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Many processes during the evolution of protoplanetary disks and during planetformation are highly sensitive to the sizes of dust particles that are presentin the disk: The efficiency of dust accretion in the disk and volatiletransport on dust particles, gravoturbulent instabilities leading to theformation of planetesimals, or the accretion of pebbles onto large planetaryembryos to form giant planets are typical examples of processes that depend onthe sizes of the dust particles involved. Furthermore, radiative propertieslike absorption or scattering opacities depend on the particle sizes. Tointerpret observations of dust in protoplanetary disks, a proper estimate ofthe dust particle sizes is needed.  We present DustPy - A Python package to simulate dust evolution inprotoplanetary disks. DustPy solves gas and dust transport including viscousadvection and diffusion as well as collisional growth of dust particles. DustPyis written with a modular concept, such that every aspect of the model can beeasily modified or extended to allow for a multitude of research opportunities.

DustPy: A Python Package for Dust Evolution in Protoplanetary Disks