- Page 1: Passage to a Ringed World The Cassi
- Page 6 and 7: FOREWORD This book is for you. You
- Page 8 and 9: ACKNOWLEDGMENTS This book would not
- Page 10 and 11: Three separate images, taken by Voy
- Page 12 and 13: descent to the surface. The Huygens
- Page 14 and 15: address the challenges of the missi
- Page 16 and 17: Participant Nations* * First flag i
- Page 18 and 19: PROBING A MOON OF MYSTERY Huygens
- Page 20 and 21: TOUR T18-3 TARGETED SATELLITE FLYBY
- Page 22 and 23: SATURN CASSINI-HUYGENS MISSION SCIE
- Page 24 and 25: Cassini-Huygens designed to determi
- Page 26 and 27: In this diagram from his book, Syst
- Page 28 and 29: This Voyager 1 image shows Saturn
- Page 30 and 31: An Extended Atmosphere From Liquid
- Page 32 and 33: Haze layers are also observed above
- Page 34 and 35: IN THE EYE OF THE BEHOLDER Taken fr
- Page 36 and 37: This spectacular view of the edge o
- Page 38 and 39: the interaction was described as a
- Page 40 and 41: have a signature of a tone decreasi
- Page 42 and 43: CONSTITUENTS OF THE TITAN ATMOSPHER
- Page 44 and 45: The processes of plate tectonics an
- Page 46 and 47: tan was accreting, it is possible t
- Page 48 and 49: Surface Science. The highest resolu
- Page 50 and 51: This enhanced Voyager 2 image shows
- Page 52 and 53: Voyager 1 captured this striking im
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Prometheus and Pandora, two tiny sa
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In the stellar occultation experime
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scattering than are larger particle
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In fact, Saturn’s rings — as we
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The satellites of Saturn comprise a
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Before the advent of spacecraft exp
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The bright surface of Saturn’s mo
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Galilean satellites. Most of what i
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duced that one hemisphere is compos
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patches on the surface. Although it
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Artist’s conception of Ithaca Cha
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An artist’s rendition of Saturn
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The MAPS Instruments Coordinated ob
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field reverses direction across the
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SATURN’S MAGNETIC FIELD Saturn’
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Solar Wind Magnetosheath Titan neut
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per atmosphere. Energetic particles
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and plasma wave emissions from narr
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CHAPTER 7 Space mission design aims
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(SOI) propulsive maneuver to initia
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the tour cannot continue. Of course
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crease inclination to this value. T
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This illustration shows the main de
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discussed earlier) and data handlin
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of the spacecraft! Below the oxidiz
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• Opening or shutting thermal lou
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management subsystem and the Probe
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falls below its storage temperature
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The Cassini-Huygens spacecraft stan
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The Imaging Science Subsystem (ISS)
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• Map the composition and thermal
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cise distance between the surface f
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• Study the interaction of the ma
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• Study the erosional and electro
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midway out on the magnetometer boom
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The RPWS instrument will be used to
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altitudes down to 40 kilometers abo
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dex. A group of platinum resistance
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CHAPTER 10 Mission operations are t
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PLANETARY MISSION OPERATIONS Functi
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two low-gain antennas 1 and will pr
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During much of Cassini’s orbital
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articulation control subsystem’s
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AFTERWORD It has been said that in
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Developments tied to the Cassini-Hu
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APPENDIX A Command. A data transact
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APPENDIX A 138 PASSAGE TO A RINGED
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APPENDIX A Plasma wave. A wave char
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APPENDIX A 142 PASSAGE TO A RINGED
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APPENDIX B H O 2 + Water molecule w
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APPENDIX C 146 PASSAGE TO A RINGED
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APPENDIX D 148 PASSAGE TO A RINGED
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APPENDIX D 150 PASSAGE TO A RINGED
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APPENDIX F 152 PASSAGE TO A RINGED
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APPENDIX F 154 PASSAGE TO A RINGED
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APPENDIX F Peralta, F. and S. Flana
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National Aeronautics and Space Admi