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Solar eclipse of May 31, 2003

An annular solar eclipse occurred at the Moon's ascending node of orbit on Saturday, May 31, 2003, with a magnitude of 0.9384. 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 2.6 days after apogee, the Moon's apparent diameter was smaller.

Eclipse timing
Places experiencing annular eclipse Places experiencing partial eclipse == Gallery ==
Gallery
File:Garrulus - Eclips boven Chassepierre (by).jpg|Chassepierre, Belgium File:Eclipse--31-05-2003-2.jpg|From Belfort, France File:Sunrise Eclipse 2003 May 31.jpg|Wonneberg, Germany File:20030531 Oria (30847677046).jpg|From Oria, Italy File:Sun eclipse venice 5.31.2003 (32682446663).jpg|From Venice, Italy File:Zonsverduistering mei 2003 WIlleskop.jpg|Willeskop, Netherlands File:Solareclipse1 (1683459168).jpg|From Oslo, Norway File:Solar eclipse Ringerike 2003.jpg|From Ringerike, Norway File:Annular eclipse from Tom Mor - near maximum (geograph 1662570).jpg|Grantown-on-Spey, Scotland == 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 2003 A total lunar eclipse on May 16. • An annular solar eclipse on May 31.A total lunar eclipse on November 9. • A total solar eclipse on November 23. Metonic • Preceded by: Solar eclipse of August 11, 1999 • Followed by: Solar eclipse of March 19, 2007 Tzolkinex • Preceded by: Solar eclipse of April 17, 1996 • Followed by: Solar eclipse of July 11, 2010 Half-Saros • Preceded by: Lunar eclipse of May 25, 1994 • Followed by: Lunar eclipse of June 4, 2012 Tritos • Preceded by: Solar eclipse of June 30, 1992 • Followed by: Solar eclipse of April 29, 2014 Solar Saros 147 • Preceded by: Solar eclipse of May 19, 1985 • Followed by: Solar eclipse of June 10, 2021 Inex • Preceded by: Solar eclipse of June 20, 1974 • Followed by: Solar eclipse of May 9, 2032 Triad • Preceded by: Solar eclipse of July 30, 1916 • Followed by: Solar eclipse of March 31, 2090 Solar eclipses of 2000–2003 Saros 147 Metonic series Tritos series Inex series == See also ==
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