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. |
- ^ 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.