太陽系和系外行星中恒星與行星作用及衛星與磁層作用的天文物理過程的理論模型研究(2/3)

It is becoming increasingly clear that our Solar System is unique in the sense that it is not just our home in the vast Universe, but also an experimental laboratory to decipher the mysteries of the formation of planets and origin of life in other worlds. After the voyages to the Saturnian system and Titan with the NASA-ESA Cassini mission and to comet 67P/Churyumov-Gerasimenko with the Rosetta mission of ESA, we are embarking on a new journey to exoplanets with a view to compare the physical processes in the evolutionary histories of the Solar System and the planetary systems of other low-mass stars. In the case of our own planetary system, the research will emphasize scientific problems to be clarified by ongoing and future spacecraft missions such as the BepiColombo mission to Mercury, the Parker Solar Probe and Solar Orbiter missions, the Europa Clipper of NASA and JUICE mission of ESA, and thePsyche mission of NASA. These include the injection of high-speed beta-meteoroids from a near-sun dust belt and their collisional interaction with Mercury and other planets, the satellite-magnetosphere interaction at the Jovian system, and the surface properties of asteroids. These in-depth studies will be connected to the investigation of the exo-moons, and the corresponding star-planet interaction (Space wether effects) as a result of the magnetic activities (superflares and coronal mass ejection) of the host stars of exoplanets taking advantage of the wealth of high-precision photometric data from the Kepler and TESS space telescopes as well as the ground-basedobservations on Lulin Observatory.