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We have melanin in our skin to block radiation from the sun. Now there's a difference. The sun is emitting thermal radiation of about a million degrees celcius.
by waps 13y ago
We have melanin in our skin to block radiation from the sun. Now there's a difference. The sun is emitting thermal radiation of about a million degrees celcius. The energy profile of it's radiation is very well studied. It's basically random radiation with every individual photon being in a defined (and quite low) energy interval.
Radiation in space is totally random over the entire spectrum. There aren't many events at all (compared to the sun's radiation you could be forgiven for claiming there isn't any radiation in space at all, so few photons), but the events that do happen have a totally random energy distribution. Meaning most of the rays have enough energy to knock 2 or 3 molecules from the front of your finger into your brain. Or (a very tiny) part of the casing of the ship into deep into your body. If you measure space radiation with your sensor pointed down towards this massive rock we're living on, using the entire mass of the planet to block the radiation, the meter does not go down to zero (even when you eliminate the radiation produced by the planet itself).
Metals have a bit of an advantage blocking radiation because they have collective electron orbitals. If radiation impacts an electron inside a metal structure, it's going to throw it centimeters, meters away, maybe even kilometers. But here's the difference : that energy can be dissipated all around the structure. In other words, just because an electron gets an energy boost and gets thrown all around the room does not mean it has left it's orbital at all, and so it should remain inside the metal plate. If it does, the radiation is blocked. It's a sort of "structural integrity" field : the energy delivered does not have to beat the magnetic field of a single atom, but the magnetic field of the entire lattice. Unfortunately, on a per-atom basis, metal magnetic fields are on the very low side (mostly).
Ideally you'd use compressed plasma clouds to block radiation. But the energy required for maintaining that is rather enormous. But it would block pretty much all radiation (this is the reason the early universe, despite producing more photons in essentially empty space than the fusion reaction in the sun does today, was "completely dark". Those photons couldn't travel, so they'd never hit any sensor)
This is the problem with space radiation. Once radiation energy levels go above certain "reasonable" energy levels blocking it becomes a pipe dream.
- TheEzEzz 13y ago"If you measure space radiation with your sensor pointed down towards this massive rock we're living on, using the entire mass of the planet to block the radiation, the meter does not go down to zero (even when you eliminate the radiation produced by the planet itself)." Can you explain this further? Wouldn't it suggest that we're exposed to the same radiation while on Earth?
- waps 13y agoIt's not that the atmosphere does not protect us. Just not 100%, which shows just how much energy (a tiny fraction of) these particles have. So yes, you get a few atoms in your body blown off by a cosmic ray once every few months or so. In space you can expect that to increase to several times per second (as compared to solar rays, which of course constantly hit). This was a statement meant to illustrate that so far we haven't really found an upper bound for the energy levels of these particles. Give a particle enough energy and it'll fly right through the planet. http://en.wikipedia.org/wiki/Cosmic_ray http://en.wikipedia.org/wiki/Cosmic_ray The interesting thing is that we don't actually know where most of these rays come from (about 1 in 100 million comes from a supernova/black hole/other known powerful event). So something is pretty much everywhere in space, shoots out particles like a particle accelerator, except much more powerful than the ones we can build. Yet whatever is doing this manages to avoid detection by any other means.