*Dante S Lauretta1, Hannah H Kaplan2, Humberto Campins3, Harold C Connolly4, Daniella N DellaGiustina1, Jason P Dworkin5, Heather L Enos1, Daniel P Glavin5, Timothy D Glotch6, Dathon R Golish1, Victoria E Hamilton2, Romy D Hanna7, Erica R Jawin8, Timothy J McCoy8, Amy A Simon5, Nicholas Porter1, Dennis Reuter5 (1.University of Arizona, Tucson, AZ, USA, 2.Southwest Research Institute, Boulder, CO, USA , 3.University of Central Florida, Orlando, FL, USA, 4.Rowan University, Glassboro, NJ, USA, 5.NASA Goddard Space Flight Center, Greenbelt, MD, USA, 6.Stony Brook University, Stony Brook, NY, USA, 7.University of Texas, Austin, TX, USA, 8.Smithsonian Institution National Museum of Natural History, Washington, DC, USA)
Session information
[E] Oral
P (Space and Planetary Sciences ) » P-PS Planetary Sciences
[P-PS07] Solar System Small Bodies: Explorations of Ryugu, Bennu, and the Solar System at Large
convener:Taishi Nakamoto(Tokyo Institute of Technology), Tatsuaki Okada(Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency), Dante S Lauretta(University of Arizona), Masateru Ishiguro(Department of Physics and Astronomy, Seoul National University)
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 spacecrafts 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 Ryugu and Bennu whether obtained by rendezvous spacecraft, remote sensing, or other methods.
*Michael C Moreau1, Dante Lauretta2 (1.NASA Goddard Space Flight Center, 2.University of Arizona)
*Daniel Jay Scheeres1, J W McMahon1, A S French1, A B Davis1, D N Brack1, S Chesley2, D Farnocchia2, Y Takahashi2, R S Park2, J Leonard3, P Antreasian3, K Getzandanner4, A Liounis4, D E Highsmith4, D Rowlands4, E Mazarico4, M Moreau4, P Tricarico5, O S Barnouin6, M G Daly7, R W Gaskell5, E E Palmer5, J Weirich5, C L Johnson8, M M Al Asad8, J A Seabrook7, J Roberts7, C W Hergenrother9, M C Nolan9, D S Lauretta9 (1.University of Colorado Boulder, 2.Jet Propulsion Laboratory, 3.KinetX, 4.Goddard Space Flight Center, 5.Planetary Sciences Institute, 6.Applied Physics Laboratory, 7.York University, 8.University of British Colombia, 9.Lunar and Planetary Laboratory, University of Arizona)
*Kana Ishimaru1, Dathon R Golish1, Nicholas Porter1, Manar M Al Asad3, Ronald Ballouz1, Daniellla N DellaGuistina1, Bashar Lizk1, Kevin John Walsh2, Dante S Lauretta1 (1.Lunar and Planetary Laboratory, University of Arizona, 2.Southwest Research Institute, 3.Department of Earth, Oceans, and Atmospheric Sciences, The University of British Columbia)
*Coralie Dominique Adam1, Dante S Loretta2, Carl W Hergenrother2, Steven R Chesley3 (1.KinetX Inc., Space Navigation and Flight Dynamics Practice, Simi Valley, CA, USA, 2.Lunar and Planetary Laboratory, University of Arizona, Tucson, AZ, USA, 3.Jet Propulsion Laboratory, Pasadena, CA, USA)