Physics
Scientific paper
Dec 1986
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986esasp.250b.385k&link_type=abstract
In ESA Proceedings of the 20th ESLAB Symposium on the Exploration of Halley's Comet. Volume 2: Dust and Nucleus p 385-388 (SEE N
Physics
Comet Nuclei, Comets, Cosmic Dust, Evolution (Development), Thermal Stresses, Crack Initiation, Gravitational Effects, Outgassing, Surface Properties
Scientific paper
Two processes that may have an important influence on the evolution of comets are discussed: thermal stresses and the gas-dust dynamics near the cometary surface. Thermal stresses due to the temperature differences between the surface and the core of the nucleus are calculated for different structure models. It is shown that for comets of P/Halley-type orbits thermal stresses exceed the strength of water ice near to the surface resulting in cracks, splits, and outbursts. Further it is demonstrated that due to cometary gravitation and inhomogeneous outgassing initially emitted dust can be redeposited at the cometary surface. The consequences of both processes for cometary activity are discussed.
Giese Bernd
Kuehrt Ekkehard
Moehlmann Diedrich
Tauber F.
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