Solar eclipse of April 11, 2051

Last updated
Solar eclipse of April 11, 2051
SE2051Apr11P.png
Map
Type of eclipse
NaturePartial
Gamma 1.0169
Magnitude 0.9849
Maximum eclipse
Coordinates 71°36′N32°12′E / 71.6°N 32.2°E / 71.6; 32.2
Times (UTC)
Greatest eclipse2:10:39
References
Saros 120 (63 of 71)
Catalog # (SE5000) 9621

A partial solar eclipse will occur at the Moon's descending node of orbit between Monday, April 10 and Tuesday, April 11, 2051, [1] with a magnitude of 0.9849. 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 umbral shadow of the Moon will pass just above the North Pole. It will be the largest partial solar eclipse in 21st century. [2]

The maximal phase of the partial eclipse (0.98) will be recorded in the Barents Sea. The partial solar eclipse will be visible for parts of Asia, Alaska, and western Canada.

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]

April 11, 2051 Solar Eclipse Times
EventTime (UTC)
First Penumbral External Contact2051 April 11 at 00:12:31.3 UTC
Ecliptic Conjunction2051 April 11 at 02:00:30.3 UTC
Greatest Eclipse2051 April 11 at 02:10:38.6 UTC
Equatorial Conjunction2051 April 11 at 02:41:35.1 UTC
Last Penumbral External Contact2051 April 11 at 04:08:32.1 UTC
April 11, 2051 Solar Eclipse Parameters
ParameterValue
Eclipse Magnitude0.98490
Eclipse Obscuration0.98811
Gamma1.01694
Sun Right Ascension01h18m13.3s
Sun Declination+08°15'12.8"
Sun Semi-Diameter15'57.8"
Sun Equatorial Horizontal Parallax08.8"
Moon Right Ascension01h17m01.7s
Moon Declination+09°14'52.8"
Moon Semi-Diameter16'42.8"
Moon Equatorial Horizontal Parallax1°01'20.2"
ΔT84.9 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 April 2051
April 11
Descending node (new moon)
April 26
Ascending node (full moon)
SE2051Apr11P.png Lunar eclipse chart close-2051Apr26.png
Partial solar eclipse
Solar Saros 120
Total lunar eclipse
Lunar Saros 132

Eclipses in 2051

Metonic

Tzolkinex

Half-Saros

Tritos

Solar Saros 120

Inex

Triad

Solar eclipses of 2051–2054

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 August 3, 2054 occurs in the next lunar year eclipse set.

Solar eclipse series sets from 2051 to 2054
Descending node Ascending node
SarosMapGammaSarosMapGamma
120 April 11, 2051
SE2051Apr11P.png
Partial
1.0169125 October 4, 2051
SE2051Oct04P.png
Partial
−1.2094
130 March 30, 2052
SE2052Mar30T.png
Total
0.3238135 September 22, 2052
SE2052Sep22A.png
Annular
−0.448
140 March 20, 2053
SE2053Mar20A.png
Annular
−0.4089145 September 12, 2053
SE2053Sep12T.png
Total
0.314
150 March 9, 2054
SE2054Mar09P.png
Partial
−1.1711155 September 2, 2054
SE2054Sep02P.png
Partial
1.0215

Saros 120

This eclipse is a part of Saros series 120, repeating every 18 years, 11 days, and containing 71 events. The series started with a partial solar eclipse on May 27, 933 AD. It contains annular eclipses from August 11, 1059 through April 26, 1492; hybrid eclipses from May 8, 1510 through June 8, 1564; and total eclipses from June 20, 1582 through March 30, 2033. The series ends at member 71 as a partial eclipse on July 7, 2195. 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, 24 seconds on September 11, 1113, and the longest duration of totality was produced by member 60 at 2 minutes, 50 seconds on March 9, 1997. All eclipses in this series occur at the Moon’s descending node of orbit. [5]

Series members 50–71 occur between 1801 and 2195:
505152
SE1816Nov19T.gif
November 19, 1816
SE1834Nov30T.gif
November 30, 1834
SE1852Dec11T.gif
December 11, 1852
535455
SE1870Dec22T.gif
December 22, 1870
SE1889Jan01T.png
January 1, 1889
SE1907Jan14T.png
January 14, 1907
565758
SE1925Jan24T.png
January 24, 1925
SE1943Feb04T.png
February 4, 1943
SE1961Feb15T.png
February 15, 1961
596061
SE1979Feb26T.png
February 26, 1979
SE1997Mar09T.png
March 9, 1997
SE2015Mar20T.png
March 20, 2015
626364
SE2033Mar30T.png
March 30, 2033
SE2051Apr11P.png
April 11, 2051
SE2069Apr21P.png
April 21, 2069
656667
SE2087May02P.png
May 2, 2087
Saros120 66van71 SE2105May14P.jpg
May 14, 2105
Saros120 67van71 SE2123May25P.jpg
May 25, 2123
686970
Saros120 68van71 SE2141Jun04P.jpg
June 4, 2141
Saros120 69van71 SE2159Jun16P.jpg
June 16, 2159
Saros120 70van71 SE2177Jun26P.jpg
June 26, 2177
71
Saros120 71van71 SE2195Jul07P.jpg
July 7, 2195

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 June 23, 2047 and November 16, 2134
June 22–23April 10–11January 27–29November 15–16September 3–5
118120122124126
SE2047Jun23P.png
June 23, 2047
SE2051Apr11P.png
April 11, 2051
SE2055Jan27P.png
January 27, 2055
SE2058Nov16P.png
November 16, 2058
SE2062Sep03P.png
September 3, 2062
128130132134136
SE2066Jun22A.png
June 22, 2066
SE2070Apr11T.png
April 11, 2070
SE2074Jan27A.png
January 27, 2074
SE2077Nov15A.png
November 15, 2077
SE2081Sep03T.png
September 3, 2081
138140142144146
SE2085Jun22A.png
June 22, 2085
SE2089Apr10A.png
April 10, 2089
SE2093Jan27T.png
January 27, 2093
SE2096Nov15A.png
November 15, 2096
SE2100Sep04T.png
September 4, 2100
148150152154156
SE2104Jun22T.png
June 22, 2104
SE2108Apr11P.gif
April 11, 2108
Saros152 18van70 SE2112Jan29T.jpg
January 29, 2112
SE2115Nov16A.png
November 16, 2115
Saros156 07van69 SE2119Sep05P.jpg
September 5, 2119
158160162164
Saros158 04van70 SE2123Jun23P.jpg
June 23, 2123
Saros164 03van80 SE2134Nov16P.jpg
November 16, 2134

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 2018 and 2200
SE2018Jul13P.png
July 13, 2018
(Saros 117)
SE2029Jun12P.png
June 12, 2029
(Saros 118)
SE2040May11P.png
May 11, 2040
(Saros 119)
SE2051Apr11P.png
April 11, 2051
(Saros 120)
SE2062Mar11P.png
March 11, 2062
(Saros 121)
SE2073Feb07P.png
February 7, 2073
(Saros 122)
SE2084Jan07P.png
January 7, 2084
(Saros 123)
SE2094Dec07P.png
December 7, 2094
(Saros 124)
Saros125 59van73 SE2105Nov06P.jpg
November 6, 2105
(Saros 125)
Saros126 53van72 SE2116Oct06P.jpg
October 6, 2116
(Saros 126)
Saros127 64van82 SE2127Sep06P.jpg
September 6, 2127
(Saros 127)
Saros128 65van73 SE2138Aug05P.jpg
August 5, 2138
(Saros 128)
Saros129 59van80 SE2149Jul05T.jpg
July 5, 2149
(Saros 129)
SE2160Jun04T.png
June 4, 2160
(Saros 130)
SE2171May05A.png
May 5, 2171
(Saros 131)
SE2182Apr03H.png
April 3, 2182
(Saros 132)
SE2193Mar03T.png
March 3, 2193
(Saros 133)

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
SE1819Sep19Pe.gif
September 19, 1819
(Saros 112)
SE1848Aug28P.gif
August 28, 1848
(Saros 113)
SE1877Aug09P.gif
August 9, 1877
(Saros 114)
SE1906Jul21P.png
July 21, 1906
(Saros 115)
SE1935Jun30P.png
June 30, 1935
(Saros 116)
SE1964Jun10P.png
June 10, 1964
(Saros 117)
SE1993May21P.png
May 21, 1993
(Saros 118)
SE2022Apr30P.png
April 30, 2022
(Saros 119)
SE2051Apr11P.png
April 11, 2051
(Saros 120)
SE2080Mar21P.png
March 21, 2080
(Saros 121)
Saros122 63van70 SE2109Mar01P.jpg
March 1, 2109
(Saros 122)
Saros123 60van70 SE2138Feb09P.jpg
February 9, 2138
(Saros 123)
Saros124 63van73 SE2167Jan21P.jpg
January 21, 2167
(Saros 124)
Saros125 64van73 SE2195Dec31P.jpg
December 31, 2195
(Saros 125)

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References

  1. "April 11, 2051 Partial Solar Eclipse". timeanddate. Retrieved 15 August 2024.
  2. "Catalog of Solar Eclipses: 2001 to 2100". Eclipse.gsfc.nasa.gov. Retrieved 2022-03-20.
  3. "Partial Solar Eclipse of 2051 Apr 11". EclipseWise.com. Retrieved 15 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 120". eclipse.gsfc.nasa.gov.