Introduction (1:45 PM - 1:50 PM)
Session information
[E] Oral
P (Space and Planetary Sciences ) » P-PS Planetary Sciences
[P-PS11] Mercury Science and Exploration
Mon. May 25, 2026 1:45 PM - 3:15 PM 303 (International Conference Hall, Makuhari Messe)
Chairperson:Murakami Go(Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency)
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 completed all flybys, and the two BepiColombo orbiters will arrive at Mercury in November 2026. 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 fi elds, 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.
1:50 PM - 2:05 PM
*Go Murakami1, Geraint Jones2, Sebastien Besse2 (1. Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency, 2. European Space Agency)
2:05 PM - 2:20 PM
*Ayako Matsuoka1, Daniel Schmid2, Wolfgang Baumjohann2, Werner Magnes2, Hans-Ulrich Auster3, David Fischer2, Josef Wilfinger2, Yasuhito Narita3, Rumi Nakamura2, Manabu Shinohara4, Yoshimasa Tanaka5, Akiko Fujimoto6, Masaki Matsushima7, Kazuhiro Yamamoto8 (1. Data Analysis Center for Geomagnetism and Space Magnetism, Graduate School of Science, Kyoto University, 2. The Space Research Institute, OeAW, 3. Technical University of Braunschweig, 4. Kagoshima National College of Technology, 5. National Institute of Polar Research, 6. Kyushu Institute of Technology, 7. Institute of Science Tokyo, 8. Nagoya University)
2:20 PM - 2:45 PM
I-Hsiang Chiu1, *Jih-Hong Shue1, Hiroshi Hasegawa2, Yasuhito Narita3, Jun Zhong4, Masafumi Hirahara5 (1. National Central University, Taiwan, 2. JAXA, Japan, 3. Technical University Braunschweig, Germany, 4. Chinese Academy of Sciences, China, 5. Nagoya University, Japan)
2:45 PM - 3:00 PM
*Akimasa Ieda1, Yuki Harada1, Yoshifumi Saito2, Hiroshi Hasegawa2, Shoichiro Yokota3, Wataru Miyake4, Go Murakami2 (1. Institute for Space-Earth Environmental Research, Nagoya University, 2. Institute of space and astronautical sicence, 3. Osaka university, 4. Tokai university)
3:00 PM - 3:15 PM
*Tomoki Mori1, Yuki Harada2, Ayako Matsuoka3, Sae Aizawa4, Weijie Sun5, Charles F. Bowers6 (1. Graduate School of Science, Kyoto University, 2. ISEE, Nagoya University, 3. Data Analysis Center for Geomagnetism and Space Magnetism, Graduate School of Science, Kyoto University, 4. Laboratoire de Physique des Plasmas, 5. University of California, Berkeley, 6. Dublin Institute for Advanced Studies)