Solar eclipse of June 23, 2047

Last updated
Solar eclipse of June 23, 2047
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Map
Type of eclipse
NaturePartial
Gamma 1.3766
Magnitude 0.3129
Maximum eclipse
Coordinates 65°48′N178°00′W / 65.8°N 178°W / 65.8; -178
Times (UTC)
Greatest eclipse10:52:31
References
Saros 118 (70 of 72)
Catalog # (SE5000) 9612

A partial solar eclipse will occur at the Moon's descending node of orbit on Sunday, June 23, 2047, with a magnitude of 0.3129. 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 will be the second of four partial solar eclipses in 2047, with the others occurring on January 26, July 22, and December 16.

Images

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Animated path

Eclipses in 2047

Metonic

Tzolkinex

Half-Saros

Tritos

Solar Saros 118

Inex

Triad

Solar eclipses of 2047–2050

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 lunar eclipses on January 26, 2047 and July 22, 2047 occur on the previous lunar year eclipse set.

Solar eclipse sets from 2047 to 2050
Descending node Ascending node
118 June 23, 2047
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Partial
123 December 16, 2047
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Partial
128 June 11, 2048
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Annular
133 December 5, 2048
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Total
138 May 31, 2049
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Annular
143 November 25, 2049
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Hybrid
148 May 20, 2050
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Hybrid
153 November 14, 2050
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Partial

Saros 118

It is a part of Saros cycle 118, repeating every 18 years, 11 days, containing 72 events. The series started with partial solar eclipse on May 24, 803 AD. It contains total eclipses from August 19, 947 AD through October 25, 1650, hybrid eclipses on November 4, 1668 and November 15, 1686, and annular eclipses from November 27, 1704 through April 30, 1957. The series ends at member 72 as a partial eclipse on July 15, 2083. The longest duration of total was 6 minutes, 59 seconds on May 16, 1398.

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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.