How Do Planetary Rings Form and Move?

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    Planetary Rings
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Discussion Overview

The discussion revolves around the formation and movement of planetary rings, with a focus on theories regarding their origins, stability, and the dynamics involved in their motion. Participants explore various aspects of ring formation, particularly in relation to Earth and Saturn, and the implications of gravitational interactions.

Discussion Character

  • Exploratory
  • Technical explanation
  • Debate/contested

Main Points Raised

  • Some participants propose that planetary rings are collections of small pieces rather than a solid disk, influenced by gravitational forces.
  • There is a suggestion that Earth may have had a ring system that contributed to the formation of the Moon after a giant impact.
  • Questions arise about the rapid coalescence of Earth's ring into the Moon compared to the stability of Saturn's rings.
  • One participant notes that Earth's ring formed outside the Roche limit, while Saturn's rings are within it, raising questions about the implications of this distinction.
  • Concerns are expressed about how debris from the Earth-impacting object could have ended up outside the Roche limit, with speculation about the size of Earth's Roche limit.
  • Participants discuss the temporary nature of Saturn's rings, suggesting they may not be permanently stable and could disappear over time.
  • There is a call for estimates of the physical parameters and processes needed to model the Moon's formation accurately, particularly in the context of the Mars-sized impactor theory.

Areas of Agreement / Disagreement

Participants express multiple competing views regarding the formation and stability of planetary rings, with ongoing questions and uncertainties about the processes involved. No consensus is reached on the specifics of these processes or the implications of the Roche limit.

Contextual Notes

Participants highlight limitations in understanding the dynamics of ring formation and stability, particularly regarding the assumptions about the Roche limit and the conditions following the Earth-impacting collision.

Slatiebartfarce
how do planetary rings form? how do they move? what are some theories?
 
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Originally posted by Ambitwistor
As for how they move, it's mainly just orbital motion due to gravity,

Correct. It's important to remember that planetary rings are not a single solid disk, but rather a collection of countless small pieces (each like a tiny moon).

And of course, each of the 4 gas planets in our solar system has a ring system (Saturn's being the most spectacular).

And it's possible that Earth once had a ring system (that later formed the moon).
 
Yeah, but in the time period immediately following the impact, there was a ring of debris which was still coalescing into the moon.
 
This raises a question:

What made Earth's ring coallesce into a moon so quickly, and makes the rings of saturn etc remain seemingly so stable?
 
Originally posted by FZ+
This raises a question:

What made Earth's ring coallesce into a moon so quickly, and makes the rings of saturn etc remain seemingly so stable?

Basically, the Earth's ring formed outside the Roche limit, and Saturn's rings are inside of the Roche limit.
 
Ok...

But the questions continue... how did the debris field from the proposed object/earth collision get outside the roche limit? Surely some would have ended up within it, leaving Earth still with some remnants of this dust ring?

Or is Earth's roche limit simply too small?
 
Originally posted by FZ+
But the questions continue... how did the debris field from the proposed object/earth collision get outside the roche limit? Surely some would have ended up within it, leaving Earth still with some remnants of this dust ring?

More stable, but not permanently stable. Even Saturn's rings are expected to be gone in about 100 million years, IIRC. Earth's Moon-forming collosion was like 4.5 billion years ago, so any ring remnant is long gone.
 
Originally posted by FZ+
But the questions continue... how did the debris field from the proposed object/earth collision get outside the roche limit? Surely some would have ended up within it, leaving Earth still with some remnants of this dust ring?

Or is Earth's roche limit simply too small?
Now here are some really good questions!

Anyone care to make some a priori guestimates of the physical parameters and processes which a good model of the formation of the Moon (Mars-sized Earth impactor theory) would require to answer FZ+'s questions (suitably extended and quantified), to ~10% accuracy? And which are the three (five) most imporant?

Yes, it would have been an inelastic collision; now for the details ...
 

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