Solar eclipse of October 26, 2087

Last updated
Solar eclipse of October 26, 2087
SE2087Oct26P.png
Map
Type of eclipse
NaturePartial
Gamma −1.2882
Magnitude 0.4696
Maximum eclipse
Coordinates 71°00′S130°30′W / 71°S 130.5°W / -71; -130.5
Times (UTC)
Greatest eclipse11:46:57
References
Saros 125 (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, [1] 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.

Contents

The partial solar eclipse will be visible for parts of southern South America and Antarctica.

Eclipse details

Shown below are two tables displaying details about this particular solar eclipse. The first table outlines times at which the moon's penumbra or umbra attains the specific parameter, and the second table describes various other parameters pertaining to this eclipse. [2]

October 26, 2087 Solar Eclipse Times
EventTime (UTC)
First Penumbral External Contact2087 October 26 at 10:00:50.1 UTC
Ecliptic Conjunction2087 October 26 at 11:31:59.1 UTC
Greatest Eclipse2087 October 26 at 11:46:56.7 UTC
Equatorial Conjunction2087 October 26 at 12:25:49.5 UTC
Last Penumbral External Contact2087 October 26 at 13:32:48.0 UTC
October 26, 2087 Solar Eclipse Parameters
ParameterValue
Eclipse Magnitude0.46962
Eclipse Obscuration0.34848
Gamma−1.28822
Sun Right Ascension14h04m17.3s
Sun Declination-12°36'18.7"
Sun Semi-Diameter16'05.1"
Sun Equatorial Horizontal Parallax08.8"
Moon Right Ascension14h03m06.4s
Moon Declination-13°43'47.4"
Moon Semi-Diameter14'46.3"
Moon Equatorial Horizontal Parallax0°54'12.8"
ΔT112.1 s

Eclipse season

This eclipse is part of an eclipse season, a period, roughly every six months, when eclipses occur. Only two (or occasionally three) eclipse seasons occur each year, and each season lasts about 35 days and repeats just short of six months (173 days) later; thus two full eclipse seasons always occur each year. Either two or three eclipses happen each eclipse season. In the sequence below, each eclipse is separated by a fortnight.

Eclipse season of October–November 2087
October 26
Ascending node (new moon)
November 10
Descending node (full moon)
SE2087Oct26P.png Lunar eclipse chart close-2087Nov10.png
Partial solar eclipse
Solar Saros 125
Total lunar eclipse
Lunar Saros 137

Eclipses in 2087

Metonic

Tzolkinex

Half-Saros

Tritos

Solar Saros 125

Inex

Triad

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. [3]

The partial solar eclipse on June 1, 2087 occurs in the previous lunar year eclipse set.

Solar eclipse series sets from 2087 to 2090
Descending node Ascending node
SarosMapGammaSarosMapGamma
120 May 2, 2087
SE2087May02P.png
Partial
1.1139125 October 26, 2087
SE2087Oct26P.png
Partial
−1.2882
130 April 21, 2088
SE2088Apr21T.png
Total
0.4135135 October 14, 2088
SE2088Oct14A.png
Annular
−0.5349
140 April 10, 2089
SE2089Apr10A.png
Annular
−0.3319145 October 4, 2089
SE2089Oct04T.png
Total
0.2167
150 March 31, 2090
SE2090Mar31P.png
Partial
−1.1028155 September 23, 2090
SE2090Sep23T.png
Total
0.9157

Saros 125

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. [4]

Series members 43–64 occur between 1801 and 2200:
434445
SE1817May16A.gif
May 16, 1817
SE1835May27A.gif
May 27, 1835
SE1853Jun06A.gif
June 6, 1853
464748
SE1871Jun18A.gif
June 18, 1871
SE1889Jun28A.png
June 28, 1889
SE1907Jul10A.png
July 10, 1907
495051
SE1925Jul20A.png
July 20, 1925
SE1943Aug01A.png
August 1, 1943
SE1961Aug11A.png
August 11, 1961
525354
SE1979Aug22A.png
August 22, 1979
SE1997Sep02P.png
September 2, 1997
SE2015Sep13P.png
September 13, 2015
555657
SE2033Sep23P.png
September 23, 2033
SE2051Oct04P.png
October 4, 2051
SE2069Oct15P.png
October 15, 2069
585960
SE2087Oct26P.png
October 26, 2087
Saros125 59van73 SE2105Nov06P.jpg
November 6, 2105
Saros125 60van73 SE2123Nov18P.jpg
November 18, 2123
616263
Saros125 61van73 SE2141Nov28P.jpg
November 28, 2141
Saros125 62van73 SE2159Dec09P.jpg
December 9, 2159
Saros125 63van73 SE2177Dec20P.jpg
December 20, 2177
64
Saros125 64van73 SE2195Dec31P.jpg
December 31, 2195

Metonic series

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.

22 eclipse events between June 1, 2076 and October 27, 2163
June 1–3March 21–22January 7–8October 26–27August 14–15
119121123125127
SE2076Jun01P.png
June 1, 2076
SE2080Mar21P.png
March 21, 2080
SE2084Jan07P.png
January 7, 2084
SE2087Oct26P.png
October 26, 2087
SE2091Aug15T.png
August 15, 2091
129131133135137
SE2095Jun02T.png
June 2, 2095
SE2099Mar21A.png
March 21, 2099
SE2103Jan08T.png
January 8, 2103
SE2106Oct26A.png
October 26, 2106
SE2110Aug15A.png
August 15, 2110
139141143145147
SE2114Jun03T.png
June 3, 2114
SE2118Mar22A.png
March 22, 2118
SE2122Jan08A.png
January 8, 2122
SE2125Oct26T.png
October 26, 2125
SE2129Aug15A.png
August 15, 2129
149151153155157
SE2133Jun03T.png
June 3, 2133
Saros151 21van72 SE2137Mar21A.jpg
March 21, 2137
SE2141Jan08A.png
January 8, 2141
Saros155 13van71 SE2144Oct26T.jpg
October 26, 2144
Saros157 06van70 SE2148Aug14P.jpg
August 14, 2148
159161163165
Saros159 02van70 SE2152Jun03P.jpg
June 3, 2152
Saros165 02van72 SE2163Oct27P.jpg
October 27, 2163

Tritos series

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 April 8, 1902 (part of Saros 108) and January 5, 1935 (part of Saros 111) are also a part of this series but are not included in the table below.

Series members between 2000 and 2200
SE2000Jul01P.png
July 1, 2000
(Saros 117)
SE2011Jun01P.png
June 1, 2011
(Saros 118)
SE2022Apr30P.png
April 30, 2022
(Saros 119)
SE2033Mar30T.png
March 30, 2033
(Saros 120)
SE2044Feb28A.png
February 28, 2044
(Saros 121)
SE2055Jan27P.png
January 27, 2055
(Saros 122)
SE2065Dec27P.png
December 27, 2065
(Saros 123)
SE2076Nov26P.png
November 26, 2076
(Saros 124)
SE2087Oct26P.png
October 26, 2087
(Saros 125)
SE2098Sep25P.png
September 25, 2098
(Saros 126)
Saros127 63van82 SE2109Aug26P.jpg
August 26, 2109
(Saros 127)
SE2120Jul25A.png
July 25, 2120
(Saros 128)
Saros129 58van80 SE2131Jun25T.jpg
June 25, 2131
(Saros 129)
SE2142May25T.png
May 25, 2142
(Saros 130)
SE2153Apr23A.png
April 23, 2153
(Saros 131)
SE2164Mar23H.png
March 23, 2164
(Saros 132)
SE2175Feb21T.png
February 21, 2175
(Saros 133)
SE2186Jan20A.png
January 20, 2186
(Saros 134)
SE2196Dec19A.png
December 19, 2196
(Saros 135)

Inex series

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
SE1827Apr26A.gif
April 26, 1827
(Saros 116)
SE1856Apr05T.gif
April 5, 1856
(Saros 117)
SE1885Mar16A.gif
March 16, 1885
(Saros 118)
SE1914Feb25A.png
February 25, 1914
(Saros 119)
SE1943Feb04T.png
February 4, 1943
(Saros 120)
SE1972Jan16A.png
January 16, 1972
(Saros 121)
SE2000Dec25P.png
December 25, 2000
(Saros 122)
SE2029Dec05P.png
December 5, 2029
(Saros 123)
SE2058Nov16P.png
November 16, 2058
(Saros 124)
SE2087Oct26P.png
October 26, 2087
(Saros 125)
Saros126 53van72 SE2116Oct06P.jpg
October 6, 2116
(Saros 126)
Saros127 65van82 SE2145Sep16P.jpg
September 16, 2145
(Saros 127)
Saros128 67van73 SE2174Aug27P.jpg
August 27, 2174
(Saros 128)

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References

  1. "October 26, 2087 Partial Solar Eclipse". timeanddate. Retrieved 24 August 2024.
  2. "Partial Solar Eclipse of 2087 Oct 26". EclipseWise.com. Retrieved 24 August 2024.
  3. 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.
  4. "NASA - Catalog of Solar Eclipses of Saros 125". eclipse.gsfc.nasa.gov.