Solar eclipse of January 5, 2057

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Solar eclipse of January 5, 2057
SE2057Jan05T.png
Map
Type of eclipse
NatureTotal
Gamma-0.2837
Magnitude1.0287
Maximum eclipse
Duration149 sec (2 m 29 s)
Coordinates39°12′S 35°12′E / 39.2°S 35.2°E / -39.2; 35.2
Max. width of band102 km (63 mi)
Times (UTC)
Greatest eclipse9:47:52
References
Saros142 (25 of 72)
Catalog # (SE5000)9634

A total solar eclipse will occur on January 5, 2057. 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.

Related eclipses[]

Solar eclipses 2054–2058[]

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]

Solar eclipse series sets from 2054-58
Ascending node   Descending node
Saros Map Saros Map
117 August 3, 2054
SE2054Aug03P.png
Partial 		122 January 27, 2055
SE2055Jan27P.png
Partial
127 July 24, 2055
SE2055Jul24T.png
Total 		132 January 16, 2056
SE2056Jan16A.png
Annular
137 July 12, 2056
SE2056Jul12A.png
Annular 		142 January 5, 2057
SE2057Jan05T.png
Total
147 July 1, 2057
SE2057Jul01A.png
Annular 		152 December 26, 2057
SE2057Dec26T.png
Total
157 June 21, 2058
SE2058Jun21P.png
Partial

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

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 2100
SE1805Dec21A.gif
December 21, 1805
(Saros 119) 		SE1816Nov19T.gif
November 19, 1816
(Saros 120) 		SE1827Oct20H.gif
October 20, 1827
(Saros 121)
SE1838Sep18A.gif
September 18, 1838
(Saros 122) 		SE1849Aug18T.gif
August 18, 1849
(Saros 123) 		SE1860Jul18T.gif
July 18, 1860
(Saros 124)
SE1871Jun18A.gif
June 18, 1871
(Saros 125) 		SE1882May17T.png
May 17, 1882
(Saros 126) 		SE1893Apr16T.png
April 16, 1893
(Saros 127)
SE1904Mar17A.png
March 17, 1904
(Saros 128) 		SE1915Feb14A.png
February 14, 1915
(Saros 129) 		SE1926Jan14T.png
January 14, 1926
(Saros 130)
SE1936Dec13A.png
December 13, 1936
(Saros 131) 		SE1947Nov12A.png
November 12, 1947
(Saros 132) 		SE1958Oct12T.png
October 12, 1958
(Saros 133)
SE1969Sep11A.png
September 11, 1969
(Saros 134) 		SE1980Aug10A.png
August 10, 1980
(Saros 135) 		SE1991Jul11T.png
July 11, 1991
(Saros 136)
SE2002Jun10A.png
June 10, 2002
(Saros 137) 		SE2013May10A.png
May 10, 2013
(Saros 138) 		SE2024Apr08T.png
April 8, 2024
(Saros 139)
SE2035Mar09A.png
March 9, 2035
(Saros 140) 		SE2046Feb05A.png
February 5, 2046
(Saros 141) 		SE2057Jan05T.png
January 5, 2057
(Saros 142)
SE2067Dec06H.png
December 6, 2067
(Saros 143) 		SE2078Nov04A.png
November 4, 2078
(Saros 144) 		SE2089Oct04T.png
October 4, 2089
(Saros 145)
SE2100Sep04T.png
September 4, 2100
(Saros 146)

In the 22nd century:

  • Solar saros 147: annular solar eclipse of August 4, 2111
  • Solar saros 148: total solar eclipse of July 4, 2122
  • Solar saros 149: total solar eclipse of June 3, 2133
  • Solar saros 150: annular solar eclipse of May 3, 2144
  • Solar saros 151: annular solar eclipse of April 2, 2155
  • Solar saros 152: total solar eclipse of March 2, 2166
  • Solar saros 153: annular solar eclipse of January 29, 2177
  • Solar saros 154: annular solar eclipse of December 29, 2187
  • Solar saros 155: total solar eclipse of November 28, 2198

In the 23rd century:

  • Solar saros 156: annular solar eclipse of October 29, 2209
  • Solar saros 157: annular solar eclipse of September 27, 2220
  • Solar saros 158: total solar eclipse of August 28, 2231
  • Solar saros 159: partial solar eclipse of July 28, 2242
  • Solar saros 160: partial solar eclipse of June 26, 2253
  • Solar saros 161: partial solar eclipse of May 26, 2264
  • Solar saros 162: partial solar eclipse of April 26, 2275
  • Solar saros 163: partial solar eclipse of March 25, 2286
  • Solar saros 164: partial solar eclipse of February 22, 2297

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 June 1, 2011 and June 1, 2087
May 31 – June 1 March 19–20 January 5–6 October 24–25 August 12–13
118 120 122 124 126
SE2011Jun01P.png
June 1, 2011 		SE2015Mar20T.png
March 20, 2015 		SE2019Jan06P.png
January 6, 2019 		SE2022Oct25P.png
October 25, 2022 		SE2026Aug12T.png
August 12, 2026
128 130 132 134 136
SE2030Jun01A.png
June 1, 2030 		SE2034Mar20T.png
March 20, 2034 		SE2038Jan05A.png
January 5, 2038 		SE2041Oct25A.png
October 25, 2041 		SE2045Aug12T.png
August 12, 2045
138 140 142 144 146
SE2049May31A.png
May 31, 2049 		SE2053Mar20A.png
March 20, 2053 		SE2057Jan05T.png
January 5, 2057 		SE2060Oct24A.png
October 24, 2060 		SE2064Aug12T.png
August 12, 2064
148 150 152 154 156
SE2068May31T.png
May 31, 2068 		SE2072Mar19P.png
March 19, 2072 		SE2076Jan06T.png
January 6, 2076 		SE2079Oct24A.png
October 24, 2079 		SE2083Aug13P.png
August 13, 2083
158 160 162 164 166
SE2087Jun01P.png
June 1, 2087 		SE2098Oct24P.png
October 24, 2098

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

External links[]

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