How long would it take the Universe to generate an Earth-like chemistry?

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SUMMARY

The discussion centers on the time required for the Universe to generate an Earth-like chemistry, emphasizing the role of supernovae and star formation. The Universe is approximately 14 billion years old, with Earth forming around 4.5 billion years ago, suggesting that the necessary chemical elements could have been produced within 2 billion years. Early stars formed within the first billion years, and their lifespans, alongside the mixing and dispersal of heavier elements, are crucial in determining the timeline for the emergence of life-supporting chemistry. The conversation highlights the complexity of identifying essential trace elements and their varying roles in biological functions.

PREREQUISITES
  • Understanding of stellar evolution and supernova processes
  • Familiarity with the periodic table and essential elements for life (e.g., CHONPS)
  • Knowledge of planetary formation theories
  • Basic grasp of chemical element distribution in the Universe
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  • Research the life cycles of first-generation and second-generation stars
  • Explore the role of supernovae in element synthesis and distribution
  • Study the chemical requirements for life and the significance of trace elements
  • Investigate the timeline of planetary system formation in relation to stellar events
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Astronomers, astrophysicists, and biochemists interested in the origins of life and the chemical evolution of the Universe.

BillTre
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Our planet (Earth) has a wide variety of different elements, which at some time had to be generated (presumably in stars) and distributed through space to new forming planets (like ours), when the stars exploded.
What is the minimal amount of time needed for this to happen?

It has often been hypothesized that many different elements were required for chemically based life (at least like what we are familiar with) to form. I am interested in limits that the availability of a varied chemistry could have hadon an earlier generation of life.
If we take the age of the universe as about 14 billion years, and the age of the Earth as about 4.5 billion years, the universe would have been about 9.5 billion years old.
What are the life spans of early exploding stars compared with that time?
 
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I think it's going to be hard to say without some idea of how much heavier elements is enough.
As long as one just needs any amount whatsoever - First stars started to form within the first billion years, and the most massive of those died after a few million. Add an extra few or a few dozen million for the material to disperse, mix, and start coalescing again. Probably a good bet to say less than 2 billion years overall. The longer one waits, the higher the concentrations, on average.
 
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I agree with @Bandersnatch that it's hard to pit an exact date on it because there's not a hard edge. Solar systems half as prevelent as today? One percent? One in a million? One per galaxy? Where do you draw the line?

The time scale for supernovae is a few million years. The time scale for planetary system formation is a few tens of millions. The mixing time is probably a hundred million years or so, but mixing doesn't have to be complete.
 
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Would it makes sense to approach this from a star generations point of view instead of a regular time frame? For example numerous 2nd generation stars and a handful of 3rd generation stars dieing to produce the required chemical elements perhaps? However long that may take?
 
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Thanks for the responses.

A lack of sharp resolution on the when this might have occurred is not surprising to me.

I suppose that getting enough stars to blow out the larger atoms they generate and then having that come together with some reasonable amount of heavier atoms (as some have said) could prolong how long it might take to make planets with higher atomic weights like earth.
Perhaps a lot faster where there were a lot of super big early stars (if such an area existed).
 
CHONPS are often cited as the elements that compose most of Earth's living matter.
However, there are 50 some elements found in (needed?) small amounts for modern biological functioning, due to requirements for metals and other things for catalysis (as in enzymes).
Its not easy to figure out what among all this is really needed in what amounts.
 
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What trace elements are necessary is going to lead us down the path of fruitless speculation. Is iron required? Probably not, as there are bloods that use alternatives, like copper, vanadium, and arguably magnesium. I'm not sure what a parade of counter-factuals tells us.
 
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Yeah, its kind of a mess to think about.
Fe is really common in a lot of enzymes, but as you say, it can be replaced in many cases.
 

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