Figure 11.
Threshold for catastrophic disruption over particle size for various materials and velocities, as reported by Benz & Asphaug (1999), Leinhardt & Stewart (2009), and Nakamura et al. (2015), shown alongside the constraint from our model fitting. These $Q_\mathrm{D}^\star$ laws are plotted solid at sizes $>$1 cm, the regime where these relations are founded in experiments or numerical simulation, and dashed at the extrapolated smaller sizes. Also depicted is the preferred $Q_\mathrm{D}^\star$ prescription by Pokorný et al. (2024) (dash–dotted line), constrained by fitting JFC dust models to Solar system observables.

Threshold for catastrophic disruption over particle size for various materials and velocities, as reported by Benz & Asphaug (1999), Leinhardt & Stewart (2009), and Nakamura et al. (2015), shown alongside the constraint from our model fitting. These |$Q_\mathrm{D}^\star$| laws are plotted solid at sizes |$>$|1 cm, the regime where these relations are founded in experiments or numerical simulation, and dashed at the extrapolated smaller sizes. Also depicted is the preferred |$Q_\mathrm{D}^\star$| prescription by Pokorný et al. (2024) (dash–dotted line), constrained by fitting JFC dust models to Solar system observables.

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