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Solar eclipse of January 3, 1946

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Solar eclipse of January 3, 1946
Map
Type of eclipse
NaturePartial
Gamma−1.2392
Magnitude0.5529
Maximum eclipse
Coordinates67°06′S 177°36′E / 67.1°S 177.6°E / -67.1; 177.6
Times (UTC)
Greatest eclipse12:16:11
References
Saros150 (13 of 71)
Catalog # (SE5000)9388

A partial solar eclipse occurred on January 3, 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[edit]

Solar eclipses 1942–1946[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 1942 to 1946
Ascending node   Descending node
Saros Map Gamma Saros Map Gamma
115 August 12, 1942

Partial
–1.52444 120 February 4, 1943

Total
0.87335
125 August 1, 1943

Annular
–0.80410 130 January 25, 1944

Total
0.20246
135 July 20, 1944

Annular
–0.03135 140 January 14, 1945

Annular
–0.49366
145 July 9, 1945

Total
0.73557 150 January 3, 1946

Partial
–1.23918
155 June 29, 1946

Partial
1.43612

Saros 150[edit]

It is a part of Saros cycle 150, repeating every 18 years, 11 days, containing 71 events. The series started with partial solar eclipse on August 24, 1729. It contains annular eclipses from April 22, 2126 through June 22, 2829. There are no total eclipses in this series. The series ends at member 71 as a partial eclipse on September 29, 2991. The longest duration of annularity will be 9 minutes, 58 seconds on December 19, 2522.

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]