Solar eclipse of November 22, 1919

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Solar eclipse of November 22, 1919
SE1919Nov22A.png
Map
Type of eclipse
NatureAnnular
Gamma0.4549
Magnitude0.9198
Maximum eclipse
Duration697 sec (11 m 37 s)
Coordinates6°54′N 48°54′W / 6.9°N 48.9°W / 6.9; -48.9
Max. width of band341 km (212 mi)
Times (UTC)
Greatest eclipse15:14:12
References
Saros141 (18 of 70)
Catalog # (SE5000)9327

An annular solar eclipse occurred on Saturday, November 22, 1919. 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. It occurred in over half of North America, much of South America, a part of Western Europe and about a third of Africa.

Places inside the annular eclipse included North America and the Caribbean, including Austin, San Antonio, Houston and Galveston, Texas in the United States and was close to Mexico at around 7:30 CT (13:30 UTC), more than a quarter of the Gulf of Mexico and close to the Florida Keys in the United States which occurred before 8:45 ET (13:45 UTC), it also included Cuba, most of Haiti and the southwesternmost Dominican Republic , it was almost near Venezuela and it included Saint Vincent and the Grenadines and Barbados which happened in the mid morning hours. The greatest eclipse occurred at 15:14:12 UTC. In Africa, it included the Gambia, southern Senegal including Casamance, Portuguese Guinea (now Guinea-Bissau), the northern part of French Guinea (now Guinea) which occurred before 15:45 (16:45 UTC) and southeasternmost Mauritania and the middle portion of the French Sudan (now Mali) which included Bamako and Timbuktu, it occurred in the late afternoon before sunset at 17:00 UTC.

The duration of annularity at maximum eclipse (closest to but slightly shorter than the longest duration) was 11 minutes, 36.56 seconds in the Atlantic Ocean north of Brazil. It was the longest annular solar eclipse since January 5, 1647, but the Solar eclipse of December 2, 1937 lasted longer.[1]

Related eclipses[]

Solar eclipses 1916–1920[]

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]

Solar eclipse series sets from 1916–1920
Ascending node   Descending node
111 December 24, 1916
SE1916Dec24P.png
Partial
116 June 19, 1917
SE1917Jun19P.png
Partial
121 December 14, 1917
SE1917Dec14A.png
Annular
126 June 8, 1918
SE1918Jun08T.png
Total
131 December 3, 1918
SE1918Dec03A.png
Annular
136 May 29, 1919
SE1919May29T.png
Total
141 November 22, 1919
SE1919Nov22A.png
Annular
146 May 18, 1920
SE1920May18P.png
Partial
151 November 10, 1920
SE1920Nov10P.png
Partial

Saros 141[]

Solar saros 141, repeating every about 18 years, 11 days, and 8 hours, contains 70 events. The series started with partial solar eclipse on May 19, 1613. It contains 41 annular eclipses from August 4, 1739, to October 14, 2460. There are no total eclipses in this series. The series ends at member 70 as a partial eclipse on June 13, 2857. The longest annular eclipse occurred on December 14, 1955, with maximum duration of annularity at 12 minutes and 9 seconds. All eclipses in this series occur at the Moon’s ascending node.[3]

Series members 17–36 occur between 1901 and 2259
17 18 19
SE1901Nov11A.png
November 11, 1901
SE1919Nov22A.png
November 22, 1919
SE1937Dec02A.png
December 2, 1937
20 21 22
SE1955Dec14A.png
December 14, 1955
SE1973Dec24A.png
December 24, 1973
SE1992Jan04A.png
January 4, 1992
23 24 25
SE2010Jan15A.png
January 15, 2010
SE2028Jan26A.png
January 26, 2028
SE2046Feb05A.png
February 5, 2046
26 27 28
SE2064Feb17A.png
February 17, 2064
SE2082Feb27A.png
February 27, 2082
SE2100Mar10A.png
March 10, 2100
29 30 31
SE2118Mar22A.png
March 22, 2118
SE2136Apr01A.png
April 1, 2136
SE2154Apr12A.png
April 12, 2154
32 33 34
SE2172Apr23A.png
April 23, 2172
SE2190May04A.png
May 4, 2190
SE2208May15A.png
May 15, 2208
35 36
SE2226May27A.png
May 27, 2226
SE2244Jun06A.png
June 6, 2244

Inex series[]

This eclipse is a part of the long period inex cycle, repeating at alternating nodes, every 358 synodic months (≈ 10,571.95 days, or 29 years minus 20 days). Their appearance and longitude are irregular due to a lack of synchronization with the anomalistic month (period of perigee). However, groupings of 3 inex cycles (≈ 87 years minus 2 months) comes close (≈ 1,151.02 anomalistic months), so eclipses are similar in these groupings.

Notes[]

  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. ^ Saros Series Catalog of Solar Eclipses NASA Eclipse Web Site.

References[]

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