Watch: Sept. 22 Prof. Yuhui ZHAO: Sublimation induced shape and morphology evolution of small icy bodies

Speaker: Prof. Yuhui ZHAO (Purple Mountain Observatory, CAS) 
Sept.22, 2022
3PM GMT +8
Watch it on Bilibili



Images of the solar system's small icy bodies show great varieties of nuclei shapes and morphologies on their surface. The formation and evolution mechanism of these shapes and surface features such as sinks, pits, cliffs, fractures and pinnacles may indicate a distinct thermal, dynamic and chemical history of the body. The unprecedented amount high resolution data obtained by the Rosetta mission to 67P/Churyumov-Gerasimenko (67P/CG) provided us an opportunity to better understand and further investigate properties of its shape and local surface morphologies and study in better details the process of sublimation in its role in shape evolution. Furthermore, recent results from NASA mission New Horizons revealed the unexpected flattened shape of the Kuiper Belt Object (486958) Arroktoh . How significant is sublimation activities on small icy bodies at such large solar distance? Is it responsible for their peculiar shape formation. Combined with the MONET (mass-loss-driven shape evolution) model, we are able to qualitatively learn the sublimation induced shape and morphology evolution of small icy bodies.

About the speaker



Yuhui Zhao is now a researcher at the Purple Mountain Observatory, working in the field of planetary science. She is the PI of 5 NSFC projects and has published 29 papers in the field of planetary science. She is interested in the study of cometary science, the dynamics of small bodies, and the orbital mechanics of deep space exploration. She has participated in the pre-study of orbital design of several Chinese space missions, including the sample return lunar missions and the Mars missions and was involved in the implementation and data analysis of the CE-2’s Toutatis flyby mission. In recent years, she has participated in study of solar system small bodies combined with observational data obtained by space missions, mainly focusing on the dynamic history, rotational dynamics, shape formation and cometary activities.

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