Title: CassiniHuygens: Mission to Saturn
1Cassini/Huygens Mission to Saturn
- Maj Christian Ready
- Tri-Wing Encampment
2Saturn Facts
- Second largest
- 6th from Sun
- Titan has nitrogen-rich
atmosphere - Emits 79 more energy than it receives from Sun
- Receives 1/90th as much sunlight as Earth
- Largest, complex ring system
- 32 known moons
3Saturn Facts
- Diameter 120,660 Km
- Mass 569x1024Kg
- Rotation Period 10hr 40m
4Saturns Atmosphere
- Hydrogen (94)
- Helium (5)
- Other (1)
- ammonia, methane, ethane, phosphine, acetylene,
methylacetylene, and propane
5Saturns Winds
- 1,100 mph equatorial
- Second fastest in solar system
- Compared to
- Jet airplane (550mph)
- Cat 5 hurricane (220mph)
- Tsunami in open water (550mph)
- Speed of sound (660mph _at_ 30,000 feet)
6Saturn Earth Compared
- Earth-Moon distance 384,000 km (239,000 miles)
- Saturn and ring system diameter 340,000 km
(211,310 miles)
7Mission Overview
- Two Spacecraft
- Cassini (Orbiter)
- Huygens (Titan Lander)
- 4-year exploration
- Saturn
- Titan
- Ring System
- Other Satellites
8Launch
- Titan IVB/Centaur
- Cape Canaveral, FL
- 15 October 1997
9Oct 15 1997 0443 EDT
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12Cassini/Huygens Interplanetary Trajectory
13Earth-Moon Flyby
14August 17, 1999
15Jupiter Flyby
16Jupiter and Io October 2000
17Jupiter October 23 2000
18Jupiter Ganymede November 18 2000
19Jupiter Io December 01 2000
20Jupiter Ganymede December 03 2000
21Callisto, Europa, Jupiter December 07 2000
22Jupiter Io December 12 2000
23December 13 2000
24Closest Approach December 29 2000
25Jupiter Io January 01 2001
26Jupiter Io January 17 2001
27From Jupiter to Saturn
28Saturn Science Objectives
- Atmosphere temperature and composition
- Measure the global wind field
- Cloud features and processes
- Infer internal structure and rotation of the deep
atmosphere - Daily variations of the ionosphere
- Saturns formation and evolution
- Investigate sources of Saturn lightning
29Titan Saturn October 21 2002
30March 27 2004
31May 21 2004
32May 25 2004
33Arrival at Saturn
34Phoebe June 12 2004
35Titan June 21 2004
36Ring System June 21 2004
37Ring System June 21 2004
38Rings Science Objectives
- How were rings formed?
- What is the age of the rings?
- How are rings maintained?
- How do they interact with Saturn, other
satellites and electromagnetic fields?
39Orbit Insertion
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43Touring Saturn
44Highlights of the Saturn Tour
- 74 Orbits of Saturn
- 45 Close flybys of Titan
- 8 close "targeted" flybys of other satellites
- Enceladus, Phoebe, Hyperion, Dione, Rhea, Iapetus
- 30 additional satellite flybys at distances less
than 100,000 kilometers
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46July 02 2004 Feb 15 2005
47Icy Satellite Science Objectives
- Determine general characteristics and histories
- Understand how/why their surfaces change, and
what they are made of - Infer their bulk compositions and internal
structures. - Investigate interactions with the magnetosphere
and ring systems and possible gas injections into
the magnetosphere.
48Rhea July 02 2004
49Dione July 02 2004
50Tethys July 03 2004
51Iapetus July 03 2004
52Mimas July 03 2004
53Titan July 02 2004
54Titan July 03 2004
55Titan July 03 2004
56Enceladus July 03 2004
57Rings July 03 2004
58Saturn July 13 2004
59Huygens Probe Deployment to Titan
60Titan Science Objectives
- Determine the abundance of atmospheric
constituents - Infer evolution and formation of Titan
- Measure winds and global temperatures
- Investigate cloud physics, general circulation,
and seasonal effects in Titans atmosphere - Search for lightning discharges.
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67Occultation Sequence
- February 15 2005 September 5 2005
68 Feb 15 2005 Sep 7 2005
69Magnetosphere Study
- September 7 2005 July 22 2006
70Sep 7 2005 Jul 22 2006
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72Titan 180-Degree Transfer
- July 22 2006 June 30 2007
73Jul 22 2006 June 07 2007
74Icy Satellite Study
- June 30 2007 August 31 2007
75Jun 07 2007 Aug 31 2007
76High-Inclination Sequence
- August 31 2007 July 1 2008
77Aug 31 2007 Jul 01 2008
78Cassini/Huygens Web Site
- http//saturn.jpl.nasa.gov/