Solar eclipse of June 2, 2095 | |
---|---|
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 |
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.
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 |
Solar eclipse of June 2, 2095 | |
---|---|
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 |
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.
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 |