Solar eclipse of May 20, 2012
The solar eclipse of May 20, 2012 (May 21, 2012 local time in the Eastern Hemisphere) was an annular solar eclipse that was visible in a band spanning through Eastern Asia, the Pacific Ocean, and North America. As a partial solar eclipse, it was visible from northern Greenland to Hawaii, and from eastern Indonesia at sunrise to northwestern Mexico at sunset. The moon's apparent diameter was smaller because the eclipse was occurring only 32 1/2 hours after apogee.
Solar eclipse of May 20, 2012 | |
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Composite image taken from Red Bluff, California | |
Map | |
Type of eclipse | |
Nature | Annular |
Gamma | 0.4828 |
Magnitude | 0.9439 |
Maximum eclipse | |
Duration | 346 sec (5 m 46 s) |
Coordinates | 49.1°N 176.3°E |
Max. width of band | 237 km (147 mi) |
Times (UTC) | |
(P1) Partial begin | 20:56:07 |
(U1) Total begin | 22:06:17 |
Greatest eclipse | 23:53:54 |
(U4) Total end | 1:39:11 |
(P4) Partial end | 2:49:21 |
References | |
Saros | 128 (58 of 73) |
Catalog # (SE5000) | 9535 |
A solar eclipse is an astronomical phenomenon that 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. An annular solar eclipse occurs when the Moon's apparent diameter is smaller than the Sun's, blocking most of the Sun's light and causing the Sun to look like an annulus (ring). An annular eclipse appears as a partial eclipse over a region of the Earth thousands of kilometres wide.
The annular eclipse was the first visible from the contiguous United States since the solar eclipse of May 10, 1994 (Saros 128), and the first in Asia since the solar eclipse of January 15, 2010 (Saros 141). The path of the eclipse's antumbra included heavily populated regions of China and Japan, and an estimated 100 million people in those areas were capable of viewing annularity. In the western United States, its path included 8 states, and an estimated 6 million people were capable of viewing annularity. It was the 58th eclipse of the 128th Saros cycle, which began with a partial eclipse on August 29, 984 AD and will conclude with a partial eclipse on November 1, 2282.