A reappraisal of parameters for the putative planet PTFO 8-8695b and its potentially precessing parent star

Abstract

Published photometry of fading events in the PTFO 8-8695 system is modelled using improved treatments of stellar geometry, surface intensities, and, particularly, gravity darkening, with a view to testing the planetary-transit hypothesis. Variability in the morphology of fading events can be reproduced by adopting convective-envelope gravity darkening, but near-critical stellar rotation is required. This leads to inconsistencies with spectroscopic observations; the model also predicts substantial photometric variability associated with stellar precession, contrary to observations. Furthermore, the empirical ratio of orbital to rotational angular momenta is at odds with physically plausible values. An exoplanet transiting a precessing, gravity-darkened star may not be the correct explanation of periodic fading events in this system.

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• Multi-Color Simultaneous Photometry of the T-Tauri Star Having A Planetary Candidate CVSO 30
• Evidence for planetary hypothesis for PTFO 8-8695b with five-year optical/infrared monitoring observations
• A study of the rapid rotator $\zeta$ Aql: differential surface rotation?
• Are the O stars in WR+O binaries exceptionally rapid rotators?
• PTFO 8-8695: Two Stars, Two Signals, No Planet