Solar eclipse of May 22, 2096 | |
---|---|
Type of eclipse | |
Nature | Total |
Gamma | 0.1196 |
Magnitude | 1.0737 |
Maximum eclipse | |
Duration | 367 s (6 min 7 s) |
Coordinates | 27°18′N 153°24′E / 27.3°N 153.4°E |
Max. width of band | 241 km (150 mi) |
Times (UTC) | |
Greatest eclipse | 1:37:14 |
References | |
Saros | 139 (34 of 71) |
Catalog # (SE5000) | 9724 |
A total solar eclipse will occur at the Moon's ascending node of orbit between Monday, May 21 and Tuesday, May 22, 2096,[1] with a magnitude of 1.0737. 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. Occurring about 13 hours after perigee (on May 21, 2096, at 12:30 UTC), the Moon's apparent diameter will be larger.[2]
The path of totality will be visible from parts of Indonesia and the Philippines. Totality will end approximately 1000 miles (1600 km) off the United States West Coast. A partial solar eclipse will also be visible for parts of Southeast Asia, East Asia, northern Australia, Hawaii, and northwestern North America.
Overall, at 6 minutes and 7 seconds, this will be the third longest total solar eclipse of the 21st century. The only two longer eclipses in the century are July 22, 2009 and August 2, 2027. The longest duration of this eclipse on land will be seen in Surigao del Sur, the Philippines, 4 minutes and 38 seconds.
This will be the first eclipse of saros series 139 to exceed series 136 in length of totality. The length of totality for saros 139 is increasing, while that of Saros 136 is decreasing.