Author(s): S. W. Ruff
Co-Author(s): S. W. Ruff, J. B. Dalton, J. L. Bishop, M. D. Dyar, T. Glotch, W. M. Grundy, V. E. Hamilton, J. R. Johnson, F. Marchis, R. M. Mastrapa, F. M. McCubbin, R. V. Morris, H. Nekvasil, M. S. Ramsey, D. Stillman, S. T. Stewart, S. K. Sharma, A. Wang, and R. C. Wiens
Panel Selection: Inner Planets: Mercury, Venus, and the Moon. Mars: Not Phobos and Deimos. 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.
Institution: Arizona State University
This paper demonstrates the need to support laboratory investigations related to the surface composition of planetary bodies

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