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 July 11, 1953 occurs in the next lunar year eclipse set.
| Solar eclipse series sets from 1950 to 1953 | ||||||
|---|---|---|---|---|---|---|
| Ascending node | Descending node | |||||
| Saros | Map | Gamma | Saros | Map | Gamma | |
| 119 | March 18, 1950 Annular (non-central) |
0.9988 | 124 | September 12, 1950 Total |
0.8903 | |
| 129 | March 7, 1951 Annular |
−0.242 | 134 | September 1, 1951 Annular |
0.1557 | |
| 139 | February 25, 1952 Total |
0.4697 | 144 | August 20, 1952 Annular |
−0.6102 | |
| 149 | February 14, 1953 Partial |
1.1331 | 154 | August 9, 1953 Partial |
−1.344 | |
- ^ 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.