T146 Friends of Hoth: Episode II—Icy Bodies of the Solar System
Monday, 23 October 2017
1:30 PM - 5:30 PM
Tahoma 1
CONTRASTING ALTITUDINAL TRENDS IN LAUNCH VELOCITIES OF ENCELADUS' PLUME PARTICLES
Paper number: T146-14
Program: Technical Sessions
Time: 4:45 PM – 5:00 PM
Authors
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Matthew M. HedmanUniversity of Idaho, Moscow, ID
Abstract
The trends at low altitudes do not match those expected based on extrapolations of previous observations at higher altitude (1, 2). One potential cause for the different particle launch velocity trends is the presence of more than one particle population in Enceladus’ plume. In such a scenario, at low altitudes (< 35 km), the particle population may be dominated by larger particles (> 5 µm diameter) that are launched at low velocities and would fall off rapidly with altitude giving a steeper slope for launch velocity. In contrast, the particle population at higher altitudes (>35 km) may be dominated by smaller particles (< 5 µm diameter) which would fall off much more gently giving a shallow slope w.r.t altitude. Such a stratified nature of the plume is consistent with previous ideas based on independent datasets (3).
1. Hedman M.M. et al. (2009) Astrophys. J., 693, 1749-1762
2. Hedman M.M. et al. (2013) Nature, 500, 182-184
3. Postberg F. et al. (2011) Nature, 474, 620-622
Geological Society of America Abstracts with Programs. Vol. 49, No. 6
doi: 10.1130/abs/2017AM-302246
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