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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It is a part of Saros cycle 125, repeating every 18 years, 11 days, 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. The longest duration of totality was 1 minutes, 11 seconds on June 25, 1294, and the longest duration of annularity was 7 minutes, 23 seconds on July 10, 1907.

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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