Solar eclipse of January 6, 2076

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Solar eclipse of January 6, 2076
SE2076Jan06T.png
Map
Type of eclipse
Nature Total
Gamma -0.9373
Magnitude 1.0342
Maximum eclipse
Duration 109 sec (1 m 49 s)
Coordinates 87°12′S 173°42′W / 87.2°S 173.7°W / -87.2; -173.7
Max. width of band 340 km (210 mi)
Times (UTC)
Greatest eclipse 10:07:27
References
Saros 152 (16 of 70)
Catalog # (SE5000) 9677

A total solar eclipse will occur on January 6, 2076. 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.

Related eclipses[edit]

Solar eclipses 2073-2076[edit]

Each member 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.

122 February 7, 2073
SE2073Feb07P.png
Partial
127 August 3, 2073
SE2073Aug03T.png
Total
132 January 27, 2074
SE2074Jan27A.png
Annular
137 July 24, 2074
SE2074Jul24A.png
Annular
142 January 16, 2075
SE2075Jan16T.png
Total
147 July 13, 2075
SE2075Jul13A.png
Annular
152 January 6, 2076
SE2076Jan06T.png
Total
157 July 1, 2076
SE2076Jul01P.png
Partial

Metonic series[edit]

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).

Notes[edit]

References[edit]