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November 2039 lunar eclipse
Astronomical event From Wikipedia, the free encyclopedia
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A partial lunar eclipse will occur at the Moon’s ascending node of orbit on Wednesday, November 30, 2039,[1] with an umbral magnitude of 0.9443. A lunar eclipse occurs when the Moon moves into the Earth's shadow, causing the Moon to be darkened. A partial lunar eclipse occurs when one part of the Moon is in the Earth's umbra, while the other part is in the Earth's penumbra. 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. Occurring about 1.8 days before apogee (on December 2, 2039, at 11:10 UTC), the Moon's apparent diameter will be smaller.[2]
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Visibility
The eclipse will be completely visible over northern Europe, Asia, and Australia, seen rising over Africa and western Europe and setting over the central Pacific Ocean and western North America.[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 2039
- A partial lunar eclipse on June 6.
- An annular solar eclipse on June 21.
- A partial lunar eclipse on November 30.
- A total solar eclipse on December 15.
Metonic
- Preceded by: Lunar eclipse of February 11, 2036
- Followed by: Lunar eclipse of September 19, 2043
Tzolkinex
- Preceded by: Lunar eclipse of October 18, 2032
- Followed by: Lunar eclipse of January 12, 2047
Half-Saros
- Preceded by: Solar eclipse of November 25, 2030
- Followed by: Solar eclipse of December 5, 2048
Tritos
- Preceded by: Lunar eclipse of December 31, 2028
- Followed by: Lunar eclipse of October 30, 2050
Lunar Saros 126
- Preceded by: Lunar eclipse of November 19, 2021
- Followed by: Lunar eclipse of December 11, 2057
Inex
- Preceded by: Lunar eclipse of December 21, 2010
- Followed by: Lunar eclipse of November 9, 2068
Triad
- Preceded by: Lunar eclipse of January 29, 1953
- Followed by: Lunar eclipse of October 1, 2126
Lunar eclipses of 2038–2042
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 January 21, 2038 and July 16, 2038 occur in the previous lunar year eclipse set, and the penumbral lunar eclipses on April 5, 2042 and September 29, 2042 occur in the next lunar year eclipse set.
Saros 126
This eclipse is a part of Saros series 126, repeating every 18 years, 11 days, and containing 70 events. The series started with a penumbral lunar eclipse on July 18, 1228. It contains partial eclipses from March 24, 1625 through June 9, 1751; total eclipses from June 19, 1769 through November 9, 2003; and a second set of partial eclipses from November 19, 2021 through June 5, 2346. The series ends at member 70 as a penumbral eclipse on August 19, 2472.
The longest duration of totality was produced by member 36 at 106 minutes, 27 seconds on August 13, 1859. 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 133.
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See also
Notes
External links
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