Abstract
• Sesquinary mass influx is capable of significant impact to the surface geology of Phobos . This can exceed the flux of solar system impactors . • Sesquinary impacts have likely controlled the surface properties of Phobos for the last 20–25 million years. • The top ∼30 cm of Phobos regolith may largely consist of reaccreted sesquinary ejecta material.
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