Solar eclipse of November 23, 1946

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.

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

Related eclipses edit

Solar eclipses 1946–1949 edit

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 edit

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 edit

  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 edit