Solar eclipse of December 27, 2065

Last updated
Solar eclipse of December 27, 2065
SE2065Dec27P.png
Map
Type of eclipse
NaturePartial
Gamma −1.0688
Magnitude 0.8769
Maximum eclipse
Coordinates 65°24′S149°12′W / 65.4°S 149.2°W / -65.4; -149.2
Times (UTC)
Greatest eclipse8:39:56
References
Saros 123 (56 of 70)
Catalog # (SE5000) 9655

A partial solar eclipse will occur at the Moon's ascending node of orbit on Sunday, December 27, 2065, [1] with a magnitude of 0.8769. 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

This will be the last of four partial solar eclipses in 2065, with the others occurring on February 5, July 3, and August 2.

The partial solar eclipse will be visible for parts of Antarctica and the southern half of Australia.

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]

December 27, 2065 Solar Eclipse Times
EventTime (UTC)
First Penumbral External Contact2065 December 27 at 06:45:04.9 UTC
Equatorial Conjunction2065 December 27 at 08:24:00.5 UTC
Ecliptic Conjunction2065 December 27 at 08:29:12.5 UTC
Greatest Eclipse2065 December 27 at 08:39:55.7 UTC
Last Penumbral External Contact2065 December 27 at 10:34:55.8 UTC
December 27, 2065 Solar Eclipse Parameters
ParameterValue
Eclipse Magnitude0.87691
Eclipse Obscuration0.84944
Gamma−1.06879
Sun Right Ascension18h26m44.9s
Sun Declination-23°17'20.3"
Sun Semi-Diameter16'15.7"
Sun Equatorial Horizontal Parallax08.9"
Moon Right Ascension18h27m25.5s
Moon Declination-24°21'42.8"
Moon Semi-Diameter16'37.3"
Moon Equatorial Horizontal Parallax1°01'00.2"
ΔT94.6 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 December 2065–January 2066
December 27
Ascending node (new moon)
January 11
Descending node (full moon)
SE2065Dec27P.png Lunar eclipse chart close-2066Jan11.png
Partial solar eclipse
Solar Saros 123
Total lunar eclipse
Lunar Saros 135

Eclipses in 2065

Metonic

Tzolkinex

Half-Saros

Tritos

Solar Saros 123

Inex

Triad

Solar eclipses of 2065–2069

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 February 5, 2065 and August 2, 2065 occur in the previous lunar year eclipse set, and the partial solar eclipses on April 21, 2069 and October 15, 2069 occur in the next lunar year eclipse set.

Solar eclipse series sets from 2065 to 2069
Descending node Ascending node
SarosMapGammaSarosMapGamma
118 July 3, 2065
SE2065Jul03P.png
Partial
1.4619123 December 27, 2065
SE2065Dec27P.png
Partial
−1.0688
128 June 22, 2066
SE2066Jun22A.png
Annular
0.733133 December 17, 2066
SE2066Dec17T.png
Total
−0.4043
138 June 11, 2067
SE2067Jun11A.png
Annular
−0.0387143 December 6, 2067
SE2067Dec06H.png
Hybrid
0.2845
148 May 31, 2068
SE2068May31T.png
Total
−0.797153 November 24, 2068
SE2068Nov24P.png
Partial
1.0299
158 May 20, 2069
SE2069May20P.png
Partial
−1.4852

Saros 123

This eclipse is a part of Saros series 123, repeating every 18 years, 11 days, and containing 70 events. The series started with a partial solar eclipse on April 29, 1074. It contains annular eclipses from July 2, 1182 through April 19, 1651; hybrid eclipses from April 30, 1669 through May 22, 1705; and total eclipses from June 3, 1723 through October 23, 1957. The series ends at member 70 as a partial eclipse on May 31, 2318. 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 19 at 8 minutes, 7 seconds on November 9, 1398, and the longest duration of totality was produced by member 42 at 3 minutes, 27 seconds on July 27, 1813. All eclipses in this series occur at the Moon’s ascending node of orbit. [4]

Series members 42–63 occur between 1801 and 2200:
424344
SE1813Jul27T.gif
July 27, 1813
SE1831Aug07T.gif
August 7, 1831
SE1849Aug18T.gif
August 18, 1849
454647
SE1867Aug29T.png
August 29, 1867
SE1885Sep08T.png
September 8, 1885
SE1903Sep21T.png
September 21, 1903
484950
SE1921Oct01T.png
October 1, 1921
SE1939Oct12T.png
October 12, 1939
SE1957Oct23T.png
October 23, 1957
515253
SE1975Nov03P.png
November 3, 1975
SE1993Nov13P.png
November 13, 1993
SE2011Nov25P.png
November 25, 2011
545556
SE2029Dec05P.png
December 5, 2029
SE2047Dec16P.png
December 16, 2047
SE2065Dec27P.png
December 27, 2065
575859
SE2084Jan07P.png
January 7, 2084
Saros123 58van70 SE2102Jan19P.jpg
January 19, 2102
Saros123 59van70 SE2120Jan30P.jpg
January 30, 2120
606162
Saros123 60van70 SE2138Feb09P.jpg
February 9, 2138
Saros123 61van70 SE2156Feb21P.jpg
February 21, 2156
Saros123 62van70 SE2174Mar03P.jpg
March 3, 2174
63
Saros123 63van70 SE2192Mar13P.jpg
March 13, 2192

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 ascending node.

23 eclipse events between August 3, 2054 and October 16, 2145
August 3–4May 22–24March 10–11December 27–29October 14–16
117119121123125
SE2054Aug03P.png
August 3, 2054
SE2058May22P.png
May 22, 2058
SE2062Mar11P.png
March 11, 2062
SE2065Dec27P.png
December 27, 2065
SE2069Oct15P.png
October 15, 2069
127129131133135
SE2073Aug03T.png
August 3, 2073
SE2077May22T.png
May 22, 2077
SE2081Mar10A.png
March 10, 2081
SE2084Dec27T.png
December 27, 2084
SE2088Oct14A.png
October 14, 2088
137139141143145
SE2092Aug03A.png
August 3, 2092
SE2096May22T.png
May 22, 2096
SE2100Mar10A.png
March 10, 2100
SE2103Dec29A.png
December 29, 2103
SE2107Oct16T.png
October 16, 2107
147149151153155
SE2111Aug04A.png
August 4, 2111
SE2115May24T.png
May 24, 2115
Saros151 20van72 SE2119Mar11A.jpg
March 11, 2119
Saros153 15van70 SE2122Dec28A.jpg
December 28, 2122
SE2126Oct16T.png
October 16, 2126
157159161163165
Saros157 05van70 SE2130Aug04P.jpg
August 4, 2130
Saros159 01van70 SE2134May23P.jpg
May 23, 2134
Saros165 01van72 SE2145Oct16P.jpg
October 16, 2145

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
SE1805Jun26P.gif
June 26, 1805
(Saros 114)
SE1834Jun07P.gif
June 7, 1834
(Saros 115)
SE1863May17P.gif
May 17, 1863
(Saros 116)
SE1892Apr26T.png
April 26, 1892
(Saros 117)
SE1921Apr08A.png
April 8, 1921
(Saros 118)
SE1950Mar18A.png
March 18, 1950
(Saros 119)
SE1979Feb26T.png
February 26, 1979
(Saros 120)
SE2008Feb07A.png
February 7, 2008
(Saros 121)
SE2037Jan16P.png
January 16, 2037
(Saros 122)
SE2065Dec27P.png
December 27, 2065
(Saros 123)
SE2094Dec07P.png
December 7, 2094
(Saros 124)
Saros125 60van73 SE2123Nov18P.jpg
November 18, 2123
(Saros 125)
Saros126 55van72 SE2152Oct28P.jpg
October 28, 2152
(Saros 126)
Saros127 67van82 SE2181Oct08P.jpg
October 8, 2181
(Saros 127)

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References

  1. "December 27, 2065 Partial Solar Eclipse". timeanddate. Retrieved 19 August 2024.
  2. "Partial Solar Eclipse of 2065 Dec 27". EclipseWise.com. Retrieved 19 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 123". eclipse.gsfc.nasa.gov.