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APPENDIX F 154 PASSAGE TO A RINGED WORLD Galopeau, P. H. M., P. Zarka and D. L. Quéau. Source location of Saturn’s kilometric radiation: The Kelvin-Helmholtz instability hypothesis. J. Geophys. Res. 100. 1995. Gehrels, T. and M.S. Matthews (Eds). Saturn. University of Arizona Press, Tucson, Arizona. 1984. Gibbs, R. Cassini Spacecraft Design. Cassini/Huygens: A Mission to the Saturnian System (L. Horn, Ed), Proc. SPIE 2803. 1996. Goldreich, P. and S. D. Tremaine. Towards a Theory for the Uranian Rings. Nature 277. 1979. H Harris, A. W. The Origin and Evolution of Planetary Rings. Planetary Rings (R. Greenberg and A. Brahic, Eds). University of Arizona Press, Tucson, Arizona. 1984. Hartmann, W. K. Moons and Planets, 2nd ed. Wadsworth, Belmont, California. 1983. Hassan, H., C. McCarthy and D. Wyn- Roberts. Huygens — A Technical and Programmatic Overview. ESA Bulletin No 7. Feb 1994. Horn, L. J. (Ed). Cassini/Huygens: A Mission to the Saturnian System. Proc. SPIE 2803. 1996. J Jaffe, L. D. and J.-P . Lebreton. The CRAF/Cassini Science Instruments, Spacecraft, and Missions. IAF Paper 90–436, Oct 1990, and Space Technology Vol 12. 1992. Jaffe, L. D. and L. M. Herrell. Cassini/ Huygens Science Instruments. Cassini/Huygens: A Mission to the Saturnian System (L. Horn, Ed), Proc. SPIE 2803. 1996. Jones, C. P. Cassini Program Update. AIAA Preprint 93–4745. 1993. Juergens, D., J. Duval, . PPuget, A. Soufflot, V. Formisano and V. Tarnopolsky. A Common Design Imaging Spectrometer for Planetary Exploration. AIAA/ JPL Conference on Solar System Exploration. 1989. K Kaiser, M. L., M. D. Desch, W. S. Kurth, A. Lecacheux, F. Genova, B. M. Pedersen and D. R. Evans. Saturn as a Radio Source. Saturn, (T. Gehrels and M. S. Matthews, Eds). University of Arizona Press, Tucson, Arizona. 1988. Keeler, J. E. First Observations of Saturn with the 36-inch Equatorial of the Lick Observatory, Sidereal Messenger 7. 1888. Kohlhase, C. The Cassini Mission to Saturn — Meeting With a Majestic Giant. Planetary Report, Vol 13, No 4. Jul–Aug 1993. Krimigis, S. M. A Post-Voyager View of Saturn’s Environment. Johns Hopkins APL Technical Digest 3. 1982. Kunde, V., G. Bjoraker, J. Brasunas, B. Conrath, F. M. Flasar, D. Jennings, P. Romani, R. Maichle, D. Gautier and M. Abbas. Infrared Spectroscopic Remote Sensing from the Cassini Orbiter. Optical spectroscopic instrumentation and techniques for the 1990s — Applications in astronomy, chemistry, and physics. Proc. Meeting, Las Cruces, New Mexico, Jun 4–6, 1990, SPIE. 1990. Kurth, W. S. and D. A. Gurnett. Plasma Waves in Planetary Magnetospheres. J. Geophys. Res. 96. 1991. Lebreton, J-P ., and D. L. Matson. An Overview of the Cassini Mission. Nuovo Cimento C, Vol. XV #6. 1992. L
APPENDIX F Lebreton, J.-P . and D. L. Matson. An Overview of the Cassini Mission. Nuovo Cimento C, Serie 1, Vol 15C, No 6. Nov–Dec 1992. Lebreton, J.-P . Cassini, 1991, A Mission to Saturn and Titan. Proceedings of the 24th ESLAP Symposium, Formation of Stars and Planets, and the Evolution of the Solar System, Friedrichshafen, Sep 17–19, 1990. ESA SP-315. Lebreton, J.-P ., M. Verdant and R. D. Willis. Huygens — The Science Payload and Mission Profile. ESA Bulletin No 7. Feb 1994. Lunine, J. Does Titan Have Oceans? American Scientist, Vol 82, 1994. Lyons, L. R. and D. J. Williams. Quantitative Aspects of Magnetospheric Physics. D. Reidel/Kluwer, Boston, Massachusetts. 1984. M McClintock, W. E., G. M. Lawrence, R. A. Kohnert and L. W. Esposito. Optical Design of the Ultraviolet Imaging Spectrograph for the Cassini Mission to Saturn. Instrumentation for Planetary and Terrestrial Atmospheric Remote Sensing. Proc. Meeting, San Diego, California, Jul 23–24, 1992, SPIE. 1992. Mendis, D. A., J. R. Hill, W.-H. Ip, C. K. Goertz and E. Grün, 1988. Electrodynamic Processes in the Ring System of Saturn. Saturn (T. Gehrels and M. S. Matthews, Eds). University of Arizona Press, Tucson, Arizona. 1988. Mitchell, D. G., A. F. Cheng, S. M. Krimigis, E. P. Keath, S. E. Jaskulek, B. H. Mauk, R. W. McEntire, E. C. Roelof, D. G. Williams, K. C. Hsieh and . VA. Drake. INCA: the ion neutral camera for energetic neutral atom imaging of the Saturnian magnetosphere. Optical Engineering 32. 1993. Moore, P. and G. Hunt. Atlas of the Solar System. Rand McNally, New York. 1984. Morrison, D. Voyages to Saturn. National Aeronautics and Space Administration, NASA SP-451. Superintendent of Documents, U.S. Government Printing Office, Washington, D.C. 1982. Murray, C. D. Planetary Ring Dynamics, Phil. Transactions of the Royal Society. London A 349. 1994. Murray, C. D. The Cassini Imaging Science Experiment. J. British Interplanetary Society, Vol 45, No 9. Sep 1992. National Aeronautics and Space Administration. Announcement of Opportunity, Cassini Mission: Saturn Orbiter. A.O. No. OSSA-1-89, Oct 10, 1989. National Aeronautics and Space Administration. Announcement of Opportunity, Facility Instrument Science Team for the Ion and Neutral Mass Spectrometer on the Cassini Saturn Orbiter. A.O. No. OSSA-1-91, May 20, 1991. N Nirchio, F., B. Pernice, L. Borgarelli, C. Dionisio and R. Mizzoni. Cassini Radar Radio–Frequency Subsystem Design Description and Performance Analysis. 12th Annual International Geoscience and Remote Sensing Symposium, May 26–29, 1992, IEEE. 1992, Vol 1. O Osterbrock, D. E. and D. . PCruikshank. J.E. Keeler’s Discovery of a Gap in the Outer Part of the A Ring. Icarus 53. 1983. Osterbrock, D. E. 209. 1980. Keeler’s Gap. Science P Peralta, F. and J. Smith. Cassini Trajec- tory Design Description. AAS Paper 93-568. AAS/AIAA Astrodynamics Conference, Victoria, Canada. Aug 1993. BIBLIOGRAPHY 155
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Passage to a Ringed World The Cassi
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On the Cover: A collage of images s
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FOREWORD This book is for you. You
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ACKNOWLEDGMENTS This book would not
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Three separate images, taken by Voy
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descent to the surface. The Huygens
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address the challenges of the missi
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Participant Nations* * First flag i
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PROBING A MOON OF MYSTERY Huygens
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TOUR T18-3 TARGETED SATELLITE FLYBY
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SATURN CASSINI-HUYGENS MISSION SCIE
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Cassini-Huygens designed to determi
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In this diagram from his book, Syst
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This Voyager 1 image shows Saturn
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An Extended Atmosphere From Liquid
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Haze layers are also observed above
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IN THE EYE OF THE BEHOLDER Taken fr
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This spectacular view of the edge o
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the interaction was described as a
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have a signature of a tone decreasi
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CONSTITUENTS OF THE TITAN ATMOSPHER
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The processes of plate tectonics an
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tan was accreting, it is possible t
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Surface Science. The highest resolu
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This enhanced Voyager 2 image shows
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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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Page 130 and 131: CHAPTER 10 Mission operations are t
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Page 140 and 141: AFTERWORD It has been said that in
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Page 164 and 165: APPENDIX F Peralta, F. and S. Flana
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