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Solar eclipse of May 10, 2013

An annular solar eclipse occurred at the Moon's descending node of orbit between Thursday, May 9 and Friday, May 10, 2013, with a magnitude of 0.9544. 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. An annular solar eclipse occurs when the Moon's apparent diameter is smaller than the Sun's, blocking most of the Sun's light and causing the Sun to look like an annulus (ring). An annular eclipse appears as a partial eclipse over a region of the Earth thousands of kilometres wide. Occurring about 3.6 days before apogee, the Moon's apparent diameter was smaller.

Visibility
Annularity was visible from a 171 to 225 kilometre-wide track that traversed Australia, eastern Papua New Guinea, the Solomon Islands, and the Gilbert Islands, with the maximum of 6 minutes 3 seconds visible from the Pacific Ocean east of French Polynesia. == Eclipse timing ==
Eclipse timing
Places experiencing annular eclipse Places experiencing partial eclipse == Gallery ==
Gallery
File:Sol ecl ann 2013-5-10.PNG|Simulation of greatest annularity east of Marakei, Kiribati. File:Eclipse 10th May 2013, Barkly Tablelands.JPG|Anthony Lagoon, Australia, 22:20 GMT (May 9) File:Most eclipse at 8 30am (8724535645).jpg|Partial from Manly Beach, New South Wales, 22:30 GMT (May 9) File:Annular Eclipse (on the cheap) (8724726923).jpg|Partial from Docklands, Victoria, 22:49 GMT (May 9) File:Solar eclipse (8725319204).jpg|Partial from Rockhampton, Queensland, 22:57 GMT (May 9) File:Annul (2016 03 21 21 16 42 UTC).jpg|Bairiki, Kiribati, 0:15 GMT File:Solar eclipse visible in coconut leaf shadow.jpg|Eclipse shadows from a coconut leaf shadow. From Tarawa, Kiribati at 0:30 GMT File:May 9 2013 Partial Solar Eclipse from Hawaii - 2.jpg|Partial from Waikiki, Hawaii, 2:12 GMT == 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. The first and last eclipse in this sequence is separated by one synodic month. == Related eclipses ==
Related eclipses
Eclipses in 2013 A partial lunar eclipse on April 25. • An annular solar eclipse on May 10.A penumbral lunar eclipse on May 25. • A penumbral lunar eclipse on October 18. • A hybrid solar eclipse on November 3. Metonic • Preceded by: Solar eclipse of July 22, 2009 • Followed by: Solar eclipse of February 26, 2017 Tzolkinex • Preceded by: Solar eclipse of March 29, 2006 • Followed by: Solar eclipse of June 21, 2020 Half-Saros • Preceded by: Lunar eclipse of May 4, 2004 • Followed by: Lunar eclipse of May 16, 2022 Tritos • Preceded by: Solar eclipse of June 10, 2002 • Followed by: Solar eclipse of April 8, 2024 Solar Saros 138 • Preceded by: Solar eclipse of April 29, 1995 • Followed by: Solar eclipse of May 21, 2031 Inex • Preceded by: Solar eclipse of May 30, 1984 • Followed by: Solar eclipse of April 20, 2042 Triad • Preceded by: Solar eclipse of July 9, 1926 • Followed by: Solar eclipse of March 10, 2100 Solar eclipses of 2011–2014 Saros 138 Metonic series Tritos series Inex series == Notes ==
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