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Solar eclipse of January 16, 2056

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Solar eclipse of January 16, 2056
Map
Type of eclipse
NatureAnnular
Gamma0.4199
Magnitude0.9759
Maximum eclipse
Duration172 s (2 min 52 s)
Coordinates3°54′N 153°30′W / 3.9°N 153.5°W / 3.9; -153.5
Max. width of band95 km (59 mi)
Times (UTC)
Greatest eclipse22:16:45
References
Saros132 (48 of 71)
Catalog # (SE5000)9632

An annular solar eclipse will occur on January 16, 2056. 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. An annular solar eclipse occurs when the Moon's apparent diameter is smaller than the Sun's, blocking most of the Sun's light and causing the Sun to look like an annulus (ring). An annular eclipse appears as a partial eclipse over a region of the Earth thousands of kilometres wide.

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]

The partial solar eclipses on March 9, 2054 and September 2, 2054 occur in the previous lunar year eclipse set, and the partial solar eclipses on May 22, 2058 and November 16, 2058 occur in the next lunar year eclipse set.

Solar eclipse series sets from 2054 to 2058
Ascending node   Descending node
Saros Map Gamma Saros Map Gamma
117 August 3, 2054

Partial
−1.4941 122 January 27, 2055

Partial
1.155
127 July 24, 2055

Total
−0.8012 132 January 16, 2056

Annular
0.4199
137 July 12, 2056

Annular
−0.0426 142 January 5, 2057

Total
−0.2837
147 July 1, 2057

Annular
0.7455 152 December 26, 2057

Total
−0.9405
157 June 21, 2058

Partial
1.4869

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.