Standing on the shoulders of giants: Trojan Earths and vortex trapping in low mass self-gravitating protoplanetary disks of gas and solids
W. Lyra, A. Johansen, H. Klahr, N. Piskunov

TL;DR
This study demonstrates that in low-mass, self-gravitating protoplanetary disks, solid particles can rapidly collapse into planetary bodies within stable regions near giant planets, leading to diverse planet formation scenarios.
Contribution
It provides detailed simulations showing how particles of different sizes collapse into planets at Lagrangian points and vortex edges, revealing new pathways for planet formation in protoplanetary disks.
Findings
1 cm particles collapse into Earth-mass planets in less than 200 orbits.
Vortices can trap 30 cm particles, forming Super-Earths up to 17 Earth masses.
Multiple particle sizes lead to shifted stable points and varied planet masses.
Abstract
Centimeter and meter sized solid particles in protoplanetary disks are trapped within long lived high pressure regions, creating opportunities for collapse into planetesimals and planetary embryos. We study the accumulations in the stable Lagrangian points of a giant planet, as well as in the Rossby vortices launched at the edges of the gap it carves. We employ the Pencil Code, tracing the solids with a large number of interacting Lagrangian particles, usually 100,000. For particles of 1 cm to 10 cm radii, gravitational collapse occurs in the Lagrangian points in less than 200 orbits. For 5 cm particles, a 2 Earth mass planet is formed. For 10 cm, the final maximum collapsed mass is around 3 Earth masses. The collapse of the 1 cm particles is indirect, following the timescale of depletion of gas from the tadpole orbits. In the edges of the gap vortices are excited, trapping…
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Taxonomy
TopicsAstrophysics and Star Formation Studies · Astro and Planetary Science · Stellar, planetary, and galactic studies
