Energetics of Asteroid Dynamos and the Role of Compositional Convection

Details Energetics of Asteroid Dynamos and the Role of Compositional Convection Energetics of Asteroid Dynamos and the Role of Compositional Convection

Mar 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009lpi....40.1142n&link_type=abstract

40th Lunar and Planetary Science Conference, (Lunar and Planetary Science XL), held March 23-27, 2009 in The Woodlands, Texas, i

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Scientific paper

Asteroid dynamos require core cooling rates of < 0.1 K/Myr if
compositional convection driven by a light element (e.g. sulphur)
occurs, but 1-100 K/Myr otherwise. Parent bodies of several existing
meteorites cooled fast enough to generate dynamos.

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