WASP-128b: a transiting brown dwarf in the dynamical-tide regime

TL;DR

WASP-128b is a transiting brown dwarf in a close orbit around a G dwarf star, providing a valuable case to study dynamical tides and orbital decay in star-brown dwarf systems.

Contribution

This paper reports the discovery and detailed characterization of WASP-128b, highlighting its placement in the brown dwarf desert and its potential for testing tidal theories.

Findings

Measured stellar tidal quality factor log Q' = 6.96 ± 0.19

Derived host star and companion masses and radii

Estimated orbital decay timescale similar to ultra-short period hot Jupiters

Abstract

Massive companions in close orbits around G dwarfs are thought to undergo rapid orbital decay due to runaway tidal dissipation. We report here the discovery of WASP-128b, a brown dwarf discovered by the WASP survey transiting a G0V host on a $2.2\,\mathrm{d}$ orbit, where the measured stellar rotation rate places the companion in a regime where tidal interaction is dominated by dynamical tides. Under the assumption of dynamical equilibrium, we derive a value of the stellar tidal quality factor $\log{Q_\star'} = 6.96 \pm 0.19$. A combined analysis of ground-based photometry and high-resolution spectroscopy reveals a mass and radius of the host, $M_\star = 1.16 \pm 0.04\,M_\odot$, $R_\star = 1.16 \pm 0.02\,R_\odot$, and for the companion, $M_\mathrm{b} =37.5 \pm 0.8\,M_\mathrm{Jup}$, $R_\mathrm{b} = 0.94 \pm 0.02\,R_\mathrm{Jup}$, placing WASP-128b in the driest parts of the brown dwarf desert, and suggesting a mild inflation for its age. We estimate a remaining lifetime for WASP-128b similar to that of some ultra-short period massive hot Jupiters, and note it may be a propitious candidate for measuring orbital decay and testing tidal theories.