Session Details
[P-PS04]Advancing the science of Venus in the golden age of exploration
Wed. May 24, 2023 9:00 AM - 10:15 AM JST
Wed. May 24, 2023 12:00 AM - 1:15 AM UTC
Wed. May 24, 2023 12:00 AM - 1:15 AM UTC
Exhibition Hall Special Setting (3) Exhibition Hall 8, Makuhari Messe
convener:Takehiko Satoh(Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency), George HASHIMOTO(Department of Earth Sciences, Okayama University), Moa Persson(Graduate School of Frontier Sciences, The University of Tokyo, Kashiwa, Japan), Kevin McGouldrick(University of Colorado Boulder), Chairperson:George HASHIMOTO(Department of Earth Sciences, Okayama University), Takao Sato(Hokkaido Information University)


Exploration of Venus in the 21st century was opened by two missions, polar-orbiting Venus Express (ESA, 2006 - 2014) and equatorial-orbiting Akatsuki (JAXA, 2015 to current). These two have advanced our knowledge mostly about the Venusian atmosphere (dynamics, chemistry and evolution). The upcoming 3 Venus missions, NASA's VERITAS and DAVINCI, and ESA's EnVision are more focused on the geology, interior and evolution of the
solid planet, Venus. There may be more to come, such as Chinese VOICE, Indian Shukurayaan, Russian Venera-D, and even from a private company. We are and will certainly be in a new golden age of the Venus exploration! This session will therefore cover all aspects of science related to Venus, from its interior to the surrounding plasma environment, either by observationally or by theoretically. Implications to the exoplanets are also important objectives of studies of Venus. Contributions by all levels, from early-career researchers to experts, are all welcome.
solid planet, Venus. There may be more to come, such as Chinese VOICE, Indian Shukurayaan, Russian Venera-D, and even from a private company. We are and will certainly be in a new golden age of the Venus exploration! This session will therefore cover all aspects of science related to Venus, from its interior to the surrounding plasma environment, either by observationally or by theoretically. Implications to the exoplanets are also important objectives of studies of Venus. Contributions by all levels, from early-career researchers to experts, are all welcome.
[PPS04-06]An extrapolation of mantle dynamics in Mars to Venus★Invited Papers
*Masaki Ogawa1 (1.Division of General Systems Studies, Graduate School of Arts and Sciences, University of Tokyo)
[PPS04-07]An Examination of the Interactions Between Calcium Minerals and SO2 under A Simulated Venus Environment
*Sara Taeko Port1, Alison Santos2, Dorothy Lukco3, Tibor Kremic4, Gary Hunter4 (1.Oak Ridge Associated Universities, 2Department of Earth and Environmental Sciences, 2.Department of Earth and Environmental Sciences, Wesleyan University, Middletown, CT 06459, 3.HX5, LLC, 4.NASA Glenn Research Center, 21000 Brookpark Road, Cleveland, OH 44135)
[PPS04-08]Magnetic Topology at Venus★Invited Papers
*Shaosui Xu1, Rudy A Frahm2, Yingjuan Ma3, Janet Luhmann1, David Mitchell1, Moa Brita Persson4 (1.University of California, Berkeley, United States, 2.Southwest Research Institute, TX, USA, 3.University of California Los Angeles, CA, USA, 4.The University of Tokyo, Japan)
[PPS04-09]Meridional distribution of gravity waves in the Venusian atmosphere revealed by radio occultation
Fukuoka Seiki1, *Takeshi Imamura1, Hiroki Ando2, Bernd Häusler3, Martin Pätzold4, Silvia Tellmann4 (1.Graduate School of Frontier Sciences, The University of Tokyo, 2.Kyoto Sangyo University, 3.Universitat der Bundeswehr Munchen, Germany, 4.Universitat zu Koln, Germany)
[PPS04-10]Derivation of vertical profiles of sulfur dioxide (SO2) in the Venus cloud layer by the Akatsuki radio occultation measurements
Hinako Onuma1, *Katsuyuki Noguchi1, Hiroki Ando2, Takeshi Imamura3, Hideo Sagawa2 (1.Faculty of Science, Nara Women's University, 2.Faculty of Science, Kyoto Sangyo University, 3.Graduate School of Frontier Sciences, The University of Tokyo )
