Solar eclipse of January 16, 2037

A partial solar eclipse will occur at the Moon's descending node of orbit on Friday, January 16, 2037, with a magnitude of 0.7049. 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 partial solar eclipse occurs in the polar regions of the Earth when the center of the Moon's shadow misses the Earth.

Solar eclipse of January 16, 2037
Map
Type of eclipse
NaturePartial
Gamma1.1477
Magnitude0.7049
Maximum eclipse
Coordinates68.5°N 20.8°E / 68.5; 20.8
Times (UTC)
Greatest eclipse9:48:55
References
Saros122 (59 of 70)
Catalog # (SE5000)9590

Images


Animated path

Eclipses in 2037

Metonic

Tzolkinex

Half-Saros

Tritos

Solar Saros 122

Inex

Triad

Solar eclipses of 2036–2039

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]

Note: Partial solar eclipses on February 27, 2036 and August 21, 2036 occur on the previod lunar year eclipse set.

Solar eclipse series sets from 2036 to 2039
Ascending node   Descending node
117July 23, 2036

Partial
122January 16, 2037

Partial
127July 13, 2037

Total
132January 5, 2038

Annular
137July 2, 2038

Annular
142December 26, 2038

Total
147June 21, 2039

Annular
152December 15, 2039

Total

Saros 122

It is a part of Saros cycle 122, repeating every 18 years, 11 days, containing 70 events. The series started with a partial solar eclipse on April 17, 991 AD. It contains total eclipses from July 12, 1135 through August 3, 1171, hybrid eclipses on August 13, 1189 and August 25, 1207, and annular eclipses from September 4, 1225 through October 10, 1874. The series ends at member 70 as a partial eclipse on May 17, 2235. The longest duration of totality was 1 minute, 25 seconds on July 12, 1135, and the longest duration of annularity was 6 minutes, 28 seconds on October 10, 1874.

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).

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.
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