The Tidal Downsizing hypothesis for planet formation and the composition of Solar System comets

Abstract

Comets are believed to be born in the outer Solar System where the temperature is assumed to have never exceeded T ~ 100 K. Surprisingly, observations and samples of cometary dust particles returned to Earth showed that they are in fact made of a mix of ices, as expected, but also of materials forged at high-temperatures (T ~ 1500 K). We propose a radically new view regarding the origin of the high-temperature processed materials in comets, based on the recent "Tidal Downsizing" (TD) hypothesis for planet formation. In the latter, the outer proto-planetary disc is gravitationally unstable and forms massive giant planet embryos (GEs). These hot (T ~ hundreds to 2000 K) and dense regions, immersed in the background cold and low density disc, are eventually disrupted. We propose that both planets and the high-T materials in comets are synthesised inside the GEs. Disruption of GEs separates planets and small solids as the latter are "frozen-in" into gas and are peeled off together with it. These small solids are then mixed with the ambient cold disc containing ices before being incorporated into comets. Several predictions of this picture may be testable with future observations of the Solar System and exoplanets.

Same paper; was withdrawn by mistake (the paper intended to be withdrawn should have been arXiv:1102.4297)

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Cited by in corpus (8)

• Heavy metal rules. I. Exoplanet incidence and metallicity
• Dawes Review. The tidal downsizing hypothesis of planet formation
• Tidal Downsizing model. I. Numerical methods: saving giant planets from tidal disruptions
• Fingerprints of the protosolar cloud collapse in the Solar System II: Nucleosynthetic anomalies in meteorites
• An alternative origin for debris rings of planetesimals
• Ejection of gaseous clumps from gravitationally unstable protostellar disks
• The gas disk: Evolution and chemistry
• The Migrating Embryo Model for Disk Evolution