. • An annular solar eclipse on November 1. • A penumbral lunar eclipse on November 17. Metonic • Preceded by: Solar eclipse of July 20, 1925 • Followed by: Solar eclipse of February 24, 1933 Tzolkinex • Preceded by: Solar eclipse of March 28, 1922 • Followed by: Solar eclipse of June 19, 1936 Half-Saros • Preceded by: Lunar eclipse of May 3, 1920 • Followed by: Lunar eclipse of May 14, 1938 Tritos • Preceded by: Solar eclipse of June 8, 1918 • Followed by: Solar eclipse of April 7, 1940 Solar Saros 127 • Preceded by: Solar eclipse of April 28, 1911 • Followed by: Solar eclipse of May 20, 1947 Inex • Preceded by: Solar eclipse of May 28, 1900 • Followed by: Solar eclipse of April 19, 1958 Triad • Preceded by: Solar eclipse of July 8, 1842 • Followed by: Solar eclipse of March 9, 2016 Solar eclipses of 1928–1931 Saros 127 Metonic series Tritos series Inex series ==References==
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