Solar eclipse of August 30, 1924

A partial solar eclipse occurred at the Moon's ascending node of orbit on Saturday, August 30, 1924, with a magnitude of 0.4245. 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 August 30, 1924
Map
Type of eclipse
NaturePartial
Gamma1.3123
Magnitude0.4245
Maximum eclipse
Coordinates71°30′N 172°54′E / 71.5°N 172.9°E / 71.5; 172.9
Times (UTC)
Greatest eclipse8:23:00
References
Saros153 (4 of 70)
Catalog # (SE5000)9337
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Eclipses in 1924

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Metonic

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Tzolkinex

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Half-Saros

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Tritos

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Solar Saros 153

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Inex

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Triad

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Solar eclipses of 1921–1924

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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 July 31, 1924 occurs in the next lunar year eclipse set.

Solar eclipse series sets from 1921 to 1924
Descending node   Ascending node
Saros Map Gamma Saros Map Gamma
118 April 8, 1921
 
Annular
0.8869 123 October 1, 1921
 
Total
−0.9383
128 March 28, 1922
 
Annular
0.1711 133 September 21, 1922
 
Total
−0.213
138 March 17, 1923
 
Annular
−0.5438 143 September 10, 1923
 
Total
0.5149
148 March 5, 1924
 
Partial
−1.2232 153 August 30, 1924
 
Partial
1.3123

Saros 153

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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

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  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.
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