Solar eclipse of April 6, 1913
A partial solar eclipse occurred at the Moon's ascending node of orbit on Sunday, April 6, 1913,[1][2] with a magnitude of 0.4244. 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. A partial solar eclipse occurs in the polar regions of the Earth when the center of the Moon's shadow misses the Earth.
Related eclipses
Eclipses in 1913
- A total lunar eclipse on March 22, 1913.
- A partial solar eclipse on April 6, 1913.
- A partial solar eclipse on August 31, 1913.
- A total lunar eclipse on September 15, 1913.
- A partial solar eclipse on September 30, 1913.
Metonic
- Preceded by: Solar eclipse of June 17, 1909
- Followed by: Solar eclipse of January 23, 1917
Tzolkinex
- Preceded by: Solar eclipse of February 23, 1906
- Followed by: Solar eclipse of May 18, 1920
Half-Saros
- Preceded by: Lunar eclipse of March 31, 1904
- Followed by: Lunar eclipse of April 11, 1922
Tritos
- Preceded by: Solar eclipse of May 7, 1902
- Followed by: Solar eclipse of March 5, 1924
Solar Saros 147
- Preceded by: Solar eclipse of March 26, 1895
- Followed by: Solar eclipse of April 18, 1931
Inex
- Preceded by: Solar eclipse of April 25, 1884
- Followed by: Solar eclipse of March 16, 1942
Triad
- Preceded by: Solar eclipse of June 5, 1826
- Followed by: Solar eclipse of February 5, 2000
Solar eclipses of 1910–1913
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.[3]
Solar eclipse series sets from 1910 to 1913 | ||||
---|---|---|---|---|
Ascending node | Descending node | |||
117 | May 9, 1910 Total | 122 | November 2, 1910 Partial | |
127 | April 28, 1911 Total | 132 | October 22, 1911 Annular | |
137 | April 17, 1912 Hybrid | 142 | October 10, 1912 Total | |
147 | April 6, 1913 Partial | 152 | September 30, 1913 Partial |
Saros 147
Solar saros 147, repeating every about 18 years and 11 days, contains 80 events. The series started with a partial solar eclipse on October 12, 1624. It has annular eclipses from May 31, 2003, to July 31, 2706. There are no total eclipses in this series. The series ends at member 80 as a partial eclipse on February 24, 3049. The longest annular eclipse will be on November 21, 2291, at 9 minutes and 41 seconds.[4]
Series members 17–27 occur between 1901 and 2100: | ||
---|---|---|
17 | 18 | 19 |
April 6, 1913 | April 18, 1931 | April 28, 1949 |
20 | 21 | 22 |
May 9, 1967 | May 19, 1985 | May 31, 2003 |
23 | 24 | 25 |
June 10, 2021 | June 21, 2039 | July 1, 2057 |
26 | 27 | |
July 13, 2075 | July 23, 2093 |
References
- ^ "APRIL HEAVENS ARE DESCRIBED". The Times-Democrat. New Orleans, Louisiana. 1913-04-06. p. 59. Retrieved 2023-11-03 – via Newspapers.com.
- ^ "THE HEAVENS IN APRIL". The Commercial Appeal. Memphis, Tennessee. 1913-04-06. p. 74. Retrieved 2023-11-03 – via Newspapers.com.
- ^ 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.
- ^ Saros Series Catalog of Solar Eclipses NASA Eclipse Web Site.
External links
- Earth visibility chart and eclipse statistics Eclipse Predictions by Fred Espenak, NASA/GSFC
- Besselian elements
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Annular eclipses
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- 1820
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