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Plausible compositions of the seven trappist-1 planets using long-term dynamical simulations

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Abstract

TRAPPIST-1 is a nearby ultra-cool dwarf that is host to a remarkable planetary system consisting of seven transiting planets. The orbital properties and radii of the planets have been well-constrained, and recently the masses of the inner six planets have been measured with additional ground and space-based photometric observations. Large uncertainties in these mass measurements have prevented a robust analysis of the planetary compositions. Here we perform many thousands of N-body dynamical simulations with planet properties perturbed from the observed values and identify those that are stable for millions of years. This allows us to identify self-consistent orbital solutions that can be used in future studies. From our range of dynamical masses, we find that most of the planets are consistent with an Earth-like composition, where TRAPPIST-1f is likely to have a volatile-rich envelope.

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Quarles, B., Quintana, E. V., Lopez, E., Schlieder, J. E., & Barclay, T. (2017, April 7). Plausible compositions of the seven trappist-1 planets using long-term dynamical simulations. ArXiv. arXiv. https://doi.org/10.3847/2041-8213/aa74bf

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