Billy-o
04-19-2010, 03:44 PM
Waaay back when I took a Nuclear Chemistry course in college, we learned about how elements heavier than iron are formed in supernovae, thanks to the tremendous enegies released, which allows fusion of larger nuclei.
We also learned that, although all the trans-uranium elements are radioactive and usually have short half lives, there are predicted to be some superheavy elements occupying an "island of stability" in the periodic table. These elements would have longer half lives, and might even be stable. Currently, I believe these elements are predicted to have atomic numbers 120, 124, and 126 -- significantly heavier than any man-made elements.
My question is: do supernovae produce energies high enough to synthesize these hypothetical elements? If so, can we predict what their spectral signatures would look like well enough to detect them (assuming they exist)? This would be a very cool discovery!
We also learned that, although all the trans-uranium elements are radioactive and usually have short half lives, there are predicted to be some superheavy elements occupying an "island of stability" in the periodic table. These elements would have longer half lives, and might even be stable. Currently, I believe these elements are predicted to have atomic numbers 120, 124, and 126 -- significantly heavier than any man-made elements.
My question is: do supernovae produce energies high enough to synthesize these hypothetical elements? If so, can we predict what their spectral signatures would look like well enough to detect them (assuming they exist)? This would be a very cool discovery!