Do falling planets cause stellar spin-up?

D. J. A. Brown*, A. Collier Cameron, C. Hall, L. Hebb

*Corresponding author for this work

Research output: Chapter in Book/Report/Conference proceedingConference contribution

Abstract

We investigate the tidal interactions between hot Jupiter extra-solar planets and their host stars in an effort to characterise the effects of such interactions On stellar rotation. We study the WASP-18 and WASP-19 systems, showing that in both cases tidal interactions cause the eventual spiral in of the the planet towards the Roche limit. We find that for both systems this process will cause significant spin up of the host star, independent of the precise value for the tidal quality factors. By fitting tidal evolution models to observed parameters, we are able to determine that WASP-19 b is currently spiralling in, and that it has a very short remaining lifetime similar to 3 Myr.

Original languageEnglish
Title of host publicationASTROPHYSICS OF PLANETARY SYSTEMS: FORMATION, STRUCTURE, AND DYNAMICAL EVOLUTION
EditorsA Sozzetti, MG Lattanzi, AP Boss
PublisherCambridge University Press
Pages267-270
Number of pages4
ISBN (Print)978-0-521-19652-9
DOIs
Publication statusPublished - 2011
Event276th Symposium of the International-Astronomical-Union on Astrophysics of Planetary Systems: Formation, Structure, and Dynamical Evolution - Torino, Italy
Duration: 10 Oct 201015 Oct 2010

Publication series

NameIAU Symposium Proceedings Series
PublisherCAMBRIDGE UNIV PRESS
Volume276
ISSN (Print)1743-9213

Conference

Conference276th Symposium of the International-Astronomical-Union on Astrophysics of Planetary Systems: Formation, Structure, and Dynamical Evolution
Country/TerritoryItaly
Period10/10/1015/10/10

Keywords

  • stars: rotation
  • stars: activity
  • planetary systems
  • EVOLUTION
  • GYROCHRONOLOGY

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