Solar eclipse of August 31, 1913

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 ==

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. The first and last eclipse in this sequence is separated by one synodic month. == Related eclipses ==

Eclipses in 1913 • A total lunar eclipse on March 22. • A partial solar eclipse on April 6. • A partial solar eclipse on August 31. • A total lunar eclipse on September 15. • A partial solar eclipse on September 30. Metonic • Followed by: Solar eclipse of June 19, 1917 Tzolkinex • Preceded by: Solar eclipse of July 21, 1906 Tritos • Followed by: Solar eclipse of July 31, 1924 Solar Saros 114 • Preceded by: Solar eclipse of August 20, 1895 • Followed by: Solar eclipse of September 12, 1931 Inex • Followed by: Solar eclipse of August 12, 1942 Triad • Preceded by: Solar eclipse of October 31, 1826 • Followed by: Solar eclipse of July 1, 2000 Solar eclipses of 1913–1917 Saros 114 Metonic series Tritos series Inex series ==References==