Solar eclipse of November 27, 2095

Last updated
Solar eclipse of November 27, 2095
SE2095Nov27A.png
Map
Type of eclipse
NatureAnnular
Gamma 0.4903
Magnitude 0.933
Maximum eclipse
Duration527 s (8 min 47 s)
Coordinates 7°12′N169°48′E / 7.2°N 169.8°E / 7.2; 169.8
Max. width of band285 km (177 mi)
Times (UTC)
Greatest eclipse1:02:57
References
Saros 134 (48 of 71)
Catalog # (SE5000) 9723

An annular solar eclipse will occur at the Moon's descending node of orbit between Saturday, November 26 and Sunday, November 27, 2095, [1] with a magnitude of 0.933. 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 3.8 days after apogee (on November 23, 2095, at 6:10 UTC), the Moon's apparent diameter will be smaller. [2]

Contents

The path of annularity will be visible from parts of northeastern China, North Korea, South Korea, Japan, the Marshall Islands, and Kiribati. A partial solar eclipse will also be visible for parts of East Asia, Southeast Asia, Oceania, Hawaii, and southwestern Alaska.

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]

November 27, 2095 Solar Eclipse Times
EventTime (UTC)
First Penumbral External Contact2095 November 26 at 22:08:18.5 UTC
First Umbral External Contact2095 November 26 at 23:17:51.3 UTC
First Central Line2095 November 26 at 23:21:03.1 UTC
First Umbral Internal Contact2095 November 26 at 23:24:16.3 UTC
Equatorial Conjunction2095 November 27 at 00:46:21.1 UTC
Ecliptic Conjunction2095 November 27 at 00:57:09.8 UTC
Greatest Eclipse2095 November 27 at 01:02:57.4 UTC
Greatest Duration2095 November 27 at 01:13:24.5 UTC
Last Umbral Internal Contact2095 November 27 at 02:41:51.2 UTC
Last Central Line2095 November 27 at 02:45:02.1 UTC
Last Umbral External Contact2095 November 27 at 02:48:11.5 UTC
Last Penumbral External Contact2095 November 27 at 03:57:38.7 UTC
November 27, 2095 Solar Eclipse Parameters
ParameterValue
Eclipse Magnitude0.93303
Eclipse Obscuration0.87054
Gamma0.49030
Sun Right Ascension16h12m24.6s
Sun Declination-21°07'41.4"
Sun Semi-Diameter16'12.2"
Sun Equatorial Horizontal Parallax08.9"
Moon Right Ascension16h12m56.4s
Moon Declination-20°41'58.0"
Moon Semi-Diameter14'55.2"
Moon Equatorial Horizontal Parallax0°54'45.3"
ΔT119.6 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 November–December 2095
November 27
Descending node (new moon)
 December 11
Ascending node (full moon)
SE2095Nov27A.png
Annular solar eclipse
Solar Saros 134		 Partial lunar eclipse
Lunar Saros 146

Eclipses in 2095

Metonic

Tzolkinex

Half-Saros

Tritos

Solar Saros 134

Inex

Triad

Solar eclipses of 2094–2098

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 solar eclipses on January 16, 2094 (total) and July 12, 2094 (partial) occur in the previous lunar year eclipse set, and the partial solar eclipses on April 1, 2098 and September 25, 2098 occur in the next lunar year eclipse set.

Solar eclipse series sets from 2094 to 2098
Ascending node Descending node
SarosMapGammaSarosMapGamma
119 June 13, 2094
SE2094Jun13P.png
Partial		−1.4613124 December 7, 2094
SE2094Dec07P.png
Partial		1.1547
129 June 2, 2095
SE2095Jun02T.png
Total		−0.6396134 November 27, 2095
SE2095Nov27A.png
Annular		0.4903
139 May 22, 2096
SE2096May22T.png
Total		0.1196144 November 15, 2096
SE2096Nov15A.png
Annular		−0.20
149 May 11, 2097
SE2097May11T.png
Total		0.8516154 November 4, 2097
SE2097Nov04A.png
Annular		−0.8926
159May 1, 2098164 October 24, 2098
SE2098Oct24P.png
Partial		−1.5407

Saros 134

This eclipse is a part of Saros series 134, repeating every 18 years, 11 days, and containing 71 events. The series started with a partial solar eclipse on June 22, 1248. It contains total eclipses from October 9, 1428 through December 24, 1554; hybrid eclipses from January 3, 1573 through June 27, 1843; and annular eclipses from July 8, 1861 through May 21, 2384. The series ends at member 72 as a partial eclipse on August 6, 2510. 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 11 at 1 minutes, 30 seconds on October 9, 1428, and the longest duration of annularity will be produced by member 52 at 10 minutes, 55 seconds on January 10, 2168. All eclipses in this series occur at the Moon’s descending node of orbit. [5]

Series members 32–53 occur between 1801 and 2200:
323334
SE1807Jun06H.png
June 6, 1807		 SE1825Jun16H.png
June 16, 1825		 SE1843Jun27H.png
June 27, 1843
353637
SE1861Jul08A.png
July 8, 1861		 SE1879Jul19A.png
July 19, 1879		 SE1897Jul29A.png
July 29, 1897
383940
SE1915Aug10A.png
August 10, 1915 		SE1933Aug21A.png
August 21, 1933 		SE1951Sep01A.png
September 1, 1951
414243
SE1969Sep11A.png
September 11, 1969 		SE1987Sep23A.png
September 23, 1987 		SE2005Oct03A.png
October 3, 2005
444546
SE2023Oct14A.png
October 14, 2023 		SE2041Oct25A.png
October 25, 2041 		SE2059Nov05A.png
November 5, 2059
474849
SE2077Nov15A.png
November 15, 2077 		SE2095Nov27A.png
November 27, 2095 		SE2113Dec08A.png
December 8, 2113
505152
SE2131Dec19A.png
December 19, 2131		 SE2149Dec30A.png
December 30, 2149		 SE2168Jan10A.png
January 10, 2168
53
SE2186Jan20A.png
January 20, 2186

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 descending node.

22 eclipse events between July 3, 2065 and November 26, 2152
July 3–4April 21–23February 7–8November 26–27September 13–15
118120122124126
SE2065Jul03P.png
July 3, 2065 		SE2069Apr21P.png
April 21, 2069 		SE2073Feb07P.png
February 7, 2073 		SE2076Nov26P.png
November 26, 2076 		SE2080Sep13P.png
September 13, 2080
128130132134136
SE2084Jul03A.png
July 3, 2084 		SE2088Apr21T.png
April 21, 2088 		SE2092Feb07A.png
February 7, 2092 		SE2095Nov27A.png
November 27, 2095 		SE2099Sep14T.png
September 14, 2099
138140142144146
SE2103Jul04A.png
July 4, 2103		 SE2107Apr23A.png
April 23, 2107		 SE2111Feb08T.png
February 8, 2111		 SE2114Nov27A.png
November 27, 2114		 SE2118Sep15T.png
September 15, 2118
148150152154156
Saros148 27van75 SE2122Jul04T.jpg
July 4, 2122		 Saros150 23van71 SE2126Apr22A.jpg
April 22, 2126		 Saros152 19van70 SE2130Feb08T.jpg
February 8, 2130		 Saros154 13van71 SE2133Nov26A.jpg
November 26, 2133		 Saros156 08van69 SE2137Sep15P.jpg
September 15, 2137
158160162164
Saros158 05van70 SE2141Jul03P.jpg
July 3, 2141		 Saros164 04van80 SE2152Nov26P.jpg
November 26, 2152

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
SE1801Mar14P.png
March 14, 1801
(Saros 107)		 SE1812Feb12P.gif
February 12, 1812
(Saros 108)		 SE1823Jan12P.gif
January 12, 1823
(Saros 109)		 SE1844Nov10P.gif
November 10, 1844
(Saros 111)
SE1877Aug09P.gif
August 9, 1877
(Saros 114)		 SE1888Jul09P.gif
July 9, 1888
(Saros 115)		 SE1899Jun08P.gif
June 8, 1899
(Saros 116)
SE1910May09T.png
May 9, 1910
(Saros 117)		 SE1921Apr08A.png
April 8, 1921
(Saros 118)		 SE1932Mar07A.png
March 7, 1932
(Saros 119)		 SE1943Feb04T.png
February 4, 1943
(Saros 120)		 SE1954Jan05A.png
January 5, 1954
(Saros 121)
SE1964Dec04P.png
December 4, 1964
(Saros 122)		 SE1975Nov03P.png
November 3, 1975
(Saros 123)		 SE1986Oct03H.png
October 3, 1986
(Saros 124)		 SE1997Sep02P.png
September 2, 1997
(Saros 125)		 SE2008Aug01T.png
August 1, 2008
(Saros 126)
SE2019Jul02T.png
July 2, 2019
(Saros 127)		 SE2030Jun01A.png
June 1, 2030
(Saros 128)		 SE2041Apr30T.png
April 30, 2041
(Saros 129)		 SE2052Mar30T.png
March 30, 2052
(Saros 130)		 SE2063Feb28A.png
February 28, 2063
(Saros 131)
SE2074Jan27A.png
January 27, 2074
(Saros 132)		 SE2084Dec27T.png
December 27, 2084
(Saros 133)		 SE2095Nov27A.png
November 27, 2095
(Saros 134)		 SE2106Oct26A.png
October 26, 2106
(Saros 135)		 SE2117Sep26T.png
September 26, 2117
(Saros 136)
SE2128Aug25A.png
August 25, 2128
(Saros 137)		 SE2139Jul25A.png
July 25, 2139
(Saros 138)		 SE2150Jun25T.png
June 25, 2150
(Saros 139)		 SE2161May25A.png
May 25, 2161
(Saros 140)		 SE2172Apr23A.png
April 23, 2172
(Saros 141)
SE2183Mar23T.png
March 23, 2183
(Saros 142)		 SE2194Feb21A.png
February 21, 2194
(Saros 143)

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
SE1806Jun16T.png
June 16, 1806
(Saros 124)		 SE1835May27A.gif
May 27, 1835
(Saros 125)		 SE1864May06H.gif
May 6, 1864
(Saros 126)
SE1893Apr16T.png
April 16, 1893
(Saros 127)		 SE1922Mar28A.png
March 28, 1922
(Saros 128)		 SE1951Mar07A.png
March 7, 1951
(Saros 129)
SE1980Feb16T.png
February 16, 1980
(Saros 130)		 SE2009Jan26A.png
January 26, 2009
(Saros 131)		 SE2038Jan05A.png
January 5, 2038
(Saros 132)
SE2066Dec17T.png
December 17, 2066
(Saros 133)		 SE2095Nov27A.png
November 27, 2095
(Saros 134)		 SE2124Nov06A.png
November 6, 2124
(Saros 135)
SE2153Oct17T.png
October 17, 2153
(Saros 136)		 SE2182Sep27A.png
September 27, 2182
(Saros 137)

Notes

  1. ↑ "November 26–27, 2095 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 2095 Nov 27". 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 134". eclipse.gsfc.nasa.gov.

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References

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