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Encyclopedia > Boundary to space
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Layers of Atmosphere (NOAA)

The Karman Line is an internationally designated altitude commonly used to define outer space. According to definitions by the Fédération Aéronautique Internationale (FAI), the Karman or Kármán line lies at a height of 100 km (about 62 miles) above Earth's surface (ie. in technical terms 100 km above mean sea level). It was named after Theodore von Kármán.


Around this altitude the Earth's atmosphere becomes negligible for aeronautic purposes, and there is an abrupt increase in atmospheric temperature and interaction with solar radiation.

Contents

Overview

Strictly speaking, there is no such thing as an end to Earth's atmosphere: An atmosphere doesn't technically end at any given height, but becomes progressively thinner with altitude. Also, depending on how the various layers that make up the space around the Earth are defined (and depending on whether these layers are considered as part of the actual atmosphere), the definition of the edge of space could vary considerably: If one were to consider the thermosphere and exosphere only part of the atmosphere and not of space, one might have to place the boundary to space as high as about 10,000 km (6200 miles) up. It is quite reasonable to state that attaining a height of 100 km is escaping the Earth's atmosphere, as spacecraft at this altitude can no longer rely on it for weight support or propulsion. Perhaps more importantly, the FAI's definitions regarding the boundary to space are internationally accepted.


Another hurdle to strictly defining the boundary to space is the dynamic nature of Earth's atmosphere. For example; at an altitude of 1000 km, the atmosphere's density may vary by a factor of five, depending on the time of day, time of year, AP magnetic index, and recent solar flux.


The FAI apparently doesn't itself use the precise words "boundary to space" or "edge of space"; the FAI uses the term "Kármán line" or speaks of a "100 km. altitude boundary for astronautics", as also reflected in their following two definitions (quoted verbatim from their website):

  • Aeronautics -- For FAI purposes, aerial activity, including all air sports, within 100 kilometres of Earth's surface.
  • Astronautics -- For FAI purposes, activity more than 100 kilometres above Earth's surface.

Also see the article on the Kármán line under External links below, which has an excellent explanation on how this boundary was determined.


A diluted definition

Some people (including the FAI in some of their publications) also use the expression "edge of space" to refer to a very vaguely defined (essentially undefined) region below the actual 100 km boundary to space, which is often meant to include substantially lower regions as well. Thus, certain balloon or airplane flights might be described as "reaching the edge of space", when they really don't even go half as high as 100 km up. In such statements, "reaching the edge of space" merely refers to going somewhat higher than average aeronautical vehicles would commonly go.


The U.S. definition

U.S. authorities define the boundary to space to lie at a height of 50 miles (about 80 km) above mean sea level, about where the Mesosphere ends. This definition is thought by some to be outdated, and is not commonly accepted internationally.


See also

External links

  • Article on the Karman line (http://www.fai.org/astronautics/100km.asp) at the FAI website
  • Layers of the Atmosphere _ NOAA (http://www.srh.noaa.gov/srh/jetstream/atmos/layers.htm)



  Results from FactBites:
 
Karman line - Wikipedia, the free encyclopedia (532 words)
Another hurdle to strictly defining the boundary to space is the dynamic nature of Earth's atmosphere.
Some people (including the FAI in some of their publications) also use the expression "edge of space" to refer to a very vaguely defined (essentially undefined) region below the actual 100 km boundary to space, which is often meant to include substantially lower regions as well.
U.S. authorities define the boundary to space to lie at a height of 50 miles (about 80 km) above mean sea level, about where the mesosphere ends.
Outer space - Wikipedia, the free encyclopedia (1086 words)
There is no discrete boundary between the Earth's atmosphere and space as the atmosphere gradually attenuates with increasing altitude.
Outer space within the solar system is called interplanetary space, which passes over into interstellar space at the heliopause.
The vacuum of outer space is not really empty; it is sparsely filled with several dozen organic molecules discovered to date by microwave spectroscopy, 2.7 K flbody radiation left over from the Big Bang and the origin of the universe, and cosmic rays, which include ionized atomic nuclei and various subatomic particles.
  More results at FactBites »


 

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