9:00 AM - 9:15 AM
*Linda T Elkins-Tanton1, Ben Weiss2 (1.Arizona State University, 2.Massachusetts Institute of Technology)
[EE] Oral
P (Space and Planetary Sciences) » P-PS Planetary Sciences
Sun. May 21, 2017 9:00 AM - 10:30 AM 103 (International Conference Hall 1F)
convener:eleonora ammannito(University of California Los Angeles), Taishi Nakamoto(Tokyo Institute of Technology), Masanao Abe(Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency), Christopher T Russell(University of California Los Angeles), Sei-ichiro WATANABE(Division of Earth and Planetary Sciences, Graduate School of Science, Nagoya University), Chairperson:Taishi Nakamoto(Tokyo Institute of Technology)
Small Solar System bodies, including asteroids, comets, satellites, and inter-planetary dust particles, are interesting and provide lots of information on the origin and evolution of our Solar System. They can be remotely sensed by telescopes, be visited by spacecraft and studied at high resolution in a variety of wavelengths from IR to visible, UV, X-rays, and gamma rays, and even with neutrons. In addition, recently spacecraft have been sent to return samples. In this session, all the contributions on the small solar system bodies are welcome. But this year, we especially welcome contributions on recent advances on the study of the asteroids whether obtained by rendezvous spacecraft, sample return, meteorite research or remote sensing.
9:00 AM - 9:15 AM
*Linda T Elkins-Tanton1, Ben Weiss2 (1.Arizona State University, 2.Massachusetts Institute of Technology)
9:15 AM - 9:30 AM
*Satoshi Okuzumi1 (1.Department of Earth and Planetary Sciences, Tokyo Institute of Technology)
9:30 AM - 9:45 AM
*Hsing-Wen Lin1 (1.Institute of Astronomy, National Central University)
9:45 AM - 10:00 AM
*Bjorn Johan Ragnar Davidsson1 (1.Jet Propulsion Laboratory, California Institute of Technology)
10:00 AM - 10:15 AM
*Daniel C Boice1 (1.Scientific Studies and Consulting)
10:15 AM - 10:30 AM
L.T. Elkins-Tanton1, E. Asphaug1, *James F Bell1, D. Bercovici2, B.G. Bills3, R.P. Binzel4, W.F. Bottke5, G.M. Brown3, J. Goldsten6, R. Jaumann7, I. Jun3, D.J. Lawrence6, P. Lord9, S. Marchi5, T. McCoy8, D. Oh3, R.S. Park3, P.N. Peplowski6, C.A. Polanskey3, D. Potter9, T.H. Prettyman10, C.A. Raymond3, C.T. Russell11, S. Scott9, H. Stone3, K.G. Sukhatme3, N.Z. Warner3, B.P. Weiss4, D.D. Wenkert3, M. Wieczorek12, D. Williams1, M.T. Zuber4 (1.Arizona State University, 2.Yale University, 3.Jet Propulsion Laboratory/California Institute of Technology, 4.Massachusetts Institute of Technology, 5.Southwest Research Institute, 6.Applied Physics Laboratory/Johns Hopkins University, 7.DLR/German Aerospace Center, 8.Smithsonian Institution, 9.Space Systems Loral, Inc., 10.Planetary Science Institute, 11.University of California, Los Angeles, 12.Observatoire de la Côte d'Azur)
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