Communication Dans Un Congrès Année : 2008

A Partial Sublimation of the Planetesimals that Formed Titan

Résumé

We describe a scenario of Titan's formation matching the observational constraints. We argue that Titan was formed from solids initially produced in Saturn's feeding zone and that were partially vaporized during their migration/accretion in the subdisk.

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Dates et versions

hal-00472715 , version 1 (13-04-2010)

Identifiants

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O. Mousis, J.I. Lunine, C. Thomas, M. Pasek, U. Marboeuf, et al.. A Partial Sublimation of the Planetesimals that Formed Titan. A Partial Sublimation of the Planetesimals that Formed Titan, Mar 2008, League City, United States. pp.1425. ⟨hal-00472715⟩
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