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shallowdeep -> RE: Asteroid mining (5/1/2012 11:41:22 PM)
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Radiation is obviously a concern that deserves consideration when in space, especially if not in equatorial LEO, but you did start off by writing that it would be impossible to live without "a superconducting electromagnet to deflect cosmic and solar radiation." Taken literally, that was, at best, an exaggeration. Some solar flares could potentially be lethal to astronauts with no protection, but it's relatively easy to shield against the resulting solar particle events and the risk of any acute effect while inside a spacecraft is considered to be extremely unlikely. [Source: Risk of Acute Radiation Syndromes Due to Solar Particle Events] The other major concern, galactic cosmic rays, are much more challenging to shield against due to the production of extensive secondary radiation, but the radiation is present at significantly lower levels and would not cause any acute early effects. The risk with GCRs is confined to late effects: namely cancer, but also gradual tissue damage to the eye's lens and potentially to the central nervous system. Because the biological effects of high energy heavy ion (HZE) impacts can't be studied on Earth outside of particle accelerators (that physicists are undoubtably loathe to share with mere biologists), there's still a fair bit of uncertainty about what quality factor cosmic radiation, and the HZE particles in particular, should be assigned. Still, it's clear exposure is not going to be an immediate risk to life. As part of planning for a trip to Mars, NASA studied the issue in 2001. Using the guideline that a 3% increase in cancer mortality above the background of average cancer mortality in the US population would be an acceptable level of risk, the report calculated that, with only standard shielding, there is 95% confidence that it would take 268 days or more of exposure for a 55-year-old male to reach that risk level – but the exposure duration would be less for younger astronauts and for females. [Source: Space Radiation Cancer Risk Projections For Exploration Missions] For trips to a nearby captured asteroid, the radiation risk really isn't a show-stopper. For longer trips, like to Mars, it might well be. In 2004, NASA put the most probable cancer risk of a 1000-day mission at 3.4%, but with uncertainty ranging from 1% to 19%. [Source: Can People Go to Mars?] Those sorts of extended deep space trips are where massive or novel radiation shielding against GCRs could be required. Passive mass shielding currently seems closer to being practical than any active shielding scheme, and has the benefit of being simple and guaranteed to work. The obvious downside is getting the required mass into space. To heavily shield a practically-sized crew compartment would require around 400 tons of mass by one calculation. [Source: Shielding Space Travelers] That's the equivalent of the entire ISS (or two Saturn V-equivalent payloads) just for the shielding, probably cost prohibitive with NASA's current budget and lift capacity. The motivation behind active shielding is that it might reduce the expensive mass required, but despite more than 40 years of investigation, it's not yet clear that any proposed design would actually be able to do that, even assuming the significant technical issues posed could be overcome. From the 2000 Townsend paper you cited earlier: "None of the active shielding methods proposed to date appear to offer a weight savings over bulk material shielding when considering the entire deep space environment." Similarly, a group of experts convened by NASA to investigate revolutionary alternatives for shielding concluded in 2005 that "none of the electromagnetic concepts showed clear promise." [Source: Revolutionary Concepts of Radiation Shielding for Human Exploration of Space] Some of the ideas are interesting and admittedly kind of cool, but at best they are still a ways away from any practical realization. Mining asteroids, if it pans out, actually promises a solution to the shielding problem: If it need not be launched from Earth, shielding mass suddenly becomes much more affordable. Besides use as a fuel, enough water from an asteroid could also make very effective shielding for a crewed spacecraft. quote:
ORIGINAL: FrostedFlake I know a little about radiation… Up there you also find Cosmic Radiation and X-rays, both similar enough to Gamma that you can lump them together and all susceptible to magnetic fields. I see. Is it the electric charge of a photon, or a photon's mass that makes it susceptible to magnetic fields? Can we lump gamma rays with cosmic rays because of the close similarity in mass? Or was it in velocity? Or maybe just that they both have the word "ray" in the name? Why didn't my EM theory classes or health physics text cover this stuff! :)
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