Could a collision cause Venus to rotate prograde?

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SUMMARY

The discussion centers on the theories explaining Venus' slow prograde rotation, specifically the atmospheric friction theory versus the collision theory. The atmospheric friction theory posits that over billions of years, atmospheric conditions have slowed Venus' rotation, while the collision theory suggests a massive impact with a body three times larger than the Moon during the early Solar System could have caused this change. The participant argues that tidal forces and orbital energy could explain the current rotation without necessitating a planetesimal impact. A peer-reviewed paper supporting the non-impact theory is referenced, highlighting the instability of tidal locking in dense atmospheres.

PREREQUISITES
  • Understanding of planetary rotation and atmospheric dynamics
  • Familiarity with tidal locking and spin-orbit resonance concepts
  • Knowledge of the early Solar System formation theories
  • Ability to interpret peer-reviewed scientific literature
NEXT STEPS
  • Research the effects of atmospheric friction on planetary rotation
  • Study tidal locking and its implications for planets with thick atmospheres
  • Examine peer-reviewed literature on Venus' rotation, including the referenced papers
  • Investigate the collision theory and its historical context in planetary science
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Astronomers, planetary scientists, and students interested in planetary formation and dynamics, particularly those focusing on Venus and atmospheric influences on rotation.

Alex Nesh
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I got in an argument and I was defending one of the theories about Venus' slow prograde rotation. I'm defending the theory which states that atmospheric friction, over a period of billions of years slowed initially fast rotation of Venus and made it go prograde.

My opponent says that it would only be possible as a result of collision with a body three times larger than the moon in early Solar System formation.

My point is that such a collision could disintegrate both of the bodies and after all the matter condense it would be subjected to tidal forces of the sun (due to its proximity) and orbital energy cause the protoplanet to start rotating counterclockwise.

Please help me with that.
 
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Venus has a retrograde orbit.
It's slow rotation period is exactly what you would expect for a planet with a thick atmosphere cleaose to the sun and subject to tidal locking.
It may have had surface liquids earlier in it's history which would have speeded up the tidal friction.
 
I don't know much about this, unfortunately, but a bit of research shows that it may be possible to explain Venus' rotation without a planetisimal impact.

The mere publication of this theory doesn't mean that this is necessarily the right answer though. I'm afraid I don't know what the "consensus" view is, or even if there is a consensus.

For an example of a published peer-reviewed version of the non-impact theory, see for instance http://adsabs.harvard.edu/abs/2003Icar..163...1C, available online at http://www.imcce.fr/Equipes/ASD/preprints/prep.2002/venus1.2002.pdf

One interesting quote:

We show that the capture in the 1:1 spin orbit resonance during Venus' history is unlikely and becomes impossible when the dense atmosphere is present as this resonance becomes unstable

Apparently the authors are saying that the naive "tidal lock" where Venus presents one face to the sun one would expect becomes unstable for a planet with a thick atmosphere (!).

I'd like to balance this out by finding a peer-reviewed published version of the impact theory, but so far I haven't found one (though I've seen plenty of popular references).
 

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