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Modeling Carbon Outgassing from Chondritic Planetesimals

  • Authors: Bo Peng, 博 彭, Diana Valencia

Bo Peng et al 2026 The Planetary Science Journal 7 .

  • Provider: AAS Journals

Caption: Figure 3.

The fraction of total carbon reservoir left at 10 Myr, relative to a planetesimal’s initial C abundance, for planetesimals with varying radii. Blue, green, red, and orange lines are bodies of EH, OC, CV, and CI compositions. Dashed lines are the fraction of bulk carbon in completely sintered layers.

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