Solar eclipse of November 23, 2003

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Solar eclipse of November 23, 2003
SE2003Nov23T.png
Map
Type of eclipse
NatureTotal
Gamma-0.9638
Magnitude1.0379
Maximum eclipse
Duration117 sec (1 m 57 s)
Coordinates72°42′S 88°24′E / 72.7°S 88.4°E / -72.7; 88.4
Max. width of band495 km (308 mi)
Times (UTC)
Greatest eclipse22:50:22
References
Saros152 (12 of 70)
Catalog # (SE5000)9516

A total solar eclipse took place on November 23, 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. It was visible from a corridor in the Antarctic region. A partial eclipse was seen from the much broader path of the Moon's penumbra, including the southern tip of South America and most of Australia.

For most solar eclipses the path of totality moves eastwards. In this case the path moved south and then west round Antarctica.

Images[edit]

SE2003Nov23T.gif
Animated map

Related eclipses[edit]

Solar eclipses 2000–2003[edit]

This eclipse is a member of a semester series. An eclipse in a semester series of solar eclipses repeats approximately every 177 days and 4 hours (a semester) at alternating nodes of the Moon's orbit.[1]

Note: Partial solar eclipses on February 5, 2000 and July 31, 2000 occur in the previous lunar year set.

Saros 152[edit]

Solar saros 152, repeating every about 18 years and 11 days, contains 70 events. The series started with a partial solar eclipse on July 26, 1805. It has total eclipses from November 2, 1967, to September 14, 2490; hybrid eclipses from September 26, 2508, to October 17, 2544; and annular eclipses from October 29, 2562, to June 16, 2941. The series ends at member 70 as a partial eclipse on August 20, 3049. The longest total eclipse will occur on June 9, 2328, at 5 minutes and 15 seconds; the longest annular eclipse will occur on February 16, 2743, at 5 minutes and 20 seconds.[2]

Metonic series[edit]

The metonic series repeats eclipses every 19 years (6939.69 days), lasting about 5 cycles. Eclipses occur in nearly the same calendar date. In addition, the octon subseries repeats 1/5 of that or every 3.8 years (1387.94 days). All eclipses in this table occur at the Moon's descending node.

Notes[edit]

  1. ^ van Gent, R.H. "Solar- and Lunar-Eclipse Predictions from Antiquity to the Present". A Catalogue of Eclipse Cycles. Utrecht University. Retrieved 6 October 2018.
  2. ^ Saros Series Catalog of Solar Eclipses NASA Eclipse Web Site.

References[edit]

Photos: