Radial mixing in protoplanetary accretion disks

Free access article

Issue		A&A Volume 390, Number 1, July IV 2002


Page(s)		253 - 265
Section		Formation and evolution of planetary systems
DOI		http://dx.doi.org/10.1051/0004-6361:20020614

A&A 390, 253-265 (2002)
DOI: 10.1051/0004-6361:20020614

III. Carbon dust oxidation and abundance of hydrocarbons in comets

H.-P. Gail

Institut für Theoretische Astrophysik, Universität Heidelberg, Tiergartenstraße 15, 69121 Heidelberg, Germany

(Received 3 July 2001 / Accepted 19 April 2002)

Abstract
The oxidation of carbon dust and its conversion into CO and some hydrocarbon compounds as intermediate products is studied for protoplanetary accretion discs. The disc model is based on the one-zone $\alpha$ -disc approximation. The radial mixing of the combustion products into the cold outer disc region by turbulent diffusion is considered in the transport-diffusion-reaction equations for the chemistry. It is shown that considerable amounts of CH ₄ and C ₂H ₂ formed as by-products of carbon oxidation are mixed into cold disc regions beyond a distance of 10 AU where they can be included into the ice mixture of cometary nuclei formed in that region. This may explain the high abundance of these gases recently observed in comets Hyakutake (C/1996 B2) and Hale-Bopp (C/1995 O1). This mixing of hydrocarbons from carbon oxidation cannot, however, explain the high abundance of some other molecular species like C ₂H ₆ or CH ₃OH, which have to be formed by different processes.

Key words: accretion, accreation disks -- molecular processes -- solar system: formation -- comets: general

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