NASA Home Sitemap Dictionary FAQ
+
+
+
Deep Impact Legacy Site
Solar System Exploration Home
News and Events
Planets
Missions
Science and Technology
Multimedia
People
Kids
Education
History
Gallery Education Discovery Zone Your Community Press
Home FAQ Mission Science Technology Mission Results
Objectives  |  Tempel 1  |  Why Study Comets?  |  Cratering  |  Observations 
Comets in Ancient Cultures  |  Creating Colorful Comets  |  Science Team 
Spectroscopy  |  Publications  |  Small Bodies Missions 

Science - Science Team

Peter C. Thomas
 
Institution: Cornell University
Role: Develop digital shape model of the comet nucleus from imagers on the main spacecraft and the impactor; produce image mosaics and interpretive maps of the surface features of the comet; analyze the structure of the comet from surface features.
Address: 422 Space Sciences Building
Cornell University
Ithaca, NY 14853
Bio: Dr. Thomas has an academic background in geomorphology, but did his PhD. work at Cornell on the surface features of the Martian satellites Phobos and Deimos. Since then his scientific work has included the "geology" of small bodies (asteroids and comets); shapes and surface features of ellipsoidal satellites; and eolian features and polar processes on Mars. For Deep Impact he will produce digital shape models of the nucleus for direct analysis and as a base for projections of images and construction of geologic maps of surface features. He has been, or is, a science team member on the Galileo, Cassini, NEAR, Mars Global Surveyor, Mars Climate Orbiter, Mars Polar Lander, CONTOUR, and Mars Reconnaissance Orbiter missions.

BACK

Explore more of NASA on the Web:
FirstGov - Your First Click to the U.S. Government
+
+
+
+
+
NASA Home Page
+