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Solar eclipse of January 26, 2047

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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

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.

This will be the first of four partial solar eclipses in 2047, with the others occurring on June 23, July 22, and December 16.

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]

The partial solar eclipses on June 23, 2047 and December 16, 2047 occur in the next lunar year eclipse set.

Solar eclipse series sets from 2044 to 2047
Ascending node   Descending node
Saros Map Gamma Saros Map Gamma
121 February 28, 2044

Annular
−0.9954 126 August 23, 2044

Total
0.9613
131 February 16, 2045

Annular
−0.3125 136 August 12, 2045

Total
0.2116
141 February 5, 2046

Annular
0.3765 146 August 2, 2046

Total
−0.535
151 January 26, 2047

Partial
1.045 156 July 22, 2047

Partial
−1.3477

Saros 151

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This eclipse is a part of Saros series 151, repeating every 18 years, 11 days, and containing 72 events. The series started with a 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. 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 19 at 2 minutes, 44 seconds on February 28, 2101, and the longest duration of totality will be produced by member 60 at 5 minutes, 41 seconds on May 22, 2840. All eclipses in this series occur at the Moon’s ascending node of orbit.[2]

Series members 3–24 occur between 1801 and 2200:
3 4 5

September 5, 1812

September 17, 1830

September 27, 1848
6 7 8

October 8, 1866

October 19, 1884

October 31, 1902
9 10 11

November 10, 1920

November 21, 1938

December 2, 1956
12 13 14

December 13, 1974

December 24, 1992

January 4, 2011
15 16 17

January 14, 2029

January 26, 2047

February 5, 2065
18 19 20

February 16, 2083

February 28, 2101

March 11, 2119
21 22 23

March 21, 2137

April 2, 2155

April 12, 2173
24

April 23, 2191

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
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

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.

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

December 10, 1806
(Saros 129)

November 9, 1817
(Saros 130)

October 9, 1828
(Saros 131)

September 7, 1839
(Saros 132)

August 7, 1850
(Saros 133)

July 8, 1861
(Saros 134)

June 6, 1872
(Saros 135)

May 6, 1883
(Saros 136)

April 6, 1894
(Saros 137)

March 6, 1905
(Saros 138)

February 3, 1916
(Saros 139)

January 3, 1927
(Saros 140)

December 2, 1937
(Saros 141)

November 1, 1948
(Saros 142)

October 2, 1959
(Saros 143)

August 31, 1970
(Saros 144)

July 31, 1981
(Saros 145)

June 30, 1992
(Saros 146)

May 31, 2003
(Saros 147)

April 29, 2014
(Saros 148)

March 29, 2025
(Saros 149)

February 27, 2036
(Saros 150)

January 26, 2047
(Saros 151)

December 26, 2057
(Saros 152)

November 24, 2068
(Saros 153)

October 24, 2079
(Saros 154)

September 23, 2090
(Saros 155)

August 24, 2101
(Saros 156)

July 23, 2112
(Saros 157)

June 23, 2123
(Saros 158)

May 23, 2134
(Saros 159)

Inex series

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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

July 6, 1815
(Saros 143)

June 16, 1844
(Saros 144)

May 26, 1873
(Saros 145)

May 7, 1902
(Saros 146)

April 18, 1931
(Saros 147)

March 27, 1960
(Saros 148)

March 7, 1989
(Saros 149)

February 15, 2018
(Saros 150)

January 26, 2047
(Saros 151)

January 6, 2076
(Saros 152)

December 17, 2104
(Saros 153)

November 26, 2133
(Saros 154)

November 7, 2162
(Saros 155)

October 18, 2191
(Saros 156)

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.
  2. ^ "NASA - Catalog of Solar Eclipses of Saros 151". eclipse.gsfc.nasa.gov.
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