Solar eclipse of September 3, 2081 | |
---|---|
Type of eclipse | |
Nature | Total |
Gamma | 0.3378 |
Magnitude | 1.072 |
Maximum eclipse | |
Duration | 333 s (5 min 33 s) |
Coordinates | 24°36′N53°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 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]
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 |
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 |
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) |
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