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November 2020 lunar eclipse
Penumbral lunar eclipse of 30 November 2020 From Wikipedia, the free encyclopedia
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A penumbral lunar eclipse occurred at the Moon’s ascending node of orbit on Monday, November 30, 2020,[1] with an umbral magnitude of −0.2602. A lunar eclipse occurs when the Moon moves into the Earth's shadow, causing the Moon to be darkened. A penumbral lunar eclipse occurs when part or all of the Moon's near side passes into 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 3.6 days after apogee (on November 26, 2020, at 19:30 UTC), the Moon's apparent diameter was smaller.[2]
This eclipse was the last of four penumbral lunar eclipses in 2020, with the others occurring on January 10, June 5, and July 5.
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Visibility
The eclipse was completely visible over northeast Asia and North America, seen rising over east Asia and Australia and setting over South America.[3]
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Gallery
- Minneapolis, 1:45 UT and 9:24 UT
- 9:40 UT
Eclipse details
Shown below is a table displaying details about this particular solar eclipse. It describes various parameters pertaining to this eclipse.[4]
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.
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Related eclipses
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Eclipses in 2020
- A penumbral lunar eclipse on January 10.
- A penumbral lunar eclipse on June 5.
- An annular solar eclipse on June 21.
- A penumbral lunar eclipse on July 5.
- A penumbral lunar eclipse on November 30.
- A total solar eclipse on December 14.
Metonic
- Preceded by: Lunar eclipse of February 11, 2017
- Followed by: Lunar eclipse of September 18, 2024
Tzolkinex
- Preceded by: Lunar eclipse of October 18, 2013
- Followed by: Lunar eclipse of January 12, 2028
Half-Saros
- Preceded by: Solar eclipse of November 25, 2011
- Followed by: Solar eclipse of December 5, 2029
Tritos
- Preceded by: Lunar eclipse of December 31, 2009
- Followed by: Lunar eclipse of October 30, 2031
Lunar Saros 116
- Preceded by: Lunar eclipse of November 20, 2002
- Followed by: Lunar eclipse of December 11, 2038
Inex
- Preceded by: Lunar eclipse of December 21, 1991
- Followed by: Lunar eclipse of November 9, 2049
Triad
- Preceded by: Lunar eclipse of January 30, 1934
- Followed by: Lunar eclipse of October 2, 2107
Lunar eclipses of 2020–2023
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 10, 2020 and July 5, 2020 occur in the previous lunar year eclipse set.
Saros 116
This eclipse is a part of Saros series 116, repeating every 18 years, 11 days, and containing 73 events. The series started with a penumbral lunar eclipse on March 11, 993 AD. It contains partial eclipses from June 16, 1155 through September 11, 1299; total eclipses from September 21, 1317 through July 11, 1786; and a second set of partial eclipses from July 22, 1804 through October 7, 1930. The series ends at member 73 as a penumbral eclipse on May 14, 2291.
The longest duration of totality was produced by member 40 at 102 minutes, 40 seconds on May 16, 1696. 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 partial solar eclipses of Solar Saros 123.
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See also
References
External links
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