| Solar eclipse of June 25, 2150 | |
|---|---|
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Map
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|
| Type of eclipse | |
| Nature | Total |
| Gamma | -0.091 |
| Magnitude | 1.0802 |
| Maximum eclipse | |
| Duration | 7m 14s |
| Coordinates | .3N 178.1E |
| Max. width of band | 260 km |
| Times (UTC) | |
| Greatest eclipse | 0:17:25 |
| References | |
| Saros | 139 (37 of 71) |
| Catalog # (SE5000) | 9847 |
A total solar eclipse will occur on June 25, 2150. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partially 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, blocking all direct sunlight, turning day into darkness. Totality occurs in a narrow path across the surface of the Earth, while a partial solar eclipse will be visible over a region thousands of kilometres wide.
It is a part of saros series 139, repeating every 18 years, 11 days, containing 71 events. The series started with partial solar eclipse on May 17, 1501. It contains hybrid eclipses on August 11, 1627 through December 9, 1825 and total eclipses from December 21, 1843 through March 26, 2601. The series ends at member 71 as a partial eclipse on July 3, 2763.
The solar eclipse of June 13, 2132 will be the longest total solar eclipse since July 11, 1991 at 6 minutes, 55 seconds.
The longest duration of totality will be produced by member 39 at 7 minutes, 29 seconds on July 16, 2186.[1] This is the longest solar eclipse computed between 4000BC and 6000AD.[2]
Series members 24-39 occur between 1901 and 2200:
| 24 | 25 | 26 |
|---|---|---|
February 3, 1916 |
February 14, 1934 |
February 25, 1952 |
| 27 | 28 | 29 |
March 7, 1970 |
March 18, 1988 |
March 29, 2006 |
| 30 | 31 | 32 |
April 8, 2024 |
April 20, 2042 |
April 30, 2060 |
| 33 | 34 | 35 |
May 11, 2078 |
May 22, 2096 |
June 3, 2114 |
| 36 | 37 | 38 |
June 13, 2132 |
June 25, 2150 |
July 5, 2168 |
| 39 | ||
July 16, 2186 |
