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Solar eclipse of February 7, 2092

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Solar eclipse of February 7, 2092
Map
Type of eclipse
NatureAnnular
Gamma0.4322
Magnitude0.984
Maximum eclipse
Duration108 s (1 min 48 s)
Coordinates9°54′N 48°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
Saros132 (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]

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

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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
Event Time (UTC)
First Penumbral External Contact 2092 February 07 at 12:25:43.1 UTC
First Umbral External Contact 2092 February 07 at 13:29:54.4 UTC
First Central Line 2092 February 07 at 13:30:56.4 UTC
Greatest Duration 2092 February 07 at 13:30:56.4 UTC
First Umbral Internal Contact 2092 February 07 at 13:31:58.5 UTC
First Penumbral Internal Contact 2092 February 07 at 14:59:49.7 UTC
Ecliptic Conjunction 2092 February 07 at 15:05:36.1 UTC
Greatest Eclipse 2092 February 07 at 15:10:20.2 UTC
Last Penumbral Internal Contact 2092 February 07 at 15:20:32.3 UTC
Equatorial Conjunction 2092 February 07 at 15:20:48.3 UTC
Last Umbral Internal Contact 2092 February 07 at 16:48:32.0 UTC
Last Central Line 2092 February 07 at 16:49:37.1 UTC
Last Umbral External Contact 2092 February 07 at 16:50:42.1 UTC
Last Penumbral External Contact 2092 February 07 at 17:54:58.7 UTC
February 7, 2092 Solar Eclipse Parameters
Parameter Value
Eclipse Magnitude 0.98403
Eclipse Obscuration 0.96832
Gamma 0.43217
Sun Right Ascension 21h25m01.6s
Sun Declination -15°10'15.3"
Sun Semi-Diameter 16'13.1"
Sun Equatorial Horizontal Parallax 08.9"
Moon Right Ascension 21h24m39.5s
Moon Declination -14°45'56.9"
Moon Semi-Diameter 15'43.8"
Moon Equatorial Horizontal Parallax 0°57'43.8"
ΔT 116.0 s

Eclipse season

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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)
Annular solar eclipse
Solar Saros 132
Penumbral lunar eclipse
Lunar Saros 144
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Eclipses in 2092

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Metonic

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Tzolkinex

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Half-Saros

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Tritos

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Solar Saros 132

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Inex

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Triad

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Solar eclipses of 2091–2094

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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
Saros Map Gamma Saros Map Gamma
122 February 18, 2091

Partial
1.1779 127 August 15, 2091

Total
−0.949
132 February 7, 2092

Annular
0.4322 137 August 3, 2092

Annular
−0.2044
142 January 27, 2093

Total
−0.2737 147 July 23, 2093

Annular
0.5717
152 January 16, 2094

Total
−0.9333 157 July 12, 2094

Partial
1.3150

Saros 132

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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:
34 35 36

August 17, 1803

August 27, 1821

September 7, 1839
37 38 39

September 18, 1857

September 29, 1875

October 9, 1893
40 41 42

October 22, 1911

November 1, 1929

November 12, 1947
43 44 45

November 23, 1965

December 4, 1983

December 14, 2001
46 47 48

December 26, 2019

January 5, 2038

January 16, 2056
49 50 51

January 27, 2074

February 7, 2092

February 18, 2110
52 53 54

March 1, 2128

March 12, 2146

March 23, 2164
55 56

April 3, 2182

April 14, 2200

Metonic series

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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

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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

March 25, 1819
(Saros 107)

February 23, 1830
(Saros 108)

January 22, 1841
(Saros 109)

November 21, 1862
(Saros 111)

August 20, 1895
(Saros 114)

July 21, 1906
(Saros 115)

June 19, 1917
(Saros 116)

May 19, 1928
(Saros 117)

April 19, 1939
(Saros 118)

March 18, 1950
(Saros 119)

February 15, 1961
(Saros 120)

January 16, 1972
(Saros 121)

December 15, 1982
(Saros 122)

November 13, 1993
(Saros 123)

October 14, 2004
(Saros 124)

September 13, 2015
(Saros 125)

August 12, 2026
(Saros 126)

July 13, 2037
(Saros 127)

June 11, 2048
(Saros 128)

May 11, 2059
(Saros 129)

April 11, 2070
(Saros 130)

March 10, 2081
(Saros 131)

February 7, 2092
(Saros 132)

January 8, 2103
(Saros 133)

December 8, 2113
(Saros 134)

November 6, 2124
(Saros 135)

October 7, 2135
(Saros 136)

September 6, 2146
(Saros 137)

August 5, 2157
(Saros 138)

July 5, 2168
(Saros 139)

June 5, 2179
(Saros 140)

May 4, 2190
(Saros 141)

Inex series

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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

August 28, 1802
(Saros 122)

August 7, 1831
(Saros 123)

July 18, 1860
(Saros 124)

June 28, 1889
(Saros 125)

June 8, 1918
(Saros 126)

May 20, 1947
(Saros 127)

April 29, 1976
(Saros 128)

April 8, 2005
(Saros 129)

March 20, 2034
(Saros 130)

February 28, 2063
(Saros 131)

February 7, 2092
(Saros 132)

January 19, 2121
(Saros 133)

December 30, 2149
(Saros 134)

December 9, 2178
(Saros 135)

Notes

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  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.

References

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