P41F:
The Future of Planetary Atmospheric, Surface, and Interior Science Using Radio and Laser Links I Posters
Submit an Abstract to this Session
Session ID#: 44126
Session Description:
Radio Science techniques have advanced solar system exploration for over five decades. In this session, ongoing and planned innovations that will significantly enhance the field will be presented. Session topics include investigations of planetary atmospheres, surfaces, interiors, and tests of gravity laws that contribute to expanding the frontiers of solar system exploration in diverse areas such as determining the thickness of the ice sheets of ocean worlds, constraining the interior structures of the planets and small bodies, monitoring of planetary atmospheric dynamics and improvement of climate models, characterizing the scattering and other properties of planetary surfaces, and research in fundamental physics and solar system dynamics. Technology topics include the design of small spacecraft networks and constellations, advances in flight and ground instrumentation, advancement in space clock technologies, novel communications architectures including optical links, and advances in radio and laser technologies, and new techniques and instrumentation for entry probe radio science.
Primary Convener: David H Atkinson, Jet Propulsion Laboratory, California Institute of Technology, Pasadena, United States
Conveners: Erwan Mazarico, NASA Goddard Space Flight Center, Greenbelt, MD, United States, Sami Asmar, Jet Propulsion Laboratory, California Institute of Technology, Pasadena, United States and Luciano Iess, Sapienza University of Rome, Rome, Italy
Primary Liaison: David H Atkinson, Jet Propulsion Laboratory, California Institute of Technology, Pasadena, United States
Chairs: Sami Asmar, Jet Propulsion Laboratory, California Institute of Technology, Pasadena, United States and Erwan Mazarico, NASA Goddard Space Flight Center, Greenbelt, MD, United States
OSPA Liaison: Luciano Iess, Sapienza University of Rome, Rome, Italy
Abstracts Submitted to this Session:
Yu-Ming Yang1, Dustin Buccino2, Marzia Parisi2, William M Folkner3, Phillip H Phipps2,4, Paul Withers5, Daniel S Kahan3 and Kamal Oudrhiri2, (1)Jet Propulsion Laboratory, Pasadena, CA, United States, (2)Jet Propulsion Laboratory, California Institute of Technology, Pasadena, United States, (3)Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA, United States, (4)Boston University, Boston, MA, United States, (5)Boston University, Boston, United States
Daniel Hestroffer, Observatoire de Paris, université PSL, IMCCE, Paris, France, Pascal Rosenblatt, Géoazur - Université Nice Sophia Antipolis, Valbonne, France, Marco Agnan, Odysseus Space, Co. Ltd, NCKU National Cheng Kung University, DAA, Tainan, Taiwan, Boris Segret, Observatoire de Paris, université PSL, LESIA, Meudon, France, Gary Quinsac, Observatoire de Paris, université PSL, LESIA, Paris, France, Hongru Chen, Paris Observatory, université PSL, IMCCE, Paris, France, Jordan Vannitsen, Odysseus Space, Co. Ltd., NCKU National Cheng Kung University, DAA, Tainan, Taiwan, Jiun-Jih Miau, NCKU National Cheng Kung University, DAA, Tainan, Taiwan and YueHeng LI, NCKU National Cheng Kung University, Tainan, Taiwan
Silvia Tellmann, RIU, Cologne, Planetary Research, Cologne, Germany; Rheinisches Institut für Umweltforschung (RIU), Department of Planetary Research at the University of Cologne, Cologne, Germany, Martin Paetzold, University of Cologne; Rheinisches Institut fuer Umweltforschung (RIU), Department of Planetary Research, Cologne, Germany, Bernd Häusler, Universität der Bundeswehr, Institute for Space Technology & Applications, Munich, Germany, Michael Keith Bird, Univ Bonn, Bonn, Germany; University of Cologne, Rheinisches Institut für Umweltforschung (RIU), Department of Planetary Research, Cologne, Germany, David P Hinson, SETI Institute, Mountain View, CA, United States; Stanford University, Stanford, CA, United States, Thomas Andert, Universität der Bundeswehr München, Institute for Space Technology & Applications, Munich, Germany, Graciela Gonzalez Peytavi, Universität der Bundeswehr München, Institute of Space Technology & Applications, Munich, Germany and Sami Asmar, Jet Propulsion Laboratory, California Institute of Technology, Pasadena, United States
Andre Jongeling1, Alan Tanner2, James Border2, Ezra Long3 and Hungsheng Lin3, (1)Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA, United States, (2)Jet Propulsion Laboratory, Pasadena, CA, United States, (3)Jet Propulsion Laboratory, Pasadena, United States
David H Atkinson1, Kyle Botteon2, Sami Asmar2, Robert Arthur Preston3 and Joseph Lazio1, (1)Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA, United States, (2)Jet Propulsion Laboratory, California Institute of Technology, Pasadena, United States, (3)NASA Jet Propulsion Laboratory, California Institute of Technology, Pasadena, United States
Meegyeong Paik1, James Border2, Stephan X Esterhuizen3 and Dong K Shin3, (1)JPL/NASA/Caltech, Pasadena, CA, United States, (2)Jet Propulsion Laboratory, Pasadena, CA, United States, (3)JPL/NASA/Caltech, Pasadena, United States
Maria T Zuber1, David E. Smith2, Erwan Mazarico3, Antonio Genova2, Gregory A Neumann4, Luciano Iess5, Stefano Bertone6 and Daniele Durante5, (1)Massachusetts Institute of Technology, Cambridge, MA, United States, (2)Massachusetts Institute of Technology, Cambridge, United States, (3)NASA Goddard Space Flight Center, Greenbelt, MD, United States, (4)NASA Goddard Space Flight Center, Greenbelt, Maryland, USA, Greenbelt, United States, (5)Sapienza University of Rome, Rome, Italy, (6)NASA GSFC / UMBC CRESST, Greenbelt, MD, United States
Sami W Asmar1, David H Atkinson2, David J Bell3, James Border4, Ivan S Grudinin5, Joseph Lazio6, Anthony J Mannucci6, Meegyeong Paik6 and Robert Arthur Preston7, (1)Jet Propulsion Laboratory, Pasadena, United States, (2)NASA Jet Propulsion Laboratory, Science Systems Engineering Group, Pasadena, CA, United States, (3)NASA Jet Propulsion Laboratory, Flight Communications Systems, Pasadena, CA, United States, (4)Jet Propulsion Laboratory, Pasadena, CA, United States, (5)NASA Jet Propulsion Laboratory, Pasadena, United States, (6)Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA, United States, (7)NASA Jet Propulsion Laboratory, California Institute of Technology, Pasadena, United States
Chi O Ao1, Mark Hofstadter2, Anthony J Mannucci3, Ryan S Park4, Robert A Preston3, Walton Williamson1 and Nilton O. Renno5, (1)NASA Jet Propulsion Laboratory, Pasadena, CA, United States, (2)Jet Propulsion Laboratory, California Institute of Technology, Pasadena, United States, (3)Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA, United States, (4)NASA Jet Propulsion Laboratory, La Cañada Flintridge, United States, (5)University of Michigan Ann Arbor, Climate and Space Sciences and Engineering, Ann Arbor, United States
Panagiotis Vergados1, Chi O Ao1, Attila Komjathy2, Robert Arthur Preston1, Thomas Navarro3, Gerald Schubert3, Joseph Lazio4, Sami Asmar5 and David H Atkinson5, (1)NASA Jet Propulsion Laboratory, California Institute of Technology, Pasadena, United States, (2)NASA Jet Propulsion Laboratory, Pasadena, CA, United States, (3)UCLA, Los Angeles, CA, United States, (4)Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA, United States, (5)Jet Propulsion Laboratory, California Institute of Technology, Pasadena, United States
Sean Bruinsma1, Jean-charles Marty1, Ingo C F Mueller-Wodarg2, Håkan Svedhem3 and Michela Muñoz4, (1)CNES French National Center for Space Studies, Toulouse Cedex 09, France, (2)Imperial College London, London, SW7, United Kingdom, (3)ESTEC, Noordwijk, Netherlands, (4)ESA/ESAC, Villanueva de la Cañada, Spain
