Solar eclipse of January 27, 2093

Last updated
Solar eclipse of January 27, 2093
SE2093Jan27T.png
Map
Type of eclipse
NatureTotal
Gamma −0.2737
Magnitude 1.034
Maximum eclipse
Duration178 s (2 min 58 s)
Coordinates 34°06′S136°24′E / 34.1°S 136.4°E / -34.1; 136.4
Max. width of band119 km (74 mi)
Times (UTC)
Greatest eclipse3:22:16
References
Saros 142 (27 of 72)
Catalog # (SE5000) 9716

A total solar eclipse will occur at the Moon's descending node of orbit on Tuesday, January 27, 2093, [1] with a magnitude of 1.034. 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 1.3 days after perigee (on January 25, 2093, at 18:45 UTC), the Moon's apparent diameter will be larger. [2]

Contents

The path of totality will be visible from parts of Australia, New Caledonia, and Vanuatu. A partial solar eclipse will also be visible for parts of Antarctica, Australia, Indonesia, and Oceania.

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]

January 27, 2093 Solar Eclipse Times
EventTime (UTC)
First Penumbral External Contact2093 January 27 at 00:43:54.5 UTC
First Umbral External Contact2093 January 27 at 01:41:24.0 UTC
First Central Line2093 January 27 at 01:41:54.0 UTC
First Umbral Internal Contact2093 January 27 at 01:42:24.1 UTC
First Penumbral Internal Contact2093 January 27 at 02:44:05.0 UTC
Equatorial Conjunction2093 January 27 at 03:17:37.4 UTC
Greatest Duration2093 January 27 at 03:19:14.3 UTC
Greatest Eclipse2093 January 27 at 03:22:16.1 UTC
Ecliptic Conjunction2093 January 27 at 03:25:06.9 UTC
Last Penumbral Internal Contact2093 January 27 at 04:00:33.7 UTC
Last Umbral Internal Contact2093 January 27 at 05:02:13.3 UTC
Last Central Line2093 January 27 at 05:02:41.8 UTC
Last Umbral External Contact2093 January 27 at 05:03:10.2 UTC
Last Penumbral External Contact2093 January 27 at 06:00:43.1 UTC
January 27, 2093 Solar Eclipse Parameters
ParameterValue
Eclipse Magnitude1.03403
Eclipse Obscuration1.06923
Gamma−0.27372
Sun Right Ascension20h41m22.6s
Sun Declination-18°16'28.3"
Sun Semi-Diameter16'14.6"
Sun Equatorial Horizontal Parallax08.9"
Moon Right Ascension20h41m33.8s
Moon Declination-18°32'48.9"
Moon Semi-Diameter16'31.4"
Moon Equatorial Horizontal Parallax1°00'38.7"
ΔT116.9 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 January 2093
January 12
Ascending node (full moon)
January 27
Descending node (new moon)
SE2093Jan27T.png
Penumbral lunar eclipse
Lunar Saros 116
Total solar eclipse
Solar Saros 142

Eclipses in 2093

Metonic

Tzolkinex

Half-Saros

Tritos

Solar Saros 142

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 142

This eclipse is a part of Saros series 142, repeating every 18 years, 11 days, and containing 72 events. The series started with a partial solar eclipse on April 17, 1624. It contains a hybrid eclipse on July 14, 1768, and total eclipses from July 25, 1786 through October 29, 2543. There are no annular eclipses in this set. The series ends at member 72 as a partial eclipse on June 5, 2904. 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 will be produced by member 38 at 6 minutes, 34 seconds on May 28, 2291. All eclipses in this series occur at the Moon’s descending node of orbit. [5]

Series members 11–32 occur between 1801 and 2200:
111213
SE1804Aug05T.png
August 5, 1804
SE1822Aug16T.png
August 16, 1822
SE1840Aug27T.png
August 27, 1840
141516
SE1858Sep07T.png
September 7, 1858
SE1876Sep17T.png
September 17, 1876
SE1894Sep29T.png
September 29, 1894
171819
SE1912Oct10T.png
October 10, 1912
SE1930Oct21T.png
October 21, 1930
SE1948Nov01T.png
November 1, 1948
202122
SE1966Nov12T.png
November 12, 1966
SE1984Nov22T.png
November 22, 1984
SE2002Dec04T.png
December 4, 2002
232425
SE2020Dec14T.png
December 14, 2020
SE2038Dec26T.png
December 26, 2038
SE2057Jan05T.png
January 5, 2057
262728
SE2075Jan16T.png
January 16, 2075
SE2093Jan27T.png
January 27, 2093
SE2111Feb08T.png
February 8, 2111
293031
SE2129Feb18T.png
February 18, 2129
SE2147Mar02T.png
March 2, 2147
SE2165Mar12T.png
March 12, 2165
32
SE2183Mar23T.png
March 23, 2183

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 1801 and 2200
SE1809Apr14A.gif
April 14, 1809
(Saros 116)
SE1820Mar14T.gif
March 14, 1820
(Saros 117)
SE1831Feb12A.gif
February 12, 1831
(Saros 118)
SE1842Jan11A.gif
January 11, 1842
(Saros 119)
SE1852Dec11T.gif
December 11, 1852
(Saros 120)
SE1863Nov11A.png
November 11, 1863
(Saros 121)
SE1874Oct10An.gif
October 10, 1874
(Saros 122)
SE1885Sep08T.png
September 8, 1885
(Saros 123)
SE1896Aug09T.png
August 9, 1896
(Saros 124)
SE1907Jul10A.png
July 10, 1907
(Saros 125)
SE1918Jun08T.png
June 8, 1918
(Saros 126)
SE1929May09T.png
May 9, 1929
(Saros 127)
SE1940Apr07A.png
April 7, 1940
(Saros 128)
SE1951Mar07A.png
March 7, 1951
(Saros 129)
SE1962Feb05T.png
February 5, 1962
(Saros 130)
SE1973Jan04A.png
January 4, 1973
(Saros 131)
SE1983Dec04A.png
December 4, 1983
(Saros 132)
SE1994Nov03T.png
November 3, 1994
(Saros 133)
SE2005Oct03A.png
October 3, 2005
(Saros 134)
SE2016Sep01A.png
September 1, 2016
(Saros 135)
SE2027Aug02T.png
August 2, 2027
(Saros 136)
SE2038Jul02A.png
July 2, 2038
(Saros 137)
SE2049May31A.png
May 31, 2049
(Saros 138)
SE2060Apr30T.png
April 30, 2060
(Saros 139)
SE2071Mar31A.png
March 31, 2071
(Saros 140)
SE2082Feb27A.png
February 27, 2082
(Saros 141)
SE2093Jan27T.png
January 27, 2093
(Saros 142)
SE2103Dec29A.png
December 29, 2103
(Saros 143)
SE2114Nov27A.png
November 27, 2114
(Saros 144)
SE2125Oct26T.png
October 26, 2125
(Saros 145)
SE2136Sep26T.png
September 26, 2136
(Saros 146)
Saros147 30van80 SE2147Aug26A.jpg
August 26, 2147
(Saros 147)
SE2158Jul25T.png
July 25, 2158
(Saros 148)
Saros149 29van71 SE2169Jun25T.jpg
June 25, 2169
(Saros 149)
Saros150 26van71 SE2180May24A.jpg
May 24, 2180
(Saros 150)
SE2191Apr23A.png
April 23, 2191
(Saros 151)

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
SE1803Aug17A.png
August 17, 1803
(Saros 132)
SE1832Jul27T.gif
July 27, 1832
(Saros 133)
SE1861Jul08A.gif
July 8, 1861
(Saros 134)
SE1890Jun17A.gif
June 17, 1890
(Saros 135)
SE1919May29T.png
May 29, 1919
(Saros 136)
SE1948May09A.png
May 9, 1948
(Saros 137)
SE1977Apr18A.png
April 18, 1977
(Saros 138)
SE2006Mar29T.png
March 29, 2006
(Saros 139)
SE2035Mar09A.png
March 9, 2035
(Saros 140)
SE2064Feb17A.png
February 17, 2064
(Saros 141)
SE2093Jan27T.png
January 27, 2093
(Saros 142)
SE2122Jan08A.png
January 8, 2122
(Saros 143)
SE2150Dec19A.png
December 19, 2150
(Saros 144)
SE2179Nov28T.png
November 28, 2179
(Saros 145)

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References

  1. "January 27, 2093 Total Solar Eclipse". timeanddate. Retrieved 24 August 2024.
  2. "Moon Distances for London, United Kingdom, England". timeanddate. Retrieved 24 August 2024.
  3. "Total Solar Eclipse of 2093 Jan 27". 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 142". eclipse.gsfc.nasa.gov.