Probabilistic Constraints on the Mass and Composition of Proxima b

Abstract

Recent studies regarding the habitability, observability, and possible orbital evolution of the indirectly detected exoplanet Proxima b have mostly assumed a planet with $M\sim 1.3$ $M_{\oplus }$, a rocky composition, and an Earth-like atmosphere or none at all. In order to assess these assumptions, we use previous studies of the radii, masses, and compositions of super-Earth exoplanets to probabilistically constrain the mass and radius of Proxima b, assuming an isotropic inclination probability distribution. We find it is ~90% likely that the planet's density is consistent with a rocky composition; conversely, it is at least 10% likely that the planet has a significant amount of ice or an H/He envelope. If the planet does have a rocky composition, then we find expectation values and 95% confidence intervals of ${⟨M⟩}_{\text{rocky}}=1.63_{-0.72}^{+1.66}$ $M_{\oplus }$ for its mass and ${⟨R⟩}_{\text{rocky}}=1.07_{-0.31}^{+0.38}$ $R_{\oplus }$ for its radius.

6 pages, 3 figures, 1 table. Accepted for publication in ApJL

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