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(Top)
 


1 Related eclipses  



1.1  Eclipses in 1943  





1.2  Metonic  





1.3  Tzolkinex  





1.4  Half-Saros  





1.5  Tritos  





1.6  Solar Saros 125  





1.7  Inex  





1.8  Triad  





1.9  Solar eclipses of 19421946  





1.10  Saros 125  





1.11  Metonic series  







2 Notes  





3 References  














Solar eclipse of August 1, 1943






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Solar eclipse of August 1, 1943

Map

Type of eclipse
NatureAnnular
Gamma−0.8041
Magnitude0.9409
Maximum eclipse
Duration419 s (6 min 59 s)
Coordinates34°48′S 108°36′E / 34.8°S 108.6°E / -34.8; 108.6
Max. width of band367 km (228 mi)
Times (UTC)
Greatest eclipse4:16:13
References
Saros125 (50 of 73)
Catalog # (SE5000)9383

An annular solar eclipse occurred at the Moon's ascending node of orbit on Sunday, August 1, 1943, with a magnitude of 0.9409. 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. An annular solar eclipse occurs when the Moon's apparent diameter is smaller than the Sun's, blocking most of the Sun's light and causing the Sun to look like an annulus (ring). An annular eclipse appears as a partial eclipse over a region of the Earth thousands of kilometres wide. Annularity was visible in the southern Indian Ocean, with the only land being Île AmsterdaminFrench Madagascar (now belonging to French Southern and Antarctic Lands). A partial solar eclipse was visible from Australia, Indonesia, Malaysia, eastern Madagascar, Antarctica's Wilkes Land.

[edit]

Eclipses in 1943

[edit]

Metonic

[edit]

Tzolkinex

[edit]

Half-Saros

[edit]

Tritos

[edit]

Solar Saros 125

[edit]

Inex

[edit]

Triad

[edit]

Solar eclipses of 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]

The partial solar eclipses on March 16, 1942 and September 10, 1942 occur in the previous lunar year eclipse set, and the partial solar eclipses on May 30, 1946 and November 23, 1946 occur in the next lunar year eclipse set.

Solar eclipse series sets from 1942 to 1946
Ascending node   Descending node
Saros Map Gamma Saros Map Gamma
115 August 12, 1942

Partial
−1.5244 120 February 4, 1943

Total
0.8734
125 August 1, 1943

Annular
−0.8041 130 January 25, 1944

Total
0.2025
135 July 20, 1944

Annular
−0.0314 140 January 14, 1945

Annular
−0.4937
145 July 9, 1945

Total
0.7356 150 January 3, 1946

Partial
−1.2392
155 June 29, 1946

Partial
1.4361

Saros 125

[edit]

This eclipse is a part of Saros series 125, repeating every 18 years, 11 days, and containing 73 events. The series started with a partial solar eclipse on February 4, 1060. It contains total eclipses from June 13, 1276 through July 16, 1330; hybrid eclipses on July 26, 1348 and August 7, 1366; and annular eclipses from August 17, 1384 through August 22, 1979. The series ends at member 73 as a partial eclipse on April 9, 2358. 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 totality was produced by member 14 at 1 minutes, 11 seconds on June 25, 1294, and the longest duration of annularity was produced by member 48 at 7 minutes, 23 seconds on July 10, 1907. All eclipses in this series occur at the Moon’s ascending node of orbit.[2]

Series members 43–64 occur between 1801 and 2200:
43 44 45

May 16, 1817

May 27, 1835

June 6, 1853
46 47 48

June 18, 1871

June 28, 1889

July 10, 1907
49 50 51

July 20, 1925

August 1, 1943

August 11, 1961
52 53 54

August 22, 1979

September 2, 1997

September 13, 2015
55 56 57

September 23, 2033

October 4, 2051

October 15, 2069
58 59 60

October 26, 2087

November 6, 2105

November 18, 2123
61 62 63

November 28, 2141

December 9, 2159

December 20, 2177
64

December 31, 2195

Metonic series

[edit]

The metonic series repeats eclipses every 19 years (6939.69 days), lasting about 5 cycles. Eclipses occur in nearly the same calendar date. In addition, the octon subseries repeats 1/5 of that or every 3.8 years (1387.94 days). All eclipses in this table occur at the Moon's ascending node.

22 eclipse events between December 24, 1916 and July 31, 2000
December 24–25 October 12 July 31–August 1 May 19–20 March 7
111 113 115 117 119

December 24, 1916

July 31, 1924

May 19, 1928

March 7, 1932
121 123 125 127 129

December 25, 1935

October 12, 1939

August 1, 1943

May 20, 1947

March 7, 1951
131 133 135 137 139

December 25, 1954

October 12, 1958

July 31, 1962

May 20, 1966

March 7, 1970
141 143 145 147 149

December 24, 1973

October 12, 1977

July 31, 1981

May 19, 1985

March 7, 1989
151 153 155

December 24, 1992

October 12, 1996

July 31, 2000

Notes

[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.
  • ^ "NASA - Catalog of Solar Eclipses of Saros 125". eclipse.gsfc.nasa.gov.
  • References

    [edit]
  • t
  • e

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