Capture of free-floating planets by stellar systems
Nadav Goulinski, Erez N. Ribak
(Submitted on 29 May 2017)
Evidence of exoplanets with orbits that are misaligned with the spin of the host star may suggest that not all bound planets were born in the protoplanetary disk of their current planetary system. Observations have shown that free-floating Jupiter-mass objects can exceed the number of stars in our galaxy, implying that capture scenarios may not be so rare. To address this issue, we construct a three-dimensional simulation of a three-body scattering between a free-floating planet and a star accompanied by a Jupiter-mass bound planet. We distinguish between three different possible scattering outcomes, where the free-floating planet may get captured after the interaction with the binary, remain unbound, or “kick-out” the bound planet and replace it. The simulation was performed for different masses of the free-floating planets and stars, as well as different impact parameters, inclination angles and approach velocities. The outcome statistics are used to construct an analytical approximation of the cross section for capturing a free-floating planet by fitting their dependence on the tested variables. The analytically approximated cross section is used to predict the capture rate for these kinds of objects, and to estimate that about 1\% of all stars are expected to experience a temporary capture of a free-floating planet during their lifetime. Finally, we propose additional physical processes that may increase the capture statistics and whose contribution should be considered in future simulations.
Comments: The paper was submitted to MNRAS last week using their template. For this version no template was used, but the content is exactly the same
Subjects: Earth and Planetary Astrophysics (astro-ph.EP)
Cite as: arXiv:1705.10332 [astro-ph.EP] (or arXiv:1705.10332v1 [astro-ph.EP] for this version)
Submission history
From: Nadav Goulinski
[v1] Mon, 29 May 2017 18:00:17 GMT (1127kb,D)
https://arxiv.org/abs/1705.10332
