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April 2051 lunar eclipse
Astronomical event From Wikipedia, the free encyclopedia
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A total lunar eclipse will occur at the Moon’s ascending node of orbit on Wednesday, April 26, 2051,[1] with an umbral magnitude of 1.2034. A lunar eclipse occurs when the Moon moves into the Earth's shadow, causing the Moon to be darkened. A total lunar eclipse occurs when the Moon's near side entirely passes into the Earth's umbral shadow. Unlike a solar eclipse, which can only be viewed from a relatively small area of the world, a lunar eclipse may be viewed from anywhere on the night side of Earth. A total lunar eclipse can last up to nearly two hours, while a total solar eclipse lasts only a few minutes at any given place, because the Moon's shadow is smaller. Occurring about 2.6 days after apogee (on April 23, 2051, at 12:00 UTC), the Moon's apparent diameter will be smaller.[2]
This lunar eclipse is the third of a tetrad, with four total lunar eclipses in series, the others being on May 6, 2050; October 30, 2050; and October 19, 2051.
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Visibility
The eclipse will be completely visible over South America and west Africa, seen rising over North America and the eastern Pacific Ocean and setting over central and east Africa, Europe, and west, central, and south Asia.[3]
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Eclipse details
Shown below is a table displaying details about this particular solar eclipse. It describes various parameters pertaining to this eclipse.[4]
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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.
Related eclipses
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Eclipses in 2051
- A partial solar eclipse on April 11.
- A total lunar eclipse on April 26.
- A partial solar eclipse on October 4.
- A total lunar eclipse on October 19.
Metonic
- Preceded by: Lunar eclipse of July 7, 2047
- Followed by: Lunar eclipse of February 11, 2055
Tzolkinex
- Preceded by: Lunar eclipse of March 13, 2044
- Followed by: Lunar eclipse of June 6, 2058
Half-Saros
- Preceded by: Solar eclipse of April 20, 2042
- Followed by: Solar eclipse of April 30, 2060
Tritos
- Preceded by: Lunar eclipse of May 26, 2040
- Followed by: Lunar eclipse of March 25, 2062
Lunar Saros 132
- Preceded by: Lunar eclipse of April 14, 2033
- Followed by: Lunar eclipse of May 6, 2069
Inex
- Preceded by: Lunar eclipse of May 16, 2022
- Followed by: Lunar eclipse of April 4, 2080
Triad
- Preceded by: Lunar eclipse of June 25, 1964
- Followed by: Lunar eclipse of February 24, 2138
Lunar eclipses of 2049–2052
This eclipse is a member of a semester series. An eclipse in a semester series of lunar eclipses repeats approximately every 177 days and 4 hours (a semester) at alternating nodes of the Moon's orbit.[5]
The penumbral lunar eclipse on June 15, 2049 occurs in the previous lunar year eclipse set.
Saros 132
This eclipse is a part of Saros series 132, repeating every 18 years, 11 days, and containing 71 events. The series started with a penumbral lunar eclipse on May 12, 1492. It contains partial eclipses from August 16, 1636 through March 24, 1997; total eclipses from April 4, 2015 through August 2, 2213; and a second set of partial eclipses from August 13, 2231 through November 30, 2411. The series ends at member 71 as a penumbral eclipse on June 26, 2754.
The longest duration of totality will be produced by member 36 at 106 minutes, 6 seconds on June 9, 2123. All eclipses in this series occur at the Moon’s ascending node of orbit.[6]
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.
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
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.
Half-Saros cycle
A lunar eclipse will be preceded and followed by solar eclipses by 9 years and 5.5 days (a half saros).[8] This lunar eclipse is related to two total solar eclipses of Solar Saros 139.
April 20, 2042 | April 30, 2060 |
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See also
Notes
External links
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