Document Type
Article
Publication Date
5-30-2018
Publication Title
The Astrophysical Journal
Volume
859
Issue
2
First page number:
1
Last page number:
14
Abstract
Protoplanetary disk simulations show that a single planet can excite more than one spiral arm, possibly explaining the recent observations of multiple spiral arms in some systems. In this paper, we explain the mechanism by which a planet excites multiple spiral arms in a protoplanetary disk. Contrary to previous speculations, the formation of both primary and additional arms can be understood as a linear process when the planet mass is sufficiently small. A planet resonantly interacts with epicyclic oscillations in the disk, launching spiral wave modes around the Lindblad resonances. When a set of wave modes is in phase, they can constructively interfere with each other and create a spiral arm. More than one spiral arm can form because such constructive interference can occur for different sets of wave modes, with the exact number and launching position of the spiral arms being dependent on the planet mass as well as the disk temperature profile. Nonlinear effects become increasingly important as the planet mass increases, resulting in spiral arms with stronger shocks and thus larger pitch angles. This is found to be common for both primary and additional arms. When a planet has a sufficiently large mass (gsim3 thermal masses for (h/r) p = 0.1), only two spiral arms form interior to its orbit. The wave modes that would form a tertiary arm for smaller mass planets merge with the primary arm. Improvements in our understanding of the formation of spiral arms can provide crucial insights into the origin of observed spiral arms in protoplanetary disks.
Keywords
Hydrodynamics; Planet–disk interactions; Waves
Disciplines
Astrophysics and Astronomy
File Format
application/pdf
File Size
5.020 Kb
Language
English
Creative Commons License
This work is licensed under a Creative Commons Attribution 4.0 License.
Repository Citation
Bae, J.,
Zhu, Z.
(2018).
Planet-driven Spiral Arms in Protoplanetary Disks. I. Formation Mechanism.
The Astrophysical Journal, 859(2),
1-14.
http://dx.doi.org/10.3847/1538-4357/aabf8c