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October 2032 lunar eclipse
Astronomical event From Wikipedia, the free encyclopedia
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A total lunar eclipse will occur at the Moon’s descending node of orbit on Monday, October 18, 2032,[1] with an umbral magnitude of 1.1039. 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 2.1 days after perigee (on October 16, 2032, at 17:25 UTC), the Moon's apparent diameter will be larger.[2]
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This lunar eclipse is the second of a tetrad, with four total lunar eclipses in series, the others being on April 25, 2032; April 14, 2033; and October 8, 2033.
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Visibility
The eclipse will be completely visible over east Africa, Europe, and Asia, seen rising over west Africa and eastern South America and setting over Australia and the western Pacific Ocean.[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 2032
- A total lunar eclipse on April 25.
- An annular solar eclipse on May 9.
- A total lunar eclipse on October 18.
- A partial solar eclipse on November 3.
Metonic
- Preceded by: Lunar eclipse of December 31, 2028
- Followed by: Lunar eclipse of August 7, 2036
Tzolkinex
- Preceded by: Lunar eclipse of September 7, 2025
- Followed by: Lunar eclipse of November 30, 2039
Half-Saros
- Preceded by: Solar eclipse of October 14, 2023
- Followed by: Solar eclipse of October 25, 2041
Tritos
- Preceded by: Lunar eclipse of November 19, 2021
- Followed by: Lunar eclipse of September 19, 2043
Lunar Saros 127
- Preceded by: Lunar eclipse of October 8, 2014
- Followed by: Lunar eclipse of October 30, 2050
Inex
- Preceded by: Lunar eclipse of November 9, 2003
- Followed by: Lunar eclipse of September 29, 2061
Triad
- Preceded by: Lunar eclipse of December 19, 1945
- Followed by: Lunar eclipse of August 20, 2119
Lunar eclipses of 2031–2034
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 5, 2031 occurs in the previous lunar year eclipse set.
Saros 127
This eclipse is a part of Saros series 127, repeating every 18 years, 11 days, and containing 72 events. The series started with a penumbral lunar eclipse on July 9, 1275. It contains partial eclipses from November 4, 1473 through May 18, 1780; total eclipses from May 29, 1798 through November 9, 2068; and a second set of partial eclipses from November 20, 2086 through June 17, 2429. The series ends at member 72 as a penumbral eclipse on September 2, 2555.
The longest duration of totality was produced by member 35 at 101 minutes, 46 seconds on July 23, 1888. All eclipses in this series occur at the Moon’s descending 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 partial solar eclipses of Solar Saros 134.
October 14, 2023 | October 25, 2041 |
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See also
Notes
External links
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