
Alexander Mustill
Researcher

Foretellings of Ragnarök: World-engulfing Asymptotic Giants and the Inheritance of White Dwarfs
Author
Summary, in English
The search for planets around white dwarf stars, and evidence for dynamical instability around them in the form of atmospheric pollution and circumstellar disks, raises questions about the nature of planetary systems that can survive the vicissitudes of the asymptotic giant branch (AGB). We study the competing effects, on planets at several AU from the star, of strong tidal forces arising from the star's large convective envelope, and of the planets' orbital expansion due to stellar mass loss. We study, for the first time, the evolution of planets while following each thermal pulse on the AGB. For Jovian planets, tidal forces are strong, and can pull into the envelope planets initially at ~3 AU for a 1 M ☉ star and ~5 AU for a 5 M ☉ star. Lower-mass planets feel weaker tidal forces, and terrestrial planets initially within 1.5-3 AU enter the stellar envelope. Thus, low-mass planets that begin inside the maximum stellar radius can survive, as their orbits expand due to mass loss. The inclusion of a moderate planetary eccentricity slightly strengthens the tidal forces experienced by Jovian planets. Eccentric terrestrial planets are more at risk, since their eccentricity does not decay and their small pericenter takes them inside the stellar envelope. We also find the closest radii at which planets will be found around white dwarfs, assuming that any planet entering the stellar envelope is destroyed. Planets are in that case unlikely to be found inside ~1.5 AU of a white dwarf with a 1 M ☉ progenitor and ~10 AU of a white dwarf with a 5 M ☉ progenitor.
Publishing year
2012
Language
English
Publication/Series
The Astrophysical Journal
Volume
761
Issue
2
Document type
Journal article
Publisher
American Astronomical Society
Topic
- Astronomy, Astrophysics and Cosmology
- Physical Sciences
Keywords
- Astrophysics - Earth and Planetary Astrophysics
- Astrophysics - Solar and Stellar Astrophysics
- planets and satellites: dynamical evolution and stability
- stars: AGB and post-AGB
- stars: evolution
Status
Published