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Pebble Accretion at the Origin of Water in Europa

  • Authors: Thomas Ronnet, Olivier Mousis, and Pierre Vernazza

2017 The Astrophysical Journal 845 92.

  • Provider: AAS Journals

Caption: Figure 1.

Surface density and temperature profiles of the CPD, with the distance from Jupiter expressed in units of Jovian radii (RJup) calculated for ﹩{\dot{M}}_{p}=1\times {10}^{-7}\,{M}_{\mathrm{Jup}}\,{\mathrm{yr}}^{-1}﹩ and α = 10−3. The vertical bars designated by the letters I, E, G, and C correspond to the current orbits of Io, Europe, Ganymede, and Callisto, respectively.

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