Solar eclipse of December 17, 2066

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Solar eclipse of December 17, 2066
SE2066Dec17T.png
Map
Type of eclipse
Nature Total
Gamma -0.4043
Magnitude 1.0416
Maximum eclipse
Duration 194 sec (3 m 14 s)
Coordinates Lua error in package.lua at line 80: module 'strict' not found.
Max. width of band 152 km (94 mi)
Times (UTC)
Greatest eclipse 0:23:40
References
Saros 133 (48 of 72)
Catalog # (SE5000) 9657

A total solar eclipse will occur on December 17, 2066. 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.

Related eclipses

Solar eclipses 2065-2069

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.

118 July 3, 2065
SE2065Jul03P.png
Partial
123 December 27, 2065
SE2065Dec27P.png
Partial
128 June 22, 2066
SE2066Jun22A.png
Annular
133 December 17, 2066
SE2066Dec17T.png
Total
138 June 11, 2067
SE2067Jun11A.png
Annular
143 December 6, 2067
SE2067Dec06H.png
Hybrid
148 May 31, 2068
SE2068May31T.png
Total
153 November 24, 2068
SE2068Nov24P.png
Partial
158 May 20, 2069
SE2069May20P.png
Partial

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.

Series members 30-49 occur between 1742 and 2100
30 31 32
June 3, 1742 June 13, 1760 150px
June 24, 1778
33 34 35
July 4, 1796 July 17, 1814 July 27, 1832
36 37 38
August 7, 1850 150px
August 18, 1868
150px
August 29, 1886
39 40 41
SE1904Sep09T.png
September 9, 1904
150px
September 21, 1922
150px
October 1, 1940
42 43 44
SE1958Oct12T.png
October 12, 1958
SE1976Oct23T.png
October 23, 1976
SE1994Nov03T.png
November 3, 1994
45 46 47
SE2012Nov13T.png
November 13, 2012
SE2030Nov25T.png
November 25, 2030
SE2048Dec05T.png
December 5, 2048
48 49 50
SE2066Dec17T.png
December 17, 2066
150px
December 27, 2084
January 8, 2103

Notes

References


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