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Cited by 308

The DOI matches its Crossref record; 53 of the 53 references it cites were found in a registry or an index.

THE COMPOSITIONAL DIVERSITY OF EXTRASOLAR TERRESTRIAL PLANETS. I. IN SITU SIMULATIONS

Open access
Bond, Jade C., O'Brien, David P., Lauretta, Dante S.·2010·The Astrophysical Journal

Abstract

Extrasolar planet host stars have been found to be enriched in key planet-building elements. These enrichments have the potential to drastically alter the composition of material available for terrestrial planet formation. Here, we report on the combination of dynamical models of late-stage terrestrial planet formation within known extrasolar planetary systems with chemical equilibrium models of the composition of solid material within the disk. This allows us to determine the bulk elemental composition of simulated extrasolar terrestrial planets. A wide variety of resulting planetary compositions are found, ranging from those that are essentially "Earth like," containing metallic Fe and Mg silicates, to those that are dominated by graphite and SiC. This shows that a diverse range of terrestrial planets may exist within extrasolar planetary systems.

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Crossref · 10.1088/0004-637x/715/2/1050

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Metadata

Authors
Bond, J. C., O'Brien, D. P., & Lauretta, D. S.
Venue
The Astrophysical Journal
Published
2010-05-06
Volume
715
Issue
2
Pages
1050-1070
ISSN
  • 0004-637X (ISSN-L)
  • 1538-4357
OpenAlex
W2207684159
Cited by
308
References
53
FWCI
8.39
Type
journal article
Language
en
Open access
bronze

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CoChat. (2026). Citation check: THE COMPOSITIONAL DIVERSITY OF EXTRASOLAR TERRESTRIAL PLANETS. I. IN SITU SIMULATIONS. https://app.cochat.ai/papers/10.1088/0004-637x/715/2/1050
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Bond, J. C., O'Brien, D. P., & Lauretta, D. S. (2010). THE COMPOSITIONAL DIVERSITY OF EXTRASOLAR TERRESTRIAL PLANETS. I. IN SITU SIMULATIONS. The Astrophysical Journal. https://doi.org/10.1088/0004-637x/715/2/1050

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Semantic Scholar’s data is described in: Kinney, R., et al. (2023). The Semantic Scholar Open Data Platform. arXiv:2301.10140.