paper

The Radial and Rotational Velocities of PSO J318.533822.8603, a Newly Confirmed Planetary-Mass Member of the Pictoris Moving Group

arXiv:1601.04717 · doi:10.3847/0004-637X/819/2/133

Abstract

PSO J318.533822.8603 is an extremely-red planetary-mass object that has been identified as a candidate member of the Pictoris moving group based on its spatial position and tangential velocity. We present a high resolution -band spectrum of PSO J318.533822.8603. Using a forward-modeling Markov Chain Monte Carlo approach, we report the first measurement of the radial velocity and sin() of PSO J318.522, 6.0 km s and 17.5 km s, respectively. We calculate the space velocity and position of PSO J318.522 and confirm that it is a member of the Pictoris moving group. Adopting an age of 233 Myr for PSO J318.522, we determine a mass of and effective temperature of K using evolutionary models. PSO J318.533822.8603 is intermediate in mass and temperature to the directly-imaged planets Pictoris b and 51 Eridani b, making it an important benchmark object in the sequence of planetary-mass members of the Pictoris moving group. Combining our sin() measurement with recent photometric variability data, we constrain the inclination of PSO J318.522 to and its rotational period to 5-10.2 hours. The equatorial velocity of PSO J318.522 indicates that its rotation is consistent with an extrapolation of the velocity-mass relationship for solar system planets.

8 pages, 5 figures, 2 tables, ApJ accepted

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