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Planetary Rings and the Cassini Mission Lecture #1

Mark R. Showalter SETI Institute

COSPAR WORKSHOP Wednesday, July 23, 2007

1 Jupiter Saturn

Uranus Neptune

2 Why Study Rings?

Orion Nebula in HST

3 Protoplanetary Disks in the Orion Nebula

4 Artist’s Conception of a Protoplanetary Disk

5 Cassini Crosses the Ring Plane

6 Cassini Crosses the Ring Plane

7 Cassini Crosses the Ring Plane

8 Cassini Approaches Saturn

http://saturn.jpl.nasa.gov/ http://saturn.jpl.nasa.gov/multimedia/images/raw/

9 10 Low-Gain Antenna High-Gain (1 of 2) Antenna

Magnetometer Boom

Radar Bay

Fields Radio/Plasma and Wave Subsystem Particles Antenna (1 of 3) Pallet

Remote Sensing Pallet Huygens Probe

Radioisotope Thermoelectric Generator Engine (1 of 3) (1 of 2)

11 October 15, 1997

12 Saturn Arrival 1 July 2004

Jupiter Swingby 30 Dec 2000

Venus Swingby 24 June 1999 Venus Swingby Sun 26 April 1998

Launch Earth Swingby 15 Oct 1997 18 Aug 1999

13 Phoebe

(Best views from Voyager)

14 Saturn Orbit Insertion

15 16 B Ring at 150 meter resolution: There’s structure all the way down!

Voyager 2 image 3 km resolution

17 F Ring at Fine Resolution

18 A Ring, Outer Edge of the Encke Gap

Pan Wake

19 Outer A Ring Density Waves

20 Keeler Gap, Outer A Ring

21 of Saturn Janus

Rhea

Mimas

22 Saturn’s North Pole

23 Views of Titan

IR wavelengths

Visual wavelengths

24 Radar Image

Titan Probe Camera 25 The View from Saturn’s Shadow

26 The View from Saturn’s Shadow

26 Ice Geysers on

27 The Shadow of Enceladus in the E Ring

28 A new feature 200 km inward from the F ring core

29 What is this ?!?!? The aftermath of a ring impact?

30 Spokes in the B Ring

31 The Opposition Surge in the Rings

32 Satellite Mutual Event

33 Cassini Extended Mission has been approved by NASA: 2 more years and probably 4. 34 What Mission Work is Really Like...

Tour Plan Presentations

Science Planning Process Context

Long-Range Mission Planning Process

MP Updates MP Updates MP Updates MP Updates

Uplinked Tour Science and Sequences and SOP SOP Aftermarket SOP Update Sequencing R/T Commands Development Aftermarket Aftermarket Aftermarket PrAofcteersmsarket PAroftceersmsarket UpdatAef tPerromcMaePrskset Process Process ProcUepsdsates Process Process (SSPUroPc)ess

Integration/ Activity Conflict SPVT Tour Atlas Request Resolution Implementaton Process & Merge Process Process

Science Planning Process (SPP)

B. Paczkowski 4 3/03/2004 Science Planning Team

35

36

New Horizons at Jupiter February 28, 2007

http://pluto.jhuapl.edu/

37 Jupiter’s Storms February 27, 2007

False Color from IR images 1.25–2.5 µm

38 Low-Resolution Color Imaging

Io & Together March 2, 2007

39 Active volcano on

40 Active volcano on Io

40 Jupiter’s Rings in backscatter

Boulders {

Dust

Metis

Adrastea

41 Clumps in Jupiter’s Ring, Trailing Adrastea

42 Backscatter

Forward-Scatter

Dust

43 Voyager Images, January 1986

True color Enhanced color http://photojournal.jpl.nasa.gov/

44 epsilon Uranian Rings in back-scattered light lambda delta gamma eta

beta alpha

4 5 6

45 Uranian dust belts in forward-scattered light

46

Two small moons “shepherd” the ε ring

47 Uranus: August 2003

48 Uranus: August 2003

48 Recovery of “Perdita” Discovery of “” Orbit 1

Credit: Science Magazine/M. Showalter

49 Recovery of “Perdita” Orbit 2 Discovery of “

Credit: Science Magazine/M.

Showalter 50 Uranus: August 2003

Mab

51 Uranus: August 2003

Mab

µ ring ν ring

51 G Ring E Ring

Blue color indicates tinier dust particles

μ ring ν ring

52 Equinox 2007

2003

2005

2007 53 Uranian Ring Plane Crossing 2007–2008 6

4

Su ) b-S ° o

( la r La e 2 titu d de u t i t a L

c

i 0 r

t Jan Apr Jul Oct Jan Apr Jun n e c

o Sub-Earth Latitude t

e -2 n a l P

-4

2007 2008 -6 Date

54 The Uranian Ring System Through the Years:

Keck Telescope Adaptive Optics

D G E H B A 6 Z 5 4

July 2004 August 2006 May 2007

55