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Solar eclipse of September 10, 1942

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Solar eclipse of September 10, 1942
Map
Type of eclipse
NaturePartial
Gamma1.2571
Magnitude0.523
Maximum eclipse
Coordinates71°54′N 50°00′E / 71.9°N 50°E / 71.9; 50
Times (UTC)
Greatest eclipse15:39:32
References
Saros153 (5 of 70)
Catalog # (SE5000)9380

A partial solar eclipse occurred at the Moon's ascending node of orbit on Thursday, September 10, 1942, with a magnitude of 0.523. 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]

Eclipses in 1942[edit]

Metonic[edit]

Tzolkinex[edit]

Half-Saros[edit]

Tritos[edit]

Solar Saros 153[edit]

Inex[edit]

Triad[edit]

Solar eclipses of 1939–1942[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]

The partial solar eclipse on August 12, 1942 occurs in the next lunar year eclipse set.

Solar eclipse series sets from 1939 to 1942
Descending node   Ascending node
Saros Map Gamma Saros Map Gamma
118 April 19, 1939

Annular
0.9388 123 October 12, 1939

Total
−0.9737
128 April 7, 1940

Annular
0.219 133 October 1, 1940

Total
−0.2573
138 March 27, 1941

Annular
−0.5025 143 September 21, 1941

Total
0.4649
148 March 16, 1942

Partial
−1.1908 153 September 10, 1942

Partial
1.2571

Saros 153[edit]

This eclipse is a part of Saros series 153, repeating every 18 years, 11 days, and containing 70 events. The series started with a partial solar eclipse on July 28, 1870. It contains annular eclipses from December 17, 2104 through May 26, 2970. There are no hybrid or total eclipses in this set. The series ends at member 70 as a partial eclipse on August 22, 3114. Its eclipses are tabulated in three columns; every third eclipse in the same column is one exeligmos apart, so they all cast shadows over approximately the same parts of the Earth.

The longest duration of annularity will be produced by member 38 at 7 minutes, 1 seconds on September 5, 2537. All eclipses in this series occur at the Moon’s ascending node of orbit.[2]

Series members 1–19 occur between 1870 and 2200:
1 2 3

July 28, 1870

August 7, 1888

August 20, 1906
4 5 6

August 30, 1924

September 10, 1942

September 20, 1960
7 8 9

October 2, 1978

October 12, 1996

October 23, 2014
10 11 12

November 3, 2032

November 14, 2050

November 24, 2068
13 14 15

December 6, 2086

December 17, 2104

December 28, 2122
16 17 18

January 8, 2141

January 19, 2159

January 29, 2177
19

February 10, 2195

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.
  2. ^ "NASA - Catalog of Solar Eclipses of Saros 153". eclipse.gsfc.nasa.gov.

External links[edit]