Electrical conductivity of carbonaceous chondrites and electric heating of meteorite parent bodies

Details Electrical conductivity of carbonaceous chondrites and electric heating of meteorite parent bodies Electrical conductivity of carbonaceous chondrites and electric heating of meteorite parent bodies

Nov 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987eprs.nasar....d&link_type=abstract

In NASA, Lyndon B. Johnson Space Center, Experiments in Planetary and Related Sciences and the Space Station 3 p (SEE N89-14998

Computer Science

Carbonaceous Chondrites, Electrical Resistivity, Heating, Kinetics, Meteorites, Chemical Reactions, Grain Boundaries, Pyrolysis

Scientific paper

Electromagnetic heating of rock-forming materials most probably was an important process in the early history of the solar system. Electrical conductivity experiments of representative materials such as carbonaceous chondrites are necessary to obtain data for use in electromagnetic heating models. With the assumption that carbon was present at grain boundaries in the material that comprised the meteorite parent bodies, the electrical heating of such bodies was calculated as a function of body size and solar distance using the T-Tauri model of Sonett and Herbert (1977). The results are discussed.

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