Solar eclipse of September 3, 2081
Solar eclipse of September 3, 2081 | |
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Map | |
Type of eclipse | |
Nature | Total |
Gamma | 0.3378 |
Magnitude | 1.072 |
Maximum eclipse | |
Duration | 333 sec (5 m 33 s) |
Coordinates | 24°36′N 53°36′E / 24.6°N 53.6°E |
Max. width of band | 247 km (153 mi) |
Times (UTC) | |
Greatest eclipse | 9:07:31 |
References | |
Saros | 136 (41 of 71) |
Catalog # (SE5000) | 9690 |
A total solar eclipse will occur on September 3, 2081. 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 2080-2083
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.
121 | March 21, 2080 Partial |
126 | September 13, 2080 Partial |
131 | March 10, 2081 Annular |
136 | September 3, 2081 Total |
141 | February 27, 2082 Annular |
146 | August 24, 2082 Total |
151 | February 16, 2083 Partial |
156 | August 13, 2083 Partial |
Saros 136
Solar Saros 136, repeating every 18 years, 11 days, contains 71 events. The series started with partial solar eclipse on Jun 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, 8 seconds.[1]
Series members 29–43 occur between 1865 and 2117:
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Notes
References
- Earth visibility chart and eclipse statistics Eclipse Predictions by Fred Espenak, NASA/GSFC
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