- #1
yotta
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Main Question or Discussion Point
How much radioactive warming would occur in the astronomical body specified below?
I want to write a story about a very advanced civilization, not yet of Dyson Sphere capability, able to artificially create large planets up to Saturn's mass, of any composition. They decide to create one not orbiting any star, a "rogue" planet, using the radioactivity of one of the very long half-life isotopes to provide warmth for at least 10^21 years.
Composition:100% germanium-76, decay: β-β-, T1/2 ≈ 1.8×10^21y, decay energy = 2.039 MeV, incl. antineutrinos. Statistics relative to Earth: density ≈ 5.5 g/cm3, or ≈ 1.0⨁, radius ≈ 2.0⨁, mass ≈ 8.0⨁, gravity ≈ 2.0⨁. (This ignores gravitational compression, reducing the size and increasing the gravity somewhat.)
For a ballpark estimate, if all of the energy of radioactive decay occurring at the moment of T=0 arrived at the surface instantaneously, how close would the energy flux be to 20mW/m2? Of course, this first-approximation model ignores the heat absorbed by the planet, and the time for it to arrive at the surface. These can be dealt with later.
If it's too hot,* then they'd use <100% radioactive material. *I'm not sure exactly what "too hot" is; I'll want to see what I'm dealing with first to make that determination. Likewise for "too cold." Perhaps, a really thick layer of aerogel, say one kilometer, might be able to prevent any more than one mW/m2 of energy escaping, or even less.
2x Earth atmospheric pressure is desirable to fully protect the surface, which would be the mass of one atmosphere above any given area. It would be 100% helium-3, because all other gases would freeze, and this very light gas would be easily retained by 2x Earth gravity, in the absence of any star. (O2 is provided in underground rooms for breathing.)
The ability to create this planet is, of course, highly speculative, and is not what my question is about, which is the quantity of heat generated by radioactive decay within this body in our known universe. If the heat generated is truly insufficient, then other somewhat "faster" decay isotopes could be used.
The purpose of the planet is to be a great repository of knowledge, to be to "all races in physical reality" what the Library at Alexandria was on Earth. Movies, music, and news videos are of particular interest to alien races, as they are informative of a civilization, but need for someone to explain them, in order to be entirely so. And, individuals from each species to observe in person. Hidden video cameras might be placed in civilizations not having video media.
How much radioactive warming would occur in the astronomical body specified below?
I want to write a story about a very advanced civilization, not yet of Dyson Sphere capability, able to artificially create large planets up to Saturn's mass, of any composition. They decide to create one not orbiting any star, a "rogue" planet, using the radioactivity of one of the very long half-life isotopes to provide warmth for at least 10^21 years.
Composition:100% germanium-76, decay: β-β-, T1/2 ≈ 1.8×10^21y, decay energy = 2.039 MeV, incl. antineutrinos. Statistics relative to Earth: density ≈ 5.5 g/cm3, or ≈ 1.0⨁, radius ≈ 2.0⨁, mass ≈ 8.0⨁, gravity ≈ 2.0⨁. (This ignores gravitational compression, reducing the size and increasing the gravity somewhat.)
For a ballpark estimate, if all of the energy of radioactive decay occurring at the moment of T=0 arrived at the surface instantaneously, how close would the energy flux be to 20mW/m2? Of course, this first-approximation model ignores the heat absorbed by the planet, and the time for it to arrive at the surface. These can be dealt with later.
If it's too hot,* then they'd use <100% radioactive material. *I'm not sure exactly what "too hot" is; I'll want to see what I'm dealing with first to make that determination. Likewise for "too cold." Perhaps, a really thick layer of aerogel, say one kilometer, might be able to prevent any more than one mW/m2 of energy escaping, or even less.
2x Earth atmospheric pressure is desirable to fully protect the surface, which would be the mass of one atmosphere above any given area. It would be 100% helium-3, because all other gases would freeze, and this very light gas would be easily retained by 2x Earth gravity, in the absence of any star. (O2 is provided in underground rooms for breathing.)
The ability to create this planet is, of course, highly speculative, and is not what my question is about, which is the quantity of heat generated by radioactive decay within this body in our known universe. If the heat generated is truly insufficient, then other somewhat "faster" decay isotopes could be used.
The purpose of the planet is to be a great repository of knowledge, to be to "all races in physical reality" what the Library at Alexandria was on Earth. Movies, music, and news videos are of particular interest to alien races, as they are informative of a civilization, but need for someone to explain them, in order to be entirely so. And, individuals from each species to observe in person. Hidden video cameras might be placed in civilizations not having video media.
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