Solar eclipse of May 9, 1967

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 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

Related eclipses edit

Solar eclipses of 1964–1967 edit

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 to 1967
Ascending node   Descending node
Saros Map Gamma Saros Map Gamma
117  
1964 June 10
Partial
−1.13926 122  
1964 December 04
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 09
Partial
1.14218 152  
1967 November 02
Total (non-central)
−1.00067

Metonic series edit

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 edit

External links edit