Solar eclipse of November 15, 2096

Last updated
Solar eclipse of November 15, 2096
SE2096Nov15A.png
Map
Type of eclipse
NatureAnnular
Gamma −0.20
Magnitude 0.9237
Maximum eclipse
Duration533 s (8 min 53 s)
Coordinates 29°42′S163°18′E / 29.7°S 163.3°E / -29.7; 163.3
Max. width of band294 km (183 mi)
Times (UTC)
Greatest eclipse0:36:15
References
Saros 144 (21 of 70)
Catalog # (SE5000) 9725

An annular solar eclipse will occur at the Moon's descending node of orbit between Wednesday, November 14 and Thursday, November 15, 2096, [1] with a magnitude of 0.9237. 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 1.2 days before apogee (on November 16, 2096, at 5:05 UTC), the Moon's apparent diameter will be smaller. [2]

Contents

The path of annularity will be visible from parts of Malaysia, Brunei, Indonesia, Papua New Guinea, northeastern Australia, and New Zealand. A partial solar eclipse will also be visible for parts of Southeast Asia, Australia, Oceania, 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. [3]

November 15, 2096 Solar Eclipse Times
EventTime (UTC)
First Penumbral External Contact2096 November 14 at 21:30:31.9 UTC
First Umbral External Contact2096 November 14 at 22:36:23.1 UTC
First Central Line2096 November 14 at 22:39:40.3 UTC
First Umbral Internal Contact2096 November 14 at 22:42:57.9 UTC
First Penumbral Internal Contact2096 November 14 at 23:51:31.4 UTC
Greatest Eclipse2096 November 15 at 00:36:14.8 UTC
Ecliptic Conjunction2096 November 15 at 00:38:40.8 UTC
Equatorial Conjunction2096 November 15 at 00:45:04.6 UTC
Greatest Duration2096 November 15 at 00:52:33.0 UTC
Last Penumbral Internal Contact2096 November 15 at 01:20:44.7 UTC
Last Umbral Internal Contact2096 November 15 at 02:29:25.5 UTC
Last Central Line2096 November 15 at 02:32:43.9 UTC
Last Umbral External Contact2096 November 15 at 02:36:02.1 UTC
Last Penumbral External Contact2096 November 15 at 03:41:56.0 UTC
November 15, 2096 Solar Eclipse Parameters
ParameterValue
Eclipse Magnitude0.92371
Eclipse Obscuration0.85323
Gamma−0.20182
Sun Right Ascension15h25m10.4s
Sun Declination-18°40'58.6"
Sun Semi-Diameter16'10.0"
Sun Equatorial Horizontal Parallax08.9"
Moon Right Ascension15h24m54.6s
Moon Declination-18°51'10.6"
Moon Semi-Diameter14'42.9"
Moon Equatorial Horizontal Parallax0°54'00.1"
ΔT120.5 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. The first and last eclipse in this sequence is separated by one synodic month.

Eclipse season of October–November 2096
October 31
Ascending node (full moon)
 November 15
Descending node (new moon)
 November 29
Ascending node (full moon)
SE2096Nov15A.png
Penumbral lunar eclipse
Lunar Saros 118		 Annular solar eclipse
Solar Saros 144		 Penumbral lunar eclipse
Lunar Saros 156

Eclipses in 2096

Metonic

Tzolkinex

Half-Saros

Tritos

Solar Saros 144

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 144

This eclipse is a part of Saros series 144, repeating every 18 years, 11 days, and containing 70 events. The series started with a partial solar eclipse on April 11, 1736. It contains annular eclipses from July 7, 1880 through August 27, 2565. There are no hybrid or total eclipses in this set. The series ends at member 70 as a partial eclipse on May 5, 2980. 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 will be produced by member 51 at 9 minutes, 52 seconds on December 29, 2168. All eclipses in this series occur at the Moon’s descending node of orbit. [5]

Series members 5–26 occur between 1801 and 2200:
567
SE1808May25P.png
May 25, 1808		 SE1826Jun05P.png
June 5, 1826		 SE1844Jun16P.png
June 16, 1844
8910
SE1862Jun27P.png
June 27, 1862		 SE1880Jul07A.png
July 7, 1880		 SE1898Jul18A.png
July 18, 1898
111213
SE1916Jul30A.png
July 30, 1916 		SE1934Aug10A.png
August 10, 1934 		SE1952Aug20A.png
August 20, 1952
141516
SE1970Aug31A.png
August 31, 1970 		SE1988Sep11A.png
September 11, 1988 		SE2006Sep22A.png
September 22, 2006
171819
SE2024Oct02A.png
October 2, 2024 		SE2042Oct14A.png
October 14, 2042 		SE2060Oct24A.png
October 24, 2060
202122
SE2078Nov04A.png
November 4, 2078 		SE2096Nov15A.png
November 15, 2096 		SE2114Nov27A.png
November 27, 2114
232425
SE2132Dec07A.png
December 7, 2132		 SE2150Dec19A.png
December 19, 2150		 SE2168Dec29A.png
December 29, 2168
26
SE2187Jan09A.png
January 9, 2187

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 June 23, 2047 and November 16, 2134
June 22–23April 10–11January 27–29November 15–16September 3–5
118120122124126
SE2047Jun23P.png
June 23, 2047 		SE2051Apr11P.png
April 11, 2051 		SE2055Jan27P.png
January 27, 2055 		SE2058Nov16P.png
November 16, 2058 		SE2062Sep03P.png
September 3, 2062
128130132134136
SE2066Jun22A.png
June 22, 2066 		SE2070Apr11T.png
April 11, 2070 		SE2074Jan27A.png
January 27, 2074 		SE2077Nov15A.png
November 15, 2077 		SE2081Sep03T.png
September 3, 2081
138140142144146
SE2085Jun22A.png
June 22, 2085 		SE2089Apr10A.png
April 10, 2089 		SE2093Jan27T.png
January 27, 2093 		SE2096Nov15A.png
November 15, 2096 		SE2100Sep04T.png
September 4, 2100
148150152154156
SE2104Jun22T.png
June 22, 2104		 SE2108Apr11P.gif
April 11, 2108		 Saros152 18van70 SE2112Jan29T.jpg
January 29, 2112		 SE2115Nov16A.png
November 16, 2115		 Saros156 07van69 SE2119Sep05P.jpg
September 5, 2119
158160162164
Saros158 04van70 SE2123Jun23P.jpg
June 23, 2123		 Saros164 03van80 SE2134Nov16P.jpg
November 16, 2134

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
SE1802Mar04T.png
March 4, 1802
(Saros 117)		 SE1813Feb01A.gif
February 1, 1813
(Saros 118)		 SE1824Jan01A.gif
January 1, 1824
(Saros 119)		 SE1834Nov30T.gif
November 30, 1834
(Saros 120)		 SE1845Oct30H.png
October 30, 1845
(Saros 121)
SE1856Sep29A.gif
September 29, 1856
(Saros 122)		 SE1867Aug29T.png
August 29, 1867
(Saros 123)		 SE1878Jul29T.png
July 29, 1878
(Saros 124)		 SE1889Jun28A.png
June 28, 1889
(Saros 125)		 SE1900May28T.png
May 28, 1900
(Saros 126)
SE1911Apr28T.png
April 28, 1911
(Saros 127)		 SE1922Mar28A.png
March 28, 1922
(Saros 128)		 SE1933Feb24A.png
February 24, 1933
(Saros 129)		 SE1944Jan25T.png
January 25, 1944
(Saros 130)		 SE1954Dec25A.png
December 25, 1954
(Saros 131)
SE1965Nov23A.png
November 23, 1965
(Saros 132)		 SE1976Oct23T.png
October 23, 1976
(Saros 133)		 SE1987Sep23A.png
September 23, 1987
(Saros 134)		 SE1998Aug22A.png
August 22, 1998
(Saros 135)		 SE2009Jul22T.png
July 22, 2009
(Saros 136)
SE2020Jun21A.png
June 21, 2020
(Saros 137)		 SE2031May21A.png
May 21, 2031
(Saros 138)		 SE2042Apr20T.png
April 20, 2042
(Saros 139)		 SE2053Mar20A.png
March 20, 2053
(Saros 140)		 SE2064Feb17A.png
February 17, 2064
(Saros 141)
SE2075Jan16T.png
January 16, 2075
(Saros 142)		 SE2085Dec16A.png
December 16, 2085
(Saros 143)		 SE2096Nov15A.png
November 15, 2096
(Saros 144)		 SE2107Oct16T.png
October 16, 2107
(Saros 145)		 SE2118Sep15T.png
September 15, 2118
(Saros 146)
SE2129Aug15A.png
August 15, 2129
(Saros 147)		 Saros148 28van75 SE2140Jul14T.jpg
July 14, 2140
(Saros 148)		 Saros149 28van71 SE2151Jun14T.jpg
June 14, 2151
(Saros 149)		 Saros150 25van71 SE2162May14A.jpg
May 14, 2162
(Saros 150)		 Saros151 23van72 SE2173Apr12A.jpg
April 12, 2173
(Saros 151)
Saros152 22van70 SE2184Mar12T.jpg
March 12, 2184
(Saros 152)		 Saros153 19van70 SE2195Feb10A.jpg
February 10, 2195
(Saros 153)

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
SE1807Jun06H.gif
June 6, 1807
(Saros 134)		 SE1836May15A.gif
May 15, 1836
(Saros 135)		 SE1865Apr25T.png
April 25, 1865
(Saros 136)
SE1894Apr06H.gif
April 6, 1894
(Saros 137)		 SE1923Mar17A.png
March 17, 1923
(Saros 138)		 SE1952Feb25T.png
February 25, 1952
(Saros 139)
SE1981Feb04A.png
February 4, 1981
(Saros 140)		 SE2010Jan15A.png
January 15, 2010
(Saros 141)		 SE2038Dec26T.png
December 26, 2038
(Saros 142)
SE2067Dec06H.png
December 6, 2067
(Saros 143)		 SE2096Nov15A.png
November 15, 2096
(Saros 144)		 SE2125Oct26T.png
October 26, 2125
(Saros 145)
SE2154Oct07T.png
October 7, 2154
(Saros 146)		 Saros147 32van80 SE2183Sep16A.jpg
September 16, 2183
(Saros 147)

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<span class="mw-page-title-main">Solar eclipse of July 9, 1926</span> 20th-century annular solar eclipse

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References

  1. ↑ "November 14–15, 2096 Annular Solar Eclipse". timeanddate. Retrieved 25 August 2024.
  2. ↑ "Moon Distances for London, United Kingdom, England". timeanddate. Retrieved 25 August 2024.
  3. ↑ "Annular Solar Eclipse of 2096 Nov 15". EclipseWise.com. Retrieved 25 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 144". eclipse.gsfc.nasa.gov.
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