Fate of outer planets after sun ends its life cycle

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SUMMARY

The discussion centers on the fate of outer planets, specifically gas giants like Jupiter and Saturn, after the Sun transitions to a white dwarf and eventually a black dwarf. It is established that planets not ejected during the red giant phase will maintain stable orbits around the white dwarf, which does not affect their dynamics significantly. The cooling of a white dwarf into a black dwarf is a lengthy process, and while black dwarfs theoretically could decay over immense timescales, they currently do not exist in the universe. The conversation also touches on gravitational waves and their potential impact on planetary orbits over time.

PREREQUISITES
  • Understanding of stellar evolution, particularly the red giant and white dwarf phases.
  • Knowledge of gravitational dynamics and orbital mechanics.
  • Familiarity with black body radiation and thermal equilibrium concepts.
  • Awareness of proton decay theories and their implications for black dwarfs.
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  • Research the process of stellar evolution from main sequence to white dwarf stages.
  • Explore the effects of gravitational waves on orbital decay and planetary dynamics.
  • Study the implications of black body radiation in astrophysical contexts.
  • Investigate theories surrounding proton decay and its potential effects on black dwarfs.
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Astronomers, astrophysicists, and students of cosmology interested in the long-term evolution of stellar systems and the fate of planetary bodies in the universe.

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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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