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The tidal downsizing hypothesis for planet formation and the composition of Solar system comets

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journal contribution
posted on 05.02.2015, 12:31 by S. Nayakshin, S-H. Cha, John C. Bridges
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’ hypothesis for planet formation. In the latter, the outer protoplanetary disc is gravitationally unstable and forms massive giant planet embryos (GEs). These hot (T ∼ 100–2000 K) and dense regions, immersed in the background cold and low-density disc, are eventually disrupted. We propose that both planets and the high-temperature materials in comets are synthesized 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 exoplanets.

Funding

Theoretical astrophysics research and cometary research at the University of Leicester are supported by STFC rolling grants.

History

Citation

Monthly Notices of the Royal Astronomical Society (2011) 416 (1): L50-L54.

Author affiliation

/Organisation/COLLEGE OF SCIENCE AND ENGINEERING/Department of Physics and Astronomy

Version

VoR (Version of Record)

Published in

Monthly Notices of the Royal Astronomical Society (2011) 416 (1): L50-L54.

Publisher

Oxford University Press (OUP), Royal Astronomical Society

issn

0035-8711

eissn

1365-2966

Copyright date

2011

Available date

05/02/2015

Publisher version

http://mnrasl.oxfordjournals.org/content/416/1/L50

Language

en