Exploring the Mysteries of Planetary Rings: Formation, Movement, and Theories

In summary, planetary rings can form through various theories such as tidal disruption of satellites and collisions with satellites, with the latter being the preferred theory today. They mainly move through orbital motion due to gravity, but there can also be collisions and electromagnetic effects. It is possible that Earth once had a ring system that later formed the moon, which formed quickly due to being outside the Roche limit. However, even Saturn's rings are not permanently stable and are expected to disappear in about 100 million years. The details of the Moon's formation, including its physical parameters and processes, are still being studied and debated.
  • #1
Slatiebartfarce
how do planetary rings form? how do they move? what are some theories?
 
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  • #2
Various theories have been proposed, including tidal disruption of satellites, and collisions with satellites. This link:

http://www-astro.physics.uiowa.edu/~lam/research/rings/

says that the latter theory is preferred today.

As for how they move, it's mainly just orbital motion due to gravity, but there are collisions too, electromagnetic effects sometimes when ring particles are charged, etc.
 
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  • #3


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).
 
  • #4


Originally posted by Phobos
And it's possible that Earth once had a ring system (that later formed the moon).

Really? I thought that the favored theory of the Moon's formation nowadays was the "giant impact" model, in which a Mars-sized object struck the Earth (thus explaining the Moon's similarity to the Earth's mantle, the Moon's iron depletion, etc.)
 
  • #5
Yeah, but in the time period immediately following the impact, there was a ring of debris which was still coalescing into the moon.
 
  • #6
  • #7
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?
 
  • #8
Originally posted by FZ+
What made Earth's ring coallesce into a moon so quickly, and makes the rings of saturn etc remain seemingly so stable?

I don't know much about the Moon's formation. Saturn's ring's aren't stable; that's how we know they weren't formed when Saturn was. But they do last for hundreds of millions of years. I think this is partly due to the shepherd moons.
 
  • #9
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.
 
  • #10
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?
 
  • #11
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.
 
  • #12
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 ...
 

1. What are planetary rings?

Planetary rings are vast, flat disks of dust, rock, and ice particles that orbit around a planet. They are most commonly found around the four gas giant planets in our solar system: Jupiter, Saturn, Uranus, and Neptune.

2. How do planetary rings form?

The exact formation of planetary rings is still a mystery, but there are several theories. One theory suggests that they formed from material left over from the formation of the planet itself. Another theory proposes that they are the remnants of a moon that was torn apart by the planet's gravity.

3. What causes the movement of planetary rings?

The movement of planetary rings is primarily influenced by the planet's gravity. The particles in the rings are constantly pulled towards the planet, but their orbital velocity keeps them in a stable orbit. Other factors such as collisions between particles and the influence of nearby moons can also affect the movement of the rings.

4. Are there different types of planetary rings?

Yes, there are different types of planetary rings depending on the composition of the particles. For example, Saturn's rings are mostly made of ice particles, while Jupiter's rings consist of mostly dust and rock. There are also differences in the density, thickness, and structure of the rings.

5. Why do some planets have rings while others don't?

There are a few reasons why some planets have rings while others don't. The first is the distance from the sun - the four gas giant planets in our solar system are far enough away from the sun that they were able to retain their rings without them being destroyed by the sun's heat and radiation. Another factor is the presence of moons - some moons may have cleared out the space around their planet, preventing the formation of rings. Finally, the composition and mass of the planet can also play a role in whether or not it has rings.

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