| Solar eclipse of August 24, 2063 | |
|---|---|
|  Map | |
| Type of eclipse | |
| Nature | Total | 
| Gamma | 0.2771 | 
| Magnitude | 1.075 | 
| Maximum eclipse | |
| Duration | 349 sec (5 m 49 s) | 
| Coordinates | 25°36′N 168°24′E / 25.6°N 168.4°E | 
| Max. width of band | 252 km (157 mi) | 
| Times (UTC) | |
| Greatest eclipse | 1:22:11 | 
| References | |
| Saros | 136 (40 of 71) | 
| Catalog # (SE5000) | 9649 | 
A total solar eclipse will occur on 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.
Related eclipses
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  Partial | 126 | September 3, 2062  Partial | 
| 131 | February 28, 2063  Annular | 136 | August 24, 2063  Total | 
| 141 | February 17, 2064  Annular | 146 | August 12, 2064  Total | 
| 151 | February 5, 2065  Partial | 156 | August 2, 2065  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 | ||
|---|---|---|
| 29 | 30 | 31 | 
|  Apr 25, 1865 |  May 6, 1883 |  May 18, 1901 | 
| 32 | 33 | 34 | 
|  May 29, 1919 |  Jun 8, 1937 |  Jun 20, 1955 | 
| 35 | 36 | 37 | 
|  Jun 30, 1973 |  Jul 11, 1991 |  Jul 22, 2009 | 
| 38 | 39 | 40 | 
|  Aug 2, 2027 |  Aug 12, 2045 |  Aug 24, 2063 | 
| 41 | 42 | 43 | 
|  Sep 3, 2081 |  Sep 14, 2099 |  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).
| 21 eclipse events between June 12, 2029, and June 12, 2105 | ||||
|---|---|---|---|---|
| June 11–12 | March 30–31 | January 16 | November 4–5 | August 23–24 | 
| 118 | 120 | 122 | 124 | 126 | 
|  June 12, 2029 |  March 30, 2033 |  January 16, 2037 |  November 4, 2040 |  August 23, 2044 | 
| 128 | 130 | 132 | 134 | 136 | 
|  June 11, 2048 |  March 30, 2052 |  January 16, 2056 |  November 5, 2059 |  August 24, 2063 | 
| 138 | 140 | 142 | 144 | 146 | 
|  June 11, 2067 |  March 31, 2071 |  January 16, 2075 |  November 4, 2078 |  August 24, 2082 | 
| 148 | 150 | 152 | 154 | |
|  June 11, 2086 |  March 31, 2090 |  January 16, 2094 |  November 4, 2097 | |
References
- ↑ 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.
- ↑ SEsaros136 at NASA.gov
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