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Solar eclipse of November 26, 2076

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Solar eclipse of November 26, 2076
Map
Type of eclipse
NaturePartial
Gamma1.1401
Magnitude0.7315
Maximum eclipse
Coordinates63°42′N 40°06′E / 63.7°N 40.1°E / 63.7; 40.1
Times (UTC)
Greatest eclipse11:43:01
References
Saros124 (58 of 73)
Catalog # (SE5000)9680

A partial solar eclipse will occur at the Moon's descending node of orbit on Thursday, November 26, 2076, with a magnitude of 0.7315. 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.

This will be the last of four solar eclipses in 2076, with the others occurring on January 6, June 1, and July 1.

Related eclipses[edit]

Eclipses in 2076[edit]

Metonic[edit]

Tzolkinex[edit]

Half-Saros[edit]

Tritos[edit]

Solar Saros 124[edit]

Inex[edit]

Triad[edit]

Solar eclipses of 2076–2079[edit]

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 2076 to 2079
Ascending node   Descending node
Saros Map Saros Map
119 June 1, 2076

Partial
124 November 26, 2076

Partial
129 May 22, 2077

Total
134 November 15, 2077

Annular
139 May 11, 2078

Total
144 November 4, 2078

Annular
149 May 1, 2079

Total
154 October 24, 2079

Annular

Saros 124[edit]

This eclipse is a part of Saros series 124, repeating every 18 years, 11 days, and containing 73 events. The series started with a partial solar eclipse on March 6, 1049. It contains total eclipses from June 12, 1211 through September 22, 1968, and a hybrid eclipse on October 3, 1986. There are no annular eclipses in this set. The series ends at member 73 as a partial eclipse on May 11, 2347. Its eclipses are tabulated in three columns; every third eclipse in the same column is one exeligmos apart, so they all cast shadows over approximately the same parts of the Earth.

The longest duration of totality was produced by member 39 at 5 minutes, 46 seconds on May 3, 1734. All eclipses in this series occur at the Moon’s descending node of orbit.[2]

Series members 43–64 occur between 1801 and 2200:
43 44 45

June 16, 1806

June 26, 1824

July 8, 1842
46 47 48

July 18, 1860

July 29, 1878

August 9, 1896
49 50 51

August 21, 1914

August 31, 1932

September 12, 1950
52 53 54

September 22, 1968

October 3, 1986

October 14, 2004
55 56 57

October 25, 2022

November 4, 2040

November 16, 2058
58 59 60

November 26, 2076

December 7, 2094

December 19, 2112
61 62 63

December 30, 2130

January 9, 2149

January 21, 2167
64

January 31, 2185

References[edit]

  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.
  2. ^ "NASA - Catalog of Solar Eclipses of Saros 124". eclipse.gsfc.nasa.gov.

External links[edit]