Solar eclipse of March 21, 2080

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.

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
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Eclipses in 2080

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Metonic

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Tzolkinex

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Half-Saros

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Tritos

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Solar Saros 121

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Inex

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Triad

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Solar eclipses of 2080–2083

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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]

The partial solar eclipse on July 15, 2083 occurs in the next lunar year eclipse set.

Solar eclipse series sets from 2080 to 2083
Ascending node   Descending node
Saros Map Gamma Saros Map Gamma
121 March 21, 2080
 
Partial
−1.0578 126 September 13, 2080
 
Partial
1.0723
131 March 10, 2081
 
Annular
−0.3653 136 September 3, 2081
 
Total
0.3378
141 February 27, 2082
 
Annular
0.3361 146 August 24, 2082
 
Total
−0.4004
151 February 16, 2083
 
Partial
1.017 156 August 13, 2083
 
Partial
−1.2064

Saros 121

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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

Tritos series

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This eclipse is a part of a tritos cycle, repeating at alternating nodes every 135 synodic months (≈ 3986.63 days, or 11 years minus 1 month). Their appearance and longitude are irregular due to a lack of synchronization with the anomalistic month (period of perigee), but groupings of 3 tritos cycles (≈ 33 years minus 3 months) come close (≈ 434.044 anomalistic months), so eclipses are similar in these groupings.

Series members between 2036 and 2200
 
July 23, 2036
(Saros 117)
 
June 23, 2047
(Saros 118)
 
May 22, 2058
(Saros 119)
 
April 21, 2069
(Saros 120)
 
March 21, 2080
(Saros 121)
 
February 18, 2091
(Saros 122)
 
January 19, 2102
(Saros 123)
 
December 19, 2112
(Saros 124)
 
November 18, 2123
(Saros 125)
 
October 17, 2134
(Saros 126)
 
September 16, 2145
(Saros 127)
 
August 16, 2156
(Saros 128)
 
July 16, 2167
(Saros 129)
 
June 16, 2178
(Saros 130)
 
May 15, 2189
(Saros 131)
 
April 14, 2200
(Saros 132)

Metonic series

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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.

22 eclipse events between June 1, 2076 and October 27, 2163
June 1–3 March 21–22 January 7–8 October 26–27 August 14–15
119 121 123 125 127
 
June 1, 2076
 
March 21, 2080
 
January 7, 2084
 
October 26, 2087
 
August 15, 2091
129 131 133 135 137
 
June 2, 2095
 
March 21, 2099
 
January 8, 2103
 
October 26, 2106
 
August 15, 2110
139 141 143 145 147
 
June 3, 2114
 
March 22, 2118
 
January 8, 2122
 
October 26, 2125
 
August 15, 2129
149 151 153 155 157
 
June 3, 2133
 
March 21, 2137
 
January 8, 2141
 
October 26, 2144
 
August 14, 2148
159 161 163 165
 
June 3, 2152
 
October 27, 2163

References

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  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.
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