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	16.7°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.

Related eclipses

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.

The solar eclipses on January 16, 2094 (total) and July 12, 2094 (partial) occur in the previous lunar year eclipse set, and the partial solar eclipses on April 1, 2098 and September 25, 2098 occur in the next lunar year eclipse set.

Solar eclipse series sets from 2094 to 2098
Ascending node				Descending node
Saros	Map	Gamma		Saros	Map	Gamma
119	June 13, 2094 Partial	−1.4613		124	December 7, 2094 Partial	1.1547
129	June 2, 2095 Total	−0.6396		134	November 27, 2095 Annular	0.4903
139	May 22, 2096 Total	0.1196		144	November 15, 2096 Annular	−0.20
149	May 11, 2097 Total	0.8516		154	November 4, 2097 Annular	−0.8926
159	May 1, 2098			164	October 24, 2098 Partial	−1.5407

References

• Earth visibility chart and eclipse statistics Eclipse Predictions by Fred Espenak, NASA/GSFC
  • Google interactive map
  • Besselian elements