Difference between revisions of "Heavy Ions"

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Heavy ions are charged particles heavier than alpha particles.<ref>Heavy ion. (1998, Jul 20). In ''Encyclopaedia Britannica. <nowiki>https://www.britannica.com/science/heavy-ion</nowiki>''</ref>  They consitute 1% of cosmic radiation.<ref>Schimmerling W. (2011, Feb 5). The Space Radiation Environment:  An Introduction. <nowiki>https://three.jsc.nasa.gov/concepts/SpaceRadiationEnviron.pdf</nowiki></ref>
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Heavy ions are charged particles heavier than alpha particles.<ref>Heavy ion. (1998, Jul 20). In ''Encyclopaedia Britannica. <nowiki>https://www.britannica.com/science/heavy-ion</nowiki>''</ref>  They constitute 1% of cosmic radiation.<ref>Schimmerling W. (2011, Feb 5). The Space Radiation Environment:  An Introduction. <nowiki>https://three.jsc.nasa.gov/concepts/SpaceRadiationEnviron.pdf</nowiki></ref>
  
  
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[[File:Cucinotta 2009 Fig. 4-3.png|thumb|412x412px|<ref name=":0">Cucinotta FA, Durante M. (2009). Risk of Radiation Carcinogenesis. In ''Human Health and Performance Risks of Space Exploration Missions''. NASA-SP-2009-3405. <nowiki>https://humanresearchroadmap.nasa.gov/Evidence/reports/EvidenceBook.pdf</nowiki></ref>Comparison of the ionization effects on nearby molecules produced by ions with different masses.]]
 
[[File:Cucinotta 2009 Fig. 4-3.png|thumb|412x412px|<ref name=":0">Cucinotta FA, Durante M. (2009). Risk of Radiation Carcinogenesis. In ''Human Health and Performance Risks of Space Exploration Missions''. NASA-SP-2009-3405. <nowiki>https://humanresearchroadmap.nasa.gov/Evidence/reports/EvidenceBook.pdf</nowiki></ref>Comparison of the ionization effects on nearby molecules produced by ions with different masses.]]
  
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Heavy ions passing through cells transfer more energy into a small volume, compared to other components of cosmic radiation.  This concentrated effect can produce qualitatively different types of cell damage.<ref name=":0" />
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Heavy ions passing through cells transfer more energy into a small volume, compared to other components of cosmic radiation.  This concentrated effect can produce qualitatively different types of cell damage.<ref name=":0" />  Linear energy transfer (LET) is a measure of the amount of energy deposited in tissue per unit length of a particle's trajectory.<ref>Wagenaar JD. (1995, Oct 6). Linear Energy Transfer. In ''Radiation Physics Principles'' (Section 7.2.3). <nowiki>http://www.med.harvard.edu/JPNM/physics/nmltd/radprin/sect7/7.2/7_2.3.html</nowiki></ref>  LET increases as a function of ion charge and mass, and decreases as a function of velocity.<ref>Wagenaar JD. (1995, Oct 6). Stopping Power. In Radiation Physics Principles (Section 7.1.2). <nowiki>http://www.med.harvard.edu/JPNM/physics/nmltd/radprin/sect7/7.1/7_1.2.html</nowiki></ref>  Experimental irradiation of mouse cell cultures has indicated that heavy ions with an LET greater than 10 keV/μm are more likely to cause irreparable cell damage, compared to protons or alpha particles.<ref>Wilson JW, Cucinotta FA, Thibeault SA, Kim M-H, Shinn JL, & Badavi FF. (1997, Dec). In JW Wilson, J Miller, A Konradi, & FA Cucinotta, (Eds.), ''Shielding Strategies for Human Space Exploration'' (pp. 109-149). NASA Conference Publication 3360. <nowiki>http://hdl.handle.net/2060/19980137598</nowiki></ref>
  
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The health effects of high doses of other types of radiation have been studied by analyzing the health of exposed groups (for example, survivors of nuclear weapon attacks or nuclear power plant accidents).  However, in the case of heavy ion radiation, estimates of the risk to astonauts are derived solely from animal model studies and application of biophysics principles.  As a result, these estimates are less certain.<ref name=":0" />
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The health effects of high doses of other types of radiation have been studied by analyzing the health of exposed groups (for example, survivors of nuclear weapon attacks or nuclear power plant accidents).  However, in the case of heavy ion radiation, estimates of the risk to astronauts are derived solely from animal model studies and application of biophysics principles.  As a result, these estimates are less certain.<ref name=":0" />
  
 
==Shielding Considerations==
 
==Shielding Considerations==

Revision as of 11:47, 26 August 2018

Heavy ions are charged particles heavier than alpha particles.[1] They constitute 1% of cosmic radiation.[2]


Exposures

[3]Abundances and energies of heavy ions in cosmic radiation.


Health Effects

[4]Comparison of the ionization effects on nearby molecules produced by ions with different masses.

Heavy ions passing through cells transfer more energy into a small volume, compared to other components of cosmic radiation.  This concentrated effect can produce qualitatively different types of cell damage.[4] Linear energy transfer (LET) is a measure of the amount of energy deposited in tissue per unit length of a particle's trajectory.[5]  LET increases as a function of ion charge and mass, and decreases as a function of velocity.[6]  Experimental irradiation of mouse cell cultures has indicated that heavy ions with an LET greater than 10 keV/μm are more likely to cause irreparable cell damage, compared to protons or alpha particles.[7]

The health effects of high doses of other types of radiation have been studied by analyzing the health of exposed groups (for example, survivors of nuclear weapon attacks or nuclear power plant accidents). However, in the case of heavy ion radiation, estimates of the risk to astronauts are derived solely from animal model studies and application of biophysics principles.  As a result, these estimates are less certain.[4]

Shielding Considerations

References

  1. ↑ Heavy ion. (1998, Jul 20). In Encyclopaedia Britannica. https://www.britannica.com/science/heavy-ion
  2. ↑ Schimmerling W. (2011, Feb 5). The Space Radiation Environment: An Introduction. https://three.jsc.nasa.gov/concepts/SpaceRadiationEnviron.pdf
  3. ↑ Schimmerling W. (2011, Feb 5). The Space Radiation Environment: An Introduction. https://three.jsc.nasa.gov/concepts/SpaceRadiationEnviron.pdf
  4. ↑ 4.0 4.1 4.2 Cucinotta FA, Durante M. (2009). Risk of Radiation Carcinogenesis. In Human Health and Performance Risks of Space Exploration Missions. NASA-SP-2009-3405. https://humanresearchroadmap.nasa.gov/Evidence/reports/EvidenceBook.pdf
  5. ↑ Wagenaar JD. (1995, Oct 6). Linear Energy Transfer. In Radiation Physics Principles (Section 7.2.3). http://www.med.harvard.edu/JPNM/physics/nmltd/radprin/sect7/7.2/7_2.3.html
  6. ↑ Wagenaar JD. (1995, Oct 6). Stopping Power. In Radiation Physics Principles (Section 7.1.2). http://www.med.harvard.edu/JPNM/physics/nmltd/radprin/sect7/7.1/7_1.2.html
  7. ↑ Wilson JW, Cucinotta FA, Thibeault SA, Kim M-H, Shinn JL, & Badavi FF. (1997, Dec). In JW Wilson, J Miller, A Konradi, & FA Cucinotta, (Eds.), Shielding Strategies for Human Space Exploration (pp. 109-149). NASA Conference Publication 3360. http://hdl.handle.net/2060/19980137598
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