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Solar eclipse of April 6, 1913

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Solar eclipse of April 6, 1913
Map
Type of eclipse
NaturePartial
Gamma1.3147
Magnitude0.4244
Maximum eclipse
Coordinates61°12′N 175°42′E / 61.2°N 175.7°E / 61.2; 175.7
Times (UTC)
Greatest eclipse17:33:07
References
Saros147 (17 of 80)
Catalog # (SE5000)9310

A partial solar eclipse occurred on April 6, 1913. 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.

Solar eclipses 1910–1913

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]

The partial solar eclipse on August 31, 1913 occurs in the next lunar year eclipse set.

Solar eclipse series sets from 1910 to 1913
Ascending node   Descending node
Saros Map Gamma Saros Map Gamma
117 May 9, 1910

Total
−0.9437 122 November 2, 1910

Partial
1.0603
127 April 28, 1911

Total
−0.2294 132 October 22, 1911

Annular
0.3224
137 April 17, 1912

Hybrid
0.528 142 October 10, 1912

Total
−0.4149
147 April 6, 1913

Partial
1.3147 152 September 30, 1913

Partial
−1.1005

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.