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 1993 to 1996 | ||||||
---|---|---|---|---|---|---|
Descending node | Ascending node | |||||
Saros | Map | Gamma | Saros | Map | Gamma | |
118 | 1993 May 21 Partial |
1.13720 | 123 | 1993 November 13 Partial |
−1.04114 | |
128 Partial from Bismarck, ND |
1994 May 10 Annular |
0.40771 | 133 Totality at Bolivia |
1994 November 3 Total |
−0.35216 | |
138 | 1995 April 29 Annular |
−0.33821 | 143 Totality at Dundlod, India |
1995 October 24 Total |
0.35176 | |
148 | 1996 April 17 Partial |
−1.05796 | 153 | 1996 October 12 Partial |
1.12265 |
- ^ 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.