Template:Solar eclipse set 1968–1971
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 July 22, 1971 occurs in the next lunar year eclipse set.
Solar eclipse series sets from 1968 to 1971 | ||||||
---|---|---|---|---|---|---|
Ascending node | Descending node | |||||
Saros | Map | Gamma | Saros | Map | Gamma | |
119 | March 28, 2968![]() Partial |
−1.037 | 124 | September 22, 1968![]() Total |
0.9451 | |
129 | March 18, 1969![]() Annular |
−0.2704 | 134 | September 11, 1969![]() Annular |
0.2201 | |
139![]() Totality in Williamston, NC USA |
March 7, 1970![]() Total |
0.4473 | 144 | August 31, 1970![]() Annular |
−0.5364 | |
149 | February 25, 1971![]() Partial |
1.1188 | 154 | August 20, 1971![]() Partial |
−1.2659 |
- ^ 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.