Solar eclipse of September 3, 2081
A total solar eclipse will occur on Wednesday, 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. The path of totality will begin at the Atlantic Ocean, off European mainland at 07:26:49 UTC and will end at Indonesian island of Java at 10:43:03 UTC.[1]
| Solar eclipse of September 3, 2081 | |
|---|---|
|  Map | |
| Type of eclipse | |
| Nature | Total | 
| Gamma | 0.3378 | 
| Magnitude | 1.072 | 
| Maximum eclipse | |
| Duration | 333 sec (5 m 33 s) | 
| Coordinates | 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 | 
Countries and territories experiencing totality
    
    
Major cities
    
    
Related eclipses
    
    Solar eclipses 2080–2083
    
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.[2]
| 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 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.[3]
| 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 | 
Inex series
    
This eclipse is a part of the long period inex cycle, repeating at alternating nodes, every 358 synodic months (≈ 10,571.95 days, or 29 years minus 20 days). Their appearance and longitude are irregular due to a lack of synchronization with the anomalistic month (period of perigee). However, groupings of 3 inex cycles (≈ 87 years minus 2 months) comes close (≈ 1,151.02 anomalistic months), so eclipses are similar in these groupings.
| Inex series members between 1901 and 2100: | ||
|---|---|---|
|  January 3, 1908 (Saros 130) |  December 13, 1936 (Saros 131) |  November 23, 1965 (Saros 132) | 
|  November 3, 1994 (Saros 133) |  October 14, 2023 (Saros 134) |  September 22, 2052 (Saros 135) | 
|  September 3, 2081 (Saros 136) | ||
Notes
    
- "3 September 2081 Total Solar Eclipse". Timeanddate.com. Retrieved 21 June 2020.
- 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
References
    
- Earth visibility chart and eclipse statistics Eclipse Predictions by Fred Espenak, NASA/GSFC

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