Solar eclipse of November 24, 2068

Last updated
Solar eclipse of November 24, 2068
SE2068Nov24P.png
Map
Type of eclipse
NaturePartial
Gamma 1.0299
Magnitude 0.9109
Maximum eclipse
Coordinates 68°30′N131°06′W / 68.5°N 131.1°W / 68.5; -131.1
Times (UTC)
Greatest eclipse21:32:30
References
Saros 153 (12 of 70)
Catalog # (SE5000) 9661

A partial solar eclipse will occur at the Moon's ascending node of orbit on Saturday, November 24, 2068, with a magnitude of 0.9109. 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

Eclipses in 2068

Metonic

Tzolkinex

Half-Saros

Tritos

Solar Saros 153

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. [1]

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 153

This eclipse is a part of Saros series 153, repeating every 18 years, 11 days, and containing 70 events. The series started with a partial solar eclipse on July 28, 1870. It contains annular eclipses from December 17, 2104 through May 26, 2970. There are no hybrid or total eclipses in this set. The series ends at member 70 as a partial eclipse on August 22, 3114. 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 will be produced by member 38 at 7 minutes, 1 seconds on September 5, 2537. All eclipses in this series occur at the Moon’s ascending node of orbit. [2]

Series members 1–19 occur between 1870 and 2200:
123
SE1870Jul28Pb.gif
July 28, 1870
SE1888Aug07P.gif
August 7, 1888
SE1906Aug20P.png
August 20, 1906
456
SE1924Aug30P.png
August 30, 1924
SE1942Sep10P.png
September 10, 1942
SE1960Sep20P.png
September 20, 1960
789
SE1978Oct02P.png
October 2, 1978
SE1996Oct12P.png
October 12, 1996
SE2014Oct23P.png
October 23, 2014
101112
SE2032Nov03P.png
November 3, 2032
SE2050Nov14P.png
November 14, 2050
SE2068Nov24P.png
November 24, 2068
131415
SE2086Dec06P.png
December 6, 2086
Saros153 14van70 SE2104Dec17A.jpg
December 17, 2104
Saros153 15van70 SE2122Dec28A.jpg
December 28, 2122
161718
Saros153 16van70 SE2141Jan08A.jpg
January 8, 2141
Saros153 17van70 SE2159Jan19A.jpg
January 19, 2159
Saros153 18van70 SE2177Jan29A.jpg
January 29, 2177
19
Saros153 19van70 SE2195Feb10A.jpg
February 10, 2195

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.

21 eclipse events between July 1, 2000 and July 1, 2076
July 1–2April 19–20February 5–7November 24–25September 12–13
117119121123125
SE2000Jul01P.png
July 1, 2000
SE2004Apr19P.png
April 19, 2004
SE2008Feb07A.png
February 7, 2008
SE2011Nov25P.png
November 25, 2011
SE2015Sep13P.png
September 13, 2015
127129131133135
SE2019Jul02T.png
July 2, 2019
SE2023Apr20H.png
April 20, 2023
SE2027Feb06A.png
February 6, 2027
SE2030Nov25T.png
November 25, 2030
SE2034Sep12A.png
September 12, 2034
137139141143145
SE2038Jul02A.png
July 2, 2038
SE2042Apr20T.png
April 20, 2042
SE2046Feb05A.png
February 5, 2046
SE2049Nov25H.png
November 25, 2049
SE2053Sep12T.png
September 12, 2053
147149151153155
SE2057Jul01A.png
July 1, 2057
SE2061Apr20T.png
April 20, 2061
SE2065Feb05P.png
February 5, 2065
SE2068Nov24P.png
November 24, 2068
SE2072Sep12T.png
September 12, 2072
157
SE2076Jul01P.png
July 1, 2076

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 December 18, 2188 (part of Saros 164) and November 18, 2199 (part of Saros 165) are also a part of this series but are not included in the table below.

Series members between 1801 and 2134
SE1806Dec10A.gif
December 10, 1806
(Saros 129)
SE1817Nov09T.gif
November 9, 1817
(Saros 130)
SE1828Oct09A.gif
October 9, 1828
(Saros 131)
SE1839Sep07A.png
September 7, 1839
(Saros 132)
SE1850Aug07T.gif
August 7, 1850
(Saros 133)
SE1861Jul08A.gif
July 8, 1861
(Saros 134)
SE1872Jun06A.gif
June 6, 1872
(Saros 135)
SE1883May06T.png
May 6, 1883
(Saros 136)
SE1894Apr06H.gif
April 6, 1894
(Saros 137)
SE1905Mar06A.png
March 6, 1905
(Saros 138)
SE1916Feb03T.png
February 3, 1916
(Saros 139)
SE1927Jan03A.png
January 3, 1927
(Saros 140)
SE1937Dec02A.png
December 2, 1937
(Saros 141)
SE1948Nov01T.png
November 1, 1948
(Saros 142)
SE1959Oct02T.png
October 2, 1959
(Saros 143)
SE1970Aug31A.png
August 31, 1970
(Saros 144)
SE1981Jul31T.png
July 31, 1981
(Saros 145)
SE1992Jun30T.png
June 30, 1992
(Saros 146)
SE2003May31A.png
May 31, 2003
(Saros 147)
SE2014Apr29A.png
April 29, 2014
(Saros 148)
SE2025Mar29P.png
March 29, 2025
(Saros 149)
SE2036Feb27P.png
February 27, 2036
(Saros 150)
SE2047Jan26P.png
January 26, 2047
(Saros 151)
SE2057Dec26T.png
December 26, 2057
(Saros 152)
SE2068Nov24P.png
November 24, 2068
(Saros 153)
SE2079Oct24A.png
October 24, 2079
(Saros 154)
SE2090Sep23T.png
September 23, 2090
(Saros 155)
Saros156 06van69 SE2101Aug24P.jpg
August 24, 2101
(Saros 156)
Saros157 04van70 SE2112Jul23P.jpg
July 23, 2112
(Saros 157)
Saros158 04van70 SE2123Jun23P.jpg
June 23, 2123
(Saros 158)
Saros159 01van70 SE2134May23P.jpg
May 23, 2134
(Saros 159)

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
SE1808May25P.gif
May 25, 1808
(Saros 144)
SE1837May04P.gif
May 4, 1837
(Saros 145)
SE1866Apr15P.gif
April 15, 1866
(Saros 146)
SE1895Mar26P.gif
March 26, 1895
(Saros 147)
SE1924Mar05P.png
March 5, 1924
(Saros 148)
SE1953Feb14P.png
February 14, 1953
(Saros 149)
SE1982Jan25P.png
January 24, 1982
(Saros 150)
SE2011Jan04P.png
January 4, 2011
(Saros 151)
SE2039Dec15T.png
December 15, 2039
(Saros 152)
SE2068Nov24P.png
November 24, 2068
(Saros 153)
SE2097Nov04A.png
November 4, 2097
(Saros 154)
Saros155 12van71 SE2126Oct16T.jpg
October 16, 2126
(Saros 155)
Saros156 09van69 SE2155Sep26A.jpg
September 26, 2155
(Saros 156)
Saros157 08van70 SE2184Sep04A.jpg
September 4, 2184
(Saros 157)

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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. "NASA - Catalog of Solar Eclipses of Saros 153". eclipse.gsfc.nasa.gov.