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Conference Paper

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

MPS-Authors

Burn,  Remo
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Alibert,  Yann
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Mordasini,  Christoph
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Leleu,  Adrien
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Schlecker,  Martin
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

External Resource

https://ui.adsabs.harvard.edu/abs/2018EPSC...12..376B
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Citation

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.


Cite as: https://hdl.handle.net/21.11116/0000-0005-CEA0-E
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.