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Fig. 3

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Depth of fractured surface layer h (isolines), expressed as a fraction of meteoroid’s radius R, which prevents propagation of the damage deeper into the core in the plane of heliocentric distance d (abscissa) and size D of the body (ordinate). The core has the thermal and mechanical properties of a carbonaceous chondrite and the spin axis is perpendicular to the orbital plane (β = 90°, implying also θ0 = 90°). Three values of the ratio ξ of the thermal conductivity in the surface layer K1 to that in the core K2 are tested: ξ = 1 (top panel), ξ = 0.5 (middle panel), and ξ = 0.1 (bottom panel).

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