Solar eclipse of January 26, 2047

A partial solar eclipse will occur at the Moon's ascending node of orbit on Saturday, January 26, 2047, with a magnitude of 0.8907. 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.

Solar eclipse of January 26, 2047
Map
Type of eclipse
NaturePartial
Gamma1.045
Magnitude0.8907
Maximum eclipse
Coordinates62°54′N 111°42′E / 62.9°N 111.7°E / 62.9; 111.7
Times (UTC)
Greatest eclipse1:33:18
References
Saros151 (16 of 72)
Catalog # (SE5000)9611

Images

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Animated path

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Eclipses in 2047

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Metonic

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Tzolkinex

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Half-Saros

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Tritos

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Solar Saros 151

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Inex

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Triad

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Solar eclipses of 2044–2047

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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 2044 to 2047
Ascending node   Descending node
121 February 28, 2044
 
Annular
126 August 23, 2044
 
Total
131 February 16, 2045
 
Annular
136 August 12, 2045
 
Total
141 February 5, 2046
 
Annular
146 August 2, 2046
 
Total
151 January 26, 2047
 
Partial
156 July 22, 2047
 
Partial
Partial solar eclipses on June 23, 2047 and December 16, 2047 occur on the next lunar year eclipse set.

Saros 151

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It is a part of Saros cycle 151, repeating every 18 years, 11 days, containing 72 events. The series started with partial solar eclipse on August 14, 1776. It contains annular eclipses from February 28, 2101, through April 23, 2191, a hybrid eclipse on May 5, 2209, and total eclipses from May 16, 2227, through July 6, 2912. The series ends at member 72 as a partial eclipse on October 1, 3056. The longest duration of totality will be 5 minutes, 41 seconds on May 22, 2840.

Tritos series

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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.

Metonic series

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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 June 21, 1982, and June 21, 2058
June 21 April 8–9 January 26 November 13–14 September 1–2
107 109 111 113 115
June 21, 1963 April 9, 1967 January 26, 1971 November 14, 1974 September 2, 1978
117 119 121 123 125
 
June 21, 1982
 
April 9, 1986
 
January 26, 1990
 
November 13, 1993
 
September 2, 1997
127 129 131 133 135
 
June 21, 2001
 
April 8, 2005
 
January 26, 2009
 
November 13, 2012
 
September 1, 2016
137 139 141 143 145
 
June 21, 2020
 
April 8, 2024
 
January 26, 2028
 
November 14, 2031
 
September 2, 2035
147 149 151 153 155
 
June 21, 2039
 
April 9, 2043
 
January 26, 2047
 
November 14, 2050
 
September 2, 2054
157
 
June 21, 2058

References

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  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.
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