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Solar eclipse of March 21, 2080

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Solar eclipse of March 21, 2080
Map
Type of eclipse
NaturePartial
Gamma−1.0578
Magnitude0.8734
Maximum eclipse
Coordinates60°54′S 85°54′E / 60.9°S 85.9°E / -60.9; 85.9
Times (UTC)
Greatest eclipse12:20:15
References
Saros121 (64 of 71)
Catalog # (SE5000)9687

A partial solar eclipse will occur at the Moon's ascending node of orbit on Thursday, March 21, 2080, with a magnitude of 0.8734. 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.

Related eclipses[edit]

Eclipses in 2080[edit]

Metonic[edit]

Tzolkinex[edit]

Half-Saros[edit]

Tritos[edit]

Solar Saros 121[edit]

Inex[edit]

Triad[edit]

Solar eclipses of 2080–2083[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]

121 March 21, 2080

Partial
126 September 13, 2080

Partial
131 March 10, 2081

Annular
136 September 3, 2081

Total
141 February 27, 2082

Annular
146 August 24, 2082

Total
151 February 16, 2083

Partial
156 August 13, 2083

Partial

Saros 121[edit]

This eclipse is a part of Saros series 121, repeating every 18 years, 11 days, and containing 71 events. The series started with a partial solar eclipse on April 25, 944 AD. It contains total eclipses from July 10, 1070 through October 9, 1809; hybrid eclipses on October 20, 1827 and October 30, 1845; and annular eclipses from November 11, 1863 through February 28, 2044. The series ends at member 71 as a partial eclipse on June 7, 2206. 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 6 minutes, 20 seconds on June 21, 1629, and the longest duration of annularity will be produced by member 62 at 2 minutes, 27 seconds on February 28, 2044. All eclipses in this series occur at the Moon’s ascending node of orbit.[2]

Series members 49–70 occur between 1801 and 2200:
49 50 51

October 9, 1809

October 20, 1827

October 30, 1845
52 53 54

November 11, 1863

November 21, 1881

December 3, 1899
55 56 57

December 14, 1917

December 25, 1935

January 5, 1954
58 59 60

January 16, 1972

January 26, 1990

February 7, 2008
61 62 63

February 17, 2026

February 28, 2044

March 11, 2062
64 65 66

March 21, 2080

April 1, 2098

April 13, 2116
67 68 69

April 24, 2134

May 4, 2152

May 16, 2170
70

May 26, 2188

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 121". eclipse.gsfc.nasa.gov.

External links[edit]