Space exposure

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Space exposure is in reference to the exposure of a human to the conditions of outer space, without protective clothing and beyond the Earth’s atmosphere in a vacuum.

Contents

[edit] Explanation and history of space exposure

The key concerns for a human without protective clothing beyond Earth’s atmosphere are the following, listed roughly in the order of mortal significance: ebullism, hypoxia, hypocapnia, decompression sickness, extreme temperature variations and cellular mutation and destruction from high energy photons and (sub-atomic) particles.[1]

[edit] Ebullism, hypoxia, hypocapnia and decompression sickness

Ebullism, the formation of bubbles in body fluids due to reduced ambient pressure, is the most severe component of the experience. Technically, ebullism is considered to begin at an elevation of around 19 km (12 mi) or pressures less than 6.3 kPa (47 mm Hg).[1] Experiments with other animals have revealed an array of symptoms that could also apply to humans. The least severe of these is the freezing of bodily secretions due to evaporative cooling. But severe symptoms such as loss of oxygen in tissue (anoxia) and multiplicative increase of body volume occur within 10 s, followed by circulatory failure and flaccid paralysis in about 30 s.[1] The lungs also collapse (atelectasis) in this process, but will continue to release water vapour leading to cooling and ice formation in the respiratory tract.[1]

A rough estimate is that a human will have about 90 seconds to be recompressed, after which death may be unavoidable.[2] The absence of oxygen outside the body causing rapid de-oxygenation of the blood (hypoxia) is the primary reason for unconsciousness within 14 s.[3] If a person is exposed to low pressures more slowly, hypoxia causes gradual loss of cognitive functions starting at about 3 km (2 mi) altitude equivalent. Less severe effects include the formation of nitrogen gas bubbles and consequent interference with organ function (decompression sickness), which is actually less severe in space than in diving. Meanwhile, reduction of blood carbon dioxide levels (hypocapnia) can alter the blood pH and indirectly contribute to nervous system malfunctions. If the person tries to hold their breath during decompression, the lungs may rupture internally.[2]

Few humans have experienced these four conditions. Joseph Kittinger experienced localised ebullism during a 31 km (19 mi) ascent in a helium-driven gondola.[1] His right-hand glove failed to pressurise and his hand expanded to roughly twice[4] its normal volume accompanied by disabling pain. His hand took about 3 hours to recover after his return to the ground. Two other people were decompressed accidentally during space mission training programs on the ground, but both incidents were less than 5 minutes in duration, and both victims survived.[1] International Space Station and Space Shuttle astronauts regularly work in Extravehicular Mobility Units (EMUs or space suits) that are at pressures less than 30% of the spacecraft to facilitate mobility, without experiencing noticeable decompression sickness.[5] Nevertheless, the decompression accident of Soyuz 11 killed all three cosmonauts on board.[5][6]

Decompression is a serious concern during the extra-vehicular activities (EVAs) of astronauts.[7] Current EMU designs take this and other issues into consideration, and have evolved over time.[8][9] A key challenge has been the competing interests of increasing astronaut mobility (which is reduced by high-pressure EMUs, analogous to the difficulty of deforming an inflated balloon relative to a deflated one) and minimising decompression risk. Investigators[10] have considered pressurising a separate head unit to the regular 71 kPa (10.3 psi) cabin pressure as opposed to the current whole-EMU pressure of 29.6 kPa (4.3 psi)[9] (for reference, by definition, the atmospheric pressure at sea level is 101.4 kPa, equal to 14.7 psi[11]). In such a design, pressurisation of the torso could be achieved mechanically, avoiding mobility reduction associated with pneumatic pressurisation.[10]

[edit] Extreme temperature variations

Extreme temperature variations are a problem in space, because heat exchange occurs primarily via infrared photons. While the absence of convection and conduction causes an insulating effect preventing rapid dissipation of body heat, localized heating can occur if exposed to starlight at distances comparable to the Earth-Sun distance.

[edit] Cellular mutation and destruction from high energy photons and (sub-atomic) particles

A more severe long-term effect would be the direct exposure to high energy photons (ultraviolet, X-ray, and gamma) and energized subatomic particles (primarily protons[12]). These can permanently denature DNA and other cellular molecules through atomic and nuclear interactions. Prolonged exposure and the ability of X and gamma photons to penetrate the entire body may cause death from organ failure, while even short-term exposure may cause cancer.[citation needed]

[edit] In science fiction

Spacing is a staple of science fiction, where it usually occurs as a method of execution (or other sort of killing) by vacuum exposure in space - usually accomplished by ejecting the subject through the airlock of a spacecraft or space station without a space suit. The primary cause of death would be asphyxia. Unlike the persistent myth, people do not explode due to vacuum exposure or explosive decompression (See Landis' article in links).

As of 2007, there are no known instances of deliberate usage, although the crew of the Russian spacecraft Soyuz 11 lost their lives due to accidental decompression.

[edit] See also

[edit] References

  1. ^ a b c d e f Pilmanis, Andrew A. and Sears, William J. (2003), doi 10.1016/S0140-6736(03)15059-3
  2. ^ a b Landis, Geoffrey A. website
  3. ^ NASAtechnical report
  4. ^ PBS report
  5. ^ a b Stewart, L. et al. (2007), doi 10.1016/j.jemermed.2006.05.031
  6. ^ Time Magazine 1971
  7. ^ Conkin, Johnny (2001), NASA technical report
  8. ^ Jordan, Nicole C. et al. (2005), doi 10.1109/RE.2005.69
  9. ^ a b Jordan, Nicole C. et al. (2006), doi 10.1016/j.actaastro.2006.04.014
  10. ^ a b Gorguinpour, Camron (2001), [http://www.lpi.usra.edu/publications/reports/CB-1106/ucb01.pdf
  11. ^ Britannica
  12. ^ Boynton, W. V. et al. (2004), doi 10.1023/B:SPAC.0000021007.76126.15