Thermal history models for KOSI sublimation experiments

Details Thermal history models for KOSI sublimation experiments Thermal history models for KOSI sublimation experiments

Oct 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990icar...87..358s&link_type=abstract

Icarus (ISSN 0019-1035), vol. 87, Oct. 1990, p. 358-371. Research supported by DFG.

Astronomy and Astrophysics

Astronomy

31

Astronomical Models, Heat Transfer, Mass Transfer, Porous Materials, Sublimation, Thermal Diffusivity, Carbon Dioxide, Heat Sinks, Icy Satellites, Solar System, Water Vapor

Scientific paper

Temperature profiles recorded during three comet nucleus simulation experiments conducted by the KOSI (Kometensimulation) team are examined. A model has been developed that is capable of explaining the observed thermal histories of the samples. The model assumes that heat is transferred into the interior by solid-state heat conduction through the ice/dust matrix and by vapor flow driven by internal pressure gradients.

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