this post was submitted on 02 Jan 2024
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"...the results indicate the potential for the existence of a Mars-sized, or even a Mercury-sized planetary body somewhere in the outer solar system..." Sounds like maybe one?
This sentence has me confused, “so if any fraction of them have regions with energy budgets that can support liquid water, “. If they are so far from a star, how would they have any energy budget for liquid water? Wouldn’t they be a complete iceball? In these scenarios, could techtonic activity create enough energy to overcome no external source of energy enough to create an environment with liquid water?