Self-preserving ice layers on CO2 clathrate particles: Implications for Enceladus, Pluto, and similar ocean worlds

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Table 2

Self-preserving ice layer thickness d for increasing values of low occupancy (LO) surface region thickness d_LO with N_g = 0 (second column).

	Ice thickness, d (nm)
d_LO (nm)	N_g = 0	N_g = 1
1	3	3
5	20	16
10	40	32
50	131	108
100	182	149

Notes. Asa comparison, we also give one example of a partially occupied surface region with N_g = 1 (third column). In these examples, the bulk region is taken as a fully occupied CO₂ clathrate structure.

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