Template:Solar eclipse set 1950–1953
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 1950 to 1953 | ||||||
|---|---|---|---|---|---|---|
| Ascending node | Descending node | |||||
| Saros | Map | Gamma | Saros | Map | Gamma | |
| 119 |  1950 March 18 Annular (non-central) |
-0.99880 | 124 |  1950 September 12 Total |
0.89030 | |
| 129 |  1951 March 7 Annular |
-0.24196 | 134 |  1951 September 1 Annular |
0.15570 | |
| 139 |  1952 February 25 Total |
0.46973 | 144 |  1952 August 20 Annular |
-0.61023 | |
| 149 |  1953 February 14 Partial |
1.13308 | 154 |  1953 August 9 Partial |
-1.34403 | |
| Solar eclipse of July 11, 1953 belongs to the next lunar year set. | ||||||
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- ^ 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.