Constraints on the Grain Size in the Mantles of Terrestrial Planets

Details Constraints on the Grain Size in the Mantles of Terrestrial Planets Constraints on the Grain Size in the Mantles of Terrestrial Planets

Mar 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002lpi....33.1446s&link_type=abstract

33rd Annual Lunar and Planetary Science Conference, March 11-15, 2002, Houston, Texas, abstract no.1446

Physics

Scientific paper

Viscosity of planetary interiors strongly depends on the grain size.
However, the grain size remains an arbitrary parameter in geodynamic
models. This study reviews relevant physical processes and provides
constraints on the grain size.

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