Planetary chaotic zone clearing: Destinations and timescales

Sarah Morrison, Renu Malhotra

Research output: Contribution to journalArticle

34 Citations (Scopus)

Abstract

We investigate the orbital evolution of particles in a planet's chaotic zone to determine their final destinations and their timescales of clearing. There are four possible final states of chaotic particles: collision with the planet, collision with the star, escape, or bounded but non-collision orbits. In our investigations, within the framework of the planar circular restricted three body problem for planet-star mass ratio μ in the range 10-9 to 10-1.5, we find no particles hitting the star. The relative frequencies of escape and collision with the planet are not scale-free, as they depend upon the size of the planet. For planet radius Rp ≥ 0.001 RH where RH is the planet's Hill radius, we find that most chaotic zone particles collide with the planet for μ ≲ 10-5; particle scattering to large distances is significant only for higher mass planets. For fixed ratio Rp /RH , the particle clearing timescale, T cl, has a broken power-law dependence on μ. A shallower power law, T cl μ-1/3, prevails at small μ where particles are cleared primarily by collisions with the planet; a steeper power law, T cl μ-3/2, prevails at larger μ where scattering dominates the particle loss. In the limit of vanishing planet radius, we find T cl 0.024 μ-3/2. The interior and exterior boundaries of the annular zone in which chaotic particles are cleared are increasingly asymmetric about the planet's orbit for larger planet masses; the inner boundary coincides well with the classical first order resonance overlap zone, Δa cl, int ≃ 1.2 μ0.28 ap ; the outer boundary is better described by Δa cl, ext ≃ 1.7 μ0.31 ap , where ap is the planet-star separation.

Original languageEnglish (US)
Article number41
JournalAstrophysical Journal
Volume799
Issue number1
DOIs
StatePublished - Jan 20 2015

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clearing
planets
planet
timescale
collision
stars
power law
escape
collisions
radii
scattering
orbits
particle
particle collisions
three body problem
mass ratios

Keywords

  • celestial mechanics
  • chaos
  • planetdisk interactions
  • planets and satellites: dynamical evolution and stability

ASJC Scopus subject areas

  • Space and Planetary Science
  • Astronomy and Astrophysics

Cite this

Planetary chaotic zone clearing : Destinations and timescales. / Morrison, Sarah; Malhotra, Renu.

In: Astrophysical Journal, Vol. 799, No. 1, 41, 20.01.2015.

Research output: Contribution to journalArticle

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