T140 From Bouncing Grains to Cemented Sandstones: Aeolian Processes and Stratigraphy in the Solar System
Monday, 26 September 2016
1:30 PM - 5:30 PM
Mile High Ballroom 2C
REDISTRIBUTION OF PARTICLES ACROSS THE NUCLEUS OF COMET 67P/CHURYUMOV-GERASIMENKO
Paper number: T140-2
Program: Technical Sessions
Time: 1:35 PM – 1:55 PM
Authors
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Bjorn DavidssonUppsala University, Uppsala
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Ramy El-MaarryBern Universität, Bern
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Sonia FornasierUPMC Univ. Paris 06, Univ. Paris Diderot, Meudon Principal Cedex
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Lorenza GiacominiUniversity of Padova, Padova
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Antonio Gracia-BernaPhys. Inst., Universität Bern,, Bern
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Stubbe HviidDeutsches Zentrum für Luft- und Raumfahrt (DLR), Institut für Planetenforschung, Berlin
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The OSIRIS TeamGöttingen
Abstract
Sublimation-driven ejection of material from an active area is the initiator of material motion in a cometary system. The non-volatile material (usually referred to as dust) is accelerated by gas, and much of it reaches escape velocity, thereby permanently leaving the cometary environment. However, it is now clear that not all non-volatile material acquires sufficient energy to escape. There is evidence in the images for the accumulation of non-escaping dust particles emitted from areas of activity in a form of “airfall”. Furthermore, there are observations of features that appear similar to aeolian ripples, dune-like structures, possible wind-tails, and near-boulder deposits, indicating that other processes may be at work in transporting non-volatile material across the surface.
We show by numerical modelling that a type of saltation is plausible even under the rarified gas densities seen at the surface of the nucleus. However, interparticle cohesive forces present difficulties for this model, and an alternative mechanism for the initiation of reptation and creep may result from the airfall mechanism. The requirements on gas density and other parameters of this alternative make it a more attractive explanation for the observations. The uncertainties and implications will be discussed, based on Thomas et al. Astron. Astrophys. 583, A17, dx.doi:10.1051/0004-6361/201526049, 2015.
Geological Society of America Abstracts with Programs. Vol. 48, No. 7
doi: 10.1130/abs/2016AM-281342
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