Solar eclipse of June 2, 2095

Solar eclipse of June 2, 2095
Map
Type of eclipse
Nature Total
Gamma -0.6396
Magnitude 1.0332
Maximum eclipse
Duration 3m s
Coordinates 16°42′S 37°12′E / 16.7°S 37.2°E / -16.7; 37.2
Max. width of band 145 km (90 mi)
Times (UTC)
Greatest eclipse 10:07:40
References
Saros 129 (56 of 80)
Catalog # (SE5000) 9722

A total solar eclipse will occur on June 2, 2095. 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.

Solar eclipses 2094-2098

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]

119June 13, 2094

Partial
124December 7, 2094

Partial
129June 2, 2095

Total
134November 27, 2095

Annular
139May 22, 2096

Total
144November 15, 2096

Annular
149May 11, 2097

Total
154November 4, 2097

Annular
  164October 24, 2098

Partial

Notes

  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.

References


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