Solar eclipse of November 1, 1929
An annular solar eclipse occurred on Friday, 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.
Related eclipses
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![]() Total (non-central) | 122 | November 12, 1928![]() Partial | |
127 | May 9, 1929![]() Total | 132 | November 1, 1929![]() Annular | |
137 | April 28, 1930![]() Hybrid | 142 | October 21, 1930![]() Total | |
147 | April 18, 1931![]() Partial | 152 | October 11, 1931![]() 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 22, 2164 and April 3, 2182 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 annularity 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: | ||
---|---|---|
28 | 29 | 30 |
![]() June 11, 1695 | ![]() June 22, 1713 | ![]() July 4, 1731 |
31 | 32 | 33 |
![]() July 14, 1749 | ![]() July 25, 1767 | ![]() August 5, 1785 |
34 | 35 | 36 |
![]() August 17, 1803 | ![]() August 27, 1821 | ![]() September 7, 1839 |
37 | 38 | 39 |
![]() September 18, 1857 | ![]() September 29, 1875 | ![]() October 9, 1893 |
40 | 41 | 42 |
![]() October 22, 1911 | ![]() November 1, 1929 | ![]() November 12, 1947 |
43 | 44 | 45 |
![]() November 23, 1965 | ![]() December 4, 1983 | ![]() December 14, 2001 |
46 | 47 | 48 |
![]() December 26, 2019 | ![]() January 5, 2038 | ![]() January 16, 2056 |
49 | 50 | |
![]() January 27, 2074 | ![]() February 7, 2092 |
Notes
- ^ 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.
References
- Earth visibility chart and eclipse statistics Eclipse Predictions by Fred Espenak, NASA/GSFC
- Google interactive map
- Besselian elements
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![21 August 2017 total solar eclipse](http://upload.wikimedia.org/wikipedia/commons/thumb/4/42/Solar_eclipse%2C_Miles_Landing_8-21-17_%2836842678271%29.jpg/80px-Solar_eclipse%2C_Miles_Landing_8-21-17_%2836842678271%29.jpg)
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![23 October 2014 partial eclipse](http://upload.wikimedia.org/wikipedia/commons/thumb/0/09/Partial_solar_eclipse_Oct_23_2014_Minneapolis_5-36pm_Ruen1.png/80px-Partial_solar_eclipse_Oct_23_2014_Minneapolis_5-36pm_Ruen1.png)
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