セッション詳細
[P-PS04]Mercury Science and Exploration
2025年5月25日(日) 17:15 〜 19:15
ポスター会場 幕張メッセ国際展示場 7・8ホール
コンビーナ:村上 豪(宇宙航空研究開発機構宇宙科学研究所)、相澤 紗絵(Laboratoire de Physique des Plasmas, CNRS)、原田 裕己(京都大学理学研究科)、鎌田 俊一(北海道大学 理学研究院)
Mercury, the innermost planet in our Solar System, with its unique features, holds vital clues to understanding the evolution of terrestrial planets and the solar system. NASA's Mariner-10 and MESSENGER missions provided valuable insights but also left outstanding questions. These will soon to be addressed by the joint ESA-JAXA two spacecraft mission, BepiColombo, which is currently en route to Mercury and has already conducted several flybys. This session welcomes contributions on all aspects of Mercury's environment, including its origin, formation, geology, surface composition, interior structure, exosphere, magnetosphere, gravity, and magnetic fields, as well as their coupling using various research methods such as modeling, laboratory experiments, and observations (ground-based, remote-sensing, and in-situ). We also encourage early analyses of BepiColombo flyby data and discussions regarding future missions to Mercury.
[PPS04-P01]Could Solar Wind Have Decreased Permeability on Mercury and Other Airless Worlds?★Invited Papers
*Alexis P. Rodriguez1、Deborah Domingue2、Chloe Marini3 (1.NASA/Marshall Space Flight Center, Huntsville, Alabama, USA. 、2.Planetary Science Institute, Tucson, Arizona, USA.、3.University of Alabama Huntsville, Huntsville, Alabama, USA. )
[PPS04-P02]The dependence of Mercury’s magnetotail protons on IMF directions: MESSENGER observations
*毛利 智紀1、原田 裕己1、相澤 紗絵2 (1.京都大学理学研究科、2.Laboratoire de Physique des Plasmas, CNRS)

[PPS04-P03]Daytime observation of Mercury with a visible adaptive otpics installed on Tohoku 60-cm telescope at Haleakala observatory
*鍵谷 将人1、笠羽 康正1、高鳥 尚子1 (1.東北大学大学院理学研究科惑星プラズマ・大気研究センター)
[PPS04-P04]Mercurian magma ocean crystallization as a function of oxygen fugacity and sulfur content
*Jiejun Jing1,2、Jurrien S. Knibbe2、Paul ten Dam2、 Yong Wu3、Qing-Han Yuan4、Ben-Xun Su4、Wim van Westrenen2 (1.Geodynamics Research Center, Ehime University、2.Departement of Earth Sciences, Vrije Universiteit Amsterdam、3.Beijing Research Institute of Uranium Geology、4.Institute of Geology and Geophysics, Chinese Academy of Sciences)
