Solar eclipse of June 2, 2095

Solar eclipse of June 2, 2095
Map
Type of eclipse
NatureTotal
Gamma−0.6396
Magnitude1.0332
Maximum eclipse
Duration3m s
Coordinates16°42′S 37°12′E / 16.7°S 37.2°E / -16.7; 37.2
Max. width of band145 km (90 mi)
Times (UTC)
Greatest eclipse10:07:40
References
Saros129 (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.

Related eclipses[edit]

Solar eclipses 2094–2098[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]

119 June 13, 2094

Partial
124 December 7, 2094

Partial
129 June 2, 2095

Total
134 November 27, 2095

Annular
139 May 22, 2096

Total
144 November 15, 2096

Annular
149 May 11, 2097

Total
154 November 4, 2097

Annular
  164 October 24, 2098

Partial

Notes[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.

References[edit]