Solar eclipse of December 26, 2038

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Solar eclipse of December 26, 2038
SE2038Dec26T.png
Map
Type of eclipse
NatureTotal
Gamma-0.2881
Magnitude1.0268
Maximum eclipse
Duration138 sec (2 m 18 s)
Coordinates40°18′S 164°00′E / 40.3°S 164°E / -40.3; 164
Max. width of band95 km (59 mi)
Times (UTC)
Greatest eclipse1:00:10
References
Saros142 (24 of 72)
Catalog # (SE5000)9594

A total solar eclipse will occur on December 26, 2038. 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.

Images[]

SE2038Dec26T.gif
Animated path

Related eclipses[]

There are 7 eclipses in 2038 (the maximum possible), included four penumbral lunar eclipses: January 21, June 17, July 16, and December 11.

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.[1]

Note: Partial solar eclipses on February 27, 2036 and August 21, 2036 occur on the previod lunar year eclipse set.

Solar eclipse series sets from 2036–2039
Ascending node   Descending node
117 July 23, 2036
SE2036Jul23P.png
Partial
122 January 16, 2037
SE2037Jan16P.png
Partial
127 July 13, 2037
SE2037Jul13T.png
Total
132 January 5, 2038
SE2038Jan05A.png
Annular
137 July 2, 2038
SE2038Jul02A.png
Annular
142 December 26, 2038
SE2038Dec26T.png
Total
147 June 21, 2039
SE2039Jun21A.png
Annular
152 December 15, 2039
SE2039Dec15T.png
Total

Saros series 142[]

It is a part of Saros cycle 142, repeating every 18 years, 11 days, containing 72 events. The series started with partial solar eclipse on April 17, 1624. It contains one hybrid eclipse on July 14, 1768, and total eclipses from July 25, 1786 through October 29, 2543. The series ends at member 72 as a partial eclipse on June 5, 2904. The longest duration of totality will be 6 minutes, 34 seconds on May 28, 2291. All eclipses in this series occurs at the Moon’s descending node.[2]

Series members 17–41 occur between 1901 and 2359
17 18 19
SE1912Oct10T.png
October 10, 1912
SE1930Oct21T.png
October 21, 1930
SE1948Nov01T.png
November 1, 1948
20 21 22
SE1966Nov12T.png
November 12, 1966
SE1984Nov22T.png
November 22, 1984
SE2002Dec04T.png
December 4, 2002
23 24 25
SE2020Dec14T.png
December 14, 2020
SE2038Dec26T.png
December 26, 2038
SE2057Jan05T.png
January 5, 2057
26 27 28
SE2075Jan16T.png
January 16, 2075
SE2093Jan27T.png
January 27, 2093
SE2111Feb08T.png
February 8, 2111
29 30 31
SE2129Feb18T.png
February 18, 2129
SE2147Mar02T.png
March 2, 2147
SE2165Mar12T.png
March 12, 2165
32 33 34
SE2183Mar23T.png
March 23, 2183
SE2201Apr04T.png
April 4, 2201
SE2219Apr15T.png
April 15, 2219
35 36 37
SE2237Apr25T.png
April 25, 2237
SE2255May07T.png
May 7, 2255
SE2273May17T.png
May 17, 2273
38 39 40
SE2291May28T.png
May 28, 2291
SE2309Jun09T.png
June 9, 2309
SE2327Jun20T.png
June 20, 2327
41
SE2345Jun30T.png
June 30, 2345

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.[3]

Octon series with 21 events between May 21, 1993 and August 2, 2065
May 20–21 March 8–9 December 25–26 October 13–14 August 1–2
98 100 102 104 106
May 21, 1955 March 9, 1959 December 26, 1962 October 14, 1966 August 2, 1970
108 110 112 114 116
May 21, 1974 March 9, 1978 December 26, 1981 October 14, 1985 August 1, 1989
118 120 122 124 126
SE1993May21P.png
May 21, 1993
SE1997Mar09T.png
March 9, 1997
SE2000Dec25P.png
December 25, 2000
SE2004Oct14P.png
October 14, 2004
SE2008Aug01T.png
August 1, 2008
128 130 132 134 136
SE2012May20A.png
May 20, 2012
SE2016Mar09T.png
March 9, 2016
SE2019Dec26A.png
December 26, 2019
SE2023Oct14A.png
October 14, 2023
SE2027Aug02T.png
August 2, 2027
138 140 142 144 146
SE2031May21A.png
May 21, 2031
SE2035Mar09A.png
March 9, 2035
SE2038Dec26T.png
December 26, 2038
SE2042Oct14A.png
October 14, 2042
SE2046Aug02T.png
August 2, 2046
148 150 152 154 156
SE2050May20H.png
May 20, 2050
SE2054Mar09P.png
March 9, 2054
SE2057Dec26T.png
December 26, 2057
SE2061Oct13A.png
October 13, 2061
SE2065Aug02P.png
August 2, 2065
158 160 162 164 166
SE2069May20P.png
May 20, 2069
March 8, 2073 December 26, 2076 October 13, 2080 August 1, 2084

References[]

  1. ^ 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.
  2. ^ http://eclipse.gsfc.nasa.gov/SEsaros/SEsaros142.html
  3. ^ Note S1: Eclipses & Predictions in Freeth, Tony (2014). "Eclipse Prediction on the Ancient Greek Astronomical Calculating Machine Known as the Antikythera Mechanism". PLOS ONE. 9 (7): e103275. Bibcode:2014PLoSO...9j3275F. doi:10.1371/journal.pone.0103275. PMC 4116162. PMID 25075747.

External links[]

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