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Cool M dwarfs outnumber sun-like G stars by ten to one in the solarneighborhood. Due to their proximity, small size, and low mass, M-dwarf starsare becoming attractive targets for exoplanet searches via almost all currentsearch methods. But what planetary systems can form around M dwarfs? Followingup on the Cool Stars~16 Splinter Session "Planet Formation Around M Dwarfs", wesummarize here our knowledge of protoplanetary disks around cool stars, howthey disperse, what planetary systems might form and can be detected withcurrent and future instruments.

Planet Formation Around M-dwarfs: From Young Disks to Planets