4800 Oak Grove Drive
Pasadena, CA 91109I am a planetary geologist studying icy surface processes on Rhea (Saturn’s second largest moon), Mars, Vesta, Ceres, Ryugu, Europa, Ganymede, Callisto utilizing various mission data including Cassini, MRO, Mars Express, Dawn, Hayabbusa2, Galileo. I have multi-disciplinary background where I try to connect bridge between remote sensing analysis and surface geological process. Throughout my PhD, I focused onto understand the influence of subsurface volatile and their distribution on the surface of Vesta and Ceres.
Specifically, I am interested in the formation and production of regolith, a cemented material covered over a stable surface, which formed by weathering, erosion, transportation, excavation and/or deposition of the relatively older subsurface mixtures. The ongoing formation of a regolith cover is considered as a final stage of surface evolution; hence their studies related to regolith morphology provide opportunity to identify and interpret the geological process which dominate on the surface of icy planetary objects.
So far, I focused my study on the image analysis, however, for my post-doctoral project I have broaden my horizon by exploring various techniques such as numerical modeling to produce the surface degradation time-line and targeted laboratory analogues to inquire the influence of heterogenous volatile distribution on the surface regolith. For my current project, I aim to anlayse small-scale surface features by investigating higher resolution Galileo mission data for Europa, Ganymede and Callisto. In preparation for the Europa Clipper mission, comparative analysis of various surface features on Galilean satellites (Europa, Ganymede, Callisto) with Ceres and Vesta will be conducted. Especially, the continuum from dominantly icy regolith (Europa, Ganymede, Callisto) to partially icy regolith (Ceres) to relatively dry regolith (Vesta) will permit understanding of the differences in regolith dynamics as related to ice content.
Planetary geology, geomorphology, laboratory analogue, spectroscopy, planetary volatiles, volcanism, surface process, icy planetary bodies, mass wasting, impact craters, surface modeling, regolith
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