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The discovery of thousands of exoplanets has shown that the birth of planetsis a very efficient process in nature. Several physical mechanisms have beenproposed to describe the assembly of planets in disks surrounding young stars.However, observational constraints have been sparse on account of insufficientsensitivity and resolution, especially for imaging the inner $10 - 20$ au fromthe star, where most of planets are observed. Thanks to its unprecedentedangular resolution and sensitivity at wavelengths where the emission from thecircumstellar material is optically thin, the ngVLA has the potential totransform our understanding of planet formation. In this chapter, we presentstate-of-the-art theoretical models of planetary systems in the act of formingthat demonstrate ngVLA capabilities of imaging and follow the temporalevolution of young solar system analogues up to the distance of the OrionNebula. These images will unveil how planets form and interact with theirparental disks, and will shed light on the diverse properties of exoplanetarysystems.

Science with a ngVLA: Imaging planetary systems in the act of forming with the ngVLA