Short-term stability of particles in the WD J0914+1914 white dwarf planetary system
Nearly all known white dwarf planetary systems contain detectable rocky debris in the stellar photosphere. A glaring exception is the young and still evolving white dwarf WD J0914+1914, which instead harbours a giant planet and a disc of pure gas. The stability boundaries of this disc and the future...
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Autores principales: | , , , |
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Formato: | Articulo Preprint |
Lenguaje: | Inglés |
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2020
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Acceso en línea: | http://sedici.unlp.edu.ar/handle/10915/125830 |
Aporte de: |
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I19-R120-10915-125830 |
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institution |
Universidad Nacional de La Plata |
institution_str |
I-19 |
repository_str |
R-120 |
collection |
SEDICI (UNLP) |
language |
Inglés |
topic |
Ciencias Astronómicas minor planets, asteroids: general comets: general protoplanetary discs planets and satellites: dynamical evolution and stability planet-star interactions stars: white dwarfs |
spellingShingle |
Ciencias Astronómicas minor planets, asteroids: general comets: general protoplanetary discs planets and satellites: dynamical evolution and stability planet-star interactions stars: white dwarfs Zotos, Euaggelos E. Veras, Dimitri Saeed, Tareq Darriba, Luciano Ariel Short-term stability of particles in the WD J0914+1914 white dwarf planetary system |
topic_facet |
Ciencias Astronómicas minor planets, asteroids: general comets: general protoplanetary discs planets and satellites: dynamical evolution and stability planet-star interactions stars: white dwarfs |
description |
Nearly all known white dwarf planetary systems contain detectable rocky debris in the stellar photosphere. A glaring exception is the young and still evolving white dwarf WD J0914+1914, which instead harbours a giant planet and a disc of pure gas. The stability boundaries of this disc and the future prospects for this white dwarf to be polluted with rocks depend upon the mass and orbit of the planet, which are only weakly constrained. Here we combine an ensemble of plausible planet orbits and masses to determine where observers should currently expect to find the outer boundary of the gas disc. We do so by performing a sweep of the entire plausible phase space with short-term numerical integrations. We also demonstrate that particle-star collisional trajectories, which would lead to the (unseen) signature of rocky metal pollution, occupy only a small fraction of the phase space, mostly limited to particle eccentricities above 0.75. Our analysis reveals that a highly inflated planet on a near-circular orbit is the type of planet which is most consistent with the current observations. |
format |
Articulo Preprint |
author |
Zotos, Euaggelos E. Veras, Dimitri Saeed, Tareq Darriba, Luciano Ariel |
author_facet |
Zotos, Euaggelos E. Veras, Dimitri Saeed, Tareq Darriba, Luciano Ariel |
author_sort |
Zotos, Euaggelos E. |
title |
Short-term stability of particles in the WD J0914+1914 white dwarf planetary system |
title_short |
Short-term stability of particles in the WD J0914+1914 white dwarf planetary system |
title_full |
Short-term stability of particles in the WD J0914+1914 white dwarf planetary system |
title_fullStr |
Short-term stability of particles in the WD J0914+1914 white dwarf planetary system |
title_full_unstemmed |
Short-term stability of particles in the WD J0914+1914 white dwarf planetary system |
title_sort |
short-term stability of particles in the wd j0914+1914 white dwarf planetary system |
publishDate |
2020 |
url |
http://sedici.unlp.edu.ar/handle/10915/125830 |
work_keys_str_mv |
AT zotoseuaggelose shorttermstabilityofparticlesinthewdj09141914whitedwarfplanetarysystem AT verasdimitri shorttermstabilityofparticlesinthewdj09141914whitedwarfplanetarysystem AT saeedtareq shorttermstabilityofparticlesinthewdj09141914whitedwarfplanetarysystem AT darribalucianoariel shorttermstabilityofparticlesinthewdj09141914whitedwarfplanetarysystem |
bdutipo_str |
Repositorios |
_version_ |
1764820452325195778 |