Solar eclipse of January 5, 2057
Template:Short description Script error: No such module "Solar eclipse". A total solar eclipse will occur at the Moon's descending node of orbit on Friday, January 5, 2057,[1] with a magnitude of 1.0287. 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 1.6 days after perigee (on January 3, 2057, at 20:00 UTC), the Moon's apparent diameter will be larger.[2]
This eclipse and May 20, 2050 are the next two total solar eclipses in which the Moon's shadow will trace a path that fails to hit land anywhere on Earth. Totality will begin 125 miles east of Belmonte in Brazil, then traverse southeast through the Atlantic Ocean where it will miss the Cape of Good Hope in South Africa by 250 miles, before winding northeast and concluding in the Indian Ocean 500 miles south of Java island. However, a partial solar eclipse will be visible for parts of eastern South America, Southern Africa, Antarctica, Southeast Asia, and western Australia.
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 | 2057 January 5 at 07:08:52.7 UTC |
| First Umbral External Contact | 2057 January 5 at 08:06:59.9 UTC |
| First Central Line | 2057 January 5 at 08:07:21.4 UTC |
| First Umbral Internal Contact | 2057 January 5 at 08:07:42.8 UTC |
| First Penumbral Internal Contact | 2057 January 5 at 09:10:27.5 UTC |
| Greatest Duration | 2057 January 5 at 09:46:16.1 UTC |
| Equatorial Conjunction | 2057 January 5 at 09:47:23.0 UTC |
| Greatest Eclipse | 2057 January 5 at 09:47:52.2 UTC |
| Ecliptic Conjunction | 2057 January 5 at 09:50:49.8 UTC |
| Last Penumbral Internal Contact | 2057 January 5 at 10:25:16.8 UTC |
| Last Umbral Internal Contact | 2057 January 5 at 11:28:04.0 UTC |
| Last Central Line | 2057 January 5 at 11:28:23.7 UTC |
| Last Umbral External Contact | 2057 January 5 at 11:28:43.3 UTC |
| Last Penumbral External Contact | 2057 January 5 at 12:26:55.7 UTC |
| Parameter | Value |
|---|---|
| Eclipse Magnitude | 1.02873 |
| Eclipse Obscuration | 1.05829 |
| Gamma | −0.28370 |
| Sun Right Ascension | 19h07m25.3s |
| Sun Declination | -22°31'37.8" |
| Sun Semi-Diameter | 16'15.9" |
| Sun Equatorial Horizontal Parallax | 08.9" |
| Moon Right Ascension | 19h07m26.6s |
| Moon Declination | -22°48'43.6" |
| Moon Semi-Diameter | 16'27.8" |
| Moon Equatorial Horizontal Parallax | 1°00'25.4" |
| ΔT | 88.4 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 22 Ascending node (full moon) |
January 5 Descending node (new moon) |
|---|---|
| File:Lunar eclipse chart close-2056Dec22.png | File:SE2057Jan05T.png |
| Penumbral lunar eclipse Lunar Saros 116 |
Total solar eclipse Solar Saros 142 |
Related eclipses
Eclipses in 2057
- A total solar eclipse on January 5.
- A partial lunar eclipse on June 17.
- An annular solar eclipse on July 1.
- A partial lunar eclipse on December 11.
- A total solar eclipse on December 26.
Metonic
- Preceded by: Solar eclipse of March 20, 2053
- Followed by: Solar eclipse of October 24, 2060
Tzolkinex
- Preceded by: Solar eclipse of November 25, 2049
- Followed by: Solar eclipse of February 17, 2064
Half-Saros
- Preceded by: Lunar eclipse of January 1, 2048
- Followed by: Lunar eclipse of January 11, 2066
Tritos
- Preceded by: Solar eclipse of February 5, 2046
- Followed by: Solar eclipse of December 6, 2067
Solar Saros 142
- Preceded by: Solar eclipse of December 26, 2038
- Followed by: Solar eclipse of January 16, 2075
Inex
- Preceded by: Solar eclipse of January 26, 2028
- Followed by: Solar eclipse of December 16, 2085
Triad
- Preceded by: Solar eclipse of March 7, 1970
- Followed by: Solar eclipse of November 7, 2143
Solar eclipses of 2054–2058
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 March 9, 2054 and September 2, 2054 occur in the previous lunar year eclipse set, and the partial solar eclipses on May 22, 2058 and November 16, 2058 occur in the next lunar year eclipse set.
| Solar eclipse series sets from 2054 to 2058 | ||||||
|---|---|---|---|---|---|---|
| Ascending node | Descending node | |||||
| Saros | Map | Gamma | Saros | Map | Gamma | |
| 117 | August 3, 2054 File:SE2054Aug03P.png Partial |
−1.4941 | 122 | January 27, 2055 File:SE2055Jan27P.png Partial |
1.155 | |
| 127 | July 24, 2055 File:SE2055Jul24T.png Total |
−0.8012 | 132 | January 16, 2056 File:SE2056Jan16A.png Annular |
0.4199 | |
| 137 | July 12, 2056 File:SE2056Jul12A.png Annular |
−0.0426 | 142 | January 5, 2057 File:SE2057Jan05T.png Total |
−0.2837 | |
| 147 | July 1, 2057 File:SE2057Jul01A.png Annular |
0.7455 | 152 | December 26, 2057 File:SE2057Dec26T.png Total |
−0.9405 | |
| 157 | June 21, 2058 File:SE2058Jun21P.png Partial |
1.4869 | ||||
Saros 142
This eclipse is a part of Saros series 142, repeating every 18 years, 11 days, and containing 72 events. The series started with a partial solar eclipse on April 17, 1624. It contains a hybrid eclipse on July 14, 1768, and total eclipses from July 25, 1786 through October 29, 2543. There are no annular eclipses in this set. The series ends at member 72 as a partial eclipse on June 5, 2904. 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 will be produced by member 38 at 6 minutes, 34 seconds on May 28, 2291. All eclipses in this series occur at the Moon’s descending node of orbit.[5]
| Series members 11–32 occur between 1801 and 2200: | ||
|---|---|---|
| 11 | 12 | 13 |
| File:SE1804Aug05T.png August 5, 1804 |
File:SE1822Aug16T.png August 16, 1822 |
File:SE1840Aug27T.png August 27, 1840 |
| 14 | 15 | 16 |
| File:SE1858Sep07T.png September 7, 1858 |
File:SE1876Sep17T.png September 17, 1876 |
File:SE1894Sep29T.png September 29, 1894 |
| 17 | 18 | 19 |
| File:SE1912Oct10T.png October 10, 1912 |
File:SE1930Oct21T.png October 21, 1930 |
File:SE1948Nov01T.png November 1, 1948 |
| 20 | 21 | 22 |
| File:SE1966Nov12T.png November 12, 1966 |
File:SE1984Nov22T.png November 22, 1984 |
File:SE2002Dec04T.png December 4, 2002 |
| 23 | 24 | 25 |
| File:SE2020Dec14T.png December 14, 2020 |
File:SE2038Dec26T.png December 26, 2038 |
File:SE2057Jan05T.png January 5, 2057 |
| 26 | 27 | 28 |
| File:SE2075Jan16T.png January 16, 2075 |
File:SE2093Jan27T.png January 27, 2093 |
File:SE2111Feb08T.png February 8, 2111 |
| 29 | 30 | 31 |
| File:SE2129Feb18T.png February 18, 2129 |
File:SE2147Mar02T.png March 2, 2147 |
File:SE2165Mar12T.png March 12, 2165 |
| 32 | ||
| File:SE2183Mar23T.png March 23, 2183 | ||
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.
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.
Inex series
Template:Solar Inex series 2028 January 26
References
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External links
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