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.