- #1
Simfish
Gold Member
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For example, here's a e-mail I recently sent to a professor.
""Hello Professor XX,
Do you know if any theoretical work has been done on the atmospheric evolution of a tidally locked planet facing a red dwarf star? Especially a planet whose atmosphere freezes over on the cold side, but re-vaporizes on the warm side? I'd be especially curious to know whether or not such an atmosphere could be stable over long periods of time [and how its stability compares to the stability of a planet whose atmosphere doesn't freeze over] (on the cold side, you might have comparatively few air molecules, so they might be able to "escape" a planet on the cold side since they don't have to deal with the numerous collisions that they have to deal with on the warm side, and there might not be as complex of an atmosphere on the dark side).
Is Triton an example where the atmosphere condenses on the cold side and re-vaporizes on the warm side? (YY told me that she made a homework problem about that, where the student had to calculate the heat of condensation). I'm extremely curious about how numerical models could be used on exoplanetary atmospheres, although I can't really find much research on that.
Thanks!
XX""
""Hello Professor XX,
Do you know if any theoretical work has been done on the atmospheric evolution of a tidally locked planet facing a red dwarf star? Especially a planet whose atmosphere freezes over on the cold side, but re-vaporizes on the warm side? I'd be especially curious to know whether or not such an atmosphere could be stable over long periods of time [and how its stability compares to the stability of a planet whose atmosphere doesn't freeze over] (on the cold side, you might have comparatively few air molecules, so they might be able to "escape" a planet on the cold side since they don't have to deal with the numerous collisions that they have to deal with on the warm side, and there might not be as complex of an atmosphere on the dark side).
Is Triton an example where the atmosphere condenses on the cold side and re-vaporizes on the warm side? (YY told me that she made a homework problem about that, where the student had to calculate the heat of condensation). I'm extremely curious about how numerical models could be used on exoplanetary atmospheres, although I can't really find much research on that.
Thanks!
XX""