*********************************
There is now a CONTENT FREEZE for Mercury while we switch to a new platform. It began on Friday, March 10 at 6pm and will end on Wednesday, March 15 at noon. No new content can be created during this time, but all material in the system as of the beginning of the freeze will be migrated to the new platform, including users and groups. Functionally the new site is identical to the old one. webteam@gatech.edu
*********************************
Andrew Newman
Summary Sentence: A seminar by Dr. Michael Sori, School of Earth and Atmospheric Sciences
Full Summary: No summary paragraph submitted.
Michael SoriCeres, the largest object in the asteroid belt, has been revealed by NASA’s Dawn mission to be a complex geophysical world. Its transitional nature – somewhere between icy and rocky, asteroid and planet – allows Ceres to elucidate a number of planetary processes.
In this talk, I will focus on icy volcanism, also called cryovolcanism. I will argue that surface features show Ceres to be geologically active, and geophysical models constrain its cryovolcanic rate. The level of activity I infer shows that cryovolcanism is an important geological process in the solar system, but is not as dominant as silicate volcanism.
I will end by discussing ways in which the geophysical techniques here can be used to study other topics on Mars, Mercury, the Moon, and Ceres, including how the Dawn data can be used to investigate ice deformation, the faint young sun, and planetary differentiation.
