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 eclipses on April 6, 1913 and September 30, 1913 occur in the previous lunar year eclipse set, and the solar eclipses on December 24, 1916 (partial), June 19, 1917 (partial), and December 14, 1917 (annular) occur in the next lunar year eclipse set.
| Solar eclipse series sets from 1913 to 1917 | ||||||
|---|---|---|---|---|---|---|
| Descending node | Ascending node | |||||
| Saros | Map | Gamma | Saros | Map | Gamma | |
| 114 | August 31, 1913 Partial |
1.4512 | 119 | February 25, 1914 Annular |
−0.9416 | |
| 124 | August 21, 1914 Total |
0.7655 | 129 | February 14, 1915 Annular |
−0.2024 | |
| 134 | August 10, 1915 Annular |
0.0124 | 139.png)
|
February 3, 1916 Total |
0.4987 | |
| 144 | July 30, 1916 Annular |
−0.7709 | 149 | January 23, 1917 Partial |
1.1508 | |
| 154 | July 19, 1917 Partial |
−1.5101 | ||||
- ^ 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.