Solar eclipse of November 22, 1919

Solar eclipse of November 22, 1919
Solar eclipse of November 22, 1919
	UTC)
Greatest eclipse	15:14:12
References
Saros	141 (18 of 70)
Catalog # (SE5000)	9327

An annular

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

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 to 1920
Ascending node		Descending node
111	December 24, 1916 Partial	116	June 19, 1917 Partial
121	December 14, 1917 Annular	126	June 8, 1918 Total
131	December 3, 1918 Annular	136	May 29, 1919 Total
141	November 22, 1919 Annular	146	May 18, 1920 Partial
151	November 10, 1920 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
November 11, 1901	November 22, 1919	December 2, 1937
20	21	22
December 14, 1955	December 24, 1973	January 4, 1992
23	24	25
January 15, 2010	January 26, 2028	February 5, 2046
26	27	28
February 17, 2064	February 27, 2082	March 10, 2100
29	30	31
March 22, 2118	April 1, 2136	April 12, 2154
32	33	34
April 23, 2172	May 4, 2190	May 15, 2208
35	36
May 27, 2226	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.

Inex series members between 1901 and 2100:
November 22, 1919 (Saros 141)	November 1, 1948 (Saros 142)	October 12, 1977 (Saros 143)
September 22, 2006 (Saros 144)	September 2, 2035 (Saros 145)	August 12, 2064 (Saros 146)
July 23, 2093 (Saros 147)