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Title: Laboratory Studies in Support of Planetary Geophysics
Primary Author: Julie Castillo-Rogez
Secondary Author(s): William B. Durham, Essam Heggy, Mathieu Choukroun, Jerome Noir, Sarah T. Stewart, Steve D. Vance, Christine M. McCarthy, Martin B. Barmatz, Pamela G. Conrad
Institution: Jet Propulsion Laboratory
Summary: We summarize the rationale for advocating a healthy and sustained program of laboratory research in support of the geophysical exploration of planetary bodies. We address the challenges inherent to this discipline, and we suggest recommendations for the review panel''s consideration.
Panel Selection: Inner Planets: Mercury, Venus, and the Moon. Mars: Not Phobos and Deimos. Giant Planets: Jupiter, Saturn, Uranus, Neptune, and exoplanets, including rings and magnetic fields, but not their satellites. Satellites: Galilean satellites, Titan, and the other satellites of the giant planets. Primitive Bodies: Asteroids, comets, Phobos, Deimos, Pluto/Charon and other Kuiper belt objects, meteorites, and interplanetary dust.
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These documents have been prepared in coordination with the National Academies of Science in support of the National Academies Planetary Science Decadal Survey. These documents are being made available for information purposes only, and any views and opinions expressed herein do not necessarily state or reflect those of NASA, JPL, or the California Institute of Technology.