Fig. 5: Disk structure at the midplane formed by an impact between icy planets (MT = 1M⊕, γ = 0.13, θ = 48. 5∘, vimp = vesc, Run ID20). | Nature Communications

Fig. 5: Disk structure at the midplane formed by an impact between icy planets (MT = 1M⊕, γ = 0.13, θ = 48. 5∘, vimp = vesc, Run ID20).

From: Large planets may not form fractionally large moons

Fig. 5

The line descriptions are the same as those in Fig. 4. The panels show (a) the surface density, (b) temperature, (c) vapor mass fraction, and (d) pressure gradient parameter η as a function of r/R⊕. The planetary radius is 1.42 R⊕.

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