Solar eclipse of December 26, 2038

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Template:Short description Script error: No such module "Solar eclipse". A total solar eclipse will occur at the Moon's descending node of orbit between Saturday, December 25 and Sunday, December 26, 2038,[1] with a magnitude of 1.0268. 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 1.7 days after perigee (on December 24, 2038, at 8:25 UTC), the Moon's apparent diameter will be larger.[2]

Totality will be visible from parts of Australia and New Zealand. A partial eclipse will be visible for parts of Southeast Asia, Australia, Antarctica, and Oceania.

In some parts of the world it will fall on Christmas Day, the first such eclipse since 2000, and the last until 2057.[3]Template:Rp

File:SE2038Dec26T.gif
Animated path

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.[4]

December 26, 2038 Solar Eclipse Times
Event Time (UTC)
First Penumbral External Contact 2038 December 25 at 22:20:51.4 UTC
First Umbral External Contact 2038 December 25 at 23:19:15.0 UTC
First Central Line 2038 December 25 at 23:19:33.4 UTC
First Umbral Internal Contact 2038 December 25 at 23:19:51.9 UTC
First Penumbral Internal Contact 2038 December 26 at 00:23:04.9 UTC
Greatest Duration 2038 December 26 at 00:59:26.3 UTC
Greatest Eclipse 2038 December 26 at 01:00:09.7 UTC
Equatorial Conjunction 2038 December 26 at 01:02:10.7 UTC
Ecliptic Conjunction 2038 December 26 at 01:03:10.7 UTC
Last Penumbral Internal Contact 2038 December 26 at 01:37:10.7 UTC
Last Umbral Internal Contact 2038 December 26 at 02:40:28.5 UTC
Last Central Line 2038 December 26 at 02:40:45.0 UTC
Last Umbral External Contact 2038 December 26 at 02:41:01.5 UTC
Last Penumbral External Contact 2038 December 26 at 03:39:31.2 UTC
December 26, 2038 Solar Eclipse Parameters
Parameter Value
Eclipse Magnitude 1.02685
Eclipse Obscuration 1.05443
Gamma −0.28813
Sun Right Ascension 18h18m51.7s
Sun Declination -23°21'47.8"
Sun Semi-Diameter 16'15.7"
Sun Equatorial Horizontal Parallax 08.9"
Moon Right Ascension 18h18m46.7s
Moon Declination -23°39'05.4"
Moon Semi-Diameter 16'25.8"
Moon Equatorial Horizontal Parallax 1°00'18.1"
ΔT 78.0 s

Eclipse season

Script error: No such module "Labelled list hatnote". 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 2038
December 11
Ascending node (full moon)
December 26
Descending node (new moon)
File:Lunar eclipse chart close-2038Dec11.png File:SE2038Dec26T.png
Penumbral lunar eclipse
Lunar Saros 116
Total solar eclipse
Solar Saros 142

Related eclipses

Eclipses in 2038

Metonic

Tzolkinex

Half-Saros

Tritos

Solar Saros 142

Inex

Triad

Solar eclipses of 2036–2039

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.[5]

The partial solar eclipses on February 27, 2036 and August 21, 2036 occur in the previous lunar year eclipse set.

Solar eclipse series sets from 2036 to 2039
Ascending node   Descending node
Saros Map Gamma Saros Map Gamma
117 July 23, 2036
File:SE2036Jul23P.png
Partial
−1.425 122 January 16, 2037
File:SE2037Jan16P.png
Partial
1.1477
127 July 13, 2037
File:SE2037Jul13T.png
Total
−0.7246 132 January 5, 2038
File:SE2038Jan05A.png
Annular
0.4169
137 July 2, 2038
File:SE2038Jul02A.png
Annular
0.0398 142 December 26, 2038
File:SE2038Dec26T.png
Total
−0.2881
147 June 21, 2039
File:SE2039Jun21A.png
Annular
0.8312 152 December 15, 2039
File:SE2039Dec15T.png
Total
−0.9458

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.[6]

Series members 11–32 occur between 1801 and 2200:
11 12 13
File:SE1804Aug05T.png
August 5, 1804
File:SE1822Aug16T.png
August 16, 1822
File:SE1840Aug27T.png
August 27, 1840
14 15 16
File:SE1858Sep07T.png
September 7, 1858
File:SE1876Sep17T.png
September 17, 1876
File:SE1894Sep29T.png
September 29, 1894
17 18 19
File:SE1912Oct10T.png
October 10, 1912
File:SE1930Oct21T.png
October 21, 1930
File:SE1948Nov01T.png
November 1, 1948
20 21 22
File:SE1966Nov12T.png
November 12, 1966
File:SE1984Nov22T.png
November 22, 1984
File:SE2002Dec04T.png
December 4, 2002
23 24 25
File:SE2020Dec14T.png
December 14, 2020
File:SE2038Dec26T.png
December 26, 2038
File:SE2057Jan05T.png
January 5, 2057
26 27 28
File:SE2075Jan16T.png
January 16, 2075
File:SE2093Jan27T.png
January 27, 2093
File:SE2111Feb08T.png
February 8, 2111
29 30 31
File:SE2129Feb18T.png
February 18, 2129
File:SE2147Mar02T.png
March 2, 2147
File:SE2165Mar12T.png
March 12, 2165
32
File: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.

21 eclipse events between May 21, 1993 and May 20, 2069
May 20–21 March 9 December 25–26 October 13–14 August 1–2
118 120 122 124 126
File:SE1993May21P.png
May 21, 1993
File:SE1997Mar09T.png
March 9, 1997
File:SE2000Dec25P.png
December 25, 2000
File:SE2004Oct14P.png
October 14, 2004
File:SE2008Aug01T.png
August 1, 2008
128 130 132 134 136
File:SE2012May20A.png
May 20, 2012
File:SE2016Mar09T.png
March 9, 2016
File:SE2019Dec26A.png
December 26, 2019
File:SE2023Oct14A.png
October 14, 2023
File:SE2027Aug02T.png
August 2, 2027
138 140 142 144 146
File:SE2031May21A.png
May 21, 2031
File:SE2035Mar09A.png
March 9, 2035
File:SE2038Dec26T.png
December 26, 2038
File:SE2042Oct14A.png
October 14, 2042
File:SE2046Aug02T.png
August 2, 2046
148 150 152 154 156
File:SE2050May20H.png
May 20, 2050
File:SE2054Mar09P.png
March 9, 2054
File:SE2057Dec26T.png
December 26, 2057
File:SE2061Oct13A.png
October 13, 2061
File:SE2065Aug02P.png
August 2, 2065
158
File:SE2069May20P.png
May 20, 2069

Tritos series

Template:Solar Tritos series 2006 March 29

Inex series

Template:Solar Inex series 2010 January 15

References

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External links

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