
Alexander Mustill
Researcher

The great escape: how exoplanets and smaller bodies desert dying stars
Author
Summary, in English
Mounting discoveries of extrasolar planets orbiting post-main-sequence stars motivate studies to understand the fate of these planets. In the traditional 'adiabatic' approximation, a secondary's eccentricity remains constant during stellar mass-loss. Here, we remove this approximation, investigate the full two-body point-mass problem with isotropic mass-loss, and illustrate the resulting dynamical evolution. The magnitude and duration of a star's mass-loss combined with a secondary's initial orbital characteristics might provoke ejection, modest eccentricity pumping, or even circularization of the orbit. We conclude that Oort Clouds and wide-separation planets may be dynamically ejected from 1-7 M☉ parent stars during AGB evolution. The vast majority of planetary material that survives a supernova from a 7-20 M☉ progenitor will be dynamically ejected from the system, placing limits on the existence of first-generation pulsar planets. Planets around >20 M☉ black hole progenitors may easily survive or readily be ejected depending on the core collapse and superwind models applied. Material ejected during stellar evolution might contribute significantly to the free-floating planetary population.
Publishing year
2011
Language
English
Pages
2104-2123
Publication/Series
Monthly Notices of the Royal Astronomical Society
Volume
417
Issue
3
Links
Document type
Journal article
Publisher
Oxford University Press
Topic
- Astronomy, Astrophysics and Cosmology
- Physical Sciences
Keywords
- Astrophysics - Earth and Planetary Astrophysics
- Astrophysics - Solar and Stellar Astrophysics
- Oort Cloud
- Physics - Classical Physics
- planet-star interactions
- planets and satellites: dynamical evolution and stability
- stars: AGB and post-AGB
- stars: evolution
- supernovae: general
Status
Published
ISBN/ISSN/Other
- ISSN: 1365-2966