How Does Gravity Influence Entropy in the Formation of Proto-Stars?

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Discussion Overview

The discussion revolves around the relationship between gravity, entropy, and the formation of proto-stars, exploring how gravitational collapse affects entropy in the context of astrophysical processes. It includes theoretical considerations and implications for both proto-stars and meteorite formation.

Discussion Character

  • Exploratory
  • Technical explanation
  • Conceptual clarification
  • Debate/contested

Main Points Raised

  • One participant questions whether a proto-star has less entropy than the gas cloud from which it formed, seeking to understand how overall entropy can be considered increased during this process.
  • Another participant suggests that heat production during the collapse contributes to the increase in global entropy.
  • A participant posits that describing the motion of tightly-packed atoms in a proto-star may require more information than describing the random diffusion of atoms in a gas cloud, expressing a sense of counter-intuition regarding this idea.
  • It is noted that to fully understand the entropy change, one must consider not only the proto-star but also the heat radiation emitted and the expansion of the outer region of the proto-stellar disc during collapse.
  • A hypothetical scenario is introduced regarding rock fragments collapsing into a meteorite, questioning whether this process would also result in a higher temperature than the original fragments.
  • Another participant responds that the meteorite would need to either be much hotter than its original constituents or emit significant heat over time to account for entropy changes.

Areas of Agreement / Disagreement

Participants express differing views on the relationship between gravity, entropy, and temperature changes during the formation of proto-stars and meteorites. The discussion remains unresolved with multiple competing perspectives presented.

Contextual Notes

Participants highlight the need for additional information regarding energy conservation and the dynamics involved in the processes discussed, indicating that assumptions about heat emission and angular momentum conservation are critical to the arguments presented.

Islam Hassan
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If gravity leads, for example to a gas cloud gradually coalescing into a proto-star, does this proto-star not have less entropy than the gas cloud that engendered it? If yes, then in what sense is overall entropy increased, in what way can we say that entropy globally has been increased via the collapse of the gas cloud into a proto-star?IH
 
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Islam Hassan said:
in what way can we say that entropy globally has been increased via the collapse of the gas cloud into a proto-star?

heat production
 
So it would require more information to describe the motion of a proto-star's tightly-packed constituent atoms than than the random gaseous diffusion of atoms in a gas cloud? Seems counter-intuitive, which doesn't mean it's wrong though...IH
 
Islam Hassan said:
So it would require more information to describe the motion of a proto-star's tightly-packed constituent atoms than than the random gaseous diffusion of atoms in a gas cloud?

It mainly requires not to consider the resulting proto-star only but also the emission of heat radiation (to ensure conservation of energy) and the expansion of the outer region of the proto-stellar disc (to ensure conservation of angular momentum) during the collapse.
 
Ok, thanks DrS.

What if we consider instead rock fragments drifting in orbit and collapsing into one solid meteorite? No significant radiation, no disk. This meteorite would likewise have to be much hotter than its original constituents?IH
 
Islam Hassan said:
This meteorite would likewise have to be much hotter than its original constituents?

This or significant heat emission (within a sufficiently long period of time).
 
Last edited:
Ok, thanx...
 

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