Solar eclipse of July 1, 2057

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Solar eclipse of July 1, 2057
SE2057Jul01A.png
Map
Type of eclipse
NatureAnnular
Gamma0.7455
Magnitude0.9464
Maximum eclipse
Duration263 sec (4 m 23 s)
Coordinates71°30′N 176°12′W / 71.5°N 176.2°W / 71.5; -176.2
Max. width of band298 km (185 mi)
Times (UTC)
Greatest eclipse23:40:15
References
Saros147 (25 of 80)
Catalog # (SE5000)9635

An annular solar eclipse will occur on July 1, 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. 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.

Related eclipses[edit]

Solar eclipses 2054-2058[edit]

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
SE2054Aug03P.png
Partial
122 January 27, 2055
SE2055Jan27P.png
Partial
127 July 24, 2055
SE2055Jul24T.png
Total
132 January 16, 2056
SE2056Jan16A.png
Annular
137 July 12, 2056
SE2056Jul12A.png
Annular
142 January 5, 2057
SE2057Jan05T.png
Total
147 July 1, 2057
SE2057Jul01A.png
Annular
152 December 26, 2057
SE2057Dec26T.png
Total
157 June 21, 2058
SE2058Jun21P.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). All eclipses in this table occur at the Moon's ascending node.

References[edit]

  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.

External links[edit]