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Title: Lunar Pyroclastic Deposits and the Origin of the Moon
Primary Author: Harrison H. Schmitt
Secondary Author(s): N/A
Institution: University of Wisconsin-Madison
Summary: he primary difficulty in accepting the computer modeled "giant impact" hypothesis for the origin of the Moon, versus independent derivation, comes from the analysis of the non-glass components of lunar pyroclastic deposits. These prove that volatile reservoirs exist in the mantle of the Moon.
Panel Selection: Inner Planets: Mercury, Venus, and the Moon.
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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.