Energy for Dust Modification in the Solar Nebula, and in the First-Formed Protoplanets and Their Present-Day Survivors

Details Energy for Dust Modification in the Solar Nebula, and in the First-Formed Protoplanets and Their Present-Day Survivors Energy for Dust Modification in the Solar Nebula, and in the First-Formed Protoplanets and Their Present-Day Survivors

Mar 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999lpi....30.1065r&link_type=abstract

30th Annual Lunar and Planetary Science Conference, March 15-29, 1999, Houston, TX, abstract no. 1065

Physics

Scientific paper

Internal chemical and structural energy of metastable, vapor-condensed
nonstoichiometric amorphous ferromagnesiosilica solids support
modification in the earliest accreted protoplanets, viz
(thermally-induced amorphization) and hydrocryogenic alteration.

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