Groove formation on Phobos: Testing the Stickney ejecta emplacement model for a subset of the groove population
Authors:
- Lionel WilsonLWLionel Wilson
- James W. HeadJHJames W. Head
- 1 January 2015
- journal article
- Published by Elsevier in Planetary and Space Science
- Vol. 105, 26-42
Abstract
No abstract availableKeywords
Funding Information
- NASA
- UK Science and Engineering Research Council (SERC) (#SGD/10498)
This publication has 40 references indexed in Scilit:
- The surface geology and geomorphology of PhobosPlanetary and Space Science, 2014
- Survival times of meter-sized boulders on the surface of the MoonPlanetary and Space Science, 2013
- Precise mass determination and the nature of PhobosGeophysical Research Letters, 2010
- The selection and characterization of the Phobos-Soil landing sitesSolar System Research, 2010
- Impact History of Eros: Craters and BouldersIcarus, 2002
- Disruption of kilometre-sized asteroids by energetic collisionsNature, 1998
- The Stickney Impact of Phobos: A Dynamical ModelIcarus, 1993
- A statistical study of impact ejecta distribution around Phobos and DeimosIcarus, 1991
- Results of TV imaging of phobos (experiment VSK-FREGAT)Planetary and Space Science, 1991
- Television observations of PhobosNature, 1989