Template:Solar eclipse set 1964–1967: Difference between revisions
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|152||[[File:SE1967Nov02T.png|150px]]<BR>[[Solar eclipse of November 2, 1967|November 2, 1967]]<BR>Total |
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Revision as of 06:21, 19 October 2015
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]
Note: Partial solar eclipses on January 14, 1964 and July 9, 1964 belong to the previous lunar year set.
| Ascending node | Descending node | |||
|---|---|---|---|---|
| Saros | Map | Saros | Map | |
| 117 |  June 10, 1964 Partial |
122 |  December 4, 1964 Partial | |
| 127 |  May 30, 1965 Total |
132 |  November 23, 1965 Annular | |
| 137 |  May 20, 1966 Annular |
142 |  November 12, 1966 Total | |
| 147 |  May 9, 1967 Partial |
152 |  November 2, 1967 Total | |
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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.