Title: Planetary Rings
1Planetary Rings
2Rings are swarms of orbiting particles
- Orbits have to be very circular
- Elliptical orbits will result in collisions,
destroying the ring
3Rings Have to be Very Flat
- Inclined orbits will result in collisions and
destruction of the ring
4Rings have to be Equatorial
- Tilted orbits precess the plane of the orbit
rotates due to the planets equatorial bulge,
other satellites, and the Suns gravity
5A tilted ring wont stay flat very long
- Particle orbits will precess at different rates
- Collisions will soon destroy the ring
6Rings, Gaps, and Resonances
- When two objects return to the same relative
positions regularly, they are said to be in
resonance - Some resonances are stable. Mercurys 32
resonance between its rotation and its orbit is
an example. - Plutos period is 3/2 that of Neptunes. This
resonance keeps the two planets from ever
colliding even though their orbits cross.
7Rings, Gaps, and Resonances
- Some resonances create gaps. There are no
asteroids with one-half Jupiters period because
repeated pulls by Jupiter eventually would change
the asteroids orbit. - Gaps in Saturns rings are due to resonances with
Saturns satellites.
8Shepherd Moons
- Shepherd Moons help maintain the sharp edges of
rings
9A Shepherd Moon Outside a Ring Tends to Drag
Stray Particles Back, Causing Them to Fall Back
Into the Ring
10Outer Shepherd Moon
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16A Shepherd Moon Inside a Ring Tends to Speed
Stray Particles Up, Causing Them to Rise Back
Into the Ring
17Inner Shepherd Moon
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23Rings Are Probably Short-Lived
- Gravity of the Sun and planets satellites
constantly disturbs orbits of particles - Collisions probably happen frequently
- Particles should drift out of the ring
- Rings around outer planets have probably come and
gone repeatedly during history of Solar System
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