Solar eclipse of November 14, 2031

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.

Solar eclipse of November 14, 2031
Map
Type of eclipse
NatureHybrid
Gamma0.3078
Magnitude1.0106
Maximum eclipse
Duration68 sec (1 m 8 s)
Coordinates0.6°S 137.6°W / -0.6; -137.6
Max. width of band38 km (24 mi)
Times (UTC)
Greatest eclipse21:07:31
References
Saros143 (24 of 72)
Catalog # (SE5000)9578

Images


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 2029–2032
Descending node   Ascending node
118June 12, 2029

Partial
123December 5, 2029

Partial
128June 1, 2030

Annular
133November 25, 2030

Total
138May 21, 2031

Annular
143November 14, 2031

Hybrid
148May 9, 2032

Annular
153November 3, 2032

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
8 9 10

May 23, 1743

June 3, 1761

June 14, 1779
11 12 13

June 24, 1797

July 6, 1815

July 17, 1833
14 15 16

July 28, 1851

August 7, 1869

August 19, 1887
17 18 19

August 30, 1905

September 10, 1923

September 21, 1941
20 21 22

October 2, 1959

October 12, 1977

October 24, 1995
23 24 25

November 3, 2013

November 14, 2031

November 25, 2049
26 27 28

December 6, 2067

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 21 April 8–9 January 26 November 13–14 September 1–2
107 109 111 113 115
June 21, 1963 April 9, 1967 January 26, 1971 November 14, 1974 September 2, 1978
117 119 121 123 125

June 21, 1982

April 9, 1986

January 26, 1990

November 13, 1993

September 2, 1997
127 129 131 133 135

June 21, 2001

April 8, 2005

January 26, 2009

November 13, 2012

September 1, 2016
137 139 141 143 145

June 21, 2020

April 8, 2024

January 26, 2028

November 14, 2031

September 2, 2035
147 149 151 153 155

June 21, 2039

April 9, 2043

January 26, 2047

November 14, 2050

September 2, 2054
157

June 21, 2058

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.
This article is issued from Wikipedia. The text is licensed under Creative Commons - Attribution - Sharealike. Additional terms may apply for the media files.