A Two-dimensional Model for the Primordial Nebula Constrained by D/H Measurements in the Solar System: Implications for the Formation of Giant Planets

By F. Hersant, D. Gautier, J. Huré. 2001

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In Astronomy and Astrophysics

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THE COMPOSITIONAL DIVERSITY OF EXTRASOLAR TERRESTRIAL PLANETS. I. IN SITU SIMULATIONS (2010, methodology): “The Hersant et al. (2001) models assumed a uniform mass accretion rate.”
The composition of ices in comet C/1995 O1 (Hale-Bopp) from radio spectroscopy (2004, background): “This possibility results from reprocessing in the Solar Nebula, as proposed by Hersant et al. (2001): gas-phase H2O and HCN, originating from ices infalling from the presolar cloud, underwent isotopic exchanges with H2 in the inner Solar Nebula; reprocessed gas then diffused by turbulence to the…”
The origin of crystalline silicates in the Herbig Be star HD 100546 and in comet Hale-Bopp (2003, background): “Also, the time scale for the formation of a giant planet in the disk region is a few Myrs (Pollack et al. 1996; Hersant et al. 2001), which can easily be accounted for giv n the estimated age of HD 100546 of>10 Myr (van den Ancker et al. 1998).”
Deuterium enrichments in chondritic macromolecular material—Implications for the origin and evolution of organics, water and asteroids (2010, methodology): “…unchanged since accretion of the OC parent bodies, a number of papers have used the D enrichments in OC water to constrain models of solar nebula evolution, as well as the formation of comets and the giant planets (Drouart et al., 1999; Mousis et al., 2000; Hersant et al., 2001; Robert, 2002).”
The evolution of the water distribution in a viscous protoplanetary disk (2005, background): “Diffusion of material along concentration gradients is expected to occur regardless of the mechanism responsible for driving disk evolution (Morfill and Völk, 1984; Stevenson and Lunine, 1988; Hersant et al., 2001; Gail, 2001; Takeuchi and Lin, 2002; Cuzzi et al., 2003; Cuzzi and Zahnle, 2004; Boss,”
Updated Big Bang nucleosynthesis confronted to WMAP observations and to the abundance of light elements (2003, background): “In addition to the high redshift data, the only D/H observations available are i) the protosolar value which is affected by a large error bar, (2.5±0.5)×10−5 (Hersant et al. 2001), and ii) the local and present value in the interstellar medium, (1.52± 0.08)× 10−5 (Moos et al. 2002).”
Turbulent Radial Mixing in the Solar Nebula as the Source of Crystalline Silicates in Comets (2000, methodology): “Hersant et al. (2001) showed that the three parameters defining the nebula can be constrained by the deuterium enrichments measured in LL3 meteorites, comets, proto-Uranian and proto-Neptunian ices, taking into account a few other physical constraints, namely: 1) the mass of the nebula cannot…”
Enrichments in Volatiles in Jupiter: A New Interpretation of the Galileo Measurements (2001, methodology): “Finally, we note that the present analysis is based on the nominal model of the solar nebula calculated by Hersant et al. (2001).”