Solar eclipse of December 5, 2048

Solar eclipse of December 5, 2048
Map
Type of eclipse
Nature Total
Gamma -0.3973
Magnitude 1.044
Maximum eclipse
Duration 208 sec (3 m 28 s)
Coordinates 46°06′S 56°24′W / 46.1°S 56.4°W / -46.1; -56.4
Max. width of band 160 km (99 mi)
Times (UTC)
Greatest eclipse 15:35:27
References
Saros 133 (47 of 72)
Catalog # (SE5000) 9616

A total solar eclipse will occur on December 5, 2048. 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.

Animated Path

Solar eclipses of 2047-2050

Each member in a semester series of solar eclipses repeats approximately every 177 days and 4 hours (a semester) at alternating nodes of the Moon's orbit.

Note: Partial lunar eclipses on January 26, 2047 and July 22, 2047 occur on the previous lunar year eclipse set.

Saros 133

Solar Saros 133, repeating every 18 years, 11 days, contains 72 events. The series started with a partial solar eclipse on July 13, 1219. It contains annular eclipses from November 20, 1435, through January 13, 1526, with a hybrid eclipse on January 24, 1544. It has total eclipses from February 3, 1562, through June 21, 2373. The series ends at member 72 as a partial eclipse on September 5, 2499. The longest duration of totality was 6 minutes, 50 seconds on August 7, 1850.[1] The total eclipses of this saros series are getting shorter and farther south with each iteration.

References

  1. ↑ http://eclipse.gsfc.nasa.gov/SEsaros/SEsaros133.html


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