Radiation issues for piloted Mars mission.
Man is now entering an era of colonizing the moon and exploration of Mars.  The crewmembers of a piloted mission to Mars will be exposed to inner belt trapped protons, the outer trapped electrons, and the galactic cosmic radiation.  In addition there is always the added risk of acute exposure to a solar particle event.  Current radiation risk is estimated using the idea of absorbed dose and ICRP-26, LET-dependent quality factors.  In a spacecraft with aluminum walls (2 g cm-2) at solar minimum the calculated dose equivalent is 0.73 Sv for a 406-day mission.  Based on the current thinking this leads to an excess cancer mortality in a 35 year male of about 1%.  About 75% of the dose equivalent is contributed by HZE particles and target fragments with average quality factors of 10.3 and 20, respectively.  The entire concept of absorbed dose, quality factor, and dose equivalent as applied to such missions needs to be reexamined, in light of the fact that less than 50% of the nuclei in the body of the astronaut would have been traversed by a single GCR nuclei in the 406-day mission.  Clearly, more biologically relevant information about the effects of heavy ions and target fragments is needed and fluence based risk estimation strategy developed for such long term stays in space.
Badhwar
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Solar System Exploration Division, NASA Johnson Space Center, Houston, TX 77058.
Nachtwey
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Yang TC-H
D000328:Adult; D000818:Animals; D016923:Cell Death; D002471:Cell Transformation, Neoplastic / Q000528:radiation effects*; D003359:Cosmic Radiation / Q000009:adverse effects; D004583:Electrons / Q000009:adverse effects; D006801:Humans; D018499:Linear Energy Transfer; D018535:Mars; D051379:Mice; D011522:Protons / Q000009:adverse effects; D011829:Radiation Dosage; D011835:Radiation Protection / Q000592:standards / Q000706:statistics & numerical data*; D012062:Relative Biological Effectiveness; D012306:Risk; D013026:Space Flight
D011522:Protons