| 词条 | Solar eclipse of May 10, 2013 | |||||||||||||||||||||||||||||||||
| 释义 |
An annular solar eclipse took place on May 9–10 (UTC), 2013, with a magnitude of 0.9544. 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. 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. Visibility
Annularity was visible from a 171 to 225 kilometre-wide track that traversed Australia, eastern Papua New Guinea, the Solomon Islands, and the Gilbert Islands, with the maximum of 6 minutes 3 seconds visible from the Pacific Ocean east of French Polynesia. ImagesRelated eclipsesSolar eclipses 2011-2014{{Solar eclipse set 2011-2014}}Saros 138It is a part of Saros cycle 138, repeating every 18 years, 11 days, containing 70 events. The series started with partial solar eclipse on June 6, 1472. It contains annular eclipses from August 31, 1598 through February 18, 2482 with a hybrid eclipse on March 1, 2500. It has total eclipses from March 12, 2518 through April 3, 2554. The series ends at member 70 as a partial eclipse on July 11, 2716. The longest duration of totality will be only 56 seconds on April 3, 2554.
Tritos series{{Solar Trito series 2002 June 10}}Metonic cycle{{Solar Metonic series 2001 December 14}}References{{reflist|group=Note}}{{commons category|Solar eclipse of 2013 May 10}}{{Solar eclipse NASA reference|2001/SE2013May10A|20130510}}
4 : Annular solar eclipses|21st-century solar eclipses|2013 in science|May 2013 events |
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