Solar eclipse of September 13, 2080

Future partial solar eclipse
61°06′N 25°48′E / 61.1°N 25.8°E / 61.1; 25.8Times (UTC)Greatest eclipse16:38:09ReferencesSaros126 (51 of 72)Catalog # (SE5000)9688

A partial solar eclipse will occur at the Moon's descending node of orbit on Friday, September 13, 2080, with a magnitude of 0.8743. 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.

Eclipses in 2080

Metonic

Tzolkinex

Half-Saros

  • Preceded by: Lunar eclipse of September 9, 2071
  • Followed by: Lunar eclipse of September 19, 2089

Tritos

Solar Saros 126

Inex

Triad

Solar eclipses of 2080–2083

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 126

This eclipse is a part of Saros series 126, repeating every 18 years, 11 days, and containing 72 events. The series started with a partial solar eclipse on March 10, 1179. It contains annular eclipses from June 4, 1323 through April 4, 1810; hybrid eclipses from April 14, 1828 through May 6, 1864; and total eclipses from May 17, 1882 through August 23, 2044. The series ends at member 72 as a partial eclipse on May 3, 2459. 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 annularity was produced by member 11 at 6 minutes, 30 seconds on June 26, 1359, and the longest duration of totality was produced by member 45 at 2 minutes, 36 seconds on July 10, 1972. All eclipses in this series occur at the Moon’s descending node of orbit.[2]

Series members 36–57 occur between 1801 and 2200:
36 37 38

April 4, 1810

April 14, 1828

April 25, 1846
39 40 41

May 6, 1864

May 17, 1882

May 28, 1900
42 43 44

June 8, 1918

June 19, 1936

June 30, 1954
45 46 47

July 10, 1972

July 22, 1990

August 1, 2008
48 49 50

August 12, 2026

August 23, 2044

September 3, 2062
51 52 53

September 13, 2080

September 25, 2098

October 6, 2116
54 55 56

October 17, 2134

October 28, 2152

November 8, 2170
57

November 18, 2188

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 descending node.

22 eclipse events between July 3, 2065 and November 26, 2152
July 3–4 April 21–23 February 7–8 November 26–27 September 13–15
118 120 122 124 126

July 3, 2065

April 21, 2069

February 7, 2073

November 26, 2076

September 13, 2080
128 130 132 134 136

July 3, 2084

April 21, 2088

February 7, 2092

November 27, 2095

September 14, 2099
138 140 142 144 146

July 4, 2103

April 23, 2107

February 8, 2111

November 27, 2114

September 15, 2118
148 150 152 154 156

July 4, 2122

April 22, 2126

February 8, 2130

November 26, 2133

September 15, 2137
158 160 162 164

July 3, 2141

November 26, 2152

Tritos series

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.

The partial solar eclipses on March 27, 1884 (part of Saros 108) and December 24, 1916 (part of Saros 111) are also a part of this series but are not included in the table below.

Series members between 1971 and 2200

July 22, 1971
(Saros 116)

June 21, 1982
(Saros 117)

May 21, 1993
(Saros 118)

April 19, 2004
(Saros 119)

March 20, 2015
(Saros 120)

February 17, 2026
(Saros 121)

January 16, 2037
(Saros 122)

December 16, 2047
(Saros 123)

November 16, 2058
(Saros 124)

October 15, 2069
(Saros 125)

September 13, 2080
(Saros 126)

August 15, 2091
(Saros 127)

July 15, 2102
(Saros 128)

June 13, 2113
(Saros 129)

May 14, 2124
(Saros 130)

April 13, 2135
(Saros 131)

March 12, 2146
(Saros 132)

February 9, 2157
(Saros 133)

January 10, 2168
(Saros 134)

December 9, 2178
(Saros 135)

November 8, 2189
(Saros 136)

October 9, 2200
(Saros 137)

Inex series

This eclipse is a part of the long period inex cycle, repeating at alternating nodes, every 358 synodic months (≈ 10,571.95 days, or 29 years minus 20 days). Their appearance and longitude are irregular due to a lack of synchronization with the anomalistic month (period of perigee). However, groupings of 3 inex cycles (≈ 87 years minus 2 months) comes close (≈ 1,151.02 anomalistic months), so eclipses are similar in these groupings.

Series members between 1801 and 2200

March 14, 1820
(Saros 117)

February 23, 1849
(Saros 118)

February 2, 1878
(Saros 119)

January 14, 1907
(Saros 120)

December 25, 1935
(Saros 121)

December 4, 1964
(Saros 122)

November 13, 1993
(Saros 123)

October 25, 2022
(Saros 124)

October 4, 2051
(Saros 125)

September 13, 2080
(Saros 126)

August 26, 2109
(Saros 127)

August 5, 2138
(Saros 128)

July 16, 2167
(Saros 129)

June 26, 2196
(Saros 130)

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.
  2. ^ "NASA - Catalog of Solar Eclipses of Saros 126". eclipse.gsfc.nasa.gov.
  • Earth visibility chart and eclipse statistics Eclipse Predictions by Fred Espenak, NASA/GSFC
    • Besselian elements


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