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Solar eclipse of July 20, 1944

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Solar eclipse of July 20, 1944
Map
Type of eclipse
NatureAnnular
Gamma−0.0314
Magnitude0.97
Maximum eclipse
Duration222 s (3 min 42 s)
Coordinates19°00′N 95°42′E / 19°N 95.7°E / 19; 95.7
Max. width of band108 km (67 mi)
Times (UTC)
Greatest eclipse5:43:13
References
Saros135 (35 of 71)
Catalog # (SE5000)9385

An annular solar eclipse occurred at the Moon's ascending node of orbit on Thursday, July 20, 1944, with a magnitude of 0.97. 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 from British Uganda (today's Uganda), Anglo-Egyptian Sudan (the part now belonging to South Sudan), British Kenya (today's Kenya), Ethiopia, British Somaliland (today's Somalia), British Raj (the part now belonging to India), Burma, Thailand, French Indochina (the parts now belonging to Laos and Vietnam), Philippines, South Seas Mandate in Japan (the part now belonging to Hatohobei, Palau) the Territory of New Guinea (now belonging to Papua New Guinea).

Related eclipses[edit]

Eclipses in 1944[edit]

Metonic[edit]

Tzolkinex[edit]

Half-Saros[edit]

Tritos[edit]

Solar Saros 135[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 135[edit]

This eclipse is a part of Saros series 135, repeating every 18 years, 11 days, and containing 71 events. The series started with a partial solar eclipse on July 5, 1331. It contains annular eclipses from October 21, 1511 through February 24, 2305; hybrid eclipses on March 8, 2323 and March 18, 2341; and total eclipses from March 29, 2359 through May 22, 2449. The series ends at member 71 as a partial eclipse on August 17, 2593. 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 was produced by member 16 at 10 minutes, 41 seconds on December 24, 1601, and the longest duration of totality will be produced by member 62 at 2 minutes, 27 seconds on May 12, 2431. All eclipses in this series occur at the Moon’s ascending node of orbit.[2]

Series members 28–49 occur between 1801 and 2200:
28 29 30

May 5, 1818

May 15, 1836

May 26, 1854
31 32 33

June 6, 1872

June 17, 1890

June 28, 1908
34 35 36

July 9, 1926

July 20, 1944

July 31, 1962
37 38 39

August 10, 1980

August 22, 1998

September 1, 2016
40 42 42

September 12, 2034

September 22, 2052

October 4, 2070
43 44 45

October 14, 2088

October 26, 2106

November 6, 2124
46 47 48

November 17, 2142

November 27, 2160

December 9, 2178
49

December 19, 2196

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).

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.
  2. ^ "NASA - Catalog of Solar Eclipses of Saros 135". eclipse.gsfc.nasa.gov.

References[edit]