Physics
Scientific paper
Jan 1999
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999m%26ps...34..121g&link_type=abstract
Meteoritics & Planetary Science, vol. 34, no. 1, pp. 121-127 (1999).
Physics
17
Scientific paper
Asteroid thermal models have typically employed a constant value of specific heat capacity, although this parameter is a function of temperature. We examine whether incorporation of the temperature dependence of specific heat capacity is a necessary refinement and find that including it produces considerable differences in thermal history. Though the temperature effect is demonstrated in a representative calculation for a chondritic asteroid with 26Al decay as a heat source, this result also has implications for asteroidal thermal models based on electromagnetic induction heating or heating by impact, as well as for thermal models of the terrestrial planets.
Ghosh Amitabha
McSween Harry Y. Jr.
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