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Solar eclipse of May 9, 1967

From Wikipedia, the free encyclopedia

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.

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Transcription

Related eclipses

Solar eclipses of 1964–1967

This eclipse is a member of a 1964–1967 series at alternating nodes every 6 synodic months.

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 Gamma Saros Map Gamma
117

1964 June 10
Partial
−1.13926 122

1964 December 4
Partial
1.11929
127

1965 May 30
Total
−0.42251 132

1965 November 23
Annular
0.39061
137

1966 May 20
Annular
0.34672 142

1966 November 12
Total
−0.33001
147

1967 May 9
Partial
1.14218 152

1967 November 2
Total (non-central)
−1.00067

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

External links

This page was last edited on 26 February 2022, at 14:44
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