Solar eclipse of February 7, 2092

Last updated
Solar eclipse of February 7, 2092
SE2092Feb07A.png
Map
Type of eclipse
NatureAnnular
Gamma 0.4322
Magnitude 0.984
Maximum eclipse
Duration108 s (1 min 48 s)
Coordinates 9°54′N48°42′W / 9.9°N 48.7°W / 9.9; -48.7
Max. width of band62 km (39 mi)
Times (UTC)
Greatest eclipse15:10:20
References
Saros 132 (50 of 71)
Catalog # (SE5000) 9714

An annular solar eclipse will occur at the Moon's descending node of orbit on Thursday, February 7, 2092, [1] with a magnitude of 0.984. 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. An annular solar eclipse occurs when the Moon's apparent diameter is smaller than the Sun's, blocking most of the Sun's light and causing the Sun to look like an annulus (ring). An annular eclipse appears as a partial eclipse over a region of the Earth thousands of kilometres wide. Occurring about 6.25 days before perigee (on February 2, 2092, at 9:00 UTC), the Moon's apparent diameter will be larger. [2]

Contents

The path of annularity will be visible from parts of Panama, Colombia, Venezuela, Guyana, the Canary Islands, Morocco, Algeria, and Tunisia. A partial solar eclipse will also be visible for parts of North America, Central America, the Caribbean, northern South America, West Africa, Northwest Africa, and Western Europe.

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]

February 7, 2092 Solar Eclipse Times
EventTime (UTC)
First Penumbral External Contact2092 February 07 at 12:25:43.1 UTC
First Umbral External Contact2092 February 07 at 13:29:54.4 UTC
First Central Line2092 February 07 at 13:30:56.4 UTC
Greatest Duration2092 February 07 at 13:30:56.4 UTC
First Umbral Internal Contact2092 February 07 at 13:31:58.5 UTC
First Penumbral Internal Contact2092 February 07 at 14:59:49.7 UTC
Ecliptic Conjunction2092 February 07 at 15:05:36.1 UTC
Greatest Eclipse2092 February 07 at 15:10:20.2 UTC
Last Penumbral Internal Contact2092 February 07 at 15:20:32.3 UTC
Equatorial Conjunction2092 February 07 at 15:20:48.3 UTC
Last Umbral Internal Contact2092 February 07 at 16:48:32.0 UTC
Last Central Line2092 February 07 at 16:49:37.1 UTC
Last Umbral External Contact2092 February 07 at 16:50:42.1 UTC
Last Penumbral External Contact2092 February 07 at 17:54:58.7 UTC
February 7, 2092 Solar Eclipse Parameters
ParameterValue
Eclipse Magnitude0.98403
Eclipse Obscuration0.96832
Gamma0.43217
Sun Right Ascension21h25m01.6s
Sun Declination-15°10'15.3"
Sun Semi-Diameter16'13.1"
Sun Equatorial Horizontal Parallax08.9"
Moon Right Ascension21h24m39.5s
Moon Declination-14°45'56.9"
Moon Semi-Diameter15'43.8"
Moon Equatorial Horizontal Parallax0°57'43.8"
ΔT116.0 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 February 2092
February 7
Descending node (new moon)
 February 23
Ascending node (full moon)
SE2092Feb07A.png
Annular solar eclipse
Solar Saros 132		 Penumbral lunar eclipse
Lunar Saros 144

Eclipses in 2092

Metonic

Tzolkinex

Half-Saros

Tritos

Solar Saros 132

Inex

Triad

Solar eclipses of 2091–2094

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 eclipses on June 13, 2094 and December 7, 2094 occur in the next lunar year eclipse set.

Solar eclipse series sets from 2091 to 2094
Descending node Ascending node
SarosMapGammaSarosMapGamma
122 February 18, 2091
SE2091Feb18P.png
Partial		1.1779127 August 15, 2091
SE2091Aug15T.png
Total		−0.949
132 February 7, 2092
SE2092Feb07A.png
Annular		0.4322137 August 3, 2092
SE2092Aug03A.png
Annular		−0.2044
142 January 27, 2093
SE2093Jan27T.png
Total		−0.2737147 July 23, 2093
SE2093Jul23A.png
Annular		0.5717
152 January 16, 2094
SE2094Jan16T.png
Total		−0.9333157 July 12, 2094
SE2094Jul12P.png
Partial		1.3150

Saros 132

This eclipse is a part of Saros series 132, repeating every 18 years, 11 days, and containing 71 events. The series started with a partial solar eclipse on August 13, 1208. It contains annular eclipses from March 17, 1569 through March 12, 2146; hybrid eclipses on March 23, 2164 and April 3, 2182; and total eclipses from April 14, 2200 through June 19, 2308. The series ends at member 71 as a partial eclipse on September 25, 2470. 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 25 at 6 minutes, 56 seconds on May 9, 1641, and the longest duration of totality will be produced by member 61 at 2 minutes, 14 seconds on June 8, 2290. All eclipses in this series occur at the Moon’s descending node of orbit. [5]

Series members 34–56 occur between 1801 and 2200:
343536
SE1803Aug17A.png
August 17, 1803		 SE1821Aug27A.png
August 27, 1821		 SE1839Sep07A.png
September 7, 1839
373839
SE1857Sep18A.png
September 18, 1857		 SE1875Sep29A.png
September 29, 1875		 SE1893Oct09A.png
October 9, 1893
404142
SE1911Oct22A.png
October 22, 1911 		SE1929Nov01A.png
November 1, 1929 		SE1947Nov12A.png
November 12, 1947
434445
SE1965Nov23A.png
November 23, 1965 		SE1983Dec04A.png
December 4, 1983 		SE2001Dec14A.png
December 14, 2001
464748
SE2019Dec26A.png
December 26, 2019 		SE2038Jan05A.png
January 5, 2038 		SE2056Jan16A.png
January 16, 2056
495051
SE2074Jan27A.png
January 27, 2074 		SE2092Feb07A.png
February 7, 2092 		SE2110Feb18A.png
February 18, 2110
525354
SE2128Mar01A.png
March 1, 2128		 SE2146Mar12A.png
March 12, 2146		 SE2164Mar23H.png
March 23, 2164
5556
SE2182Apr03H.png
April 3, 2182		 SE2200Apr14T.png
April 14, 2200

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.

Series members between 1801 and 2200
SE1819Mar25P.gif
March 25, 1819
(Saros 107)		 SE1830Feb23P.gif
February 23, 1830
(Saros 108)		 SE1841Jan22P.gif
January 22, 1841
(Saros 109)		 SE1862Nov21P.gif
November 21, 1862
(Saros 111)
SE1895Aug20P.gif
August 20, 1895
(Saros 114)		 SE1906Jul21P.png
July 21, 1906
(Saros 115)		 SE1917Jun19P.png
June 19, 1917
(Saros 116)
SE1928May19T.png
May 19, 1928
(Saros 117)		 SE1939Apr19A.png
April 19, 1939
(Saros 118)		 SE1950Mar18A.png
March 18, 1950
(Saros 119)		 SE1961Feb15T.png
February 15, 1961
(Saros 120)		 SE1972Jan16A.png
January 16, 1972
(Saros 121)
SE1982Dec15P.png
December 15, 1982
(Saros 122)		 SE1993Nov13P.png
November 13, 1993
(Saros 123)		 SE2004Oct14P.png
October 14, 2004
(Saros 124)		 SE2015Sep13P.png
September 13, 2015
(Saros 125)		 SE2026Aug12T.png
August 12, 2026
(Saros 126)
SE2037Jul13T.png
July 13, 2037
(Saros 127)		 SE2048Jun11A.png
June 11, 2048
(Saros 128)		 SE2059May11T.png
May 11, 2059
(Saros 129)		 SE2070Apr11T.png
April 11, 2070
(Saros 130)		 SE2081Mar10A.png
March 10, 2081
(Saros 131)
SE2092Feb07A.png
February 7, 2092
(Saros 132)		 SE2103Jan08T.png
January 8, 2103
(Saros 133)		 SE2113Dec08A.png
December 8, 2113
(Saros 134)		 SE2124Nov06A.png
November 6, 2124
(Saros 135)		 SE2135Oct07T.png
October 7, 2135
(Saros 136)
SE2146Sep06A.png
September 6, 2146
(Saros 137)		 SE2157Aug05A.png
August 5, 2157
(Saros 138)		 SE2168Jul05T.png
July 5, 2168
(Saros 139)		 SE2179Jun05A.png
June 5, 2179
(Saros 140)		 SE2190May04A.png
May 4, 2190
(Saros 141)

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
SE1802Aug28A.png
August 28, 1802
(Saros 122)		 SE1831Aug07T.gif
August 7, 1831
(Saros 123)		 SE1860Jul18T.png
July 18, 1860
(Saros 124)
SE1889Jun28A.png
June 28, 1889
(Saros 125)		 SE1918Jun08T.png
June 8, 1918
(Saros 126)		 SE1947May20T.png
May 20, 1947
(Saros 127)
SE1976Apr29A.png
April 29, 1976
(Saros 128)		 SE2005Apr08H.png
April 8, 2005
(Saros 129)		 SE2034Mar20T.png
March 20, 2034
(Saros 130)
SE2063Feb28A.png
February 28, 2063
(Saros 131)		 SE2092Feb07A.png
February 7, 2092
(Saros 132)		 SE2121Jan19T.png
January 19, 2121
(Saros 133)
SE2149Dec30A.png
December 30, 2149
(Saros 134)		 SE2178Dec09A.png
December 9, 2178
(Saros 135)

Notes

  1. ↑ "February 7, 2092 Annular Solar Eclipse". timeanddate. Retrieved 24 August 2024.
  2. ↑ "Moon Distances for London, United Kingdom, England". timeanddate. Retrieved 24 August 2024.
  3. ↑ "Annular Solar Eclipse of 2092 Feb 07". 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 132". eclipse.gsfc.nasa.gov.

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References

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