Presentation: Venus hot break hypothesis

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SUMMARY

The discussion centers on the "Venus hot break hypothesis," which will be presented at the Ancient Venus Conference in Houston on July 25. The hypothesis suggests that a glancing collision between proto-Mercury and proto-Venus could explain the slow rotation of both planets and their differing densities. Specifically, the collision may have canceled the rotational momentum of both bodies and transferred mantle material from proto-Mercury to proto-Venus, contributing to Venus's counter-rotation. The presenter invites experts to conduct the necessary calculations to validate this hypothesis.

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Astronomers, planetary scientists, and astrophysicists interested in planetary formation, dynamics, and the specific characteristics of Venus and Mercury.

Andre
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Announcement Venus exchanged rotational energy into heat
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I have thought that a glancing collision between a proto-Mercury and a proto-Venus might explain many characteristics of the two bodies. A glancing collision of two bodies with the same rotation should be expected to cancel some or all of the rotational momentum of both bodies, perhaps explaining the slow rotation of Mercury and Venus. If the collision resulted in transfer of some of the mantle of the proto-Mercury to the proto-Venus this would explain the higher density of Mercury and lower density of Venus. https://nssdc.gsfc.nasa.gov/planetary/factsheet/
Re-accretion of the transferred material to Venus might contribute to its counter rotation.
I do not have the expertise or facilities to do the necessary calculations but perhaps you do.
 

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