Introduction to a “Radical” Working Hypothesis about a Hemisphere-Scale Impact on Dione (Saturn)
Author:
Affiliation:
1. Faculty of Oceanology, Kobe University, 5-1-1 Fukaeminami-machi, Higashinada-ku, Kobe 658-0022, Japan
Publisher
MDPI
Link
https://www.mdpi.com/2673-9984/7/1/14/pdf
Reference21 articles.
1. Dione’s resurfacing history as determined from a global impact crater database;Kirchoff;Icarus,2015
2. Crater modification and geologic activity in Enceladus’ heavily cratered plains: Evidence from the impact crater distribution;Kirchoff;Icarus,2009
3. Plasma, plumes and rings: Saturn system dynamics as recorded in global color patterns on its midsize icy satellites;Schenk;Icarus,2011
4. Tidal dissipation, surface heat flow, and figure of viscoelastic models of Io;Segatz;Icarus,1988
5. Implications from Ithaca Chasma for the thermal and orbital history of Tethys;Chen;Geophys. Res. Lett.,2008
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