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Physical aging in cometsThe question of physical aging in cometary nuclei is addressed in order to elucidate the relationship between the past conditions in the protosolar nebula and the present state of the cometary nucleus, and to understand the processes that will physically and chemically alter the nucleus as a function of time. Attention is given to some of the processes that might be responsible for causing aging in comets, namely, radiation damage in the upper layers of the nucleus during the long residences in the Oort cloud, processing from heating and collisions within the Oort cloud, loss of highly volatile species from the nucleus on the first passage through the inner solar system, buildup of a dusty mantle, which can eventually prohibit further sublimation, and a change in the porosity, and hence the thermal properties, of the nucleus. Recent observations suggest that there are distinct differences between 'fresh' Oort cloud comets and thermally processed periodic comets with respect to intrinsic brightness and rate of change of activity as a function of distance.
Document ID
19930029579
Acquisition Source
Legacy CDMS
Document Type
Conference Proceedings
Authors
Meech, Karen J.
(Hawaii Univ. Honolulu, United States)
Date Acquired
August 15, 2013
Publication Date
January 1, 1991
Publication Information
Publication: In: Comets in the post-Halley era. Vol. 1 (A93-13551 02-90)
Publisher: Kluwer Academic Publishers
Subject Category
Astrophysics
Accession Number
93A13576
Funding Number(s)
CONTRACT_GRANT: NGL-12-001-057
CONTRACT_GRANT: NSF AST-88-02726
Distribution Limits
Public
Copyright
Other

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