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The Stickney Crater ejecta secondary impact crater spike on Phobos: Implications for the age of Stickney and the surface of Phobos

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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

Keywords: stickney crater; phobos; secondary impact; stickney

Journal Title: Planetary and Space Science
Year Published: 2017

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