Solar eclipse of November 14, 2031

Last updated
Solar eclipse of November 14, 2031
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Map
Type of eclipse
NatureHybrid
Gamma 0.3078
Magnitude 1.0106
Maximum eclipse
Duration68 s (1 min 8 s)
Coordinates 0°36′S137°36′W / 0.6°S 137.6°W / -0.6; -137.6
Max. width of band38 km (24 mi)
Times (UTC)
Greatest eclipse21:07:31
References
Saros 143 (24 of 72)
Catalog # (SE5000) 9578

A total solar eclipse will occur on Friday, November 14, 2031. It is a hybrid event, with portions of its central path near sunrise and sunset as an annular eclipse. 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 total solar eclipse occurs when the Moon's apparent diameter is larger than the Sun's, blocking all direct sunlight, turning day into darkness. Totality occurs in a narrow path across Earth's surface, with the partial solar eclipse visible over a surrounding region thousands of kilometres wide.

Contents

Images

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Animated path

Solar eclipses 2029–2032

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]

Note: Partial solar eclipses on January 14, 2029 and July 11, 2029 occur on the previous lunar year eclipse set.

Solar eclipse series sets from 2029 to 2032
Descending node Ascending node
118 June 12, 2029
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Partial
123 December 5, 2029
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Partial
128 June 1, 2030
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Annular
133 November 25, 2030
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Total
138 May 21, 2031
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Annular
143 November 14, 2031
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Hybrid
148 May 9, 2032
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Annular
153 November 3, 2032
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Partial

Saros 143

It is a part of Saros cycle 143, repeating every 18 years, 11 days, containing 72 events. The series started with partial solar eclipse on March 7, 1617 and total event from June 24, 1797 through October 24, 1995. It has hybrid eclipses from November 3, 2013 through December 6, 2067, and annular eclipses from December 16, 2085 through September 16, 2536. The series ends at member 72 as a partial eclipse on April 23, 2873. The longest duration of totality was 3 minutes, 50 seconds on August 19, 1887. All eclipses in this series occurs at the Moon’s ascending node.

Series members 17–28 occur between 1741 and 2100
8910
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May 23, 1743
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June 3, 1761
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June 14, 1779
111213
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June 24, 1797
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July 6, 1815
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July 17, 1833
141516
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July 28, 1851
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August 7, 1869
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August 19, 1887
171819
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August 30, 1905
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September 10, 1923
SE1941Sep21T.png
September 21, 1941
202122
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October 2, 1959
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October 12, 1977
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October 24, 1995
232425
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November 3, 2013
SE2031Nov14H.png
November 14, 2031
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November 25, 2049
262728
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December 6, 2067
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December 16, 2085

Metonic series

The metonic series repeats eclipses every 19 years (6939.69 days), lasting about 5 cycles. Eclipses occur in nearly the same calendar date. In addition, the octon subseries repeats 1/5 of that or every 3.8 years (1387.94 days). All eclipses in this table occur at the Moon's ascending node.

21 eclipse events between June 21, 1982, and June 21, 2058
June 21April 8–9January 26November 13–14September 1–2
107109111113115
June 21, 1963April 9, 1967January 26, 1971November 14, 1974September 2, 1978
117119121123125
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June 21, 1982
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April 9, 1986
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January 26, 1990
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November 13, 1993
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September 2, 1997
127129131133135
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June 21, 2001
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April 8, 2005
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January 26, 2009
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November 13, 2012
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September 1, 2016
137139141143145
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June 21, 2020
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April 8, 2024
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January 26, 2028
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November 14, 2031
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September 2, 2035
147149151153155
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June 21, 2039
SE2043Apr09T.png
April 9, 2043
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January 26, 2047
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November 14, 2050
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September 2, 2054
157
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June 21, 2058

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References

  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.