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chemcomp models and enables the study of the formation of planets in 1D protoplanetary disks. It includes disk physics for viscous disk evolution, pebble growth and evolution applying the two populations model, evaporation and condensation at evaporation lines, and chemical compositions. Written in Python, chemcomp also includes planet physics for type-I and type-II migration, thermal and dynamical torques, and pebble and gas accretion.