Iron Fusion in Stars: Uncovering the Mysteries of Heavy Elements on Earth

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SUMMARY

Heavier elements found on Earth, such as plutonium, originate from supernovae and other energetic cosmological events, rather than from stellar fusion processes that cease at iron. The discussion clarifies that all plutonium used in nuclear industries is artificially produced by bombarding uranium with slow neutrons. The half-life of heavy elements, like plutonium's 24,000 years, indicates their decay rate but does not preclude their presence on Earth in excavatable quantities due to their long-term stability over multiple half-lives.

PREREQUISITES
  • Understanding of stellar fusion processes, specifically the role of iron as the last fusion stage.
  • Knowledge of supernova events and their significance in element formation.
  • Familiarity with radioactive decay and half-life concepts.
  • Basic principles of nuclear chemistry, particularly plutonium production methods.
NEXT STEPS
  • Research the process of element formation during supernova events.
  • Learn about the methods of plutonium production in nuclear reactors.
  • Explore the implications of half-life in the context of radioactive elements.
  • Investigate the differences between nova and supernova phenomena.
USEFUL FOR

Astronomers, nuclear physicists, and anyone interested in the origins of heavy elements and their implications in both cosmic and terrestrial contexts.

Atload
[SOLVED] Iron Fusion In Stars

If iron is said to be the last stage of fusion in stars, how is it that heavier elements are found on earth, where there seems to be less likely a chance for such fusion to occur? Where do these elements come from? Moreover, the half-life of a heavy element on the order of plutonium is only 24,000 years--how did such an element wind up on Earth in quantities that can be excavated? How is it that these elements were created?
 
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Originally posted by Atload
If iron is said to be the last stage of fusion in stars, how is it that heavier elements are found on earth, where there seems to be less likely a chance for such fusion to occur? Where do these elements come from? Moreover, the half-life of a heavy element on the order of plutonium is only 24,000 years--how did such an element wind up on Earth in quantities that can be excavated? How is it that these elements were created?
http://aether.lbl.gov/www/tour/elements/stellar/stellar_a.html

And:

http://photon.phys.clemson.edu/wwwpages/StarLife.html
 
Originally posted by Atload
Moreover, the half-life of a heavy element on the order of plutonium is only 24,000 years--how did such an element wind up on Earth in quantities that can be excavated?

It doesn't. All the plutonium used in today's nuclear industries is bred by bombarding uranium with slow neutrons.
 
Naturally occurring elements heavier then Iron are a result of a star going Nova or other such energetic cosomologic events. The energies present in such an event create the heavier elements.
 
how did such an element wind up on Earth in quantities that can be excavated?
The half life is a measure of the exponential decay of these elements. It is a record of how often they randomly decay, a matter of statistical probability than absolute. In two half lives, you have a quarter of the atoms still around. So, the element can last for a very long time with a relatively short half-life. Just significantly smaller numbers than originally.
 
Originally posted by Integral
Naturally occurring elements heavier then Iron are a result of a star going Nova or other such energetic cosomologic events. The energies present in such an event create the heavier elements.

supernova...not nova
(different phenomena, but similar names)
 

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