Solar eclipse of November 23, 1946

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Solar eclipse of November 23, 1946
Map
Type of eclipse
NaturePartial
Gamma1.105
Magnitude0.7758
Maximum eclipse
Coordinates63°24′N 45°18′W / 63.4°N 45.3°W / 63.4; -45.3
Times (UTC)
Greatest eclipse17:37:12
References
Saros122 (54 of 70)
Catalog # (SE5000)9391

A partial solar eclipse occurred on November 23, 1946. 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 1946–1949

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]

Solar eclipse series sets from 1946 to 1949
Ascending node   Descending node
Saros Map Gamma Saros Map Gamma
117 1946 May 30

Partial
-1.07105 122 1946 November 23

Partial
1.10500
127 1947 May 20

Total
-0.35279 132 1947 November 12

Annular
0.37431
137 1948 May 9

Annular
0.41332 142 1948 November 1

Total
-0.35172
147 1949 April 28

Partial
1.20682 152 1949 October 21

Partial
-1.02696

Tritos series

This eclipse is a part of a tritos cycle, repeating at alternating nodes every 135 synodic months (≈ 3986.63 days, or 11 years minus 1 month). Their appearance and longitude are irregular due to a lack of synchronization with the anomalistic month (period of perigee), but groupings of 3 tritos cycles (≈ 33 years minus 3 months) come close (≈ 434.044 anomalistic months), so eclipses are similar in these groupings.

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.

External links