Solar eclipse of September 23, 2090

Last updated
Solar eclipse of September 23, 2090
SE2090Sep23T.png
Map
Type of eclipse
NatureTotal
Gamma 0.9157
Magnitude 1.0562
Maximum eclipse
Duration216 s (3 min 36 s)
Coordinates 60°42′N40°30′W / 60.7°N 40.5°W / 60.7; -40.5
Max. width of band463 km (288 mi)
Times (UTC)
Greatest eclipse16:56:36
References
Saros 155 (10 of 71)
Catalog # (SE5000) 9711

A total solar eclipse will occur at the Moon's ascending node of orbit on Saturday, September 23, 2090, [1] with a magnitude of 1.0562. 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 total solar eclipse occurs when the Moon's apparent diameter is larger than the Sun's, blocking all direct sunlight, turning day into darkness. Totality occurs in a narrow path across Earth's surface, with the partial solar eclipse visible over a surrounding region thousands of kilometres wide. Occurring about 4 hours after perigee (on September 23, 2090, at 12:40 UTC), the Moon's apparent diameter will be larger. [2]

Contents

The path of totality will be visible from parts of northern Canada, Greenland, southern Ireland, the southern United Kingdom, France, and Belgium. A partial solar eclipse will also be visible for parts of North America, Western Europe, and West Africa.

This solar eclipse will be the first total solar eclipse visible from Great Britain since August 11, 1999, and the first visible from Ireland since May 22, 1724. The totality will be visible in southern Greenland, Valentia, West Cork, Poole, Newquay, Plymouth, Southampton, Isle of Wight, northern France (including Paris and Rennes) and south Belgium and a partially eclipsed sun will be visible in Birmingham, London, Exeter, Cardiff, Belfast, Dublin, Weston Super Mare, Bristol and Oxford.

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. [3]

September 23, 2090 Solar Eclipse Times
EventTime (UTC)
First Penumbral External Contact2090 September 23 at 14:50:25.0 UTC
First Umbral External Contact2090 September 23 at 16:12:55.8 UTC
First Central Line2090 September 23 at 16:16:08.2 UTC
First Umbral Internal Contact2090 September 23 at 16:19:34.4 UTC
Equatorial Conjunction2090 September 23 at 16:26:17.0 UTC
Greatest Eclipse2090 September 23 at 16:56:36.3 UTC
Greatest Duration2090 September 23 at 16:56:43.3 UTC
Ecliptic Conjunction2090 September 23 at 17:05:47.3 UTC
Last Umbral Internal Contact2090 September 23 at 17:34:01.1 UTC
Last Central Line2090 September 23 at 17:37:26.6 UTC
Last Umbral External Contact2090 September 23 at 17:40:38.4 UTC
Last Penumbral External Contact2090 September 23 at 19:03:02.8 UTC
September 23, 2090 Solar Eclipse Parameters
ParameterValue
Eclipse Magnitude1.05615
Eclipse Obscuration1.11546
Gamma0.91569
Sun Right Ascension12h04m19.6s
Sun Declination-00°28'06.5"
Sun Semi-Diameter15'56.2"
Sun Equatorial Horizontal Parallax08.8"
Moon Right Ascension12h05m28.3s
Moon Declination+00°25'15.5"
Moon Semi-Diameter16'43.4"
Moon Equatorial Horizontal Parallax1°01'22.6"
ΔT114.8 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 2090
September 8
Descending node (full moon)
 September 23
Ascending node (new moon)
Lunar eclipse chart close-2090Sep08.png SE2090Sep23T.png
Total lunar eclipse
Lunar Saros 129		 Total solar eclipse
Solar Saros 155

Eclipses in 2090

Metonic

Tzolkinex

Half-Saros

Tritos

Solar Saros 155

Inex

Triad

Solar eclipses of 2087–2090

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. [4]

The partial solar eclipse on June 1, 2087 occurs in the previous lunar year eclipse set.

Solar eclipse series sets from 2087 to 2090
Descending node Ascending node
SarosMapGammaSarosMapGamma
120 May 2, 2087
SE2087May02P.png
Partial		1.1139125 October 26, 2087
SE2087Oct26P.png
Partial		−1.2882
130 April 21, 2088
SE2088Apr21T.png
Total		0.4135135 October 14, 2088
SE2088Oct14A.png
Annular		−0.5349
140 April 10, 2089
SE2089Apr10A.png
Annular		−0.3319145 October 4, 2089
SE2089Oct04T.png
Total		0.2167
150 March 31, 2090
SE2090Mar31P.png
Partial		−1.1028155 September 23, 2090
SE2090Sep23T.png
Total		0.9157

Saros 155

This eclipse is a part of Saros series 155, repeating every 18 years, 11 days, and containing 71 events. The series started with a partial solar eclipse on June 17, 1928. It contains total eclipses from September 12, 2072 through August 30, 2649; hybrid eclipses from September 10, 2667 through October 2, 2703; and annular eclipses from October 13, 2721 through May 8, 3064. The series ends at member 71 as a partial eclipse on July 24, 3190. 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 will be produced by member 14 at 4 minutes, 5 seconds on November 6, 2162, and the longest duration of annularity will be produced by member 63 at 5 minutes, 31 seconds on April 28, 3046. All eclipses in this series occur at the Moon’s ascending node of orbit. [5]

Series members 1–16 occur between 1928 and 2200:
123
SE1928Jun17P.png
June 17, 1928 		SE1946Jun29P.png
June 29, 1946 		SE1964Jul09P.png
July 9, 1964
456
SE1982Jul20P.png
July 20, 1982 		SE2000Jul31P.png
July 31, 2000 		SE2018Aug11P.png
August 11, 2018
789
SE2036Aug21P.png
August 21, 2036 		SE2054Sep02P.png
September 2, 2054 		SE2072Sep12T.png
September 12, 2072
101112
SE2090Sep23T.png
September 23, 2090 		Saros155 11van71 SE2108Oct05T.jpg
October 5, 2108		 Saros155 12van71 SE2126Oct16T.jpg
October 16, 2126
131415
Saros155 13van71 SE2144Oct26T.jpg
October 26, 2144		 Saros155 14van71 SE2162Nov07T.jpg
November 7, 2162		 Saros155 15van71 SE2180Nov17T.jpg
November 17, 2180
16
Saros155 16van71 SE2198Nov28T.jpg
November 28, 2198

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 ascending node.

21 eclipse events between July 13, 2018 and July 12, 2094
July 12–13April 30–May 1February 16–17December 5–6September 22–23
117119121123125
SE2018Jul13P.png
July 13, 2018 		SE2022Apr30P.png
April 30, 2022 		SE2026Feb17A.png
February 17, 2026 		SE2029Dec05P.png
December 5, 2029 		SE2033Sep23P.png
September 23, 2033
127129131133135
SE2037Jul13T.png
July 13, 2037 		SE2041Apr30T.png
April 30, 2041 		SE2045Feb16A.png
February 16, 2045 		SE2048Dec05T.png
December 5, 2048 		SE2052Sep22A.png
September 22, 2052
137139141143145
SE2056Jul12A.png
July 12, 2056 		SE2060Apr30T.png
April 30, 2060 		SE2064Feb17A.png
February 17, 2064 		SE2067Dec06H.png
December 6, 2067 		SE2071Sep23T.png
September 23, 2071
147149151153155
SE2075Jul13A.png
July 13, 2075 		SE2079May01T.png
May 1, 2079 		SE2083Feb16P.png
February 16, 2083 		SE2086Dec06P.png
December 6, 2086 		SE2090Sep23T.png
September 23, 2090
157
SE2094Jul12P.png
July 12, 2094

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 December 18, 2188 (part of Saros 164) and November 18, 2199 (part of Saros 165) are also a part of this series but are not included in the table below.

Series members between 1801 and 2134
SE1806Dec10A.gif
December 10, 1806
(Saros 129)		 SE1817Nov09T.gif
November 9, 1817
(Saros 130)		 SE1828Oct09A.gif
October 9, 1828
(Saros 131)		 SE1839Sep07A.png
September 7, 1839
(Saros 132)		 SE1850Aug07T.gif
August 7, 1850
(Saros 133)
SE1861Jul08A.gif
July 8, 1861
(Saros 134)		 SE1872Jun06A.gif
June 6, 1872
(Saros 135)		 SE1883May06T.png
May 6, 1883
(Saros 136)		 SE1894Apr06H.gif
April 6, 1894
(Saros 137)		 SE1905Mar06A.png
March 6, 1905
(Saros 138)
SE1916Feb03T.png
February 3, 1916
(Saros 139)		 SE1927Jan03A.png
January 3, 1927
(Saros 140)		 SE1937Dec02A.png
December 2, 1937
(Saros 141)		 SE1948Nov01T.png
November 1, 1948
(Saros 142)		 SE1959Oct02T.png
October 2, 1959
(Saros 143)
SE1970Aug31A.png
August 31, 1970
(Saros 144)		 SE1981Jul31T.png
July 31, 1981
(Saros 145)		 SE1992Jun30T.png
June 30, 1992
(Saros 146)		 SE2003May31A.png
May 31, 2003
(Saros 147)		 SE2014Apr29A.png
April 29, 2014
(Saros 148)
SE2025Mar29P.png
March 29, 2025
(Saros 149)		 SE2036Feb27P.png
February 27, 2036
(Saros 150)		 SE2047Jan26P.png
January 26, 2047
(Saros 151)		 SE2057Dec26T.png
December 26, 2057
(Saros 152)		 SE2068Nov24P.png
November 24, 2068
(Saros 153)
SE2079Oct24A.png
October 24, 2079
(Saros 154)		 SE2090Sep23T.png
September 23, 2090
(Saros 155)		 Saros156 06van69 SE2101Aug24P.jpg
August 24, 2101
(Saros 156)		 Saros157 04van70 SE2112Jul23P.jpg
July 23, 2112
(Saros 157)		 Saros158 04van70 SE2123Jun23P.jpg
June 23, 2123
(Saros 158)
Saros159 01van70 SE2134May23P.jpg
May 23, 2134
(Saros 159)

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
SE1801Apr13P.png
April 13, 1801
(Saros 145)		 SE1830Mar24P.gif
March 24, 1830
(Saros 146)		 SE1859Mar04P.gif
March 4, 1859
(Saros 147)
SE1888Feb11P.gif
February 11, 1888
(Saros 148)		 SE1917Jan23P.png
January 23, 1917
(Saros 149)		 SE1946Jan03P.png
January 3, 1946
(Saros 150)
SE1974Dec13P.png
December 13, 1974
(Saros 151)		 SE2003Nov23T.png
November 23, 2003
(Saros 152)		 SE2032Nov03P.png
November 3, 2032
(Saros 153)
SE2061Oct13A.png
October 13, 2061
(Saros 154)		 SE2090Sep23T.png
September 23, 2090
(Saros 155)		 Saros156 07van69 SE2119Sep05P.jpg
September 5, 2119
(Saros 156)
Saros157 06van70 SE2148Aug14P.jpg
August 14, 2148
(Saros 157)		 Saros158 07van70 SE2177Jul25P.jpg
July 25, 2177
(Saros 158)

Notes

  1. ↑ "September 23, 2090 Total Solar Eclipse". timeanddate. Retrieved 24 August 2024.
  2. ↑ "Moon Distances for London, United Kingdom, England". timeanddate. Retrieved 24 August 2024.
  3. ↑ "Total Solar Eclipse of 2090 Sep 23". EclipseWise.com. Retrieved 24 August 2024.
  4. ↑ 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.
  5. ↑ "NASA - Catalog of Solar Eclipses of Saros 155". eclipse.gsfc.nasa.gov.

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References

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