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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 5.

Cumulative mass distribution of planetesimals/planets at different times during the fiducial simulation (described in the text). The curves show the initial distribution and at 90, 300, 600, and 3000 yr (light to dark solid curves, respectively), as well as at 106 and 5 × 106 yr (dashed and dotted, respectively).

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