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Sori_et_al-2017-Geophysical_Re ...
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Author
Sori, Michael M.
Byrne, Shane

Bland, Michael T.
Bramson, A. M.

Ermakov, Anton I.

Hamilton, Christopher W.

Otto, Katharina A.

Ruesch, Ottaviano
Russell, C. T.

Affiliation
Univ Arizona, Lunar & Planetary LabIssue Date
2017-02-16
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AMER GEOPHYSICAL UNIONCitation
The vanishing cryovolcanoes of Ceres 2017, 44 (3):1243 Geophysical Research LettersJournal
Geophysical Research LettersRights
© 2017. American Geophysical Union. All Rights Reserved.Collection Information
This item from the UA Faculty Publications collection is made available by the University of Arizona with support from the University of Arizona Libraries. If you have questions, please contact us at repository@u.library.arizona.edu.Abstract
Ahuna Mons is a 4 km tall mountain on Ceres interpreted as a geologically young cryovolcanic dome. Other possible cryovolcanic features are more ambiguous, implying that cryovolcanism is only a recent phenomenon or that other cryovolcanic structures have been modified beyond easy identification. We test the hypothesis that Cerean cryovolcanic domes viscously relax, precluding ancient domes from recognition. We use numerical models to predict flow velocities of Ahuna Mons to be 10-500 m/Myr, depending upon assumptions about ice content, rheology, grain size, and thermal parameters. Slower flow rates in this range are sufficiently fast to induce extensive relaxation of cryovolcanic structures over 10(8)-10(9) years, but gradual enough for Ahuna Mons to remain identifiable today. Positive topographic features, including a tholus underlying Ahuna Mons, may represent relaxed cryovolcanic structures. A composition for Ahuna Mons of >40% ice explains the observed distribution of cryovolcanic structures because viscous relaxation renders old cryovolcanoes unrecognizable.Note
6 month embargo; First published: 10 February 2017ISSN
00948276Version
Final published versionAdditional Links
http://doi.wiley.com/10.1002/2016GL072319ae974a485f413a2113503eed53cd6c53
10.1002/2016GL072319