Session Details
[P-PS01]Outer Solar System Exploration Today, and Tomorrow
Thu. May 25, 2023 3:30 PM - 5:00 PM JST
Thu. May 25, 2023 6:30 AM - 8:00 AM UTC
Thu. May 25, 2023 6:30 AM - 8:00 AM UTC
Online Poster Zoom Room (1) Online Poster
convener:Jun Kimura(Osaka University), Kunio M. Sayanagi(NASA Langley Research Center ), Fuminori Tsuchiya(Planetary Plasma and Atmospheric Research Center, Graduate School of Science, Tohoku University)
On-site poster schedule(2023/5/25 17:15-18:45)
The giant planets provide many keys to understanding planetary processes. They play an important role in shaping our solar system, and the physical and chemical processes they harbor also provide a unique opportunity to study the phenomena relevant for studying Earth and other planets, including exoplanetary systems. In this session, we discuss a wide range of topics encompassing the giant planets and their moons, including their origins, interiors, atmospheres, compositions, surface features, and electromagnetic fields. To advocate for current and future outer planets exploration (Juno, New Horizons, JUICE, Europa Clipper, Dragonfly and beyond), we also call for discussions on future missions to explore giant planet systems, including how to develop better international cooperation. Discussion in this latter category will include progress in developing a solar sail mission concept for observing the Jupiter system and its Trojan asteroids. We also solicit presentations about new scientific results generated using data returned by space telescopes such as the James Webb Space Telescope (JWST).
[PPS01-P01]Update on Japanese Participation in JUICE (Jupiter Icy Moons Explorer)
*Yoshifumi Saito1, Yasuhito Sekine2, Yasumasa Kasaba3, Keigo Enya1, Kazushi Asamura1, YASUKO KASAI4, Junichi Haruyama1, Ayako Matsuoka5, Kazuyuki Tohara1 (1.Solar System Science Division, Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency, 2.Tokyo Institute of Technology, 3.Tohoku University, Graduate School of Science, 4.National Institute of Information and Communications Technology, 5.Kyoto University, Graduate School of Science)
[PPS01-P02]JUICE in Japan and its science goals
*Yasuhito Sekine1, Yoshifumi Saito2, Kazushi Asamura2, Keigo Enya2, Yasumasa Kasaba3, YASUKO KASAI4, Junichi Haruyama2, Ayako Matsuoka5 (1.Earth-Life Science Insitute, Tokyo Institute of Technology, 2.ISAS, JAXA, 3.Tohoku University, 4.NICT, 5.Kyoto University)
[PPS01-P03]The Ganymede Laser Altimeter (GALA) for the Jupiter Icy Moons Explorer (JUICE): Science objectives
*Jun Kimura1, Hauke Hussmann2, Shunichi Kamata4, Koji Matsumoto5, Jurgen Oberst2, Gregor Steinbrugge6, Alexander Stark2, Klaus Gwinner2, Shoko Oshigami3, Noriyuki Namiki5, Kay Lingenauber2, Keigo Enya3, Kiyoshi Kuramoto4, Sho Sasaki1 (1.Osaka University, 2.DLR, 3.JAXA, 4.Hokkaido University, 5.NAOJ, 6.NASA Jet Propulsion Laboratory)
[PPS01-P04]The Ganymede Laser Altimeter (GALA) for the Jupiter Icy Moons Explorer (JUICE): Performance Model Simulation
*Hiroshi Araki1, Ishibashi Ko2, Noriyuki Namiki1, Hirotomo Noda1, Masanori Kobayashi2, Keigo Enya3, Masanobu Ozaki1, Mizuno Takahide3, Yoshihumi Saito3, Kazuyuki Touhara3, Shoko Oshigami3, Shingo Kashima1, Jun Kimura4, Gregor Steinbrugge5, Alexander Stark5, Christian Althaus5, Simone Del Togno5, Kay Lingenauber5, Hauke Hussmann5 (1.National Astronomical Observatory of Japan, 2.Chiba Institute of Technology Planetary Exploration Research Center, 3.Institute of Space and Astronautical Science, 4.Osaka University, 5.German Aerospace Center)
[PPS01-P05]The Ganymede Laser Altimeter (GALA) for the Jupiter Icy Moons Explorer (JUICE): The Backend Optics (BEO) mocule and the Focal Plane Assembly (FPA) module
*Keigo Enya1, Masanori Kobayashi2, Satoru Iwamura3, Naofumi Fujishiro4, Shingo Kashima5, Hiroshi Araki5, Hirotomo Noda5, Noriyuki Namiki5, Shoko Oshigami1, Ko Ishibashi2, Jun Kimura6, Kazuyuki Touhara1, Yoshifumi Saito1, Christian Althaus7, Simone del Togno7, Lingenauber Kay7, Reinald Kallenbach7, Hauke Hussmann7 (1.JAXA/ISAS, 2.CIT, 3.MRJ, 4.AstroOpt, 5.NAOJ, 6.Osaka University, 7.DLR)
[PPS01-P06]The Ganymede Laser Altimeter (GALA) for the Jupiter Icy Moons Explorer (JUICE): APD and Electronics
*Kobayashi Masanori1, Ko Ishibashi1, Osamu Okudaira1, Keigo Enya2, Takahide Mizuno2, Yoshifumi Saito2, Kazuyuki Touhara2, Masayuki Fujii3, Thomas Behnke4, Hauke Hussmann4, Reinald Kallenbach4, Kay Lingenauber4, Simone del Togno4 (1.Chiba Institute of Technology, 2.Japan Aerospace Exploration Agency, 3.FAM Science Co., Ltd., 4.Deutsches Zentrum für Luft- und Raumfahrt)
[PPS01-P07]Magnetic field experiment at Jupiter icy moons (JUICE J-MAG) and in-flight sensor alignment calibration
*Ayako Matsuoka1, Michele Dougherty2, Patrick Brown2, Hans-Ulrich Auster3, Hisayoshi Shimizu4, Futoshi Takahashi5 (1.Data Analysis Center for Geomagnetism and Space Magnetism, Graduate School of Science, Kyoto University, 2.Imperial College London, 3.Institut für Geophysik und extraterrestrische Physik, Technische Universität Braunschweig, 4.Earthquake Research Institute, The University of Tokyo, 5.Faculty of Science, Kyushu University)
[PPS01-P08]A putative model region for Wilson-cycles on icy satellites: Dione´s Wispy Terrain
*Balazs Bradak1, Jun Kimura2, Christopher A Gomez1, Roland Novak1 (1.Faculty of Oceanology, Kobe University , 2.Department of Earth and Space Science, Osaka University)
[PPS01-P09]Reorientation of Ganymede induced by furrow-forming impact
*Naoyuki Hirata1 (1.Kobe University)
[PPS01-P10]Investigations of ice properties on Galilean satellites through telescope observations and laboratory experiments in wavelengths of 1.0-1.5 μm
*Shuya Tan1, Masayuki Kuzuhara2,3, Yasuhito Sekine1, Gabriel Tobie4, Erwan Le Menn4, Benoit Jabaud4 (1.Earth-Life Science Institute, Tokyo Institute of Technology, 2.Astrobiology Center, 3.National Astronomical Observatory of Japan, 4.Nantes University)
[PPS01-P11]Toward measurements of elastic wave velocities of laboratory analogs of Titan’s organic materials
*Eito Hirai1,2, Yasuhito Sekine2,3, Takeshi Tsuji4, Osamu Nishizawa, Tomohiro Ohuchi5, Yuji Higo6 (1.Department of Earth and Planetary Sciences, School of Science, Tokyo Institute of Technology, 2.Earth–Life Science Institute (ELSI), Tokyo Institute of Technology, 3.Institute of Nature and Environmental Technology, Kanazawa University, 4.Department of Systems Innovation, the University of Tokyo, 5.Geodynamics Research Center, Ehime University, 6.Japan Synchrotron Radiation Research Institute)
[PPS01-P12]Long-term monitoring of Jupiter’s aurora and Io torus by Hisaki EXCEED
*Hajime Kita1, Tomoki Kimura2, Fuminori Tsuchiya3, Go Murakami4, Atsushi Yamazaki4, Chihiro Tao5, Ryoichi Koga6, Reina Hikida7, Kazuo Yoshioka8, Ichiro Yoshikawa8 (1.Tohoku Institute of Technology, 2.Tokyo University of Science, 3.Tohoku University, 4.ISAS/JAXA, 5.NICT, 6.Nagoya University, 7.JAXA, 8.The University of Tokyo)
[PPS01-P13]Localized hot electron injection on the dusk side during transient brightening in Io plasma torus observed by Hisaki
Kento Furukawa1, *Fuminori Tsuchiya1, Masato Kagitani1, Kazuo Yoshioka2, Ichiro Yoshikawa2, Tomoki Kimura3, Hajime Kita4, Go Murakami5, Atsushi Yamazaki5, Hiroaki Misawa1, Yasumasa Kasaba1, Masafumi Imai6 (1.Tohoku University, 2.The University of TThe , 3.Tokyo University of Science, 4.Tohoku Institute of Technology, 5.Japan Aerospace and Exploration Agency, 6.National Institute of Technology, Niihama College)
[PPS01-P14]Numerical simulation of passive radar for ionospheric explorations at Jupiter's icy moons
*Rikuto Yasuda1, Tomoki Kimura2, Hiroaki Misawa1, Fuminori Tsuchiya1, Shinnosuke Satoh1, Yasumasa Kasaba1, Shotaro Sakai1, Atsushi Kumamoto1, Baptiste Cecconi3, Corentin Louis4, Philippe Zarka3 (1.TOHOKU UNIVERSITY, 2.TOKYO UNIVERSITY OF SCIENCE, 3.OBSERVATOIRE DE PARIS, 4.DIAS DUNSINK OBSERVATORY)
[PPS01-P15]Kronian current sheet geometry and its link to reconnection
*Cristian Robert Radulescu1,2, Andrew Coates1,2, Geraint Jones1,2, Nick Achilleos2,3, Yasumasa Kasaba4 (1.Mullard Space Science Laboratory, UCL, Dorking, UK, 2.Center for Planetary Sciences at UCL/Birkbek, London, UK, 3.Dept. of Physics and Astronomy, UCL, London, UK, 4.Tohoku University, Japan )
[PPS01-P16]Polarization characteristics of Jupiter's hectometric radio emission
*Hiroaki Misawa1, Fuminori Tsuchiya1, Atsushi Kumamoto2, Rikuto Yasuda1, Yoshiya Kasahara3, Yoshizumi Miyoshi4, Satoko Nakamura4 (1.Planetary Plasma and Atmospheric Research Center, Graduate School of Science, Tohoku University, 2.Department of Geophysics, Graduate School of Science, Tohoku University, 3.ARC-SAT, Kanazawa University, 4.ISEE, Nagoya University)
[PPS01-P17]Physics-based computational capabilities for investigating the radio and energetic neutral atom emissions originated from the radiation belts of the Gas and Ice Giants
*Daniel Santos-Costa1, Quentin Nénon2, Nicolas André2, Imke de Pater3, Peter Kollmann4, Henry B. Garrett5, Insoo Jun6, Emma Woodfield7, Angélica Sicard8 (1.Southwest Research Institute, 2.IRAP, 3.University of California, Berkeley, 4.JHU/APL, 5.Consultant, 6.JPL/Caltech, 7.British Antarctic Survey, 8.ONERA)
[PPS01-P18]Implications of short-term variations in Jupiter's inner electron belts observed with the Very Large Array's high sensitivity and angular resolution capabilities
*Daniel Santos-Costa1, Imke de Pater2, Robert J. Sault3, Bryan Butler4, Chris Moeckel2, Tim Keebler5, Julien N. Girard6, Philippe Zarka6, Emma Woodfield7, Quentin Nénon8, Nicolas André8, Fuminori Tsuchiya9, Chihiro Tao10, Hajime Kita11 (1.Southwest Research Institute, 2.University of California, Berkeley, 3.Consultant, 4.NRAO, 5.University of Michigan, 6.LESIA, Observatoire de Paris, 7.British Antarctic Survey, 8.IRAP, 9.PPARC, Tohoku University, 10.NICT, 11.Tohoku Institute of Technology)