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February 2036 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 Monday, February 11, 2036,[1] with an umbral magnitude of 1.3007. 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 1.2 days after perigee (on February 10, 2036, at 16:00 UTC), the Moon's apparent diameter will be larger.[2]
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Visibility
The eclipse will be completely visible over Africa, Europe, and west, central, and south Asia, seen rising over much of North and South America and setting over east Asia and Australia.[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 2036
- A total lunar eclipse on February 11.
- A partial solar eclipse on February 27.
- A partial solar eclipse on July 23.
- A total lunar eclipse on August 7.
- A partial solar eclipse on August 21.
Metonic
- Preceded by: Lunar eclipse of April 25, 2032
- Followed by: Lunar eclipse of November 30, 2039
Tzolkinex
- Preceded by: Lunar eclipse of December 31, 2028
- Followed by: Lunar eclipse of March 25, 2043
Half-Saros
- Preceded by: Solar eclipse of February 6, 2027
- Followed by: Solar eclipse of February 16, 2045
Tritos
- Preceded by: Lunar eclipse of March 14, 2025
- Followed by: Lunar eclipse of January 12, 2047
Lunar Saros 124
- Preceded by: Lunar eclipse of January 31, 2018
- Followed by: Lunar eclipse of February 22, 2054
Inex
- Preceded by: Lunar eclipse of March 3, 2007
- Followed by: Lunar eclipse of January 22, 2065
Triad
- Preceded by: Lunar eclipse of April 13, 1949
- Followed by: Lunar eclipse of December 13, 2122
Lunar eclipses of 2035–2038
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 eclipses on June 17, 2038 and December 11, 2038 occur in the next lunar year eclipse set.
Saros 124
This eclipse is a part of Saros series 124, repeating every 18 years, 11 days, and containing 73 events. The series started with a penumbral lunar eclipse on August 17, 1152. It contains partial eclipses from March 21, 1513 through June 15, 1639; total eclipses from June 25, 1657 through April 18, 2144; and a second set of partial eclipses from April 29, 2162 through July 14, 2288. The series ends at member 73 as a penumbral eclipse on October 21, 2450.
The longest duration of totality was produced by member 39 at 101 minutes, 27 seconds on August 30, 1765. 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 131.
February 6, 2027 | February 16, 2045 |
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Notes
External links
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