Ceres: Predictions for near-surface water ice stability and implications for plume generating processes

Abstract

This paper will constrain the possible sources and processes for the formation of recently observed H2O vapor plumes above the surface of the dwarf planet Ceres. Two hypotheses have been proposed: (1) cryovolcanism where the water source is the mantle and the heating source is still unknown or (2) comet-like sublimation where near-surface water ice is vaporized by seasonally increasing solar insolation. We test hypothesis 2, comet-like near-surface sublimation, by using a thermal model to examine the stability of water ice in the near surface. For a reasonable range of physical parameters (thermal inertia, surface roughness, and slopes), we find that water ice is only stable at latitudes higher than ∼40-60 . These results indicate that either (a) the physical properties of Ceres are unlike our expectations or (b) an alternative to comet-like sublimation, such as the cryovolcanism hypothesis, must be invoked.