Solar eclipse of September 23, 2090

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Template:Short description Script error: No such module "Solar eclipse". 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]

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
Event Time (UTC)
First Penumbral External Contact 2090 September 23 at 14:50:25.0 UTC
First Umbral External Contact 2090 September 23 at 16:12:55.8 UTC
First Central Line 2090 September 23 at 16:16:08.2 UTC
First Umbral Internal Contact 2090 September 23 at 16:19:34.4 UTC
Equatorial Conjunction 2090 September 23 at 16:26:17.0 UTC
Greatest Eclipse 2090 September 23 at 16:56:36.3 UTC
Greatest Duration 2090 September 23 at 16:56:43.3 UTC
Ecliptic Conjunction 2090 September 23 at 17:05:47.3 UTC
Last Umbral Internal Contact 2090 September 23 at 17:34:01.1 UTC
Last Central Line 2090 September 23 at 17:37:26.6 UTC
Last Umbral External Contact 2090 September 23 at 17:40:38.4 UTC
Last Penumbral External Contact 2090 September 23 at 19:03:02.8 UTC
September 23, 2090 Solar Eclipse Parameters
Parameter Value
Eclipse Magnitude 1.05615
Eclipse Obscuration 1.11546
Gamma 0.91569
Sun Right Ascension 12h04m19.6s
Sun Declination -00°28'06.5"
Sun Semi-Diameter 15'56.2"
Sun Equatorial Horizontal Parallax 08.8"
Moon Right Ascension 12h05m28.3s
Moon Declination +00°25'15.5"
Moon Semi-Diameter 16'43.4"
Moon Equatorial Horizontal Parallax 1°01'22.6"
ΔT 114.8 s

Eclipse season

Script error: No such module "Labelled list hatnote". 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)
File:Lunar eclipse chart close-2090Sep08.png File:SE2090Sep23T.png
Total lunar eclipse
Lunar Saros 129		 Total solar eclipse
Solar Saros 155

Related eclipses

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
Saros Map Gamma Saros Map Gamma
120 May 2, 2087
File:SE2087May02P.png
Partial 		1.1139 125 October 26, 2087
File:SE2087Oct26P.png
Partial 		−1.2882
130 April 21, 2088
File:SE2088Apr21T.png
Total 		0.4135 135 October 14, 2088
File:SE2088Oct14A.png
Annular 		−0.5349
140 April 10, 2089
File:SE2089Apr10A.png
Annular 		−0.3319 145 October 4, 2089
File:SE2089Oct04T.png
Total 		0.2167
150 March 31, 2090
File:SE2090Mar31P.png
Partial 		−1.1028 155 September 23, 2090
File:SE2090Sep23T.png
Total 		0.9157

Saros 155

Template:Solar Saros series 155

Metonic series

Template:Solar Metonic series 2018–2094

Tritos series

Template:Solar Tritos series 2003 May 31

Inex series

Template:Solar Inex series 2003 November 23

Notes

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References

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