Solar eclipse of January 27, 2055

Last updated
Solar eclipse of January 27, 2055
SE2055Jan27P.png
Map
Type of eclipse
NaturePartial
Gamma 1.155
Magnitude 0.6932
Maximum eclipse
Coordinates 69°30′N112°12′W / 69.5°N 112.2°W / 69.5; -112.2
Times (UTC)
Greatest eclipse17:54:05
References
Saros 122 (60 of 70)
Catalog # (SE5000) 9630

A partial solar eclipse will occur at the Moon's descending node of orbit on Wednesday, January 27, 2055, [1] with a magnitude of 0.6932. 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 partial solar eclipse will be visible for most of North America.

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. [2]

January 27, 2055 Solar Eclipse Times
EventTime (UTC)
First Penumbral External Contact2055 January 27 at 15:49:08.2 UTC
Ecliptic Conjunction2055 January 27 at 17:40:43.6 UTC
Greatest Eclipse2055 January 27 at 17:54:05.3 UTC
Equatorial Conjunction2055 January 27 at 18:16:10.6 UTC
Last Penumbral External Contact2055 January 27 at 19:58:56.1 UTC
January 27, 2055 Solar Eclipse Parameters
ParameterValue
Eclipse Magnitude0.69325
Eclipse Obscuration0.59655
Gamma1.15497
Sun Right Ascension20h40m41.0s
Sun Declination-18°19'18.9"
Sun Semi-Diameter16'14.5"
Sun Equatorial Horizontal Parallax08.9"
Moon Right Ascension20h39m58.6s
Moon Declination-17°17'11.5"
Moon Semi-Diameter14'53.3"
Moon Equatorial Horizontal Parallax0°54'38.4"
ΔT87.2 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 August–September 2055
January 27
Descending node (new moon)
February 11
Ascending node (full moon)
SE2055Jan27P.png Lunar eclipse chart close-2055Feb11.png
Partial solar eclipse
Solar Saros 122
Total lunar eclipse
Lunar Saros 134

Eclipses in 2055

Metonic

Tzolkinex

Half-Saros

Tritos

Solar Saros 122

Inex

Triad

Solar eclipses of 2054–2058

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. [3]

The partial solar eclipses on March 9, 2054 and September 2, 2054 occur in the previous lunar year eclipse set, and the partial solar eclipses on May 22, 2058 and November 16, 2058 occur in the next lunar year eclipse set.

Solar eclipse series sets from 2054 to 2058
Ascending node Descending node
SarosMapGammaSarosMapGamma
117 August 3, 2054
SE2054Aug03P.png
Partial
−1.4941122 January 27, 2055
SE2055Jan27P.png
Partial
1.155
127 July 24, 2055
SE2055Jul24T.png
Total
−0.8012132 January 16, 2056
SE2056Jan16A.png
Annular
0.4199
137 July 12, 2056
SE2056Jul12A.png
Annular
−0.0426142 January 5, 2057
SE2057Jan05T.png
Total
−0.2837
147 July 1, 2057
SE2057Jul01A.png
Annular
0.7455152 December 26, 2057
SE2057Dec26T.png
Total
−0.9405
157 June 21, 2058
SE2058Jun21P.png
Partial
1.4869

Saros 122

This eclipse is a part of Saros series 122, repeating every 18 years, 11 days, and containing 70 events. The series started with a partial solar eclipse on April 17, 991 AD. It contains total eclipses from July 12, 1135 through August 3, 1171; hybrid eclipses on August 13, 1189 and August 25, 1207; and annular eclipses from September 4, 1225 through October 10, 1874. The series ends at member 70 as a partial eclipse on May 17, 2235. 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 was produced by member 9 at 1 minutes, 25 seconds on July 12, 1135, and the longest duration of annularity was produced by member 50 at 6 minutes, 28 seconds on October 10, 1874. All eclipses in this series occur at the Moon’s descending node of orbit. [4]

Series members 46–68 occur between 1801 and 2200:
464748
SE1802Aug28A.png
August 28, 1802
SE1820Sep07A.gif
September 7, 1820
SE1838Sep18A.gif
September 18, 1838
495051
SE1856Sep29A.gif
September 29, 1856
SE1874Oct10An.gif
October 10, 1874
SE1892Oct20P.gif
October 20, 1892
525354
SE1910Nov02P.png
November 2, 1910
SE1928Nov12P.png
November 12, 1928
SE1946Nov23P.png
November 23, 1946
555657
SE1964Dec04P.png
December 4, 1964
SE1982Dec15P.png
December 15, 1982
SE2000Dec25P.png
December 25, 2000
585960
SE2019Jan06P.png
January 6, 2019
SE2037Jan16P.png
January 16, 2037
SE2055Jan27P.png
January 27, 2055
616263
SE2073Feb07P.png
February 7, 2073
SE2091Feb18P.png
February 18, 2091
Saros122 63van70 SE2109Mar01P.jpg
March 1, 2109
646566
Saros122 64van70 SE2127Mar13P.jpg
March 13, 2127
Saros122 65van70 SE2145Mar23P.jpg
March 23, 2145
Saros122 66van70 SE2163Apr03P.jpg
April 3, 2163
6768
Saros122 67van70 SE2181Apr14P.jpg
April 14, 2181
Saros122 68van70 SE2199Apr25P.jpg
April 25, 2199

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.

The partial solar eclipses on April 8, 1902 (part of Saros 108) and January 5, 1935 (part of Saros 111) are also a part of this series but are not included in the table below.

Series members between 2000 and 2200
SE2000Jul01P.png
July 1, 2000
(Saros 117)
SE2011Jun01P.png
June 1, 2011
(Saros 118)
SE2022Apr30P.png
April 30, 2022
(Saros 119)
SE2033Mar30T.png
March 30, 2033
(Saros 120)
SE2044Feb28A.png
February 28, 2044
(Saros 121)
SE2055Jan27P.png
January 27, 2055
(Saros 122)
SE2065Dec27P.png
December 27, 2065
(Saros 123)
SE2076Nov26P.png
November 26, 2076
(Saros 124)
SE2087Oct26P.png
October 26, 2087
(Saros 125)
SE2098Sep25P.png
September 25, 2098
(Saros 126)
Saros127 63van82 SE2109Aug26P.jpg
August 26, 2109
(Saros 127)
SE2120Jul25A.png
July 25, 2120
(Saros 128)
Saros129 58van80 SE2131Jun25T.jpg
June 25, 2131
(Saros 129)
SE2142May25T.png
May 25, 2142
(Saros 130)
SE2153Apr23A.png
April 23, 2153
(Saros 131)
SE2164Mar23H.png
March 23, 2164
(Saros 132)
SE2175Feb21T.png
February 21, 2175
(Saros 133)
SE2186Jan20A.png
January 20, 2186
(Saros 134)
SE2196Dec19A.png
December 19, 2196
(Saros 135)

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
SE1823Jul08P.gif
July 8, 1823
(Saros 114)
SE1852Jun17P.gif
June 17, 1852
(Saros 115)
SE1881May27P.gif
May 27, 1881
(Saros 116)
SE1910May09T.png
May 9, 1910
(Saros 117)
SE1939Apr19A.png
April 19, 1939
(Saros 118)
SE1968Mar28P.png
March 28, 1968
(Saros 119)
SE1997Mar09T.png
March 9, 1997
(Saros 120)
SE2026Feb17A.png
February 17, 2026
(Saros 121)
SE2055Jan27P.png
January 27, 2055
(Saros 122)
SE2084Jan07P.png
January 7, 2084
(Saros 123)
Saros124 60van73 SE2112Dec19P.jpg
December 19, 2112
(Saros 124)
Saros125 61van73 SE2141Nov28P.jpg
November 28, 2141
(Saros 125)
Saros126 56van72 SE2170Nov08P.jpg
November 8, 2170
(Saros 126)
Saros127 68van82 SE2199Oct19P.jpg
October 19, 2199
(Saros 127)

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References

  1. "January 27, 2055 Partial Solar Eclipse". timeanddate. Retrieved 15 August 2024.
  2. "Partial Solar Eclipse of 2055 Jan 27". EclipseWise.com. Retrieved 15 August 2024.
  3. 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.
  4. "NASA - Catalog of Solar Eclipses of Saros 122". eclipse.gsfc.nasa.gov.