外太空
外太空简介
外太空指的是地球稠密大气层之外的空间区域,并没有明确的界线分野。一般定义为大约距离地球表面1000千米之外的空间。
人类对外太空的好奇和探索从未停止过,中国“神五”、“神六”的成功发射标志着中国对外太空的探索步入了世界的先进行列。
Outer space
人类对外太空的好奇和探索从未停止过,中国“神五”、“神六”的
![Layers of Atmosphere - not to scale (NOAA)[1]](http://upload.wikimedia.org/wikipedia/en/f/f9/AtmosphereLayers.jpg)
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 actually 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.
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Earth's boundary
There is no clear boundary between the 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
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
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
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 10-15 kPa[2]. For comparison, the pressure at sea level (as defined in the atm) is about 101 kPa
Contrary to popular belief[1], a person suddenly exposed to the vacuum would not explode, freeze to death, 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 equalise 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 the Earth, including geosynchronous communication satellites 35,786
Milestones on the way to space
- Sea level - 101.3 kPa (1 atm; 1 bar; 29.92 in Hg; 760 mm Hg; 14.5 lbf/
in²) of atmospheric pressure - 4.6 km (15,000 ft) - FAA requires supplemental oxygen for aircraft pilots and passengers.
- 5.0 km (16,000 ft) - 50 kPa of atmospheric pressure
- 5.3 km (17,400 ft) - Half of the Earth's atmosphere is below this altitude.
- 8.0
km - Death zone for human climbers(26,200 ft) - 8.8 km (29,035 ft) - Summit of Mount Everest, the highest mountain on Earth (26 kPa)
- 16 km (52,500 ft) - Pressurized cabin or pressure suit required.
- 18 km (59,000 ft) - Boundary between troposphere and stratosphere
- 20 km (65,600 ft) - 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) - Regular aircraft pressurization systems no longer function.
- 32 km (105,000 ft) - Turbojets no longer function.
- 34.7 km (113,740 ft) - Altitude record for manned balloon flight
- 45 km (148,000 ft) - Ramjets no longer function.
- 50 km (164,000 ft) - Boundary between stratosphere and mesosphere
- 80 km (262,000 ft / 50 mi) - Boundary between mesosphere and thermosphere. USA definition of space flight.
- 100 km (328,084 ft) - 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 (400,000 ft) - First noticeable atmospheric drag during re-entry from orbit
- 200
km (120 mi) - Lowest possible orbit with short-term stability (stable for a few days) - 307 km (166 nm) - STS-1 mission orbit
- 350
km (220 mi) - Lowest possible orbit with long-term stability (stable for many years) - 360 km - ISS average orbit, which still varies due to drag and periodic boosting.
- 390 km - Mir mission orbit
- 440 km - Skylab mission orbit
- 587 km (317 nm) - STS-103 / HST orbit
- 690 km - Boundary between thermosphere and exosphere
- 780 km (485 miles) - Iridium orbit
- 1,374
km (850 mi) - Highest altitude by a manned Earth-orbiting flight (Gemini XI with Agena Target Vehicle) - 20,200 km (12,600 mi) - GPS orbit
- 35,786
km (22,237 mi) - Geostationary orbit height - 320,000
km (200,000 mi) - Lunar gravity exceeds Earth's (at L-1) - 348,200 km - minimum altitude that the moon passes through (surface to surface) at lunar perigee
- 402,100 km - maximum altitude that the moon passes through (surface to far side) at lunar apogee
Regions of outer space
Space does not equal orbit
To perform an orbital spaceflight, a spacecraft must travel away from the 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 caused being 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
There is a major difference between sub-orbital and orbital spaceflights. The minimum altitude for a stable orbit around the Earth (that
is, one without significant atmospheric drag), begins at around 350
See also
- Outer Space Treaty
- NASA
- Astronaut Badge
- Extraterrestrial life
- Interplanetary Internet
- 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
- ^ NASA Human Body in a Vacuum
External links
- 最后由 58.100.71.* 更新于 2007年7月9日
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