Session outline
| Space and Planetary Sciences (P) | ||
|---|---|---|
| Session Sub-category | Planetary Sciences(PS) | |
| Session ID | P-PS11 | |
| Title | Mercury Science and Exploration | |
| Short Title | Mercury Science and Exploration | |
| Main Convener | Name | Go Murakami |
| Affiliation | Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency | |
| Co-Convener 1 | Name | Yuki Harada |
| Affiliation | ISEE, Nagoya University | |
| Co-Convener 2 | Name | Shunichi Kamata |
| Affiliation | Faculty of Science, Hokkaido University | |
| Co-Convener 3 | Name | Sae Aizawa |
| Affiliation | Laboratoire de Physique des Plasmas | |
| Session Language |
E |
|
| Scope |
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. |
|
| Presentation Format | Oral and Poster presentation | |
| Time | Presentation No | Title | Presenter |
|---|---|---|---|
| Oral Presentation May 25 PM1 | |||
| 13:50 - 14:05 | PPS11-01 | Updated status and upcoming plans of the BepiColombo mission | Go Murakami |
| 14:05 - 14:20 | PPS11-02 | Magnetic field measurement during cruising and observation plan at Mercury of BepiColombo MIO MGF | Ayako Matsuoka |
| 14:20 - 14:45 | PPS11-03 | A Survey of Reconnection Layer around Mercury's Magnetopause | Jih-Hong Shue |
| 14:45 - 15:00 | PPS11-04 | Ion bursts in Mercury’s Magnetotail during BepiColombo’s second flyby | Akimasa Ieda |
| 15:00 - 15:15 | PPS11-05 | A Statistical Study of the Dependence of Magnetic Field and Proton Structures in Mercury’s Magnetotail on Upstream IMF Directions | Tomoki Mori |
| Oral Presentation May 25 PM2 | |||
| 15:30 - 15:55 | PPS11-06 | Modeling Na spectral line shapes in Mercury’s exosphere and its implications for BepiColombo/MSASI observations | Yudai Suzuki |
| 15:55 - 16:10 | PPS11-07 | Development of a New Emission-Line Spectral Analysis Method to Constrain the Energy Distribution of Mercury’s Sodium Exosphere | Ukyo Kitamura |
| 16:10 - 16:25 | PPS11-08 | Seasonal Variations and Source Processes of Mercury's Sodium Atmosphere | Kouki Masaki |
| 16:25 - 16:50 | PPS11-09 | First global map of Mercury's surface roughness implies previous underestimation of the planet's radial contraction | Gaku Nishiyama |
| Presentation No | Title | Presenter |
|---|---|---|
| Poster Presentation May 25 PM3 | ||
| PPS11-P01 | Observation of spatio-temporal variations in Mercury's sodium exosphere using the Haleakala T60 telescope with the fiber-fed spectrograph | Naoko Takatori |
| PPS11-P02 | Insights into Mercury's Hydrogen Exosphere: Characterization and First Detection of H2 Molecules | Fabian Weichbold |
| PPS11-P03 | Observation of Mercury's Potassium and Sodium Exosphere using the Haleakala T60 Telescope | Masato Kagitani |
| PPS11-P04 | EMIC Waves in Mercury's Magnetosphere: Statistical Analysis by the MESSENGER Spacecraft | Riku Kikuchi |
| PPS11-P05 | Magnetic Field Analysis of Field-Aligned Currents in Mercury’s Magnetosphere | Takuro OGAWA |
| PPS11-P06 | Mercury's Internal Structure Model Based on Geodetic and Cosmochemical Constraints | Kazuki Takahashi |
| PPS11-P07 | Mercury's Tidal Response: Investigating the Cause of Its Soft Interior Structure | Shunichi Kamata |