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What the heck is spalling? Didn't Al Bean himself admit they were too dumb to make it so they faked their way through van Allen?
Originally posted by Zaphod58
“We have also confirmed a new type of hydrogen storage material holds particular promise,” said Alessandra Menicucci, who is overseeing the project and notes that, “in general, the lighter a material’s atomic nuclei the better the protection.”
www.gizmag.com...
Originally posted by Zaphod58
reply to post by kiwasabi
That material is new, that's for a mission to Mars. However, read the last sentence. "In general, the lighter the material's atomic nuclei, the better the protection." That's completely relevant to the discussion.
Again, the shuttle wasn't designed to go through the Van Allen Belt, so it didn't have quite the same protection as the Apollo capsules did. The shuttle would stay up longer, but they were still in the magnetic field of the earth, so they were still somewhat protected by that, as well as their shielding. In 1998 they went into the Belt, so they were exposed to more than normal. Thus the difference.
And if you're going to keep talking about the Empire State Building crash, at least get it right. It was a B-25, not a B-52.
Originally posted by Zaphod58
reply to post by kiwasabi
The shuttle went into the lower bands of the Belts occasionally depending on the mission. The shuttle servicing missions for the Hubble would pass through the Belts during their orbit, because of the altitude of the Hubble. It depends on the experiments, and what altitude they had to be at. Some experiments required higher altitudes than others, to get clear of certain phenomenon around the Earth.
Originally posted by Zaphod58
reply to post by kiwasabi
Apollo relied a lot on the duration of the mission. They were looking at short term durations, and again, solar radiation can be stopped by relatively thin shielding. There was water circulating through their suits, which would help with some protection. The various layers of suits would also provide some shielding. Alpha particles are stopped by normal clothing. Beta particles aren't much stronger.
Originally posted by Zaphod58
It doesn't matter how many particles we're talking about, because they were there for a short time. You can have more particles, but that doesn't change the strength of the particles.
"We are in a period when the radiation risks are elevated, but still tolerable," Spence said, adding that the levels were about what an X-ray technician or uranium miner might normally experience in a year.
Originally posted by Zaphod58
reply to post by kiwasabi
"We are in a period when the radiation risks are elevated, but still tolerable," Spence said, adding that the levels were about what an X-ray technician or uranium miner might normally experience in a year.
news.discovery.com...
The sun is actually a very inefficient emitter when it comes to Gamma rays. I'll look up emissions from the sun tomorrow when I have time, but I remember reading that it's surprisingly low, so it's entirely possible for the moon to emit more than the sun, and still be well in the safe levels.
Actually, the Sun does not only produce IR, visible light, and UV. Fusion in the core actually gives off high energy gamma rays. However, as the gamma ray photons make their arduous journey to the surface of the Sun, they are continuously absorbed by the solar plasma and re-emitted to lower frequencies. By the time they get to the surface, their frequencies are mostly only within the IR/visible light/UV spectrum.
Apollo 11 was on the moon for nearly a full day, that is enough time for the radiation to seep through the suits and cause serious damage.
Naturally occurring background radiation is the main source of exposure for most people, and provides some perspective on radiation exposure from nuclear energy. The average dose received by all of us from background radiation is around 2.4 mSv/yr, which can vary depending on the geology and altitude where people live – ranging between 1 and 10 mSv/yr, but can be more than 50 mSv/yr. The highest known level of background radiation affecting a substantial population is in Kerala and Madras states in India where some 140,000 people receive doses which average over 15 millisievert per year from gamma radiation, in addition to a similar dose from radon. Comparable levels occur in Brazil and Sudan, with average exposures up to about 40 mSv/yr to many people.
Several places are known in Iran, India and Europe where natural background radiation gives an annual dose of more than 100 mSv and up to 260 mSv (at Ramsar in Iran, where some 200,000 people are exposed to more than 10 mSv/yr). Lifetime doses from natural radiation range up to several thousand millisievert. However, there is no evidence of increased cancers or other health problems arising from these high natural levels. The millions of nuclear workers that have been monitored closely for 50 years have no higher cancer mortality than the general population but have had up to ten times the average dose. People living in Colorado and Wyoming have twice the annual dose as those in Los Angeles, but have lower cancer rates.