Solar eclipse of November 15, 2096

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Template:Short description Script error: No such module "Solar eclipse". 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]

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
Event Time (UTC)
First Penumbral External Contact 2096 November 14 at 21:30:31.9 UTC
First Umbral External Contact 2096 November 14 at 22:36:23.1 UTC
First Central Line 2096 November 14 at 22:39:40.3 UTC
First Umbral Internal Contact 2096 November 14 at 22:42:57.9 UTC
First Penumbral Internal Contact 2096 November 14 at 23:51:31.4 UTC
Greatest Eclipse 2096 November 15 at 00:36:14.8 UTC
Ecliptic Conjunction 2096 November 15 at 00:38:40.8 UTC
Equatorial Conjunction 2096 November 15 at 00:45:04.6 UTC
Greatest Duration 2096 November 15 at 00:52:33.0 UTC
Last Penumbral Internal Contact 2096 November 15 at 01:20:44.7 UTC
Last Umbral Internal Contact 2096 November 15 at 02:29:25.5 UTC
Last Central Line 2096 November 15 at 02:32:43.9 UTC
Last Umbral External Contact 2096 November 15 at 02:36:02.1 UTC
Last Penumbral External Contact 2096 November 15 at 03:41:56.0 UTC
November 15, 2096 Solar Eclipse Parameters
Parameter Value
Eclipse Magnitude 0.92371
Eclipse Obscuration 0.85323
Gamma −0.20182
Sun Right Ascension 15h25m10.4s
Sun Declination -18°40'58.6"
Sun Semi-Diameter 16'10.0"
Sun Equatorial Horizontal Parallax 08.9"
Moon Right Ascension 15h24m54.6s
Moon Declination -18°51'10.6"
Moon Semi-Diameter 14'42.9"
Moon Equatorial Horizontal Parallax 0°54'00.1"
ΔT 120.5 s

Eclipse season

Script error: No such module "Labelled list hatnote". 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)
File:SE2096Nov15A.png
Penumbral lunar eclipse
Lunar Saros 118
Annular solar eclipse
Solar Saros 144
Penumbral lunar eclipse
Lunar Saros 156

Related eclipses

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
Saros Map Gamma Saros Map Gamma
119 June 13, 2094
File:SE2094Jun13P.png
Partial
−1.4613 124 December 7, 2094
File:SE2094Dec07P.png
Partial
1.1547
129 June 2, 2095
File:SE2095Jun02T.png
Total
−0.6396 134 November 27, 2095
File:SE2095Nov27A.png
Annular
0.4903
139 May 22, 2096
File:SE2096May22T.png
Total
0.1196 144 November 15, 2096
File:SE2096Nov15A.png
Annular
−0.20
149 May 11, 2097
File:SE2097May11T.png
Total
0.8516 154 November 4, 2097
File:SE2097Nov04A.png
Annular
−0.8926
159 May 1, 2098 164 October 24, 2098
File:SE2098Oct24P.png
Partial
−1.5407

Saros 144

Template:Solar Saros series 144

Metonic series

Template:Solar Metonic series 2047–2134

Tritos series

Template:Solar Tritos series 2009 July 22

Inex series

Template:Solar Inex series 2010 January 15

References

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  3. ↑ Script error: No such module "citation/CS1".
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External links

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