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Solar eclipse of January 25, 1944

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Solar eclipse of January 25, 1944
Map
Type of eclipse
NatureTotal
Gamma0.2025
Magnitude1.0428
Maximum eclipse
Duration249 s (4 min 9 s)
Coordinates7°36′S 50°12′W / 7.6°S 50.2°W / -7.6; -50.2
Max. width of band146 km (91 mi)
Times (UTC)
Greatest eclipse15:26:42
References
Saros130 (48 of 73)
Catalog # (SE5000)9384

A total solar eclipse occurred at the Moon's descending node of orbit on Tuesday, January 25, 1944, with a magnitude of 1.0428. 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 total solar eclipse occurs when the Moon's apparent diameter is larger than the Sun's, blocking all direct sunlight, turning day into darkness. Totality occurs in a narrow path across Earth's surface, with the partial solar eclipse visible over a surrounding region thousands of kilometres wide. Totality was visible from Peru, Brazil, British Sierra Leone (today's Sierra Leone), and French West Africa (the parts now belonging to Guinea, Mali, Burkina Faso and Niger, including Guinean capital Conakry). At greatest eclipse, the Sun was 78 degrees above horizon (just 12 degrees from zenith).

Observations[edit]

The National Astronomical Observatory in Tacubaya, Mexico sent a team to Chiclayo, Peru. The weather was clear during the eclipse, and because totality occurred shortly after sunrise with a relatively low solar zenith angle, the boundary between the corona and the background of the sky was not so obvious. Most images were taken successfully except for one with the long focus camera.[1]

Related eclipses[edit]

Eclipses in 1944[edit]

Metonic[edit]

Tzolkinex[edit]

Half-Saros[edit]

Tritos[edit]

Solar Saros 130[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.[2]

Note: The partial solar eclipse on September 10, 1942 occurs in the previous lunar year eclipse set.

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

Partial
120 February 4, 1943

Total
125 August 1, 1943

Annular
130 January 25, 1944

Total
135 July 20, 1944

Annular
140 January 14, 1945

Annular
145 July 9, 1945

Total
150 January 3, 1946

Partial
155 June 29, 1946

Partial

Saros 130[edit]

This eclipse is a part of Saros series 130, repeating every 18 years, 11 days, and containing 73 events. The series started with a partial solar eclipse on August 20, 1096. It contains total eclipses from April 5, 1475 through July 18, 2232. There are no annular or hybrid eclipses in this set. The series ends at member 73 as a partial eclipse on October 25, 2394. 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 30 at 6 minutes, 41 seconds on July 11, 1619. All eclipses in this series occur at the Moon’s descending node of orbit.[3]

Series members 41–62 occur between 1801 and 2200:
41 42 43

November 9, 1817

November 20, 1835

November 30, 1853
44 45 46

December 12, 1871

December 22, 1889

January 3, 1908
47 48 49

January 14, 1926

January 25, 1944

February 5, 1962
50 51 52

February 16, 1980

February 26, 1998

March 9, 2016
53 54 55

March 20, 2034

March 30, 2052

April 11, 2070
56 57 58

April 21, 2088

May 3, 2106

May 14, 2124
59 60 61

May 25, 2142

June 4, 2160

June 16, 2178
62

June 26, 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. ^ Harlow Shapley (1944). "Total Solar Eclipse of January 25, 1944". Popular Astronomy. 52: 107. Archived from the original on 27 August 2019.
  2. ^ 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.
  3. ^ "NASA - Catalog of Solar Eclipses of Saros 130". eclipse.gsfc.nasa.gov.

References[edit]