Reproducing the Architecture of TRAPPIST-1 using Global Formation and Evolution 
Models

Burn, Remo; Alibert, Yann; Mordasini, Christoph; Leleu, Adrien; Schlecker, Martin

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Reproducing the Architecture of TRAPPIST-1 using Global Formation and Evolution Models

Burn, R., Alibert, Y., Mordasini, C., Leleu, A., & Schlecker, M. (2018). Reproducing the Architecture of TRAPPIST-1 using Global Formation and Evolution Models. In European Planetary Science Congress.

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Item Permalink: https://hdl.handle.net/21.11116/0000-0005-CEA0-E Version Permalink: https://hdl.handle.net/21.11116/0000-0005-CEA1-D

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https://ui.adsabs.harvard.edu/abs/2018EPSC...12..376B (Any fulltext) Open Access status unknown

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Creators:
Burn, Remo¹, Author
Alibert, Yann¹, Author
Mordasini, Christoph¹, Author
Leleu, Adrien¹, Author
Schlecker, Martin¹, Author

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1Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners, ou_2421692

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Abstract: The, so far, unique and well constrained TRAPPIST-1 system can be exploited for testing planet formation theories. Because of observational biases, terrestrial planet formation models will, for the next decade, only be testable around low mass stars, showing the need for research in this area. We invoke the Bern model of global planet formation and evolution to conduct population syntheses for 0.1 solar mass stars and compare the wealth of systems to the TRAPPIST-1 system, finding reasonable consensus for many observables. However, compositions differ significantly.

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Dates: Date issued: 2018

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Title: European Planetary Science Congress

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Start-/End Date: 2018

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Title: European Planetary Science Congress

Source Genre: Proceedings

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