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Solar eclipse of November 23, 2003

A total solar eclipse occurred at the Moon's descending node of orbit between Sunday, November 23 and Monday, November 24, 2003, with a magnitude of 1.0379. 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 25 minutes before perigee, the Moon's apparent diameter was near its maximum. Perigee did occur just past the greatest point of this eclipse.

Observations
A Russian icebreaker departed from Port Elizabeth, South Africa carrying tourists to observe the eclipse near the Shackleton Ice Shelf and Novolazarevskaya Station, and then sailed to Hobart, Tasmania. About 100 people from 15 countries were on board, including Iranian amateur astronomer Babak Amin Tafreshi, NASA's Goddard Space Flight Center astrophysicist Fred Espenak, and Williams College professor Jay Pasachoff. There were also about 200 scientists and tourists taking two commercial charter flights to observe it over Antarctica. This was the first time humans observed a total solar eclipse from Antarctica. == Images ==
Eclipse timing
Places experiencing partial eclipse == 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 February 5, 2000 • Followed by: Solar eclipse of September 11, 2007 Tzolkinex • Preceded by: Solar eclipse of October 12, 1996 • Followed by: Solar eclipse of January 4, 2011 Half-Saros • Preceded by: Lunar eclipse of November 18, 1994 • Followed by: Lunar eclipse of November 28, 2012 Tritos • Preceded by: Solar eclipse of December 24, 1992 • Followed by: Solar eclipse of October 23, 2014 Solar Saros 152 • Preceded by: Solar eclipse of November 12, 1985 • Followed by: Solar eclipse of December 4, 2021 Inex • Preceded by: Solar eclipse of December 13, 1974 • Followed by: Solar eclipse of November 3, 2032 Triad • Preceded by: Solar eclipse of January 23, 1917 • Followed by: Solar eclipse of September 23, 2090 Solar eclipses of 2000–2003 Saros 152 Metonic series Tritos series Inex series ==Notes==
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