Fate of outer planets after sun ends its life cycle

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Discussion Overview

The discussion revolves around the fate of the outer planets, particularly gas giants like Jupiter and Saturn, after the sun transitions through its life cycle, culminating in the white dwarf phase and potentially becoming a black dwarf. Participants explore the implications of these stages on planetary orbits and the eventual fate of the solar system.

Discussion Character

  • Exploratory
  • Debate/contested
  • Technical explanation

Main Points Raised

  • Some participants question whether white dwarf planets can "die" and what would happen to gas giants without a sun to orbit.
  • It is proposed that planets not ejected during the red giant phase will remain in stable orbits around a white dwarf, which eventually cools to a black dwarf, but this does not affect their orbits.
  • One participant argues that the sun does not truly "end" its life cycle, as becoming a black dwarf is still part of it.
  • There are inquiries about what happens after a black dwarf and whether the sun's matter could eventually disperse, affecting the dynamics of the solar system.
  • Some participants suggest that black holes might evaporate through Hawking Radiation, raising questions about similar mechanisms for other celestial objects over vast timescales.
  • There is a discussion about the mass loss of the sun during its red giant phase and how this affects planetary orbits, with estimates varying on the percentage of mass lost.
  • Participants discuss the potential decay of black dwarfs, with some suggesting that protons could decay and lead to their eventual disappearance, while others argue they might persist indefinitely.
  • Questions are raised about the role of black body radiation in the evaporation of black dwarfs, with differing views on whether it would be sufficient to cause significant mass loss.
  • One participant mentions that cooling in the expanding universe could eventually lead to the evaporation of solid objects, albeit very slowly.
  • There are references to the concept of thermal equilibrium and whether any objects in the universe currently exist in such a state.
  • The discussion touches on the visibility of interstellar meteoroids in thermal imaging, with some asserting that those far from stars would not be detectable.

Areas of Agreement / Disagreement

Participants express multiple competing views regarding the fate of the sun and its remnants, the stability of planetary orbits, and the implications of black body radiation and thermal equilibrium. The discussion remains unresolved with no consensus on many of the speculative aspects raised.

Contextual Notes

Participants acknowledge various assumptions about mass loss during the red giant phase, the mechanisms of decay for black dwarfs, and the effects of cosmic expansion on cooling and evaporation, but these remain unresolved and depend on further clarification of definitions and theories.

gfd43tg
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Do white dwarf planets ever die and eventually there will be no remains of the sun? What will happen to the gas giants with no sun to orbit?
 
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After a star enters the white dwarf phase, any planets not ejected during the red giant phase will remain in stable orbits. A white dwarf eventually cools and becomes a black dwarf, but, this has no effect on planetary orbits. It takes a very long time and our universe is not nearly old enough for any black dwarfs to yet exist.
 
And as a somewhat nit-picky aside, the answer to your subject line question is "the sun DOESN'T end its life cycle". Even when it turns into a black dwarf in the far distant future, that is still part of its life cycle.
 
Is there anything after a black dwarf? Does that matter in the sun ever disperse and there ceases to be any remains of a sun? I'm imagining a scenario where a star eventually disperses and all it's matter disperses throughout the universe. I'm wondering what would happen to Jupiter and Saturn in a case where all the matter of the sun was gone and the ''center'' of the solar system was no more.
 
Interesting question. I don't know. A black hole will eventually evaporate through Hawking Radiation (at least that's currently the belief) so perhaps there's a similar mechanism for other objects, over really vast amounts of time.
 
Chronos said:
After a star enters the white dwarf phase, any planets not ejected during the red giant phase will remain in stable orbits. A white dwarf eventually cools and becomes a black dwarf, but, this has no effect on planetary orbits. It takes a very long time and our universe is not nearly old enough for any black dwarfs to yet exist.

Ummmm, yes. But when the outer shells of the red giant are sloughed off, the mass of the star declines (by, perhaps, 80-90%?) and that changes the dynamics of the planets. Likely they will slow down and move to orbits farther out. Once the white dwarf is formed, its gravity is too high to allow more matter to easily leave, and from then on it has constant mass regardless of temperature, rotation or whatever else.
 
(by, perhaps, 80-90%?)
More like 50% for the sun, it depends on the mass of the star.

If protons decay, then black dwarfs will disappear after a very long time. Even if there is no conventional decay mechanism (which is unclear), they might be able to decay via virtual black holes.
If they do not decay, the black dwarf will stay there forever.

All objects in an orbit will lose energy to gravitational waves, the orbits will decay and they will crash onto the black dwarf (making it hotter for a comparatively short timescale).
 
Wouldn't black body radiation alone cause it to evaporate?
 
Flatland said:
Wouldn't black body radiation alone cause it to evaporate?

The whole point of a black dwarf is that they are in thermal equilibrium with space.
 
  • #10
Flatland said:
Wouldn't black body radiation alone cause it to evaporate?
Once it is cold, the energy is not sufficient to emit a significant number of atoms - not even in infinite time as cooling goes too fast, assuming eternal accelerated expansion of the universe.

A proton needs of the order of 10 to 100 keV to escape to space, at a temperature of 1 meV (~12 K, still warmer than the current cosmic microwave background) this gives a suppression of (upper estimate) ##e^{-10^7} \approx 0##. There is still some radiation pressure increasing the chance of an escaping particle a bit, but as soon as the black dwarf is cold, even that does not help any more.
 
  • #11
Cooling stops after some time in the expanding universe because of the radiation from cosmological horizons, so all solid objects will evaporate (of course, extremely slowly)
 
  • #12
tzimie said:
Cooling stops after some time in the expanding universe because of the radiation from cosmological horizons, so all solid objects will evaporate (of course, extremely slowly)

Did you not read post #10 or did you think it is wrong? Do you have any citations to back up what appears to be a personal theory?
 
  • #13
Of course it is not my personal theory. I read about it on this forum about 5 years ago. I will try to find a link later

UPD: weird, I can't Google it now... I even remember the number: in our expanding universe temperature will never fall below 10^-33K

Regarding post 10, in.the infinity of time it is irrelevant how low the probability is, if something can happen, it happens
 
Last edited:
  • #15
QuantumPion said:
The whole point of a black dwarf is that they are in thermal equilibrium with space.

Are there any objects in the universe that is currently at thermal equilibrium with space?
 
  • #16
Flatland said:
Are there any objects in the universe that is currently at thermal equilibrium with space?

Any interstellar meteoroid.
 
  • #17
nikkkom said:
Any interstellar meteoroid.

So meteoroids won't show up on thermal camera?
 
  • #18
Flatland said:
So meteoroids won't show up on thermal camera?

The ones that are between the stars probably won't, but any nearby will be warmed by the Sun.
 

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