Solar eclipse of August 24, 2063

Last updated
Solar eclipse of August 24, 2063
SE2063Aug24T.png
Map
Type of eclipse
NatureTotal
Gamma 0.2771
Magnitude 1.075
Maximum eclipse
Duration349 s (5 min 49 s)
Coordinates 25°36′N168°24′E / 25.6°N 168.4°E / 25.6; 168.4
Max. width of band252 km (157 mi)
Times (UTC)
Greatest eclipse1:22:11
References
Saros 136 (40 of 71)
Catalog # (SE5000) 9649

A total solar eclipse will occur on Friday, August 24, 2063. 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.

Contents

Solar eclipses 2062–2065

This eclipse is a member of a semester series. An eclipse 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. [1]

121 March 11, 2062
SE2062Mar11P.png
Partial
126 September 3, 2062
SE2062Sep03P.png
Partial
131 February 28, 2063
SE2063Feb28A.png
Annular
136 August 24, 2063
SE2063Aug24T.png
Total
141 February 17, 2064
SE2064Feb17A.png
Annular
146 August 12, 2064
SE2064Aug12T.png
Total
151 February 5, 2065
SE2065Feb05P.png
Partial
156 August 2, 2065
SE2065Aug02P.png
Partial

Saros 136

Solar Saros 136, repeating every 18 years, 11 days, contains 71 events. The series started with partial solar eclipse on June 14, 1360, and reached a first annular eclipse on September 8, 1504. It was a hybrid event from November 22, 1612, through January 17, 1703, and total eclipses from January 27, 1721, through May 13, 2496. The series ends at member 71 as a partial eclipse on July 30, 2622, with the entire series lasting 1262 years. The longest eclipse occurred on June 20, 1955, with a maximum duration of totality at 7 minutes, 7.74 seconds. All eclipses in this series occurs at the Moon's descending node. [2]

Series members 29–43 occur between 1865 and 2117
293031
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Apr 25, 1865
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May 6, 1883
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May 18, 1901
323334
SE1919May29T.png
May 29, 1919
SE1937Jun08T.png
Jun 8, 1937
SE1955Jun20T.png
Jun 20, 1955
353637
SE1973Jun30T.png
Jun 30, 1973
SE1991Jul11T.png
Jul 11, 1991
SE2009Jul22T.png
Jul 22, 2009
383940
SE2027Aug02T.png
Aug 2, 2027
SE2045Aug12T.png
Aug 12, 2045
SE2063Aug24T.png
Aug 24, 2063
414243
SE2081Sep03T.png
Sep 3, 2081
SE2099Sep14T.png
Sep 14, 2099
SE2117Sep26T.png
Sep 26, 2117

Metonic cycle

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).

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References

  1. van Gent, R.H. "Solar- and Lunar-Eclipse Predictions from Antiquity to the Present". A Catalogue of Eclipse Cycles. Utrecht University. Retrieved 6 October 2018.
  2. SEsaros136 at NASA.gov