# Tag Info

19

The Sun fuses protons, and this is a very slow process because there is no bound state of two protons. Hydrogen bombs fuse deuterium and tritium, and this is much, much faster because there is a bound state of these nucleides. You might like to have a look at: How much faster is the fusion we make on earth compared to the fusion that happens in the sun? ...

4

The final stage of nucleosynthesis at the core of a massive star involves the production of iron-peak elements, mostly determined by competition between alpha capture and photodisintegration. The starting material is mostly Si28 and weak processes are unable to significantly alter the n/p ratio from unity on short enough timescales. Thus the expected outcome ...

4

Transmuting chemically significant quantities of one element to another using nuclear reactions is not cost effective for any naturally occurring element. Nuclear physics is the end of alchemy. Two examples I happen have off the top of my head: the "Fat Man" and "Little Boy" nuclear weapons deployed in the second world war each involved about $10^{24}$ ...

3

After doing some more research I found the answer to my question. The method I proposed was actually one of the first methods for hydrogen-boron fusion that was tested. It's called "fixed/solid target proton-boron-11 fusion". Experimentation very quickly showed that the method could not work because of two big problems: As #dmckee already commented above, ...

3

A very nice question about a common misconception in books on astrophysics (I've made the same mistake in a comment here). According to M.P. Fewell, the origin of this misconception lies in the theory of stellar nucleosynthesis and the abundance of the elements. While other nuclei have higher binding energy per nucleon, $^{56}\mathrm{Fe}$ is more abundant ...

2

You question isn't specific enough; it needs a little work to clarify the fusion setup. For example, what fuel type are you talking about fusing? Is there confinement, so that this is a thermal fusion reaction, or would just one fusion reaction be sufficient? For example, the temperature required to overcome the Coulomb barrier for deuterium-tritium ...

2

Jupiter will never (not on any timescale like the lifetime of the Sun anyway) accrete enough mass to begin hydrogen fusion. It would need to accrete 12 times its current mass to undergo a brief period of fusing its interior deuterium and to accrete more than 70 times its current mass to attain a central temperature high enough to sustain hydrogen (pp chain) ...

1

I'm not entirely sure what you mean about 'pulling hydrogen', all bodies, whether they be planets or literally human bodies, will pull hydrogen via gravity. Earth can lose the H it attracts as H is so light that it can have speeds greater than the escape velocity (just due to random thermal motion). Perhaps Jupiter is sufficiently massive that this happens ...

Only top voted, non community-wiki answers of a minimum length are eligible