Solar eclipse of November 27, 2095
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 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]
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]
| Event | Time (UTC) |
|---|---|
| First Penumbral External Contact | 2095 November 26 at 22:08:18.5 UTC |
| First Umbral External Contact | 2095 November 26 at 23:17:51.3 UTC |
| First Central Line | 2095 November 26 at 23:21:03.1 UTC |
| First Umbral Internal Contact | 2095 November 26 at 23:24:16.3 UTC |
| Equatorial Conjunction | 2095 November 27 at 00:46:21.1 UTC |
| Ecliptic Conjunction | 2095 November 27 at 00:57:09.8 UTC |
| Greatest Eclipse | 2095 November 27 at 01:02:57.4 UTC |
| Greatest Duration | 2095 November 27 at 01:13:24.5 UTC |
| Last Umbral Internal Contact | 2095 November 27 at 02:41:51.2 UTC |
| Last Central Line | 2095 November 27 at 02:45:02.1 UTC |
| Last Umbral External Contact | 2095 November 27 at 02:48:11.5 UTC |
| Last Penumbral External Contact | 2095 November 27 at 03:57:38.7 UTC |
| Parameter | Value |
|---|---|
| Eclipse Magnitude | 0.93303 |
| Eclipse Obscuration | 0.87054 |
| Gamma | 0.49030 |
| Sun Right Ascension | 16h12m24.6s |
| Sun Declination | -21°07'41.4" |
| Sun Semi-Diameter | 16'12.2" |
| Sun Equatorial Horizontal Parallax | 08.9" |
| Moon Right Ascension | 16h12m56.4s |
| Moon Declination | -20°41'58.0" |
| Moon Semi-Diameter | 14'55.2" |
| Moon Equatorial Horizontal Parallax | 0°54'45.3" |
| ΔT | 119.6 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.
| November 27 Descending node (new moon) |
December 11 Ascending node (full moon) |
|---|---|
| File:SE2095Nov27A.png | |
| Annular solar eclipse Solar Saros 134 |
Partial lunar eclipse Lunar Saros 146 |
Related eclipses
Eclipses in 2095
- A total solar eclipse on June 2.
- A partial lunar eclipse on June 17.
- An annular solar eclipse on November 27.
- A partial lunar eclipse on December 11.
Metonic
- Preceded by: Solar eclipse of February 7, 2092
- Followed by: Solar eclipse of September 14, 2099
Tzolkinex
- Preceded by: Solar eclipse of October 14, 2088
- Followed by: Solar eclipse of January 8, 2103
Half-Saros
- Preceded by: Lunar eclipse of November 20, 2086
- Followed by: Lunar eclipse of December 2, 2104
Tritos
- Preceded by: Solar eclipse of December 27, 2084
- Followed by: Solar eclipse of October 26, 2106
Solar Saros 134
- Preceded by: Solar eclipse of November 15, 2077
- Followed by: Solar eclipse of December 8, 2113
Inex
- Preceded by: Solar eclipse of December 17, 2066
- Followed by: Solar eclipse of November 6, 2124
Triad
- Preceded by: Solar eclipse of January 26, 2009
- Followed by: Solar eclipse of September 27, 2182
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 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: | ||
|---|---|---|
| 32 | 33 | 34 |
| File:SE1807Jun06H.png June 6, 1807 |
File:SE1825Jun16H.png June 16, 1825 |
File:SE1843Jun27H.png June 27, 1843 |
| 35 | 36 | 37 |
| File:SE1861Jul08A.png July 8, 1861 |
File:SE1879Jul19A.png July 19, 1879 |
File:SE1897Jul29A.png July 29, 1897 |
| 38 | 39 | 40 |
| File:SE1915Aug10A.png August 10, 1915 |
File:SE1933Aug21A.png August 21, 1933 |
File:SE1951Sep01A.png September 1, 1951 |
| 41 | 42 | 43 |
| File:SE1969Sep11A.png September 11, 1969 |
File:SE1987Sep23A.png September 23, 1987 |
File:SE2005Oct03A.png October 3, 2005 |
| 44 | 45 | 46 |
| File:SE2023Oct14A.png October 14, 2023 |
File:SE2041Oct25A.png October 25, 2041 |
File:SE2059Nov05A.png November 5, 2059 |
| 47 | 48 | 49 |
| File:SE2077Nov15A.png November 15, 2077 |
File:SE2095Nov27A.png November 27, 2095 |
File:SE2113Dec08A.png December 8, 2113 |
| 50 | 51 | 52 |
| File:SE2131Dec19A.png December 19, 2131 |
File:SE2149Dec30A.png December 30, 2149 |
File:SE2168Jan10A.png January 10, 2168 |
| 53 | ||
| File:SE2186Jan20A.png January 20, 2186 | ||
Metonic series
Template:Solar Metonic series 2065–2152
Tritos series
Template:Solar Tritos series 2008 August 1
Inex series
Template:Solar Inex series 2009 January 26
Notes
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References
- Earth visibility chart and eclipse statistics Eclipse Predictions by Fred Espenak, NASA/GSFC
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