Abstract A global and uniformly distributed spike of secondary impact craters on Phobos with diameters (D) effective impulse by incorporating the energy conversion inefficiencies of the crater formation process. We… Click to show full abstract
Abstract A global and uniformly distributed spike of secondary impact craters on Phobos with diameters (D) effective impulse by incorporating the energy conversion inefficiencies of the crater formation process. We also calculate the pre- and post-impact Phobos moment of inertia that further contributes to the desynchronizing effect. The majority of the Stickney ejecta that exited from Phobos was trapped in orbits around Mars until it later accumulated back onto Phobos over a period of
               
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