Turbulent Radial Mixing in the Solar Nebula as the Source of Crystalline Silicates in Comets
By D. Bockelée-Morvan, D. Gautier, F. Hersant, J. Huré, F. Robert. 2000
242 citations recorded by the source corpus.
Subfields: Astronomy and Astrophysics
View Paper: https://www.semanticscholar.org/paper/6b6937338a31074b422c751d82967b29b9bc76ed
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In Astronomy and Astrophysics
Citations in the corpus
- The Inner Regions of Protoplanetary Disks (2010, background): “The thermally processed material that is created here in this hot “oven” may be partially transported outward to the planet- and comet-forming region of the disk, for instance through radial mixing (e.g. Gail 2001; Bockelée-Morvan et al. 2002).”
- ISO Spectroscopy of Gas and Dust: From Molecular Clouds to Protoplanetary Disks (2004, background): “Since the crystalline material is observed at lower temperatures further out in the disk, this implies that some radial mixing process must occur (see also Bockelée-Morvan et al. 2002), although the mechanisms are not yet well understood.”
- CRYSTALLINE SILICATES AND DUST PROCESSING IN THE PROTOPLANETARY DISKS OF THE TAURUS YOUNG CLUSTER (2007, methodology): “…(800–1200 K), such as can be found at r 1 AU when viscous heating of the disk by accretion processes is substantial (Nuth et al. 2000; Gail 2001; Bockelée-Morvan et al. 2002; Wehrstedt & Gail 2002); or as can be produced over the central 10 AU by spiral density wave shocks which grow from…”
- The origin of crystalline silicates in the Herbig Be star HD 100546 and in comet Hale-Bopp (2003, result): “Similar results are found in recent models by Bockelée-Morvan et al. (2002) & Gail (2001).”
- A 10 μm spectroscopic survey of Herbig Ae star disks: Grain growth and crystallization (2005, background): “This is expected to enable radial mixing of material (Bockelée-Morvan et al. 2002; Gail 2004).”
- Global Simulations of the Inner Regions of Protoplanetary Disks with Comprehensive Disk Microphysics (2017, background): “Evidence for such radial mixing in the solar system has been mounting, especially based on the findings of crystalline silicates in comets (e.g., Bockelée-Morvan et al. 2002 and references therein), and more directly from samples collected from comet 81P/Wild 2 (Brownlee et al. 2006; Nakamura et…”