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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 Journal 148 109.

  • Provider: AAS Journals

Caption: Figure 7.

Semimajor axis of particles as a function of time. Planets are color-coded by mass. Those >100 M, between 10 and 100 M, between 1 and 10 M, and between 0.1 and 1 M are indicated by large green points, medium red points, small black points, and gray points, respectively.

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