Solar eclipse of June 21, 2058

Last updated
Solar eclipse of June 21, 2058
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Map
Type of eclipse
NaturePartial
Gamma 1.4869
Magnitude 0.126
Maximum eclipse
Coordinates 65°54′N9°54′E / 65.9°N 9.9°E / 65.9; 9.9
Times (UTC)
Greatest eclipse0:19:35
References
Saros 157 (1 of 70)
Catalog # (SE5000) 9637

A partial solar eclipse will occur on Friday, June 21, 2058. 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.

Contents

This event will mark the beginning of Saros series 157.

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]

Solar eclipse series sets from 2054-58
Ascending node Descending node
SarosMapSarosMap
117 August 3, 2054
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Partial
122 January 27, 2055
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Partial
127 July 24, 2055
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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

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.

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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.