Are falling planets spinning up their host stars?
D. J. A. Brown, A. Collier Cameron, C. Hall, L. Hebb, B. Smalley

TL;DR
This study models tidal interactions in the WASP-18 and WASP-19 systems to constrain stellar and planetary tidal quality factors, revealing potential spin-up of stars and the planets' spiral-in stages.
Contribution
It provides new estimates of tidal quality factors and system ages, and explores the evolutionary history and future of these planetary systems.
Findings
WASP-18 system has a system age of about 0.58 Gyr.
WASP-19 is likely in the final spiral-in stage, with a possible remaining lifetime.
Stars in these systems have been spun up by tidal interactions.
Abstract
We investigate the effects of tidal interactions on the planetary orbits and stellar spin rates of the WASP-18 and WASP-19 planetary systems using a forward integration scheme. By fitting the resulting evolutionary tracks to the observed eccentricity, semi-major axis and stellar rotation rate, and to the stellar age derived from isochronal fitting, we are able to place constraints on the stellar and planetary reduced tidal quality factors, Q's and Q'p. We find that for WASP-18, log(Q's)=8.21+0.90-0.52 and log(Q'p)=7.77+1.54-1.25, implying a system age of 0.579+0.305-0.250 Gyr. For WASP-19 we obtain values of log(Q's)=6.47+2.19-0.95 and log(Q'p)=6.75+1.86-1.77, suggesting a system age of 1.60+2.84-0.79 Gyr and a remaining lifetime of 0.0067+1.1073-0.0061 Gyr. We investigate a range of evolutionary histories consistent with these results and the observed parameters for both systems, and…
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