
Imaging of protoplanets
Observations of protoplanets provide critical insights into the earliest stages of planetary formation. By directly imaging these forming planets within their protoplanetary disks, we can study their masses, compositions, and interactions with the surrounding material, shedding light on the processes that shape planetary systems

Protoplanetary disks
Protoplanetary disks are the birthplaces of planets. Understanding their physical properties, chemical composition, and evolution over time is crucial to unraveling the complex processes behind planet formation

From clouds to stars
Through observational studies of star formation, we examine how clouds of gas and dust collapse to form new stars. By analyzing the physical conditions and processes within these stellar nurseries, we uncover how stars evolve, interact with their environments, and shape the development of planetary systems and galaxies