Solar eclipse of September 3, 2081

Last updated
Solar eclipse of September 3, 2081
SE2081Sep03T.png
Map
Type of eclipse
NatureTotal
Gamma 0.3378
Magnitude 1.072
Maximum eclipse
Duration333 s (5 min 33 s)
Coordinates 24°36′N53°36′E / 24.6°N 53.6°E / 24.6; 53.6
Max. width of band247 km (153 mi)
Times (UTC)
Greatest eclipse9:07:31
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]

Contents

Countries and territories experiencing totality

Major cities

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
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Partial
126 September 13, 2080
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Partial
131 March 10, 2081
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Annular
136 September 3, 2081
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Total
141 February 27, 2082
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Annular
146 August 24, 2082
SE2082Aug24T.png
Total
151 February 16, 2083
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Partial
156 August 13, 2083
SE2083Aug13P.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. [3]

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

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.

Notes

  1. "3 September 2081 Total Solar Eclipse". Timeanddate.com. Retrieved 21 June 2020.
  2. 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.
  3. SEsaros136 at NASA.gov

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References