Solar eclipse of October 26, 2087

A partial solar eclipse will occur at the Moon's ascending node of orbit on Sunday, October 26, 2087, with a magnitude of 0.4696. 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 October 26, 2087
Map
Type of eclipse
NaturePartial
Gamma−1.2882
Magnitude0.4696
Maximum eclipse
Coordinates71°00′S 130°30′W / 71°S 130.5°W / -71; -130.5
Times (UTC)
Greatest eclipse11:46:57
References
Saros125 (58 of 73)
Catalog # (SE5000)9705
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Eclipses in 2087

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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 125

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Inex

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Triad

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Solar eclipses of 2087–2090

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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]

120 May 2, 2087
 
Partial
125 October 26, 2087
 
Partial
130 April 21, 2088
 
Total
135 October 14, 2088
 
Annular
140 April 10, 2089
 
Annular
145 October 4, 2089
 
Total
150 March 31, 2090
 
Partial
155 September 23, 2090
 
Total

Saros 125

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This eclipse is a part of Saros series 125, repeating every 18 years, 11 days, and containing 73 events. The series started with a partial solar eclipse on February 4, 1060. It contains total eclipses from June 13, 1276 through July 16, 1330; hybrid eclipses on July 26, 1348 and August 7, 1366; and annular eclipses from August 17, 1384 through August 22, 1979. The series ends at member 73 as a partial eclipse on April 9, 2358. 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 totality was produced by member 14 at 1 minutes, 11 seconds on June 25, 1294, and the longest duration of annularity was produced by member 48 at 7 minutes, 23 seconds on July 10, 1907. All eclipses in this series occur at the Moon’s ascending node of orbit.[2]

Series members 43–64 occur between 1801 and 2200:
43 44 45
 
May 16, 1817
 
May 27, 1835
 
June 6, 1853
46 47 48
 
June 18, 1871
 
June 28, 1889
 
July 10, 1907
49 50 51
 
July 20, 1925
 
August 1, 1943
 
August 11, 1961
52 53 54
 
August 22, 1979
 
September 2, 1997
 
September 13, 2015
55 56 57
 
September 23, 2033
 
October 4, 2051
 
October 15, 2069
58 59 60
 
October 26, 2087
 
November 6, 2105
 
November 18, 2123
61 62 63
 
November 28, 2141
 
December 9, 2159
 
December 20, 2177
64
 
December 31, 2195

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 125". eclipse.gsfc.nasa.gov.
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