Solar eclipse of September 13, 2080

Last updated
Solar eclipse of September 13, 2080
SE2080Sep13P.png
Map
Type of eclipse
NaturePartial
Gamma 1.0723
Magnitude 0.8743
Maximum eclipse
Coordinates 61°06′N25°48′E / 61.1°N 25.8°E / 61.1; 25.8
Times (UTC)
Greatest eclipse16:38:09
References
Saros 126 (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, [1] 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.

Contents

The partial solar eclipse will be visible for parts of northern North America, Europe, West Africa, and North Africa.

Eclipse details

Shown below are two tables displaying details about this particular solar eclipse. The first table outlines times at which the moon's penumbra or umbra attains the specific parameter, and the second table describes various other parameters pertaining to this eclipse. [2]

September 13, 2080 Solar Eclipse Times
EventTime (UTC)
First Penumbral External Contact2080 September 13 at 14:42:59.9 UTC
Equatorial Conjunction2080 September 13 at 15:36:33.0 UTC
Ecliptic Conjunction2080 September 13 at 16:27:19.9 UTC
Greatest Eclipse2080 September 13 at 16:38:09.2 UTC
Last Penumbral External Contact2080 September 13 at 18:33:46.9 UTC
September 13, 2080 Solar Eclipse Parameters
ParameterValue
Eclipse Magnitude0.87434
Eclipse Obscuration0.84863
Gamma1.07235
Sun Right Ascension11h29m55.2s
Sun Declination+03°14'46.9"
Sun Semi-Diameter15'53.7"
Sun Equatorial Horizontal Parallax08.7"
Moon Right Ascension11h31m59.3s
Moon Declination+04°11'17.0"
Moon Semi-Diameter16'24.7"
Moon Equatorial Horizontal Parallax1°00'13.7"
ΔT106.0 s

Eclipse season

This eclipse is part of an eclipse season, a period, roughly every six months, when eclipses occur. Only two (or occasionally three) eclipse seasons occur each year, and each season lasts about 35 days and repeats just short of six months (173 days) later; thus two full eclipse seasons always occur each year. Either two or three eclipses happen each eclipse season. In the sequence below, each eclipse is separated by a fortnight.

Eclipse season of September 2080
September 13
Descending node (new moon)
September 29
Ascending node (full moon)
SE2080Sep13P.png
Partial solar eclipse
Solar Saros 126
Total lunar eclipse
Lunar Saros 138

Eclipses in 2080

Metonic

Tzolkinex

Half-Saros

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. [3]

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
SarosMapGammaSarosMapGamma
121 March 21, 2080
SE2080Mar21P.png
Partial
−1.0578126 September 13, 2080
SE2080Sep13P.png
Partial
1.0723
131 March 10, 2081
SE2081Mar10A.png
Annular
−0.3653136 September 3, 2081
SE2081Sep03T.png
Total
0.3378
141 February 27, 2082
SE2082Feb27A.png
Annular
0.3361146 August 24, 2082
SE2082Aug24T.png
Total
−0.4004
151 February 16, 2083
SE2083Feb16P.png
Partial
1.017156 August 13, 2083
SE2083Aug13P.png
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. [4]

Series members 36–57 occur between 1801 and 2200:
363738
SE1810Apr04A.gif
April 4, 1810
Saros126 37van72 SE1828Apr14H.jpg
April 14, 1828
SE1846Apr25H.gif
April 25, 1846
394041
SE1864May06H.gif
May 6, 1864
SE1882May17T.png
May 17, 1882
SE1900May28T.png
May 28, 1900
424344
SE1918Jun08T.png
June 8, 1918
SE1936Jun19T.png
June 19, 1936
SE1954Jun30T.png
June 30, 1954
454647
SE1972Jul10T.png
July 10, 1972
SE1990Jul22T.png
July 22, 1990
SE2008Aug01T.png
August 1, 2008
484950
SE2026Aug12T.png
August 12, 2026
SE2044Aug23T.png
August 23, 2044
SE2062Sep03P.png
September 3, 2062
515253
SE2080Sep13P.png
September 13, 2080
SE2098Sep25P.png
September 25, 2098
Saros126 53van72 SE2116Oct06P.jpg
October 6, 2116
545556
Saros126 54van72 SE2134Oct17P.jpg
October 17, 2134
Saros126 55van72 SE2152Oct28P.jpg
October 28, 2152
Saros126 56van72 SE2170Nov08P.jpg
November 8, 2170
57
Saros126 57van72 SE2188Nov18P.jpg
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 3–4April 21–23February 7–8November 26–27September 13–15
118120122124126
SE2065Jul03P.png
July 3, 2065
SE2069Apr21P.png
April 21, 2069
SE2073Feb07P.png
February 7, 2073
SE2076Nov26P.png
November 26, 2076
SE2080Sep13P.png
September 13, 2080
128130132134136
SE2084Jul03A.png
July 3, 2084
SE2088Apr21T.png
April 21, 2088
SE2092Feb07A.png
February 7, 2092
SE2095Nov27A.png
November 27, 2095
SE2099Sep14T.png
September 14, 2099
138140142144146
SE2103Jul04A.png
July 4, 2103
SE2107Apr23A.png
April 23, 2107
SE2111Feb08T.png
February 8, 2111
SE2114Nov27A.png
November 27, 2114
SE2118Sep15T.png
September 15, 2118
148150152154156
Saros148 27van75 SE2122Jul04T.jpg
July 4, 2122
Saros150 23van71 SE2126Apr22A.jpg
April 22, 2126
Saros152 19van70 SE2130Feb08T.jpg
February 8, 2130
Saros154 13van71 SE2133Nov26A.jpg
November 26, 2133
Saros156 08van69 SE2137Sep15P.jpg
September 15, 2137
158160162164
Saros158 05van70 SE2141Jul03P.jpg
July 3, 2141
Saros164 04van80 SE2152Nov26P.jpg
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
SE1971Jul22P.png
July 22, 1971
(Saros 116)
SE1982Jun21P.png
June 21, 1982
(Saros 117)
SE1993May21P.png
May 21, 1993
(Saros 118)
SE2004Apr19P.png
April 19, 2004
(Saros 119)
SE2015Mar20T.png
March 20, 2015
(Saros 120)
SE2026Feb17A.png
February 17, 2026
(Saros 121)
SE2037Jan16P.png
January 16, 2037
(Saros 122)
SE2047Dec16P.png
December 16, 2047
(Saros 123)
SE2058Nov16P.png
November 16, 2058
(Saros 124)
SE2069Oct15P.png
October 15, 2069
(Saros 125)
SE2080Sep13P.png
September 13, 2080
(Saros 126)
SE2091Aug15T.png
August 15, 2091
(Saros 127)
SE2102Jul15A.png
July 15, 2102
(Saros 128)
SE2113Jun13T.png
June 13, 2113
(Saros 129)
SE2124May14T.png
May 14, 2124
(Saros 130)
SE2135Apr13A.png
April 13, 2135
(Saros 131)
SE2146Mar12A.png
March 12, 2146
(Saros 132)
SE2157Feb09T.png
February 9, 2157
(Saros 133)
SE2168Jan10A.png
January 10, 2168
(Saros 134)
SE2178Dec09A.png
December 9, 2178
(Saros 135)
SE2189Nov08T.png
November 8, 2189
(Saros 136)
SE2200Oct09A.png
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
SE1820Mar14T.gif
March 14, 1820
(Saros 117)
SE1849Feb23A.gif
February 23, 1849
(Saros 118)
SE1878Feb02A.gif
February 2, 1878
(Saros 119)
SE1907Jan14T.png
January 14, 1907
(Saros 120)
SE1935Dec25A.png
December 25, 1935
(Saros 121)
SE1964Dec04P.png
December 4, 1964
(Saros 122)
SE1993Nov13P.png
November 13, 1993
(Saros 123)
SE2022Oct25P.png
October 25, 2022
(Saros 124)
SE2051Oct04P.png
October 4, 2051
(Saros 125)
SE2080Sep13P.png
September 13, 2080
(Saros 126)
Saros127 63van82 SE2109Aug26P.jpg
August 26, 2109
(Saros 127)
Saros128 65van73 SE2138Aug05P.jpg
August 5, 2138
(Saros 128)
Saros129 60van80 SE2167Jul16T.jpg
July 16, 2167
(Saros 129)
SE2196Jun26T.png
June 26, 2196
(Saros 130)

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References

  1. "September 13, 2080 Partial Solar Eclipse". timeanddate. Retrieved 22 August 2024.
  2. "Partial Solar Eclipse of 2080 Sep 13". EclipseWise.com. Retrieved 22 August 2024.
  3. 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.
  4. "NASA - Catalog of Solar Eclipses of Saros 126". eclipse.gsfc.nasa.gov.