Thermal history of the parent bodies of meteorites

Details Thermal history of the parent bodies of meteorites Thermal history of the parent bodies of meteorites

Jan 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986avest..19..211k&link_type=abstract

(Astronomicheskii Vestnik, vol. 19, July-Sept. 1985, p. 211-223) Solar System Research (ISSN 0038-0946), vol. 19, no. 3, Jan. 19

Astronomy and Astrophysics

Astronomy

Asteroids, Meteoritic Composition, Temperature Distribution, Aluminum 26, Cooling, Melting, Thermal Conductivity

Scientific paper

Thermal histories of asteroids have been calculated for the first 300 million years after their formation, with heating depending on the decay of Al-26 and the energy of the impacts of the asteroid-forming bodies. The calculations were made taking into account the growth of the asteroids and changes in the thermal conductivity of their surface layers; these considerations have a substantial influence on the results. The calculated rates of cooling were found to agree with meteoritic data.

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