Solar eclipse of October 14, 2004

A partial solar eclipse occurred on October 13–14, 2004. 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 partial solar eclipse occurs in the polar regions of the Earth when the center of the Moon's shadow misses the Earth. It was the 54th eclipse of the 124th Saros cycle, which began with a partial eclipse on March 6, 1049 and will conclude with a partial eclipse on May 11, 2347.

Solar eclipse of October 14, 2004
Map
Type of eclipse
NaturePartial
Gamma1.0348
Magnitude0.9282
Maximum eclipse
Coordinates61.2°N 153.7°W / 61.2; -153.7
Times (UTC)
Greatest eclipse3:00:23
References
Saros124 (54 of 73)
Catalog # (SE5000)9518

Images


Animated path

Eclipses of 2004

Solar eclipses 2004–2007

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]

Metonic series

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.[2]

References

  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. Freeth, Tony. "Note S1: Eclipses & Predictions". plos.org. Retrieved 6 October 2018.

Photos:

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