Solar eclipse of December 26, 2057

A total solar eclipse will occur on December 26, 2057. 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.

Solar eclipse of December 26, 2057
Map
Type of eclipse
NatureTotal
Gamma-0.9405
Magnitude1.0348
Maximum eclipse
Duration110 sec (1 m 50 s)
Coordinates84.9°S 21.8°E / -84.9; 21.8
Max. width of band355 km (221 mi)
Times (UTC)
Greatest eclipse1:14:35
References
Saros152 (15 of 70)
Catalog # (SE5000)9636

Solar eclipses 2054–2058

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.[1]

Solar eclipse series sets from 2054-58
Ascending node   Descending node
Saros Map Saros Map
117August 3, 2054

Partial		 122January 27, 2055

Partial
127July 24, 2055

Total		 132January 16, 2056

Annular
137July 12, 2056

Annular		 142January 5, 2057

Total
147July 1, 2057

Annular		 152December 26, 2057

Total
157June 21, 2058

Partial

Saros 152

Solar saros 152, repeating every about 18 years and 11 days, contains 70 events. The series started with a partial solar eclipse on July 26, 1805. It has total eclipses from November 2, 1967, to September 14, 2490; hybrid eclipses from September 26, 2508, to October 17, 2544; and annular eclipses from October 29, 2562, to June 16, 2941. The series ends at member 70 as a partial eclipse on August 20, 3049. The longest total eclipse will occur on June 9, 2328, at 5 minutes and 15 seconds; the longest annular eclipse will occur on February 16, 2743, at 5 minutes and 20 seconds.[2]

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.

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 descending node.[3]

gollark: And controversial stuff has never arisen from discussing something else?
gollark: The idea of a "ControversialEsolangs" for that probably wouldn't work well for various reasons, including the difficulty of moving active conversations, cognitive overhead of switching and lots of overhead deciding when to switch, a smaller set of people there even if they could otherwise participate interestingly, and somewhat more difficult-to-express issues like, er, selection effects.
gollark: I think it's a nice-to-have property but not worth sacrificing much else for.
gollark: You can see when it is *happening*, if you happen to be active, and ignore it for a bit.
gollark: You can just mute them *when* discomforting things happen, or possibly mute <#348702212110680064> if you mostly care about esolangs.

References
  1. van Gent, R.H. "Solar- and Lunar-Eclipse Predictions from Antiquity to the Present". A Catalogue of Eclipse Cycles. Utrecht University. Retrieved 6 October 2018.
  2. Saros Series Catalog of Solar Eclipses NASA Eclipse Web Site.
  3. Freeth, Tony. "Note S1: Eclipses & Predictions". plos.org. Retrieved 6 October 2018.
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