Challenges in Forming the Solar System's Giant Planet Cores via Pebble Accretion
Authors: K. A. Kretke and H. F. Levison
Kretke & Levison
2014 The Astronomical Journal148109.
Provider: AAS Journals
Caption: Figure 2.
Growth of planetesimals of initial radius 200, 300, 500, 1000, and 2000 km (red, cyan, blue, green, and magenta, respectively). We show multiple runs for each initial planetesimal size to demonstrate the stochastic nature of LIPAD.