How did elements and building blocks of life arrive on Earth?

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Discussion Overview

The discussion revolves around the origins of elements and the building blocks of life on Earth, exploring how these materials arrived from space and their implications for the development of life. The conversation touches on theories of element formation in stars, the role of supernovae, and the processes involved in the early Earth's chemical composition.

Discussion Character

  • Exploratory
  • Debate/contested
  • Technical explanation

Main Points Raised

  • One participant questions how heavier elements arrived on Earth, noting the necessity of large amounts of carbon for the emergence of life and the challenges posed by the distances of stars.
  • Another participant states that the Solar System formed from a nebula created by a supernova, asserting that all naturally occurring isotopes beyond iron are produced in such events.
  • It is suggested that while some of Earth's minerals were deposited by meteors and comets, the majority coalesced from the original nebula, which was enriched by multiple supernovae.
  • A participant raises a question about whether the original nebula was the result of a single supernova or a collection of supernovae, highlighting the complexity of the galaxy's history.
  • Another participant emphasizes the improbability that all elements originated from a single supernova, noting the historical prevalence of supernovae in the galaxy.
  • A later post mentions the discovery of a building block of RNA in an asteroid, suggesting that not only elements but also essential compounds for life may have arrived on Earth from extraterrestrial sources.

Areas of Agreement / Disagreement

Participants express differing views on the origins of elements, particularly regarding the role of supernovae and whether a single event or multiple events contributed to the material present on Earth. The discussion remains unresolved with multiple competing perspectives.

Contextual Notes

Participants acknowledge the complexity of the processes involved in the formation and cooling of the Earth, which leads to a heterogeneous distribution of materials. There are also references to the limitations of current models regarding the origins of elements and the early Earth's conditions.

Aziza
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we are currently learning about radioactivity and i have become curious of how these heavier elements came to Earth in the first place? From what i understand, the lighter elements are formed by fusion in stars, but even so, how could these lighter elements reach us when the stars are so far away? I could see perhaps some of the elements reaching us as dust or something, but how did enough of it reach us to allow for start of life? I mean carbon for example is absolutely essential to life, so we would need extremely large amount of it for the first living cells to begin synthesizing themselves.

Also, according to current model, the early Earth was big glob of lava and whatnot, so all of the chemicals must have been mixing around all together, so then why today we have more or less even "deposits" of certain chemicals, like uranium? I mean if in liquid form the Earth was all mixed up, then how come when it cooled, it became more ordered in terms of chemical composition?
 
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The nebula from which the Solar system was created was from a Supernova from a previous generation. All naturally occurring isotopes beyond [itex]^{56}\mathrm{Fe}[/itex] are created that way.
 
Yup, while a nonzero potion of the Earth's minerals were deposited by meteors, comets and falling space dust, the vast bulk of the Earth coalesced at the same time as the the other planets and the sun from the original collapsing nebula. That original nebula of gas an dust is the remnants of earlier supernovae ejecta.

The reason it isn't all perfectly homogenous is because parts of the Earth cool at different rates, heavier parts sink, lighter parts float so you get sedimentation layers - and then - tectonic activity stirs it all up.

And that's an ubersimplification. The dynamics of a forming and cooling planet are very complex and result in a great degree of heterogeny in materials.
 
Dickfore said:
The nebula from which the Solar system was created was from a Supernova from a previous generation.

Are sure that is was a single supernova and not a protostellar nebula enriched with metals by many supernovas?
 
DrStupid said:
Are sure that is was a single supernova and not a protostellar nebula enriched with metals by many supernovas?

It is highly unlikely that ALL of the elements came from 1 supernova. The galaxy has been riddled with supernovae since it's initial formation 12+ billion years ago.
 
Just heard on tv a few nights ago something even more astonishing: One of the four building blocks of RNA [AGTC] was found just a few years ago in an asteroid or meteor found here on earth...I think it was "G"...

So not only the elements above Fe are here from supernovas, which is correct, but the building blocks for life may have arrived here from elsewhere as well...
 

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