Remains of collapsed stars as touching binary planets?

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Discussion Overview

The discussion revolves around the hypothetical scenario of a binary star system evaporating or exploding, leaving behind two solid metallic spheres, specifically focusing on the feasibility of such an event and the nature of the remnants. Participants explore the implications of stellar events on the formation of heavy elements like gold and the dynamics of contact binary systems.

Discussion Character

  • Exploratory
  • Conceptual clarification
  • Debate/contested

Main Points Raised

  • One participant questions the physical possibility of a binary star system leaving behind solid metallic spheres that maintain their shapes rather than collapsing into a larger sphere.
  • Another participant references Kleopatra as an example of a non-spherical object but argues that planet-sized objects typically do not remain as solid spheres due to gravitational forces.
  • It is proposed that stellar events do not produce alloys of scarce elements, suggesting that remnants would primarily consist of iron or carbon.
  • A participant inquires whether any stellar event could produce an Earth's mass of gold and discusses the conditions under which two such masses could remain in contact without aggregating.
  • Concerns are raised about the likelihood of producing gold through stellar events, with one participant likening it to an improbable random event.

Areas of Agreement / Disagreement

Participants express differing views on the feasibility of producing solid metallic remnants from stellar events, particularly regarding the formation of gold and the dynamics of contact binary systems. The discussion remains unresolved with multiple competing perspectives presented.

Contextual Notes

Participants note the complexity of stellar processes and the rarity of certain events, highlighting the dependence on specific conditions and definitions related to stellar remnants and gravitational interactions.

Who May Find This Useful

Writers and enthusiasts interested in astrophysics, particularly those exploring the physical accuracy of speculative scenarios involving stellar remnants and binary systems.

dconnell
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Would it be in any way physically possible for a binary star system to evaporate / explode, leaving behind two spheres of a solid metal such as gold (or an alloy), which were then rigid enough to drift together and maintain their shapes, rather than just collapsing into a larger sphere?

And, for bonus points, does anyone know any kind of gravity simulation software I could use to map what that combined field would look like?

Thanks.
 
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Kleopatra fits that description.

Not a planet. Planet sized objects always morph into spheroids or bud off moons and/or debris.

Stars won't leave behind any alloy made of scarce elements. You could get a ball of mostly iron or one made of mostly carbon etc. Events that create gold will also create the other heavy elements.

The Rouche lobe might be the model you want.
 
Thanks for the reply. This is for a story I'm writing, which I want to be as physically accurate as possible, but I'm not a physicist...

A couple follow on questions if that's ok (I've googled but not quite found the answers):

Could any stellar event produce about an Earth's mass of gold?

If that mass was homogeneous/solid, ie not a rubble pile, and cold without a distinct core, would two of these masses in contact still definitely aggregate?

What if they were orbiting each other such that the centrifugal force was enough to keep them touching but separate, even if only for a couple million years or so?

None of this has to be at all likely, just not physically impossible under exactly the right conditions.

And what keeps contact binary stars which don't combine from doing so?

Cheers.
 
dconnell said:
Could any stellar event produce about an Earth's mass of gold?
You mean a 'random' event, as opposed to some 'Engineered' event? Pretty definitely NO, I'm afraid.
Like throwing a shuffled pack of cards on the table and picking them up in order without looking - but much more so.
 

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