2. Bit of Administration …. ReadingReading –BSNV Chap. 13 PortfoliosPortfolios –Due Thursday, April 29, because of possible TAA strike Put in box outside 6522 SterlingPut in box outside 6522 Sterling –All 5 must be securely bound together, including ones already graded –Late portfolios will lose credit Lab 3Lab 3 –Due Thursday, April 29, because of possible TAA strike Put in box outside 6522 SterlingPut in box outside 6522 Sterling –Problem 5, HW 1 is a good starting point for the lab questions –Note typo in Question 3 - “Jupiter” => “Saturn”

3. Jovian Rings Saturn Neptune Jupiter Uranus

4. Saturn Saturn Cassini’s Division A B C

5. Jovian Rings Saturn Saturn 70, 000 km across …. 20 m thick!

6. Jovian Rings Saturn Saturn S A B Redshift Blueshift Velocity A > Velocity B Keplerian! Earth

7. Jovian Rings Saturn Saturn Snowflakes (few microns) to Boulders (10 m) Snowflakes (few microns) to Boulders (10 m)

8. Jovian Rings Dynamics - Roche Limit Dynamics - Roche Limit Radius Inside Which Large Bodies Fragment Due to Tidal Forces Radius Inside Which Large Bodies Fragment Due to Tidal Forces (i.e., differences in gravitational forces) (i.e., differences in gravitational forces) Sat 12 1000 km 1 km Gravitational Force on Moon 2 Gravitational Force on Moon 1 1.002 x Greater

9. Jovian Rings Gravitational Force on Moon 2 Gravitational Force on Moon 1 4 x Greater! Dynamics - Roche Limit Dynamics - Roche Limit Radius Inside Which Large Bodies Fragment Due to Tidal Forces Radius Inside Which Large Bodies Fragment Due to Tidal Forces (i.e., differences in gravitational forces) (i.e., differences in gravitational forces) 12 1 km Sat

10. Jovian Rings Dynamics - Roche Limit Dynamics - Roche Limit Radius Inside Which Large Bodies Fragment Due to Tidal Forces Radius Inside Which Large Bodies Fragment Due to Tidal Forces (i.e., differences in gravitational forces) (i.e., differences in gravitational forces) Rings formed by … Rings formed by … Moon entering within Roche limit? Moon entering within Roche limit? Material originally inside Roche limit that never Material originally inside Roche limit that never formed a moon? formed a moon? Slow destruction of small moons within Roche limit Slow destruction of small moons within Roche limit by micrometeorites? by micrometeorites?

11. Jovian Rings Dynamics - Cassini Division - Tidal Resonance Dynamics - Cassini Division - Tidal Resonance Suppose …. Suppose ….

12. Jovian Rings Dynamics - Cassini Division - Tidal Resonance Dynamics - Cassini Division - Tidal Resonance Suppose …. Suppose …. S S S Mimas

13. Jovian Rings Dynamics - Cassini Division - Tidal Resonance Dynamics - Cassini Division - Tidal Resonance Orbital Period of Mimas is 2x Orbital Period Orbital Period of Mimas is 2x Orbital Period of particles in Cassini’s Division of particles in Cassini’s Division “2 to 1 Resonance” “2 to 1 Resonance” Repeated gravitational pulls clear gap at that orbit. Repeated gravitational pulls clear gap at that orbit.

14. Jovian Rings Dynamics - Shepherd Satellites Dynamics - Shepherd Satellites 100 km

15. Jovian Rings Dynamics - Shepherd Satellites Dynamics - Shepherd Satellites Saturn

16. Jovian Rings Dynamics - Shepherd Satellites Dynamics - Shepherd Satellites

17. Jovian Rings Uranus and Neptune Uranus and Neptune

18. Jovian Rings Uranus and Neptune - Weather Uranus and Neptune - Weather

19. Jovian Rings Uranus and Neptune - Weather Uranus and Neptune - Weather

20. Jovian Rings Uranus and Neptune - Interior Structure Uranus and Neptune - Interior Structure

21. Jovian Rings Uranus and Neptune - Rotation and Magnetic Fields Uranus and Neptune - Rotation and Magnetic Fields

22. Jovian Rings Uranus and Neptune - Moons Uranus and Neptune - Moons Retrograde, inclined orbit - captured? 38 o K

23. Jovian Planets Summary Summary Weather (“Atmospheric Dynamics”) Weather (“Atmospheric Dynamics”) Driven by energy flows Driven by energy flows Thermal from interior Thermal from interior Residual heat from formation Ongoing contraction Gravity (highs to lows) Gravity (highs to lows) Solar radiation Solar radiation Rapid rotation + Coriolis leads to twisting motions Rapid rotation + Coriolis leads to twisting motions Magnetic fields Magnetic fields Result from Result from Liquid metallic interiors Liquid metallic interiors Rotation Rotation Convection Convection

24. Jovian Planets Summary Summary Giant Moons Giant Moons Ice and rock (from condensation sequence) Ice and rock (from condensation sequence) Dynamically active (due to tidal forces) Dynamically active (due to tidal forces) Atmospheres (Io, Titan, Triton) Atmospheres (Io, Titan, Triton) Liquid oceans (Europa?, Titan?) Liquid oceans (Europa?, Titan?) Life ? Life ?

25. Asteroids, Comets, Meteors, and Pluto

27. Asteroids Asteroids

28. Asteroids, Comets, Meteors, and Pluto Asteroids Asteroids