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June 2058 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 Thursday, June 6, 2058,[1] with an umbral magnitude of 1.6628. It will be a central lunar eclipse, in which part of the Moon will pass through the center of the Earth's shadow. 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 1.6 days before perigee (on June 8, 2058, at 9:30 UTC), the Moon's apparent diameter will be larger.[2]
During the eclipse, IC 4634 will be occulted by the Moon over Antarctica. Deep-sky objects are rarely occulted during a total eclipse from any given spot on Earth.[3]: 161
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Visibility
The eclipse will be completely visible over east Africa, Antarctica, west, central, and south Asia, and western Australia, seen rising over west Africa, Europe, and eastern South America and setting over east Asia and eastern Australia.[4]
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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.[5]
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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. The first and last eclipse in this sequence is separated by one synodic month.
Related eclipses
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Eclipses in 2058
- A partial solar eclipse on May 22.
- A total lunar eclipse on June 6.
- A partial solar eclipse on June 21.
- A partial solar eclipse on November 16.
- A total lunar eclipse on November 30.
Metonic
- Preceded by: Lunar eclipse of August 18, 2054
- Followed by: Lunar eclipse of March 25, 2062
Tzolkinex
- Preceded by: Lunar eclipse of April 26, 2051
- Followed by: Lunar eclipse of July 17, 2065
Half-Saros
- Preceded by: Solar eclipse of May 31, 2049
- Followed by: Solar eclipse of June 11, 2067
Tritos
- Preceded by: Lunar eclipse of July 7, 2047
- Followed by: Lunar eclipse of May 6, 2069
Lunar Saros 131
- Preceded by: Lunar eclipse of May 26, 2040
- Followed by: Lunar eclipse of June 17, 2076
Inex
- Preceded by: Lunar eclipse of June 26, 2029
- Followed by: Lunar eclipse of May 17, 2087
Triad
- Preceded by: Lunar eclipse of August 6, 1971
- Followed by: Lunar eclipse of April 7, 2145
Lunar eclipses of 2056–2060
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.[6]
The penumbral lunar eclipses on February 1, 2056 and July 26, 2056 occur in the previous lunar year eclipse set, and the penumbral lunar eclipses on April 15, 2060 and October 9, 2060 occur in the next lunar year eclipse set.
Saros 131
This eclipse is a part of Saros series 131, repeating every 18 years, 11 days, and containing 72 events. The series started with a penumbral lunar eclipse on May 10, 1427. It contains partial eclipses from July 25, 1553 through March 22, 1932; total eclipses from April 2, 1950 through September 3, 2202; and a second set of partial eclipses from September 13, 2220 through April 9, 2563. The series ends at member 72 as a penumbral eclipse on July 7, 2707.
The longest duration of totality will be produced by member 38 at 100 minutes, 36 seconds on June 28, 2094. All eclipses in this series occur at the Moon’s descending node of orbit.[7]
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).[9] This lunar eclipse is related to two annular solar eclipses of Solar Saros 138.
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See also
Notes
External links
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