Solar eclipse of November 2, 1910

A partial solar eclipse occurred on November 2, 1910. 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 eclipse of November 2, 1910
Map
Type of eclipse
NaturePartial
Gamma1.0603
Magnitude0.8515
Maximum eclipse
Coordinates61.9°N 155.1°W / 61.9; -155.1
Times (UTC)
Greatest eclipse2:08:32
References
Saros122 (52 of 70)
Catalog # (SE5000)9305

Solar eclipses of 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]

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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.
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