Ejecta from impact craters

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COLLISIONS BETWEEN GRAVITY-DOMINATED BODIES. I. OUTCOME REGIMES AND SCALING LAWS (2011, methodology): “Finally, Housen & Holsapple (2011) provide scaling laws for the gravitationally escaping ejecta from the target in the impact cratering regime.”
THE ACTIVE ASTEROIDS (2011, background): “Experiments at laboratory scales show that the ratio ofme, the mass ejected faster than speed v, to the projectile mass, M , is me M = A ( v U )α (6) with A ∼ 0.01 and, very roughly, α ∼ -1.5 (Housen and Holsapple 2011).”