Computer Science
Scientific paper
Jun 1990
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990em%26p...49..239y&link_type=abstract
Earth, Moon, and Planets (ISSN 0167-9295), vol. 49, June 1990, p. 239-245.
Computer Science
Comet Nuclei, Radiation Effects, Stellar Radiation, Supernovae, Halley'S Comet, Oort Cloud, Radiation Dosage
Scientific paper
Effect of stellar and supernova radiations on cometary nuclei in the Oort cloud is investigated. Radiation dose received by a comet is calculated and compared with the one which Halley's comet receives by one perihelion passage. Stellar radiation provides 10 to 50 percent of Halley unit over 4 billion years. Inclusion of sublimation of volatile molecules such as CO or N2 does not allow the temperature to rise to 30 K by irradiation of bright OB stars, contrary to the claim of Stern and Shull. A chance encounter with an SN provides radiation dose which is just sufficient to raise to 30 K the surface layer which is 1 m thick on the assumption that the radiation is wholly communicated to the interior. Thus, the comets remain pristine under the effect of stellar and SN radiations.
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