A partial solar eclipse occurred on September 30, 1913.[1][2][3][4] 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 September 30, 1913 | |
---|---|
Map | |
Type of eclipse | |
Nature | Partial |
Gamma | −1.1005 |
Magnitude | 0.8252 |
Maximum eclipse | |
Coordinates | 61°00′S 11°36′E / 61°S 11.6°E |
Times (UTC) | |
Greatest eclipse | 4:45:49 |
References | |
Saros | 152 (7 of 70) |
Catalog # (SE5000) | 9311 |
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.[5]
Solar eclipse series sets from 1910 to 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 |