Solar eclipse of September 26, 2117
| Solar eclipse of September 26, 2117 | |
|---|---|
| Type of eclipse | |
| Nature | Total |
| Gamma | 0.4442 |
| Magnitude | 1.0645 |
| Maximum eclipse | |
| Duration | 303 sec (5 m 3 s) |
| Coordinates | 21°54′N 178°24′E / 21.9°N 178.4°E Fatal error: The format of the coordinate could not be determined. Parsing failed. |
| Max. width of band | 233 km (145 mi) |
| Times (UTC) | |
| Greatest eclipse | 0:55:42 |
| References | |
| Saros | 136 (43 of 71) |
| Catalog # (SE5000) | 9773 |
A total solar eclipse will occur on September 26, 2117. 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.
Visibility
It will be visible at sunrise across eastern Asia, Sakhalin and Kuril Islands, and then crossing the Pacific Ocean, including Kiribati. It will be visible as a partial eclipse over Hawaii, and at sunset partial eclipse over parts of Alaska.
Saros 136
Solar Saros 136, repeating every 18 years, 11 days, contains 71 events. The series started with partial solar eclipse on June 14, 1360, and reached a first annular eclipse on September 8, 1504. It was a hybrid event from November 22, 1612, through January 17, 1703, and total eclipses from January 27, 1721 through May 13, 2496. The series ends at member 71 as a partial eclipse on July 30, 2622, with the entire series lasting 1262 years. The longest eclipse occurred on June 20, 1955, with a maximum duration of totality at 7 minutes, 7.74 seconds. All eclipses in this series occurs at the Moon’s descending node.[1]
Notes
References
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