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Solar eclipse of December 2, 1937

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Solar eclipse of December 2, 1937
Map
Type of eclipse
NatureAnnular
Gamma0.4389
Magnitude0.9184
Maximum eclipse
Duration720 s (12 min 0 s)
Coordinates4°00′N 167°48′W / 4°N 167.8°W / 4; -167.8
Max. width of band344 km (214 mi)
Times (UTC)
Greatest eclipse23:05:45
References
Saros141 (19 of 70)
Catalog # (SE5000)9370

An annular solar eclipse occurred at the Moon's ascending node of orbit on Thursday, December 2, 1937, with a magnitude of 0.9184. 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 Ogasawara, Tokyo and South Seas Mandate (the part now belonging to Marshall Islands) in Japan, and Gilbert and Ellice Islands (the part now belonging to Kiribati).

The duration of annularity at maximum eclipse (closest to but slightly shorter than the longest duration) was 12 minutes, 0.33 seconds in the Pacific Ocean. It was the longest annular solar eclipse since December 25, 1628, but the Solar eclipse of December 14, 1955 lasted longer.[1]

Related eclipses[edit]

Eclipses in 1937[edit]

Metonic[edit]

Tzolkinex[edit]

Half-Saros[edit]

Tritos[edit]

Solar Saros 141[edit]

Inex[edit]

Triad[edit]

Solar eclipses of 1935–1938[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]

The partial solar eclipses on February 3, 1935 and July 30, 1935 occur in the previous lunar year eclipse set.

Solar eclipse series sets from 1935 to 1938
Ascending node   Descending node
Saros Map Gamma Saros Map Gamma
111 January 5, 1935

Partial
−1.5381 116 June 30, 1935

Partial
1.3623
121 December 25, 1935

Annular
−0.9228 126 June 19, 1936

Total
0.5389
131 December 13, 1936

Annular
−0.2493 136

Totality in Kanton Island,
Kiribati
June 8, 1937

Total
−0.2253
141 December 2, 1937

Annular
0.4389 146 May 29, 1938

Total
−0.9607
151 November 21, 1938

Partial
1.1077

Saros 141[edit]

This eclipse is a part of Saros series 141, repeating every 18 years, 11 days, and containing 70 events. The series started with a partial solar eclipse on May 19, 1613. It contains annular eclipses from August 4, 1739 through October 14, 2640. There are no hybrid or total eclipses in this set. The series ends at member 70 as a partial eclipse on June 13, 2857. 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 20 at 12 minutes, 9 seconds on December 14, 1955. All eclipses in this series occur at the Moon’s ascending node of orbit.[3]

Series members 12–33 occur between 1801 and 2200:
12 13 14

September 17, 1811

September 28, 1829

October 9, 1847
15 16 17

October 19, 1865

October 30, 1883

November 11, 1901
18 19 20

November 22, 1919

December 2, 1937

December 14, 1955
21 22 23

December 24, 1973

January 4, 1992

January 15, 2010
24 25 26

January 26, 2028

February 5, 2046

February 17, 2064
27 28 29

February 27, 2082

March 10, 2100

March 22, 2118
30 31 32

April 1, 2136

April 12, 2154

April 23, 2172
33

May 4, 2190

Tritos series[edit]

This eclipse is a part of a tritos cycle, repeating at alternating nodes every 135 synodic months (≈ 3986.63 days, or 11 years minus 1 month). Their appearance and longitude are irregular due to a lack of synchronization with the anomalistic month (period of perigee), but groupings of 3 tritos cycles (≈ 33 years minus 3 months) come close (≈ 434.044 anomalistic months), so eclipses are similar in these groupings.

Notes[edit]

  1. ^ "Annular Solar Eclipses with Durations Exceeding 11m 00s: -3999 to 6000". NASA Eclipse Web Site.
  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 141". eclipse.gsfc.nasa.gov.

References[edit]

External links[edit]