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A total solar eclipse will occur on January 5, 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 January 5, 2057
SE2057Jan05T.png
Map
Type of eclipse
NatureTotal
Gamma-0.2837
Magnitude1.0287
Maximum eclipse
Duration149 sec (2 m 29 s)
Coordinates39°12′S 35°12′E / 39.2°S 35.2°E / -39.2; 35.2
Max. width of band102 km (63 mi)
Times (UTC)
Greatest eclipse9:47:52
References
Saros142 (25 of 72)
Catalog # (SE5000)9634

Contents

Related eclipsesEdit

Solar eclipses 2054-2058Edit

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]

117 August 3, 2054
 
Partial
122 January 27, 2055
 
Partial
127 July 24, 2055
 
Total
132 January 16, 2056
 
Annular
137 July 12, 2056
 
Annular
142 January 5, 2057
 
Total
147 July 1, 2057
 
Annular
152 December 26, 2057
 
Total
157 June 21, 2058
 
Partial

Saros series 142Edit

It is a part of Saros cycle 142, repeating every 18 years, 11 days, containing 72 events. The series started with partial solar eclipse on April 17, 1624. It contains one hybrid eclipse on July 14, 1768, and total eclipses from July 25, 1786 through October 29, 2543. The series ends at member 72 as a partial eclipse on June 5, 2904. The longest duration of totality will be 6 minutes, 34 seconds on May 28, 2291. All eclipses in this series occurs at the Moon’s descending node.[2]

Tritos seriesEdit

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 seriesEdit

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.

ReferencesEdit

  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. ^ http://eclipse.gsfc.nasa.gov/SEsaros/SEsaros142.html

External linksEdit