Evaporation metamorphism of primitive dust material in the early solar nebula

Details Evaporation metamorphism of primitive dust material in the early solar nebula Evaporation metamorphism of primitive dust material in the early solar nebula

Apr 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979e%26psl..43...13h&link_type=abstract

Earth and Planetary Science Letters, vol. 43, no. 1, Apr. 1979, p. 13-21.

Computer Science

21

Evaporation, Interplanetary Medium, Metamorphism (Geology), Protoplanets, Solar System, Aluminum Oxides, Calcium Oxides, Chemical Composition, Gas Analysis, Mass Spectroscopy, Residues, Silicates, Solid Phases

Scientific paper

An evaporation experiment on matrix material of the Murchison (C2) meteorite up to 1900 C in vacuo has revealed the evaporation sequence of primitive dust material and the associated evolution of residual solid phases from hydrous silicates through magnesium silicates and iron-metal to calcium-aluminum oxides. The comparison with primitive meteorites suggests that the evaporation metamorphism coupled with the recondensation may have played an important role in the generation of diverse primitive meteorites in the early solar nebula.

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