Template:Solar eclipse set 1910–1913
Appearance
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 |
- ^ 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.