Can We Detect Uranium and Thorium Fusion in Stars Through Spectral Analysis?

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The discussion centers on the possibility of detecting uranium and thorium fusion in stars through spectral analysis. Participants question whether these heavy elements form in stars similarly to lighter elements like helium and carbon-iron. There is a consensus that if fusion occurs, it should be detectable by analyzing the light emitted from stars. References to supernova nucleosynthesis suggest that heavy elements are primarily formed in such explosive events. Overall, the feasibility of identifying uranium and thorium fusion in stellar environments remains an open question.
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If elements like uranium and thorium in fact did form the same way helium and carbon-iron do, which is through fusion. would we be able to know? Is there a way to tell if those elements are forming through fusion in the cores of stars? Like would it be possible to analyze the light coming from stars and determine whether not uranium/thorium fusion takes place

thanks
 
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dangerbird said:
If elements like uranium and thorium in fact did form the same way helium and carbon-iron do, which is through fusion. would we be able to know? Is there a way to tell if those elements are forming through fusion in the cores of stars? Like would it be possible to analyze the light coming from stars and determine whether not uranium/thorium fusion takes place

thanks

Well, I don't believe we have any alternate hypothesis about how heavy elements form. If not in stars, then where?
 
vibjwb said:
Supernova
Yes. I wasn't making a distinction about how stars do it, just that it's stars. That was misleading.
 
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