碩博班專題討論(Colloquium)
Origin of Neutral Gas with Peculiar Velocity in the Saturn E-ring
演講者 : Prof. Yueh-ning Li 李悅寧 教授 (National Taiwan Normal University)
演講地點 :
理學教學新大樓物理系1F 36102教室
演講時間 :
2023 / 09 / 08
14:10
The materials of Saturn E-ring are known to have originated from the satellite Enceladus. Once leaving the satellite, either by surface sputtering, outgassing plumes, or other mechanisms, the ejected material is subject to several forces in synergy, among which gravity, electromagnetic forces, and radiation forces. In consequence, unlike Enceladus, which is massive enough to follow a Keplerian orbit, all kinds of trajectories are manifested by small particles. Particles with a large mass-to-charge ratio barely feel the sweeping magnetic field that is co-rotating with Saturn. On the other hand, particles with small mass-to-charge ratio have small gyro-radius, and thus are bound to the magnetic field lines. Through Hamiltonian analysis, we discovered that particles with intermediate mass-to-charge ratio may form a distinct population of ring particles. This population can exhibit some peculiar velocity signatures that are verifiable through observations.