Image Details

Choose export citation format:

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 3.

Pebble accretion rate as a function of mass from the LIPAD simulations overlaid on the results of Equation (3) (with the Ormel & Klahr 2010 hyperbolic regime cross section for low-mass planetesimals).

Other Images in This Article

Show More

Copyright and Terms & Conditions