Solar eclipse of November 2, 1967

Solar eclipse of November 2, 1967
Map
Type of eclipse
Nature Total
Gamma 1.0007
Magnitude 1.0126
Maximum eclipse
Duration -
Coordinates 62°00′S 27°48′W / 62°S 27.8°W / -62; -27.8
Max. width of band - km
Times (UTC)
Greatest eclipse 5:38:56
References
Saros 152 (10 of 70)
Catalog # (SE5000) 9437

A total solar eclipse occurred on November 2, 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 total solar eclipse occurs when the Moon's apparent diameter is larger than the Sun's, blocking all direct sunlight, turning day into darkness. Totality occurs in a narrow path across Earth's surface, with the partial solar eclipse visible over a surrounding region thousands of kilometres wide.

Solar eclipses of 1964-1967

Each member 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.

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
SarosMap SarosMap
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

Notes

    References

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