How did the planets acquire their spin?

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Discussion Overview

The discussion centers on how planets acquire their spin, exploring the role of angular momentum from the gas clouds from which they formed. It encompasses theoretical aspects of planetary formation, angular momentum conservation, and the effects of collisions and tidal locking.

Discussion Character

  • Exploratory
  • Technical explanation
  • Debate/contested
  • Conceptual clarification

Main Points Raised

  • Some participants propose that planets acquire spin from the angular momentum of the rotating gas cloud from which they formed, suggesting that conservation of angular momentum plays a key role.
  • Others argue that the relationship between orbital angular momentum and spin angular momentum is complex, and that the conservation of angular momentum does not straightforwardly explain the spin of planets.
  • A participant questions why the Moon does not rotate in the opposite direction if collisions can affect planetary spin, suggesting that tidal locking and the nature of impacts are significant factors.
  • Some contributions highlight that the majority of angular momentum ends up in the central star, with only a small fraction contributing to the spin of planets, indicating a potential imbalance in the distribution of angular momentum during formation.
  • There is mention of ongoing research into the specifics of how coalescing gas clouds translate into planetary spin, with no consensus on a definitive explanation.

Areas of Agreement / Disagreement

Participants generally agree that angular momentum is a crucial factor in understanding planetary spin, but multiple competing views remain regarding the mechanisms and implications of this relationship. The discussion is unresolved, with significant complexity acknowledged in the formation processes.

Contextual Notes

Limitations include the lack of clarity on how orbital and spin angular momentum interact, the dependence on specific conditions during planetary formation, and the unresolved nature of the effects of collisions and tidal locking on planetary spin.

  • #31
Never. Too early, I mean.
 

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