Solar eclipse of November 26, 2076

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.

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

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

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.
edit