Why We Have Heavy Elements on Earth

  • Context: Graduate 
  • Thread starter Thread starter paweld
  • Start date Start date
  • Tags Tags
    Earth Elements
Click For Summary
SUMMARY

Heavy elements on Earth, such as uranium and lead, originate from supernova explosions, not from the Big Bang or stellar nucleosynthesis processes, which only produce elements up to iron and nickel. The "S-process" and "R-process" in stellar nucleosynthesis are responsible for the creation of these heavier elements during supernova events. The Milky Way has experienced approximately one supernova per century over billions of years, contributing to the interstellar material from which the solar system formed. Consequently, the solar system had access to a rich supply of heavy elements due to the numerous supernovae that occurred 6-9 billion years ago.

PREREQUISITES
  • Understanding of stellar nucleosynthesis, specifically the "S-process" and "R-process".
  • Knowledge of supernova mechanics and their role in element formation.
  • Familiarity with the timeline of the Milky Way's formation and evolution.
  • Basic concepts of interstellar material and its significance in planetary formation.
NEXT STEPS
  • Research the "S-process" and "R-process" in detail to understand how heavy elements are synthesized.
  • Explore the impact of supernova explosions on galactic evolution and interstellar material distribution.
  • Study the timeline of the Milky Way's formation and the frequency of supernovae over its history.
  • Investigate the role of heavy elements in planetary formation and their significance for life on Earth.
USEFUL FOR

Astronomers, astrophysicists, students of cosmology, and anyone interested in the origins of heavy elements and their implications for planetary formation.

paweld
Messages
253
Reaction score
0
Why we have (although very little) on Earth heavy elemnents such
as uranium, lead, ... if they weren't created in Big Bang or stellar nucleosynthesis
(these proceses don't produce elements heavier than iron and nickel).
Any guesses?
 
Astronomy news on Phys.org
No need to guess - these processes are well understood. Elements heavier than iron are produced primarily in supernova explosions, where there is a flood of neutrons which builds up the heavier elements. Look up the "S-process" and the "R-process" in stellar nucleosynthesis.
 
But is there any supernove near Earth?
 
Supernovae create massive shock waves which blow material out into the host galaxy. A galaxy like the Milky Way has on the order of about 1 supernova per century. Since the Milky Way was in existence for billions of years before the sun formed, there were millions of prior supernovae within the Milky Way, all churning up the interstellar material. So, when the solar system formed, there was an ample supply of heavy elements from supernovae with which to build the planets. As the song goes, "...we are stardust..."
 
Yes, it's now clear.
Thanks.
 
Numerous supernova contributed matter to the proto cloud from which the solar system formed. Mostly from 6-9 billion years ago.
 

Similar threads

  • · Replies 28 ·
Replies
28
Views
4K
  • · Replies 34 ·
2
Replies
34
Views
6K
  • · Replies 3 ·
Replies
3
Views
2K
  • · Replies 2 ·
Replies
2
Views
3K
Replies
0
Views
1K
  • · Replies 10 ·
Replies
10
Views
3K
  • · Replies 6 ·
Replies
6
Views
2K
  • · Replies 7 ·
Replies
7
Views
5K
  • · Replies 4 ·
Replies
4
Views
3K
  • · Replies 12 ·
Replies
12
Views
2K