Thermal radiation pressure as a possible mechanism for losing small particles on asteroids

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Fig. 13

Similar figures to Fig. 12, but the thermal inertia Γ is corrected based on Eq. (20). We note that many more cases are flagged as (A), i.e., escape-guaranteed. (a, c) Olivine; (b, d) magnetite particles. (a, b) morning terminator; (c, d) evening terminator.

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