Solar eclipse of October 26, 2087

Future partial solar eclipse

71°00′S 130°30′W / 71°S 130.5°W / -71; -130.5Times (UTC)Greatest eclipse11:46:57ReferencesSaros125 (58 of 73)Catalog # (SE5000)9705

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.

Related eclipses

Eclipses in 2087

A partial solar eclipse on May 2, 2087.
A total lunar eclipse on May 17, 2087.
A partial solar eclipse on June 1, 2087.
A partial solar eclipse on October 26, 2087.
A total lunar eclipse on November 10, 2087.

Metonic

Preceded by: Solar eclipse of January 7, 2084
Followed by: Solar eclipse of August 15, 2091

Tzolkinex

Preceded by: Solar eclipse of September 13, 2080
Followed by: Solar eclipse of December 7, 2094

Half-Saros

Preceded by: Lunar eclipse of October 21, 2078
Followed by: Lunar eclipse of October 31, 2096

Tritos

Preceded by: Solar eclipse of November 26, 2076
Followed by: Solar eclipse of September 25, 2098

Solar Saros 125

Preceded by: Solar eclipse of October 15, 2069
Followed by: Solar eclipse of November 6, 2105

Inex

Preceded by: Solar eclipse of November 16, 2058
Followed by: Solar eclipse of October 6, 2116

Triad

Preceded by: Solar eclipse of December 25, 2000
Followed by: Solar eclipse of August 27, 2174

Solar eclipses of 2087–2090

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

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.

Series members 48–64 occur between 1900 and 2200:
48	49	50
July 10, 1907	July 20, 1925	August 1, 1943
51	52	53
August 11, 1961	August 22, 1979	September 2, 1997
54	55	56
September 13, 2015	September 23, 2033	October 4, 2051
57	58	59
October 15, 2069	October 26, 2087	November 6, 2105
60	61	62
November 18, 2123	November 28, 2141	December 9, 2159
63	64
December 20, 2177	December 31, 2195

References

^ 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.

External links

http://eclipse.gsfc.nasa.gov/SEplot/SEplot2051/SE2087Oct26P.GIF

Solar eclipses

Features

Lists of eclipses

By era	Antiquity Middle Ages Modern era 16th 17th 18th 19th 20th 21st 22nd Future
Saros series (list)	109 110 111 112 113 114 115 116 117 118 119 120 121 122 123 124 125 126 127 128 129 130 131 132 133 134 135 136 137 138 139 140 141 142 143 144 145 146 147 148 149 150 151 152 153 154 155 156 157 158 159 160 161 162
Visibility	Australia British Isles China Israel Philippines Russia Turkey Ukraine United States
Historical	Mursili's eclipse (1312 BC) Assyrian eclipse (763 BC) Eclipse of Thales (585 BC) Muhammad's eclipse (632 AD)