Session Details

[P-PS01]Outer Solar System Exploration Today, and Tomorrow

Thu. May 25, 2023 1:45 PM - 3:00 PM JST
Thu. May 25, 2023 4:45 AM - 6:00 AM UTC
106 International Conference Hall, Makuhari Messe
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), Chairperson:Kunio M. Sayanagi(NASA Langley Research Center), Jun Kimura(Osaka University)
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).

[PPS01-11]Investigations of Giant Planet Upper Atmospheres: Past, Present and Future★Invited Papers

*James O Donoghue1, Luke Moore2, Chihiro Tao4, Go Murakami1, Tom Stallard3, Henrik Melin3, Hajime Kita5 (1.JAXA Institute of Space and Astronautical Science, 2.Boston University, 3.University of Leicester, 4.National Institute Of Information And Communications Technology (NICT), 5.Tohoku University)

[PPS01-12]Jupiter’s Magnetic Field and Secular Variation: Implications for the Interior, Rotation Rate, and Particle Motion

*John E P Connerney1 (1.Space Research Corporation)

[PPS01-13]Jovian auroral radio source occultation modelling and application to the JUICE science mission planning

*Baptiste Cecconi1, Corentin K Louis2, Claudio Muñoz Crego3, Claire Vallat4 (1.LESIA, Observatoire de Paris, CNRS, PSL Research University, 2.School of Cosmic Physics, DIAS Dunsink Observatory, Dublin Institute for Advanced Studies, Dublin, Ireland, 3.Aurora B.V., for European Space Agency, ESAC, Madrid, Spain, 4.Rhea Group, for European Space Agency, ESAC, Madrid, Spain)

[PPS01-14]Developing a next generation community modeling framework for the upper atmosphere of Uranus, using the Global Ionosphere-Thermosphere Model (GITM).

*Jared Bell1, Kunio M. Sayanagi2 (1.NASA Goddard Space Flight Center, 2.NASA Langley Research Center)

[PPS01-15]Shadow Chaser: a SmallSat for stellar-occultation measurements of Uranus and Neptune’s thermospheres from Earth orbit

*Kunio M. Sayanagi1, Cindy L Young1, William R Saunders2, Joshua F Carden1, Katherine T McBrayer1, Vianni Ricano Cadenas1, Madison L Hanrahan3, Jonathan D Chrone1, Jared M Bell4, Michael J Person5, Paul Withers2, Joseph F Gasbarre1, Jordan J Klovstad1 (1.NASA Langley Research Center , 2.Boston University, 3.Deep Creek High School, 4.NASA Goddard Space Flight Center, 5.Massachusetts Institute of Technology)