Solar eclipse of November 14, 2031

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Solar eclipse of November 14, 2031
SE2031Nov14H.png
Map
Type of eclipse
Nature Hybrid
Gamma 0.3078
Magnitude 1.0106
Maximum eclipse
Duration 68 sec (1 m 8 s)
Coordinates Lua error in package.lua at line 80: module 'strict' not found.
Max. width of band 38 km (24 mi)
Times (UTC)
Greatest eclipse 21:07:31
References
Saros 143 (24 of 72)
Catalog # (SE5000) 9578

A total solar eclipse will occur on 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.

Images

File:SE2031Nov14H.gif
Animated path

Related eclipses

Solar eclipses 2029-2032

Each member 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.

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 2029-2032
Descending node   Ascending node
118 June 12, 2029
SE2029Jun12P.png
Partial
123 December 5, 2029
SE2029Dec05P.png
Partial
128 June 1, 2030
SE2030Jun01A.png
Annular
133 November 25, 2030
SE2030Nov25T.png
Total
138 May 21, 2031
SE2031May21A.png
Annular
143 November 14, 2031
SE2031Nov14H.png
Hybrid
148 May 9, 2032
SE2032May09A.png
Annular
153 November 3, 2032
SE2032Nov03P.png
Partial

Solar 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.[1]

Series members 17-28 occur between 1901 and 2100:

17 18 19
SE1905Aug30T.png
August 30, 1905
SE1923Sep10T.png
September 10, 1923
SE1941Sep21T.png
September 21, 1941
20 21 22
SE1959Oct02T.png
October 2, 1959
SE1977Oct12T.png
October 12, 1977
SE1995Oct24T.png
October 24, 1995
23 24 25
SE2013Nov03H.png
November 3, 2013
SE2031Nov14H.png
November 14, 2031
SE2049Nov25H.png
November 25, 2049
26 27 28
SE2067Dec06H.png
December 6, 2067
SE2085Dec16A.png
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).

This series has 21 eclipse events between June 21, 1982, and June 21, 2058.

June 21 April 8-9 January 26 November 13-14 September 1-2
117 119 121 123 125
SE1982Jun21P.png
June 21, 1982
SE1986Apr09P.png
April 9, 1986
SE1990Jan26A.png
January 26, 1990
SE1993Nov13P.png
November 13, 1993
SE1997Sep02P.png
September 2, 1997
127 129 131 133 135
SE2001Jun21T.png
June 21, 2001
SE2005Apr08H.png
April 8, 2005
SE2009Jan26A.png
January 26, 2009
SE2012Nov13T.png
November 13, 2012
150px
September 1, 2016
137 139 141 143 145
SE2020Jun21A.png
June 21, 2020
SE2024Apr08T.png
April 8, 2024
SE2028Jan26A.png
January 26, 2028
SE2031Nov14H.png
November 14, 2031
SE2035Sep02T.png
September 2, 2035
147 149 151 153 155
SE2039Jun21A.png
June 21, 2039
SE2043Apr09T.png
April 9, 2043
150px
January 26, 2047
SE2050Nov14P.png
November 14, 2050
SE2054Sep02P.png
September 2, 2054
157
SE2058Jun21P.png
June 21, 2058

References

External links


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