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. Author manuscript; available in PMC: 2019 May 1.
Published in final edited form as: Icarus. 2019 Jan 21;323:1–15. doi: 10.1016/j.icarus.2019.01.012

Figure 4.

Figure 4.

Plot of the ratio of net flux to evaporation flux vs dimensionless time ξ for an evaporating spherical body according to Equation (7) with DMg evaluated at 2000 K and 10−8 bar total pressure. Contours for three planetesimal radii, s, are shown.