Solar eclipse of May 31, 2068

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Solar eclipse of May 31, 2068
SE2068May31T.png
Map
Type of eclipse
Nature Total
Gamma -0.797
Magnitude 1.011
Maximum eclipse
Duration 66 sec (1 m 6 s)
Coordinates 31°00′S 123°12′E / 31°S 123.2°E / -31; 123.2
Max. width of band 63 km (39 mi)
Times (UTC)
Greatest eclipse 3:56:39
References
Saros 148 (24 of 75)
Catalog # (SE5000) 9660

A total solar eclipse will occur on May 31, 2068. 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[edit]

Solar eclipses 2065-2069[edit]

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

Metonic series[edit]

The metonic series repeats eclipses every 19 years (6939.69 days), lasting about 5 cycles. Eclipses occur in nearly the same calendar date. In addition the octon subseries repeats 1/5 of that or every 3.8 years (1387.94 days).

Notes[edit]

References[edit]