Staff Scientist
Lunar and Planetary Institute
3600 Bay Area Blvd.,
Houston, Texas 77058
schenk@lpi.usra.edu
281 486-2157

Current activities include the study of impact crater morphology on Ganymede and on other icy satellites, including the impact of split comets on the Galilean Satellites. I have also been using stereo images to map the shape and topography of mountains and shield volcanos on Io, including the largest known landslide in the solar system at Euboea Montes (paper to be published in Science on March 6, 1998), and the flow of lava around topographic obstacles at Ra Patera. Other projects include the topography of lava flows and craters on small icy satellites, and the geology of the odd landscape of Triton, including cantaloupe terrain.
Ganymede and Callisto Crater Database
3-D Tour of the Solar System (now available on CD-ROM!)
Topography of Valhalla and Gilgamesh impact basins, Callisto and Ganymede -
ABSTRACT (.PDF), FIGURES
Stereo Topography of the Ra Patera volcano, Io -
PREPRINT (.PDF), (.TXT), FIGURES
Origin of Mountains on Io by Thrust Faulting and
Large-scale Mass Movements -
Figures.
This paper will be published in
Science magazine on March 6, 1998.
Schenk, P., and W. McKinnon, 1989. Fault offsets and lateral crustal movement on Europa: Evidence for a mobile ice shell, Icarus, 79, p. 75-100.
Schenk, P., and M.P.A. Jackson, 1993. Diapirism on Triton: A record of crustal layering and instability, Geology, 21, p. 299-302.
Schenk, P., and J. Moore, 1995. Volcanic constructs on Ganymede and Enceladus, J. Geophysical Res., 100, p. 19009-19022.
Schenk, P., E. Asphaug, W. McKinnon, H. Melosh, and P. Weissman, 1996. Cometary nuclei and tidal disruption: The geologic record of crater chains on Callisto and Ganymede, Icarus, 121, p. 249-274.
Schenk, P., A. McEwen, A. Davies, T. Davenport, K. Jones, and B. Fessler, Geology and topography of Ra Patera, Io, in the Voyager era: Prelude to eruption, Geophysical Research Letters, 24, 2468, 1997.
Schenk, P., and M.H. Bulmer, Thrust faulting, block rotation and large-scale mass movements at Euboea Montes, Io, submitted, Science, October, 1997.


©Lunar and Planetary Institute, Houston, Texas, 1997