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Solar eclipse of September 14, 2099

Total eclipse


Summary

Total eclipse

FieldValue
previousSolar eclipse of March 21, 2099
nextSolar eclipse of March 10, 2100

A total solar eclipse will occur at the Moon's descending node of orbit on Monday, September 14, 2099, with a magnitude of 1.0684. 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. Occurring about 5 hours before perigee (on September 15, 2099, at 12:20 UTC), the Moon's apparent diameter will be larger.

Locations experiencing totality

The eclipse 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 (Montana, North Dakota, South Dakota, Minnesota, Wisconsin, Illinois, Indiana, Michigan, Ohio, Pennsylvania, West Virginia, Maryland, Virginia and North Carolina). The eclipse will end in the Atlantic Ocean, with partial visibility in parts of Central America, the Caribbean, northern South America, the Iberian Peninsula, West Africa and throughout the entirety of North.

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, and April 18, 1558.

British Columbia

  • Williams Lake

Alberta

  • Calgary
  • Medicine Hat

Saskatchewan

  • Swift Current

Montana

  • Plentywood

North Dakota

  • Williston
  • Minot
  • Fargo
  • Grand Forks

Minnesota

  • Saint Cloud
  • Minneapolis
  • Saint Paul

Wisconsin

  • Eau Claire
  • Wausau
  • La Crosse
  • Oshkosh
  • Sheboygan
  • Madison
  • Janesville
  • Milwaukee
  • Kenosha

Illinois

  • Chicago
  • Waukegan
  • Evanston

Michigan

  • Grand Rapids
  • Lansing
  • Kalamazoo
  • Ann Arbor

Indiana

  • South Bend
  • Fort Wayne

Ohio

  • Toledo
  • Lima
  • Sandusky
  • Mansfield
  • Columbus
  • Canton
  • Zanesville

Pennsylvania

  • Waynesburg

West Virginia

  • Parkersburg
  • Wheeling
  • Clarksburg
  • Morgantown
  • Martinsburg

Virginia

  • Staunton
  • Harrisonburg
  • Charlottesville
  • Lynchburg
  • Richmond
  • Newport News
  • Norfolk
  • Virginia Beach

North Carolina

  • Elizabeth City
  • Kill Devil Hills
  • Kitty Hawk
  • Swan Quarter
  • Washington

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. Moreover, in Canada, the cities of Moose Jaw and Regina will be directly north of the path, but not in it.

Eclipse details

Shown below are two tables displaying details about this particular solar eclipse. The first table outlines times at which the Moon's penumbra or umbra attains the specific parameter, and the second table describes various other parameters pertaining to this eclipse.

EventTime (UTC)
First Penumbral External Contact2099 September 14 at 14:25:44.7 UTC
First Umbral External Contact2099 September 14 at 15:22:08.5 UTC
First Central Line2099 September 14 at 15:23:37.5 UTC
First Umbral Internal Contact2099 September 14 at 15:25:06.8 UTC
First Penumbral Internal Contact2099 September 14 at 16:32:45.5 UTC
Equatorial Conjunction2099 September 14 at 16:35:31.9 UTC
Ecliptic Conjunction2099 September 14 at 16:53:52.7 UTC
Greatest Duration2099 September 14 at 16:56:49.2 UTC
Greatest Eclipse2099 September 14 at 16:57:53.0 UTC
Last Penumbral Internal Contact2099 September 14 at 17:23:30.3 UTC
Last Umbral Internal Contact2099 September 14 at 18:30:52.9 UTC
Last Central Line2099 September 14 at 18:32:22.2 UTC
Last Umbral External Contact2099 September 14 at 18:33:51.3 UTC
Last Penumbral External Contact2099 September 14 at 19:30:09.7 UTC
ParameterValue
Eclipse Magnitude1.06844
Eclipse Obscuration1.14156
Gamma0.39422
Sun Right Ascension11h31m25.7s
Sun Declination+03°05'04.1"
Sun Semi-Diameter15'53.8"
Sun Equatorial Horizontal Parallax08.7"
Moon Right Ascension11h32m12.4s
Moon Declination+03°26'11.8"
Moon Semi-Diameter16'43.1"
Moon Equatorial Horizontal Parallax1°01'21.6"
ΔT123.3 s

Eclipse season

This eclipse is part of an eclipse season, a period, roughly every six months, when eclipses occur. Only two (or occasionally three) eclipse seasons occur each year, and each season lasts about 35 days and repeats just short of six months (173 days) later; thus two full eclipse seasons always occur each year. Either two or three eclipses happen each eclipse season. In the sequence below, each eclipse is separated by a fortnight.

September 14
Descending node (new moon)
September 29
Ascending node (full moon)
[[File:SE2099Sep14T.png200px]][[File:Lunar eclipse chart close-2099Sep29.png200px]]
Total solar eclipse
Solar Saros 136Penumbral lunar eclipse
Lunar Saros 148

Notes

References

References

  1. "September 14, 2099 Total Solar Eclipse". timeanddate.
  2. "Moon Distances for London, United Kingdom, England". timeanddate.
  3. [http://webpages.charter.net/darksky25/Astronomy/Articles/WIEclipses.html Madison's Eclipse Drought] {{Webarchive. link. (2017-09-24 by John Rummel)
  4. "1379-05-16.gif".
  5. [http://eclipse.gsfc.nasa.gov/JSEX/JSEX-NA.html JavaScript Solar Eclipse Explorer] by NASA
  6. [https://www.timeanddate.com/eclipse/map/2099-september-14 Eclipse Path of Total Solar Eclipse on September 14, 2099]
  7. "Total Solar Eclipse of 2099 Sep 14". EclipseWise.com.
Wikipedia Source

This article was imported from Wikipedia and is available under the Creative Commons Attribution-ShareAlike 4.0 License. Content has been adapted to SurfDoc format. Original contributors can be found on the article history page.

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