Nonthermal crystallization of amorphous silicates in comets

Recent observations show the ubiquity of crystalline silicate in various objects, among which comets provide the best opportunity to study possible processing of pristine matter during their formation and evolution. While thermal processing of bare amorphous silicates in the hot inner solar nebula h...

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Bibliographic Details
Published in:Earth, planets, and space planets, and space, 2010-01, Vol.62 (1), p.23-27
Main Authors: Yamamoto, Tetsuo, Chigai, Takeshi, Kimura, Hiroshi, Tanaka, Kyoko K.
Format: Article
Language:English
Subjects:
Earth and Environmental Science
Earth Sciences
Geology
Geophysics/Geodesy
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Summary:Recent observations show the ubiquity of crystalline silicate in various objects, among which comets provide the best opportunity to study possible processing of pristine matter during their formation and evolution. While thermal processing of bare amorphous silicates in the hot inner solar nebula has been invoked, its drawback is a difficulty in explaining the interstellar composition of cometary ices. Here we apply a model of core-mantle interstellar grains to propose nonthermal crystallization of the amorphous silicate core due to the energy released by chemical reactions in the organic refractory mantle when moderately heated by solar radiation. By formulating the nonthermal crystallization, we find that the degree of crystallinity is determined by a single parameter that is proportional to the amount of the released energy. We show that the present mechanism of crystallization is capable of reproducing the strengths of crystalline silicate features observed in comets. Our model can reconcile crystalline silicate in the comae of comets with the interstellar composition of ices in their nuclei.
ISSN:1343-8832
1880-5981
DOI:10.5047/eps.2008.11.002