Information about Outer Space

For the Atari video game, see Outer Space (video game).

"Deep space" redirects here. For the NASA space probes, see Deep Space 1 and Deep Space 2.

Outer space, sometimes simply called space, refers to the relatively empty regions of the universe outside the atmospheres of celestial bodies. Outer space is used to distinguish it from airspace (and terrestrial locations). Contrary to popular understanding, outer space is not completely empty (i.e. a perfect vacuum) but contains a low density of particles, predominantly hydrogen plasma, as well as electromagnetic radiation, dark matter and dark energy.

Earth's boundary

There is no clear boundary between Earth's atmosphere and space as the density of the atmosphere gradually decreases as the altitude increases. Nevertheless, the Fédération Aéronautique Internationale has established the Kármán line at an altitude of 100 km (62 miles) as a working definition for the boundary between aeronautics and astronautics. This is used because above an altitude of roughly 100 km, as Theodore von Kármán calculated, a vehicle would have to travel faster than orbital velocity in order to derive sufficient aerodynamic lift from the atmosphere to support itself. The United States designates people who travel above an altitude of 80 km (50 statute miles) as astronauts. During re-entry, roughly 120 km (75 miles) marks the boundary where atmospheric drag becomes noticeable, depending on the ballistic coefficient of the vehicle.

Solar system

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 types of organic molecules discovered to date by microwave spectroscopy. According to the Big bang theory, 2.7 K blackbody radiation was left over from the 'big bang' and the origin of the universe, and cosmic rays, which include ionized atomic nuclei and various subatomic particles. There is also gas, plasma and dust, and small meteors and material left over from previous manned and unmanned launches that are a potential hazard to spacecraft. Some of this debris re-enters the atmosphere periodically.

The absence of air makes outer space (and the surface of the Moon) ideal locations for astronomy at all wavelengths of the electromagnetic spectrum, as evidenced by the spectacular pictures sent back by the Hubble Space Telescope, allowing light from about 13.7 billion years ago — almost to the time of the Big Bang — to be observed. Pictures and other data from unmanned space vehicles have provided invaluable information about the planets, asteroids and comets in our solar system.

The "vacuum of space"

While not being an actual perfect vacuum, outer space contains such sparse matter that it can be effectively thought of as one. The pressure of interstellar space is about 10 pPa (1×10^-11 Pa). For comparison, the pressure at sea level (as defined in the unit of atmospheric pressure) is about 101 kPa (1×10⁵ Pa).

Contrary to popular belief,^[1] a person suddenly exposed to the vacuum would not explode, freeze to death (space may be cold, but it's mostly vacuum, a perfect insulator; the main temperature worry for space suits is how to get rid of naturally generated body heat), or die from boiling blood, but would take a short while to die by asphyxiation (suffocation). Air would immediately leave the lungs due to the enormous pressure gradient. Any oxygen dissolved in the blood would empty into the lungs to try to equalize the partial pressure gradient. Once the deoxygenated blood arrived at the brain, death would quickly follow. Water vapor would also rapidly evaporate off from exposed areas such as the lungs, cornea of the eye and mouth, cooling the body.

Satellites

There are many artificial satellites orbiting Earth, including geosynchronous communication satellites 35,786 km (22,241 miles) above mean sea level at the Equator. There is also increasing reliance, for both military and civilian uses, on satellites which enable the Global Positioning System (GPS). A common misconception is that people in orbit are outside Earth's gravity because they are "floating". They are floating because they are in "free fall": the force of gravity is creating an inward centripetal force which is stopping them from flying out into space, balanced by the (reactive) centrifugal force induced by their linear velocity. Earth's gravity reaches out far past the Van Allen belt and keeps the Moon in orbit at an average distance of 384,403 km (238,857 miles).

According to the theory of gravity, the gravity of all celestial bodies drops off toward zero with the inverse square of the distance.

Milestones on the way to space

• Sea level - 101.3 kPa (1 atm; 1.013 bar; 29.92 in Hg; 760 mm Hg; 14.5 lbf/in²) of atmospheric pressure
• 3.0 km (10,000 ft)(1.9 miles) - FAA requires supplemental oxygen for aircraft pilots in unpressurized aircraft.^[2]
• 5.0 km (16,400 ft)(3.1 miles) - 50 kPa of atmospheric pressure
• 5.3 km (17,400 ft)(3.3 miles) - Half of the Earth's atmosphere is below this altitude.
• 8.0 km (26,200 ft)(5 miles) - Death zone for human climbers
• 8.85 km (29,035 ft)(5.5 miles) - Summit of Mount Everest, the highest mountain on Earth (26 kPa)
• 16 km (52,500 ft)(9.9 miles) - Pressurized cabin or pressure suit required.
• 18 km (59,100 ft)(11.2 miles) - Boundary between troposphere and stratosphere
• 20 km (65,600 ft)(12.4 miles) - Water at room temperature boils without a pressurized container. (The popular notion that bodily fluids would start to boil at this point is false because the body generates enough internal pressure to prevent it.)
• 24 km (78,700 ft)(14.9 miles) - Regular aircraft pressurization systems no longer function.
• 32 km (105,000 ft)(19.9 miles) - Turbojets no longer function.
• 34.7 km (113,740 ft)(21.5 miles) - Altitude record for manned balloon flight
• 45 km (147,600 ft)(28 miles) - Ramjets no longer function.
• 50 km (164,000 ft)(31 miles) - Boundary between stratosphere and mesosphere
• 80.5 km (264,000 ft)(50 miles) - Boundary between mesosphere and thermosphere. USA definition of space flight.
• 100 km (328,100 ft)(62.1 miles) - Kármán line, defining the limit of outer space according to the Fédération Aéronautique Internationale. Aerodynamic surfaces ineffective due to low atmospheric density. Lift speed generally exceeds orbital velocity. Turbopause.
• 120 km (393,400 ft)(74.6 miles) - First noticeable atmospheric drag during re-entry from orbit
• 200 km (124.2 miles) - Lowest possible orbit with short-term stability (stable for a few days)
• 307 km (190.8 miles) - STS-1 mission orbit
• 350 km (217.4 miles) - Lowest possible orbit with long-term stability (stable for many years)
• 360 km (223.7 miles) - ISS average orbit, which still varies due to drag and periodic boosting.
• 390 km (242.3 miles) - Mir mission orbit
• 440 km (273.4 miles) - Skylab mission orbit
• 587 km (364.8 miles) - HST orbit
• 690 km (428.7 miles) - Boundary between thermosphere and exosphere
• 780 km (484.7 miles) - Iridium orbit
• 1,374 km (850 miles) - Highest altitude by a manned Earth-orbiting flight (Gemini XI with Agena Target Vehicle)
• 20,200 km (12,600 miles) - GPS orbit
• 35,786 km (22,237 miles) - Geostationary orbit height
• 320,000 km (200,000 miles) - Lunar gravity exceeds Earth's (at Lagrange point)
• 348,200 km (238,700 miles) - lunar perigee (closet approach of the Moon)
• 402,100 km (249,900 miles) - lunar apogee (largest distance between Earth and Moon)

Regions of outer space

• Cislunar space
• Interplanetary space
• Interstellar medium
• Intergalactic space

Space does not equal orbit

To perform an orbital spaceflight, a spacecraft must travel away from Earth faster than it must for a sub-orbital spaceflight. A spacecraft has not entered orbit until it is traveling with a sufficiently great horizontal velocity such that the acceleration due to gravity on the spacecraft is less than or equal to the centripetal acceleration being caused by its horizontal velocity (see circular motion). So to enter orbit, a spacecraft must not only reach space, but must also achieve a sufficient orbital speed (angular velocity). For a low-Earth orbit, this is about 7.9 km/s (18,000 mph). Konstantin Tsiolkovsky was the first to realize that, given the energy available from any available chemical fuel, a several-stage rocket would be required. The escape velocity to pull free of Earth's gravitational field altogether and move into interplanetary space is about 40,000 km/h (25,000 mph or 11,000 m/s). The energy required to reach velocity for low Earth orbit (32 MJ/kg) is about twenty times the energy required simply to climb to the corresponding altitude (10 kJ/(km·kg)).

There is a major difference between sub-orbital and orbital spaceflights. The minimum altitude for a stable orbit around Earth (that is, one without significant atmospheric drag) begins at around 350 km (220 miles) above mean sea level. A common misunderstanding about the boundary to space is that orbit occurs simply by reaching this altitude. Achieving orbital speed can theoretically occur at any altitude, although atmospheric drag precludes an orbit that is too low. At sufficient speed, an airplane would need a way to keep it from flying off into space, but at present, this speed is several times greater than anything within reasonable technology.

See also

• Outer Space Treaty
• NASA
• Astronaut Badge
• Extraterrestrial life
• Interplanetary Internet
• Spaceflight
• Space station
• Space and survival
• Space colonization
• Space exploration
• Private space flight
• Space science
• Space technology
• Solar wind
• Karman line
• List of space flights

References

External links

• Morgan Freeman's Space Exploration Channel "Our Space" on ClickStar
• Profits set to soar in outer space
• Newscientist Space.
• X PRIZE Foundation.
• Images of Earth and space taken from outer space
• and

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