Physics
Scientific paper
Mar 2011
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011lpi....42.2526h&link_type=abstract
42nd Lunar and Planetary Science Conference, held March 7–11, 2011 at The Woodlands, Texas. LPI Contribution No. 1608, p.2526
Physics
Scientific paper
As characterized by TEM and PSD-XRD the products resemble hydrated
protosilicates in primitive meteorites. The optimal hydration
temperature is about 291 K, a new constraint for models of early solar
system formation.
Abreu Neyda M.
Hoffman Jennifer E.
Howard Tatiana K.
Veblen Linda A.
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