How Do Planetary Rings Form and Move?

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    Planetary Rings
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Planetary rings form primarily from debris left over after collisions or the remnants of moons that have been torn apart by gravitational forces. Their movement is governed by orbital dynamics, with rings consisting of numerous small particles rather than a solid structure. Each gas giant in the solar system has a ring system, with Saturn's being the most prominent. The discussion highlights the rapid formation of Earth's moon from a debris ring following a giant impact, raising questions about the stability of Saturn's rings compared to Earth's transient ring. Ultimately, the stability of these rings is influenced by their position relative to the Roche limit, with Saturn's rings expected to dissipate in about 100 million years.
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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