Solar eclipse of May 9, 1967
| Solar eclipse of May 9, 1967 | |
|---|---|
 Map | |
| Type of eclipse | |
| Nature | Partial |
| Gamma | 1.1422 |
| Magnitude | 0.7201 |
| Maximum eclipse | |
| Coordinates | 62°30′N 168°06′W / 62.5°N 168.1°W |
| Times (UTC) | |
| Greatest eclipse | 14:42:48 |
| References | |
| Saros | 147 (20 of 80) |
| Catalog # (SE5000) | 9436 |
A partial solar eclipse occurred on May 9, 1967. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth. A partial solar eclipse occurs in the polar regions of the Earth when the center of the Moon's shadow misses the Earth.
Related eclipses
Solar eclipses of 1964-1967
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.
| Solar eclipse series sets from 1964-1967 | ||||
|---|---|---|---|---|
| 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 | |
References
- ↑ 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.
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External links
- Earth visibility chart and eclipse statistics Eclipse Predictions by Fred Espenak, NASA/GSFC
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