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Solar eclipse of May 9, 1967

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Solar eclipse of May 9, 1967
Map
Type of eclipse
NaturePartial
Gamma1.1422
Magnitude0.7201
Maximum eclipse
Coordinates62°30′N 168°06′W / 62.5°N 168.1°W / 62.5; -168.1
Times (UTC)
Greatest eclipse14:42:48
References
Saros147 (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.

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]

The partial solar eclipses on January 14, 1964 and July 9, 1964 occur in the previous lunar year eclipse set.

Solar eclipse series sets from 1964 to 1967
Ascending node   Descending node
Saros Map Gamma Saros Map Gamma
117 June 10, 1964

Partial
−1.1393 122 December 4, 1964

Partial
1.1193
127 May 30, 1965

Total
−0.4225 132 November 23, 1965

Annular
0.3906
137 May 20, 1966

Annular
0.3467 142 November 12, 1966

Total
−0.33
147 May 9, 1967

Partial
1.1422 152 November 2, 1967

Total (non-central)
1.0007

Metonic series

The metonic series repeats eclipses every 19 years (6939.69 days), lasting about 5 cycles. Eclipses occur in nearly the same calendar date. In addition, the octon subseries repeats 1/5 of that or every 3.8 years (1387.94 days).

References

  1. ^ 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.