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Mass and energy transport in sublimating cometary ice cracks

Journal Article · · Icarus (International Journal of the Solar System); (USA)
;  [1]
  1. Observatorium Lustbuehel, Graz (Austria) DLR, Institut fuer Experimentelle Stroemungsmechanik, Goettingen (Germany, F.R.)

A model is developed for the mass and energy transport characteristics of the gas in a rectangular crack of arbitrary depth and cross section on a cometary surface, under the assumptions that the gas sublimates from the walls according to the local ice temperature and that the molecules hitting the ice walls recondense there. The sublimation rate from an icy surface with many small pores is found to be virtually the same as in the case of a flat surface; the existence of a few larger holes which lead to the same total pore cross section, however, can drop the surface sublimation rate to 80 percent. Gaps will constitute a major emission source if an inward-increasing temperature profile occurs in the ice. An additional major factor is cooling by net sublimation from the ice walls. 15 refs.

OSTI ID:
5974699
Journal Information:
Icarus (International Journal of the Solar System); (USA), Journal Name: Icarus (International Journal of the Solar System); (USA) Vol. 89; ISSN ICRSA; ISSN 0019-1035
Country of Publication:
United States
Language:
English