Solar eclipse of December 17, 2066
Template:Short description Script error: No such module "Solar eclipse". A total solar eclipse will occur at the Moon's ascending node of orbit between Thursday, December 16 and Friday, December 17, 2066,[1] with a magnitude of 1.0416. 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. A total solar eclipse occurs when the Moon's apparent diameter is larger than the Sun's, blocking all direct sunlight, turning day into darkness. Totality occurs in a narrow path across Earth's surface, with the partial solar eclipse visible over a surrounding region thousands of kilometres wide. Occurring about 18.5 hours before perigee (on December 17, 2066, at 19:00 UTC), the Moon's apparent diameter will be larger.[2]
The path of totality will be visible from parts of southwestern Australia and Stewart Island of New Zealand. A partial solar eclipse will also be visible for parts of Indonesia, Australia, Antarctica, and Oceania.
This total eclipse follows a similar path to the eclipse on December 25–26, 2038.
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 | 2066 December 16 at 21:49:58.3 UTC |
| First Umbral External Contact | 2066 December 16 at 22:48:21.3 UTC |
| First Central Line | 2066 December 16 at 22:49:05.7 UTC |
| First Umbral Internal Contact | 2066 December 16 at 22:49:50.2 UTC |
| First Penumbral Internal Contact | 2066 December 17 at 00:01:22.6 UTC |
| Ecliptic Conjunction | 2066 December 17 at 00:19:30.7 UTC |
| Equatorial Conjunction | 2066 December 17 at 00:20:59.4 UTC |
| Greatest Duration | 2066 December 17 at 00:23:31.6 UTC |
| Greatest Eclipse | 2066 December 17 at 00:23:39.9 UTC |
| Last Penumbral Internal Contact | 2066 December 17 at 00:46:01.7 UTC |
| Last Umbral Internal Contact | 2066 December 17 at 01:57:30.4 UTC |
| Last Central Line | 2066 December 17 at 01:58:15.8 UTC |
| Last Umbral External Contact | 2066 December 17 at 01:59:01.2 UTC |
| Last Penumbral External Contact | 2066 December 17 at 02:57:20.6 UTC |
| Parameter | Value |
|---|---|
| Eclipse Magnitude | 1.04155 |
| Eclipse Obscuration | 1.08483 |
| Gamma | −0.40428 |
| Sun Right Ascension | 17h39m46.4s |
| Sun Declination | -23°20'56.0" |
| Sun Semi-Diameter | 16'15.1" |
| Sun Equatorial Horizontal Parallax | 08.9" |
| Moon Right Ascension | 17h39m53.3s |
| Moon Declination | -23°45'32.9" |
| Moon Semi-Diameter | 16'39.9" |
| Moon Equatorial Horizontal Parallax | 1°01'09.6" |
| ΔT | 95.3 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.
| December 17 Ascending node (new moon) |
December 31 Descending node (full moon) |
|---|---|
| File:SE2066Dec17T.png | |
| Total solar eclipse Solar Saros 133 |
Penumbral lunar eclipse Lunar Saros 145 |
Related eclipses
Eclipses in 2066
- A total lunar eclipse on January 11.
- An annular solar eclipse on June 22.
- A partial lunar eclipse on July 7.
- A total solar eclipse on December 17.
- A penumbral lunar eclipse on December 31.
Metonic
- Preceded by: Solar eclipse of February 28, 2063
- Followed by: Solar eclipse of October 4, 2070
Tzolkinex
- Preceded by: Solar eclipse of November 5, 2059
- Followed by: Solar eclipse of January 27, 2074
Half-Saros
- Preceded by: Lunar eclipse of December 11, 2057
- Followed by: Lunar eclipse of December 22, 2075
Tritos
- Preceded by: Solar eclipse of January 16, 2056
- Followed by: Solar eclipse of November 15, 2077
Solar Saros 133
- Preceded by: Solar eclipse of December 5, 2048
- Followed by: Solar eclipse of December 27, 2084
Inex
- Preceded by: Solar eclipse of January 5, 2038
- Followed by: Solar eclipse of November 27, 2095
Triad
- Preceded by: Solar eclipse of February 16, 1980
- Followed by: Solar eclipse of October 17, 2153
Solar eclipses of 2065–2069
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 eclipses on February 5, 2065 and August 2, 2065 occur in the previous lunar year eclipse set, and the partial solar eclipses on April 21, 2069 and October 15, 2069 occur in the next lunar year eclipse set.
| Solar eclipse series sets from 2065 to 2069 | ||||||
|---|---|---|---|---|---|---|
| Descending node | Ascending node | |||||
| Saros | Map | Gamma | Saros | Map | Gamma | |
| 118 | July 3, 2065 File:SE2065Jul03P.png Partial |
1.4619 | 123 | December 27, 2065 File:SE2065Dec27P.png Partial |
−1.0688 | |
| 128 | June 22, 2066 File:SE2066Jun22A.png Annular |
0.733 | 133 | December 17, 2066 File:SE2066Dec17T.png Total |
−0.4043 | |
| 138 | June 11, 2067 File:SE2067Jun11A.png Annular |
−0.0387 | 143 | December 6, 2067 File:SE2067Dec06H.png Hybrid |
0.2845 | |
| 148 | May 31, 2068 File:SE2068May31T.png Total |
−0.797 | 153 | November 24, 2068 File:SE2068Nov24P.png Partial |
1.0299 | |
| 158 | May 20, 2069 File:SE2069May20P.png Partial |
−1.4852 | ||||
Saros 133
This eclipse is a part of Saros series 133, repeating every 18 years, 11 days, and containing 72 events. The series started with a partial solar eclipse on July 13, 1219. It contains annular eclipses from November 20, 1435 through January 13, 1526; a hybrid eclipse on January 24, 1544; and total eclipses from February 3, 1562 through June 21, 2373. The series ends at member 72 as a partial eclipse on September 5, 2499. 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 25 at 1 minutes, 14 seconds on November 30, 1453, and the longest duration of totality was produced by member 61 at 6 minutes, 50 seconds on August 7, 1850. All eclipses in this series occur at the Moon’s ascending node of orbit.[5]
| Series members 34–55 occur between 1801 and 2200: | ||
|---|---|---|
| 34 | 35 | 36 |
| File:SE1814Jul17T.png July 17, 1814 |
File:SE1832Jul27T.png July 27, 1832 |
File:SE1850Aug07T.png August 7, 1850 |
| 37 | 38 | 39 |
| File:SE1868Aug18T.png August 18, 1868 |
File:SE1886Aug29T.png August 29, 1886 |
File:SE1904Sep09T.png September 9, 1904 |
| 40 | 41 | 42 |
| File:SE1922Sep21T.png September 21, 1922 |
File:SE1940Oct01T.png October 1, 1940 |
File:SE1958Oct12T.png October 12, 1958 |
| 43 | 44 | 45 |
| File:SE1976Oct23T.png October 23, 1976 |
File:SE1994Nov03T.png November 3, 1994 |
File:SE2012Nov13T.png November 13, 2012 |
| 46 | 47 | 48 |
| File:SE2030Nov25T.png November 25, 2030 |
File:SE2048Dec05T.png December 5, 2048 |
File:SE2066Dec17T.png December 17, 2066 |
| 49 | 50 | 51 |
| File:SE2084Dec27T.png December 27, 2084 |
File:SE2103Jan08T.png January 8, 2103 |
File:SE2121Jan19T.png January 19, 2121 |
| 52 | 53 | 54 |
| File:SE2139Jan30T.png January 30, 2139 |
File:SE2157Feb09T.png February 9, 2157 |
File:SE2175Feb21T.png February 21, 2175 |
| 55 | ||
| File:SE2193Mar03T.png March 3, 2193 | ||
Metonic series
Template:Solar Metonic series 2036–2112
Tritos series
Template:Solar Tritos series 2001 June 21
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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