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Kant and Laplace suggested the Solar System formed from a rotating gaseousdisk in the 18th century, but convincing evidence that young stars are indeedsurrounded by such disks was not presented for another 200 years. As we moveinto the 21st century the emphasis is now on disk formation, the role of disksin star formation, and on how planets form in those disks. Radio wavelengthsplay a key role in these studies, currently providing some of the highestspatial resolution images of disks, along with evidence of the growth of dustgrains into planetesimals. The future capabilities of EVLA and ALMA provideextremely exciting prospects for resolving disk structure and kinematics,studying disk chemistry, directly detecting proto-planets, and imaging disks information.

Disks, young stars, and radio waves: the quest for forming planetary systems