Solar eclipse of June 2, 2095

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Solar eclipse of June 2, 2095
SE2095Jun02T.png
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
SE2094Jun13P.png
Partial
124 December 7, 2094
SE2094Dec07P.png
Partial
129 June 2, 2095
SE2095Jun02T.png
Total
134 November 27, 2095
SE2095Nov27A.png
Annular
139 May 22, 2096
SE2096May22T.png
Total
144 November 15, 2096
SE2096Nov15A.png
Annular
149 May 11, 2097
SE2097May11T.png
Total
154 November 4, 2097
SE2097Nov04A.png
Annular
  164 October 24, 2098
SE2098Oct24P.png
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]