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The Bulk Densities of Small Solar System Bodies as a Probe of Planetesimal Formation

  • Authors: Misako Tatsuuma, Akimasa Kataoka, Hidekazu Tanaka, Tristan Guillot

Misako Tatsuuma et al 2024 The Astrophysical Journal 974 .

  • Provider: AAS Journals

Caption: Figure 5.

Top: central density against diameter of dust aggregates (Equation (B1)). The blue and orange lines show ice and silicate dust aggregates, whose material densities are 1.45 and 2.65 g cm−3, respectively. The solid and dashed lines show monomer radii of 0.1 and 1.0 μm, respectively. Bottom: central pressure against diameter of dust aggregates (Equation (B4)).

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