Solar eclipse of October 14, 2088

Last updated
Solar eclipse of October 14, 2088
SE2088Oct14A.png
Map
Type of eclipse
NatureAnnular
Gamma −0.5349
Magnitude 0.9727
Maximum eclipse
Duration158 s (2 min 38 s)
Coordinates 39°42′S56°00′W / 39.7°S 56°W / -39.7; -56
Max. width of band115 km (71 mi)
Times (UTC)
Greatest eclipse14:48:05
References
Saros 135 (43 of 71)
Catalog # (SE5000) 9707

An annular solar eclipse will occur at the Moon's ascending node of orbit on Thursday, October 14, 2088, [1] with a magnitude of 0.9727. 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. An annular solar eclipse occurs when the Moon's apparent diameter is smaller than the Sun's, blocking most of the Sun's light and causing the Sun to look like an annulus (ring). An annular eclipse appears as a partial eclipse over a region of the Earth thousands of kilometres wide. Occurring about 6.3 days before apogee (on October 20, 2088, at 21:10 UTC), the Moon's apparent diameter will be smaller. [2]

Contents

The path of annularity will be visible from parts of Chile and Argentina. A partial solar eclipse will also be visible for parts of South America, Antarctica, and Southern Africa.

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. [3]

October 14, 2088 Solar Eclipse Times
EventTime (UTC)
First Penumbral External Contact2088 October 14 at 12:03:04.6 UTC
First Umbral External Contact2088 October 14 at 13:11:17.2 UTC
First Central Line2088 October 14 at 13:12:48.2 UTC
First Umbral Internal Contact2088 October 14 at 13:14:19.8 UTC
Ecliptic Conjunction2088 October 14 at 14:42:05.5 UTC
Greatest Eclipse2088 October 14 at 14:48:05.1 UTC
Equatorial Conjunction2088 October 14 at 15:05:35.7 UTC
Greatest Duration2088 October 14 at 15:28:07.6 UTC
Last Umbral Internal Contact2088 October 14 at 16:21:35.2 UTC
Last Central Line2088 October 14 at 16:23:09.9 UTC
Last Umbral External Contact2088 October 14 at 16:24:44.2 UTC
Last Penumbral External Contact2088 October 14 at 17:33:04.0 UTC
October 14, 2088 Solar Eclipse Parameters
ParameterValue
Eclipse Magnitude0.97271
Eclipse Obscuration0.94616
Gamma−0.53492
Sun Right Ascension13h22m16.6s
Sun Declination-08°39'19.3"
Sun Semi-Diameter16'02.1"
Sun Equatorial Horizontal Parallax08.8"
Moon Right Ascension13h21m42.6s
Moon Declination-09°08'15.8"
Moon Semi-Diameter15'23.5"
Moon Equatorial Horizontal Parallax0°56'29.4"
ΔT113.0 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 2088
October 14
Ascending node (new moon)
 October 30
Descending node (full moon)
SE2088Oct14A.png
Annular solar eclipse
Solar Saros 135		 Partial lunar eclipse
Lunar Saros 147

Eclipses in 2088

Metonic

Tzolkinex

Half-Saros

Tritos

Solar Saros 135

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. [4]

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 135

This eclipse is a part of Saros series 135, repeating every 18 years, 11 days, and containing 71 events. The series started with a partial solar eclipse on July 5, 1331. It contains annular eclipses from October 21, 1511 through February 24, 2305; hybrid eclipses on March 8, 2323 and March 18, 2341; and total eclipses from March 29, 2359 through May 22, 2449. The series ends at member 71 as a partial eclipse on August 17, 2593. 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 was produced by member 16 at 10 minutes, 41 seconds on December 24, 1601, and the longest duration of totality will be produced by member 62 at 2 minutes, 27 seconds on May 12, 2431. All eclipses in this series occur at the Moon’s ascending node of orbit. [5]

Series members 28–49 occur between 1801 and 2200:
282930
SE1818May05A.png
May 5, 1818		 SE1836May15A.png
May 15, 1836		 SE1854May26A.png
May 26, 1854
313233
SE1872Jun06A.gif
June 6, 1872		 SE1890Jun17A.png
June 17, 1890		 SE1908Jun28A.png
June 28, 1908
343536
SE1926Jul09A.png
July 9, 1926 		SE1944Jul20A.png
July 20, 1944 		SE1962Jul31A.png
July 31, 1962
373839
SE1980Aug10A.png
August 10, 1980 		SE1998Aug22A.png
August 22, 1998 		SE2016Sep01A.png
September 1, 2016
404242
SE2034Sep12A.png
September 12, 2034 		SE2052Sep22A.png
September 22, 2052 		SE2070Oct04A.png
October 4, 2070
434445
SE2088Oct14A.png
October 14, 2088 		SE2106Oct26A.png
October 26, 2106		 SE2124Nov06A.png
November 6, 2124
464748
SE2142Nov17A.png
November 17, 2142		 SE2160Nov27A.png
November 27, 2160		 SE2178Dec09A.png
December 9, 2178
49
SE2196Dec19A.png
December 19, 2196

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.

23 eclipse events between August 3, 2054 and October 16, 2145
August 3–4May 22–24March 10–11December 27–29October 14–16
117119121123125
SE2054Aug03P.png
August 3, 2054 		SE2058May22P.png
May 22, 2058 		SE2062Mar11P.png
March 11, 2062 		SE2065Dec27P.png
December 27, 2065 		SE2069Oct15P.png
October 15, 2069
127129131133135
SE2073Aug03T.png
August 3, 2073 		SE2077May22T.png
May 22, 2077 		SE2081Mar10A.png
March 10, 2081 		SE2084Dec27T.png
December 27, 2084 		SE2088Oct14A.png
October 14, 2088
137139141143145
SE2092Aug03A.png
August 3, 2092 		SE2096May22T.png
May 22, 2096 		SE2100Mar10A.png
March 10, 2100 		SE2103Dec29A.png
December 29, 2103		 SE2107Oct16T.png
October 16, 2107
147149151153155
SE2111Aug04A.png
August 4, 2111		 SE2115May24T.png
May 24, 2115		 Saros151 20van72 SE2119Mar11A.jpg
March 11, 2119		 Saros153 15van70 SE2122Dec28A.jpg
December 28, 2122		 SE2126Oct16T.png
October 16, 2126
157159161163165
Saros157 05van70 SE2130Aug04P.jpg
August 4, 2130		 Saros159 01van70 SE2134May23P.jpg
May 23, 2134		 Saros165 01van72 SE2145Oct16P.jpg
October 16, 2145

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.

Series members between 1801 and 2200
SE1805Jan01P.gif
January 1, 1805
(Saros 109)		 SE1826Oct31P.gif
October 31, 1826
(Saros 111)		 SE1848Aug28P.gif
August 28, 1848
(Saros 113)
SE1859Jul29P.gif
July 29, 1859
(Saros 114)		 SE1870Jun28P.gif
June 28, 1870
(Saros 115)		 SE1881May27P.gif
May 27, 1881
(Saros 116)		 SE1892Apr26T.png
April 26, 1892
(Saros 117)		 SE1903Mar29A.png
March 29, 1903
(Saros 118)
SE1914Feb25A.png
February 25, 1914
(Saros 119)		 SE1925Jan24T.png
January 24, 1925
(Saros 120)		 SE1935Dec25A.png
December 25, 1935
(Saros 121)		 SE1946Nov23P.png
November 23, 1946
(Saros 122)		 SE1957Oct23T.png
October 23, 1957
(Saros 123)
SE1968Sep22T.png
September 22, 1968
(Saros 124)		 SE1979Aug22A.png
August 22, 1979
(Saros 125)		 SE1990Jul22T.png
July 22, 1990
(Saros 126)		 SE2001Jun21T.png
June 21, 2001
(Saros 127)		 SE2012May20A.png
May 20, 2012
(Saros 128)
SE2023Apr20H.png
April 20, 2023
(Saros 129)		 SE2034Mar20T.png
March 20, 2034
(Saros 130)		 SE2045Feb16A.png
February 16, 2045
(Saros 131)		 SE2056Jan16A.png
January 16, 2056
(Saros 132)		 SE2066Dec17T.png
December 17, 2066
(Saros 133)
SE2077Nov15A.png
November 15, 2077
(Saros 134)		 SE2088Oct14A.png
October 14, 2088
(Saros 135)		 SE2099Sep14T.png
September 14, 2099
(Saros 136)		 SE2110Aug15A.png
August 15, 2110
(Saros 137)		 SE2121Jul14A.png
July 14, 2121
(Saros 138)
SE2132Jun13T.png
June 13, 2132
(Saros 139)		 SE2143May14A.png
May 14, 2143
(Saros 140)		 SE2154Apr12A.png
April 12, 2154
(Saros 141)		 SE2165Mar12T.png
March 12, 2165
(Saros 142)		 SE2176Feb10A.png
February 10, 2176
(Saros 143)
SE2187Jan09A.png
January 9, 2187
(Saros 144)		 SE2197Dec09T.png
December 9, 2197
(Saros 145)

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
Saros126 37van72 SE1828Apr14H.jpg
April 14, 1828
(Saros 126)		 SE1857Mar25T.png
March 25, 1857
(Saros 127)		 SE1886Mar05A.gif
March 5, 1886
(Saros 128)
SE1915Feb14A.png
February 14, 1915
(Saros 129)		 SE1944Jan25T.png
January 25, 1944
(Saros 130)		 SE1973Jan04A.png
January 4, 1973
(Saros 131)
SE2001Dec14A.png
December 14, 2001
(Saros 132)		 SE2030Nov25T.png
November 25, 2030
(Saros 133)		 SE2059Nov05A.png
November 5, 2059
(Saros 134)
SE2088Oct14A.png
October 14, 2088
(Saros 135)		 SE2117Sep26T.png
September 26, 2117
(Saros 136)		 SE2146Sep06A.png
September 6, 2146
(Saros 137)
SE2175Aug16A.png
August 16, 2175
(Saros 138)

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References

  1. ↑ "October 14, 2088 Annular Solar Eclipse". timeanddate. Retrieved 24 August 2024.
  2. ↑ "Moon Distances for London, United Kingdom, England". timeanddate. Retrieved 24 August 2024.
  3. ↑ "Annular Solar Eclipse of 2088 Oct 14". EclipseWise.com. Retrieved 24 August 2024.
  4. ↑ 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.
  5. ↑ "NASA - Catalog of Solar Eclipses of Saros 135". eclipse.gsfc.nasa.gov.
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