Solar eclipse of April 6, 1913
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 eclipse of April 6, 1913 | |
---|---|
![]() Map | |
Type of eclipse | |
Nature | Partial |
Gamma | 1.3147 |
Magnitude | 0.4244 |
Maximum eclipse | |
Coordinates | 61.2°N 175.7°E |
Times (UTC) | |
Greatest eclipse | 17:33:07 |
References | |
Saros | 147 (17 of 80) |
Catalog # (SE5000) | 9310 |
Related eclipses
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]
Solar eclipse series sets from 1910–1913 | ||||
---|---|---|---|---|
Ascending node | Descending node | |||
117 | May 9, 1910![]() Total |
122 | November 2, 1910![]() Partial | |
127 | April 28, 1911![]() Total |
132 | October 22, 1911![]() Annular | |
137 | April 17, 1912![]() Hybrid |
142 | October 10, 1912![]() Total | |
147 | April 6, 1913![]() Partial |
152 | September 30, 1913![]() Partial |
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References
- 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.
External links
- Earth visibility chart and eclipse statistics Eclipse Predictions by Fred Espenak, NASA/GSFC
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