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Solar eclipse of September 14, 2099
Total eclipse
Total eclipse
| Field | Value |
|---|---|
| previous | Solar eclipse of March 21, 2099 |
| next | Solar 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.
| Event | Time (UTC) |
|---|---|
| First Penumbral External Contact | 2099 September 14 at 14:25:44.7 UTC |
| First Umbral External Contact | 2099 September 14 at 15:22:08.5 UTC |
| First Central Line | 2099 September 14 at 15:23:37.5 UTC |
| First Umbral Internal Contact | 2099 September 14 at 15:25:06.8 UTC |
| First Penumbral Internal Contact | 2099 September 14 at 16:32:45.5 UTC |
| Equatorial Conjunction | 2099 September 14 at 16:35:31.9 UTC |
| Ecliptic Conjunction | 2099 September 14 at 16:53:52.7 UTC |
| Greatest Duration | 2099 September 14 at 16:56:49.2 UTC |
| Greatest Eclipse | 2099 September 14 at 16:57:53.0 UTC |
| Last Penumbral Internal Contact | 2099 September 14 at 17:23:30.3 UTC |
| Last Umbral Internal Contact | 2099 September 14 at 18:30:52.9 UTC |
| Last Central Line | 2099 September 14 at 18:32:22.2 UTC |
| Last Umbral External Contact | 2099 September 14 at 18:33:51.3 UTC |
| Last Penumbral External Contact | 2099 September 14 at 19:30:09.7 UTC |
| Parameter | Value |
|---|---|
| Eclipse Magnitude | 1.06844 |
| Eclipse Obscuration | 1.14156 |
| Gamma | 0.39422 |
| Sun Right Ascension | 11h31m25.7s |
| Sun Declination | +03°05'04.1" |
| Sun Semi-Diameter | 15'53.8" |
| Sun Equatorial Horizontal Parallax | 08.7" |
| Moon Right Ascension | 11h32m12.4s |
| Moon Declination | +03°26'11.8" |
| Moon Semi-Diameter | 16'43.1" |
| Moon Equatorial Horizontal Parallax | 1°01'21.6" |
| ΔT | 123.3 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.png | 200px]] | [[File:Lunar eclipse chart close-2099Sep29.png | 200px]] |
| Total solar eclipse | |||
| Solar Saros 136 | Penumbral lunar eclipse | ||
| Lunar Saros 148 |
Notes
References
References
- "September 14, 2099 Total Solar Eclipse". timeanddate.
- "Moon Distances for London, United Kingdom, England". timeanddate.
- [http://webpages.charter.net/darksky25/Astronomy/Articles/WIEclipses.html Madison's Eclipse Drought] {{Webarchive. link. (2017-09-24 by John Rummel)
- "1379-05-16.gif".
- [http://eclipse.gsfc.nasa.gov/JSEX/JSEX-NA.html JavaScript Solar Eclipse Explorer] by NASA
- [https://www.timeanddate.com/eclipse/map/2099-september-14 Eclipse Path of Total Solar Eclipse on September 14, 2099]
- "Total Solar Eclipse of 2099 Sep 14". EclipseWise.com.
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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