Solar eclipse of September 14, 2099

Last updated
Solar eclipse of September 14, 2099
SE2099Sep14T.png
Map
Type of eclipse
NatureTotal
Gamma 0.3942
Magnitude 1.0684
Maximum eclipse
Duration318 s (5 min 18 s)
Coordinates 23°24′N62°48′W / 23.4°N 62.8°W / 23.4; -62.8
Max. width of band241 km (150 mi)
Times (UTC)
Greatest eclipse16:57:53
References
Saros 136 (42 of 71)
Catalog # (SE5000) 9732

A total solar eclipse will occur on Monday, September 14, 2099. 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.

Contents

Locations experiencing totality

It will begin at sunrise off the western coast of Canada, and move eastern across Canada (British Columbia, Alberta, and Saskatchewan) and the northern states of the United States (North Dakota, Minnesota, Wisconsin, Illinois, Indiana, Michigan, Ohio, Pennsylvania, West Virginia, Virginia and North Carolina). The eclipse will end in the Atlantic ocean, with partial visibility in parts of Europe, West Africa and throughout the entirety of North and South America.

The path of totality will pass through the cities of Madison, Wisconsin, and Grand Rapids, Michigan. The last time totality was visible over these two locations was respectively May 16, 1379, [1] [2] and April 18, 1558. [3]

British Columbia

Alberta

Saskatchewan

Montana

North Dakota

Minnesota

Wisconsin

Illinois

Michigan

Indiana

Ohio

Pennsylvania

West Virginia

Virginia

North Carolina

Although this solar eclipse does pass over a few large cities such as Minneapolis and Virginia Beach, it fails to offer totality in several major cities nearby, including most of Chicago and all of Washington D.C., Detroit, Cincinnati and Cleveland. [4] Moreover, in Canada, the cities of Moose Jaw and Regina will be directly north of the path, but not in it.

Solar eclipses 2098–2100

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. [5]

Solar eclipses 2098–2100
121 April 1, 2098
SE2098Apr01P.png
Partial		126 September 25, 2098
SE2098Sep25P.png
Partial
131 March 21, 2099
SE2099Mar21A.png
Annular		136 September 14, 2099
SE2099Sep14T.png
Total
141 March 10, 2100
SE2100Mar10A.png
Annular		146 September 4, 2100
SE2100Sep04T.png
Total

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. [6]

Series members 29–43 occur between 1865 and 2117
293031
SE1865Apr25T.gif
Apr 25, 1865 		SE1883May06T.png
May 6, 1883 		SE1901May18T.png
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.

Inex series members between 1901 and 2100:
SE1926Jan14T.png
January 14, 1926
(Saros 130)		 SE1954Dec25A.png
December 25, 1954
(Saros 131)		 SE1983Dec04A.png
December 4, 1983
(Saros 132)
SE2012Nov13T.png
November 13, 2012
(Saros 133)		 SE2041Oct25A.png
October 25, 2041
(Saros 134)		 SE2070Oct04A.png
October 4, 2070
(Saros 135)
SE2099Sep14T.png
September 14, 2099
(Saros 136)

Tritos series

This eclipse is a part of a tritos cycle, repeating at alternating nodes every 135 synodic months (≈ 3986.63 days, or 11 years minus 1 month). Their appearance and longitude are irregular due to a lack of synchronization with the anomalistic month (period of perigee), but groupings of 3 tritos cycles (≈ 33 years minus 3 months) come close (≈ 434.044 anomalistic months), so eclipses are similar in these groupings.

Notes

  1. ↑ Madison's Eclipse Drought Archived 2017-09-24 at the Wayback Machine by John Rummel
  2. ↑ "1379-05-16.gif" (GIF). nasa.gov. Archived from the original on 19 November 2021. Retrieved 18 December 2022.
  3. ↑ JavaScript Solar Eclipse Explorer by NASA
  4. ↑ Eclipse Path of Total Solar Eclipse on September 14, 2099
  5. ↑ 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.
  6. ↑ SEsaros136 at NASA.gov

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References

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