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Solar eclipse of September 12, 2053
Total eclipse From Wikipedia, the free encyclopedia
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A total solar eclipse will take place at the Moon's ascending node of orbit on Friday, September 12, 2053,[1] with a magnitude of 1.0328. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth. A total solar eclipse occurs when the Moon's apparent diameter is larger than the Sun's, blocking all direct sunlight, turning day into darkness. Totality occurs in a narrow path across Earth's surface, with the partial solar eclipse visible over a surrounding region thousands of kilometres wide. Occurring about 2.7 days after perigee (on September 9, 2053, at 16:30 UTC), the Moon's apparent diameter will be larger.[2]
The path of totality will be visible from parts of the southern tip of Spain, the northern tip of Morocco, Algeria, Tunisia, Libya, Egypt, Saudi Arabia, Yemen, the Maldives, and western Indonesia. A partial solar eclipse will also be visible for parts of north and central Africa, Europe, the Middle East, Central Asia, South Asia, and Southeast Asia.
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Eclipse details
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Shown below are two tables displaying details about this particular solar eclipse. The first table outlines times at which the moon's penumbra or umbra attains the specific parameter, and the second table describes various other parameters pertaining to this eclipse.[3]
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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.
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Related eclipses
Eclipses in 2053
- A penumbral lunar eclipse on March 4.
- An annular solar eclipse on March 20.
- A penumbral lunar eclipse on August 29.
- A total solar eclipse on September 12.
Metonic
- Preceded by: Solar eclipse of November 25, 2049
- Followed by: Solar eclipse of July 1, 2057
Tzolkinex
- Preceded by: Solar eclipse of August 2, 2046
- Followed by: Solar eclipse of October 24, 2060
Half-Saros
- Preceded by: Lunar eclipse of September 7, 2044
- Followed by: Lunar eclipse of September 18, 2062
Tritos
- Preceded by: Solar eclipse of October 14, 2042
- Followed by: Solar eclipse of August 12, 2064
Solar Saros 145
- Preceded by: Solar eclipse of September 2, 2035
- Followed by: Solar eclipse of September 23, 2071
Inex
- Preceded by: Solar eclipse of October 2, 2024
- Followed by: Solar eclipse of August 24, 2082
Triad
- Preceded by: Solar eclipse of November 12, 1966
- Followed by: Solar eclipse of July 14, 2140
Solar eclipses of 2051–2054
This eclipse is a member of a semester series. An eclipse in a semester series of solar eclipses repeats approximately every 177 days and 4 hours (a semester) at alternating nodes of the Moon's orbit.[4]
The partial solar eclipse on August 3, 2054 occurs in the next lunar year eclipse set.
Saros 145
This eclipse is a part of Saros series 145, repeating every 18 years, 11 days, and containing 77 events. The series started with a partial solar eclipse on January 4, 1639. It contains an annular eclipse on June 6, 1891; a hybrid eclipse on June 17, 1909; and total eclipses from June 29, 1927 through September 9, 2648. The series ends at member 77 as a partial eclipse on April 17, 3009. Its 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.
The longest duration of annularity was produced by member 15 at 6 seconds (by default) on June 6, 1891, and the longest duration of totality will be produced by member 50 at 7 minutes, 12 seconds on June 25, 2522. All eclipses in this series occur at the Moon’s ascending node of orbit.[5]
Metonic series
The metonic series repeats eclipses every 19 years (6939.69 days), lasting about 5 cycles. Eclipses occur in nearly the same calendar date. In addition, the octon subseries repeats 1/5 of that or every 3.8 years (1387.94 days). All eclipses in this table occur at the Moon's ascending node.
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.
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References
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