Remains of collapsed stars as touching binary planets?

In summary: 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?That is a difficult question. If they were tightly packed, then sure. If they were more loosely packed, then it would depend on how well they were held together. 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?If two objects are kept in contact by a force (such as gravity), they will stay in contact as long as the force is present. If the force is removed, the objects will eventually separate.
  • #1
dconnell
2
0
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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  • #2
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.
 
  • #3
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.
 
  • #4
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.
 

FAQ: Remains of collapsed stars as touching binary planets?

What are "Remains of collapsed stars as touching binary planets"?

"Remains of collapsed stars as touching binary planets" refers to a hypothetical scenario where two planets orbit each other so closely that their surfaces are touching. These planets are thought to have formed from the remains of a collapsed star, such as a white dwarf or neutron star.

How do these binary planets form?

It is believed that these binary planets form from the remnants of a collapsed star. As the star collapses, its outer layers are ejected into space, forming a disk of material around the remaining core. This disk can then coalesce into two planets that orbit each other closely.

Are there any known examples of "Remains of collapsed stars as touching binary planets"?

Currently, there are no confirmed examples of "Remains of collapsed stars as touching binary planets" in our own solar system or in any other known planetary systems. However, there are some binary systems where the two planets are very close together, and it is possible that they may have formed from the remains of a collapsed star.

What would be the potential implications of finding "Remains of collapsed stars as touching binary planets"?

If such a system were to be discovered, it would provide valuable insights into the formation and evolution of planetary systems. It could also challenge our understanding of how planets form and how close they can orbit each other without colliding.

How could we detect or observe "Remains of collapsed stars as touching binary planets"?

Currently, there are no specific methods for detecting or observing "Remains of collapsed stars as touching binary planets". However, future advancements in technology and space exploration may allow us to observe these systems indirectly through their gravitational effects on each other or through the detection of their atmospheres.

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