Solar eclipse of January 5, 2057

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Solar eclipse of January 5, 2057
Map
Type of eclipse
NatureTotal
Gamma−0.2837
Magnitude1.0287
Maximum eclipse
Duration149 s (2 min 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.

As of 2023, this and May 20, 2050 are the next two total solar eclipses in which the Moon's shadow will trace a path that fails to hit land anywhere on Earth. Totality will begin 125 miles east of Belmonte in Brazil, then traverse southeast through the Atlantic Ocean where it will miss the Cape of Good Hope in South Africa by 250 miles, before winding northeast and concluding in the Indian Ocean 500 miles south of Java island.

Related eclipses[edit]

Solar eclipses 2054–2058[edit]

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 to 2058
Ascending node   Descending node
Saros Map Saros Map
117 August 3, 2054

Partial
122 January 27, 2055

Partial
127 July 24, 2055

Total
132 January 16, 2056

Annular
137 July 12, 2056

Annular
142 January 5, 2057

Total
147 July 1, 2057

Annular
152 December 26, 2057

Total
157 June 21, 2058

Partial

Saros series 142[edit]

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

October 10, 1912

October 21, 1930

November 1, 1948
20 21 22

November 12, 1966

November 22, 1984

December 4, 2002
23 24 25

December 14, 2020

December 26, 2038

January 5, 2057
26 27 28

January 16, 2075

January 27, 2093

February 8, 2111
29 30 31

February 18, 2129

March 2, 2147

March 12, 2165
32 33 34

March 23, 2183

April 4, 2201

April 15, 2219
35 36 37

April 25, 2237

May 7, 2255

May 17, 2273
38 39 40

May 28, 2291

June 9, 2309

June 20, 2327
41

June 30, 2345

Tritos series[edit]

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

December 21, 1805
(Saros 119)

November 19, 1816
(Saros 120)

October 20, 1827
(Saros 121)

September 18, 1838
(Saros 122)

August 18, 1849
(Saros 123)

July 18, 1860
(Saros 124)

June 18, 1871
(Saros 125)

May 17, 1882
(Saros 126)

April 16, 1893
(Saros 127)

March 17, 1904
(Saros 128)

February 14, 1915
(Saros 129)

January 14, 1926
(Saros 130)

December 13, 1936
(Saros 131)

November 12, 1947
(Saros 132)

October 12, 1958
(Saros 133)

September 11, 1969
(Saros 134)

August 10, 1980
(Saros 135)

July 11, 1991
(Saros 136)

June 10, 2002
(Saros 137)

May 10, 2013
(Saros 138)

April 8, 2024
(Saros 139)

March 9, 2035
(Saros 140)

February 5, 2046
(Saros 141)

January 5, 2057
(Saros 142)

December 6, 2067
(Saros 143)

November 4, 2078
(Saros 144)

October 4, 2089
(Saros 145)

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[edit]

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

June 1, 2011

March 20, 2015

January 6, 2019

October 25, 2022

August 12, 2026
128 130 132 134 136

June 1, 2030

March 20, 2034

January 5, 2038

October 25, 2041

August 12, 2045
138 140 142 144 146

May 31, 2049

March 20, 2053

January 5, 2057

October 24, 2060

August 12, 2064
148 150 152 154 156

May 31, 2068

March 19, 2072

January 6, 2076

October 24, 2079

August 13, 2083
158 160 162 164 166

June 1, 2087

October 24, 2098

References[edit]

  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[edit]