REAL

Transient Chaos and Fractal Structures in Planetary Feeding Zones

Kovács, Tamás and Regály, Zsolt (2015) Transient Chaos and Fractal Structures in Planetary Feeding Zones. ASTROPHYSICAL JOURNAL LETTERS, 798 (1). ISSN 2041-8205

[img]
Preview
Text
1412.1510.pdf
Available under License Creative Commons Attribution.

Download (577kB) | Preview

Abstract

The circular restricted three body problem is investigated in the context of accretion and scatter- ing processes. In our model a large number of identical non-interacting mass-less planetesimals are considered in planar case orbiting a star-planet system. This description allows us to investigate in dynamical systems approach the gravitational scattering and possible captures of the particles by the forming planetary embryo. Although the problem serves a large variety of complex motion, the results can be easily interpreted because of the low dimensionality of the phase space. We show that initial conditions define isolated regions of the disk, where accretion or escape of the planetesimals occur, these have, in fact, a fractal structure. The fractal geometry of these ”basins” implies that the dynam- ics is very complex. Based on the calculated escape rates and escape times, it is also demonstrated that the planetary accretion rate is exponential for short times and follows a power-law for longer integration. A new numerical calculation of the maximum mass that a planet can reach (described by the expression of the isolation mass) is also derived.

Item Type: Article
Subjects: Q Science / természettudomány > QB Astronomy, Astrophysics / csillagászat, asztrofizika
SWORD Depositor: MTMT SWORD
Depositing User: MTMT SWORD
Date Deposited: 11 Oct 2023 15:22
Last Modified: 11 Oct 2023 15:22
URI: http://real.mtak.hu/id/eprint/176533

Actions (login required)

Edit Item Edit Item