Solar eclipse of November 1, 1929

Last updated
Solar eclipse of November 1, 1929
SE1929Nov01A.png
Map
Type of eclipse
NatureAnnular
Gamma 0.3514
Magnitude 0.9649
Maximum eclipse
Duration234 s (3 min 54 s)
Coordinates 4°30′N3°06′E / 4.5°N 3.1°E / 4.5; 3.1
Max. width of band134 km (83 mi)
Times (UTC)
Greatest eclipse12:05:10
References
Saros 132 (41 of 71)
Catalog # (SE5000) 9350

An annular solar eclipse occurred on November 1, 1929. 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 Spanish Sahara (today's West Sahara), French West Africa (parts now belonging to Mauritania, Mali, Burkina Faso, and southwestern tip of Benin), British Gold Coast (today's Ghana), French Togoland (today's Togo) including capital Lomé, Portuguese São Tomé and Príncipe (today's São Tomé and Príncipe), French Equatorial Africa (parts now belonging to Gabon and R. Congo) including capital Brazzaville, Belgian Congo (today's DR Congo) including capital Léopoldville, Northern Rhodesia (today's Zambia), British Tanganyika (now belonging to Tanzania) including capital Dar es Salaam, and British Seychelles (today's Seychelles) including capital Victoria.

Contents

Solar eclipses of 1928–1931

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]

Solar eclipse series sets from 1928 to 1931
Ascending node Descending node
117 May 19, 1928
SE1928May19T.png
Total (non-central)
122 November 12, 1928
SE1928Nov12P.png
Partial
127 May 9, 1929
SE1929May09T.png
Total
132 November 1, 1929
SE1929Nov01A.png
Annular
137 April 28, 1930
SE1930Apr28H.png
Hybrid
142 October 21, 1930
SE1930Oct21T.png
Total
147 April 18, 1931
SE1931Apr18P.png
Partial
152 October 11, 1931
SE1931Oct11P.png
Partial

Saros 132

This eclipse is a part of Saros cycle 132, repeating every 18 years, 11 days, containing 71 events. The series started with partial solar eclipse on August 13, 1208. It contains annular eclipses from March 17, 1569 through March 12, 2146, hybrid on March 23, 2164 and April 3, 2183 and total eclipses from April 14, 2200 through June 19, 2308. The series ends at member 71 as a partial eclipse on September 25, 2470. The longest duration of annular was 6 minutes, 56 seconds on May 9, 1641, and totality will be 2 minutes, 14 seconds on June 8, 2290. All eclipses in this series occurs at the Moon’s descending node.

Series members 28–50 occur between 1690 and 2100:
282930
SE1695Jun11A.png
June 11, 1695
SE1713Jun22A.png
June 22, 1713
SE1731Jul04A.png
July 4, 1731
313233
SE1749Jul14A.png
July 14, 1749
SE1767Jul25A.png
July 25, 1767
SE1785Aug05A.png
August 5, 1785
343536
SE1803Aug17A.png
August 17, 1803
SE1821Aug27A.png
August 27, 1821
SE1839Sep07A.png
September 7, 1839
373839
SE1857Sep18A.png
September 18, 1857
SE1875Sep29A.png
September 29, 1875
SE1893Oct09A.png
October 9, 1893
404142
SE1911Oct22A.png
October 22, 1911
SE1929Nov01A.png
November 1, 1929
SE1947Nov12A.png
November 12, 1947
434445
SE1965Nov23A.png
November 23, 1965
SE1983Dec04A.png
December 4, 1983
SE2001Dec14A.png
December 14, 2001
464748
SE2019Dec26A.png
December 26, 2019
SE2038Jan05A.png
January 5, 2038
SE2056Jan16A.png
January 16, 2056
4950
SE2074Jan27A.png
January 27, 2074
SE2092Feb07A.png
February 7, 2092

Notes

  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.

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References