Protoplanetary Disks: The Cradles of Planets
Observations of dust, gas, and substructures reveal the initial conditions for planet formation.
Observations of dust, gas, and substructures reveal the initial conditions for planet formation.
Coagulation, accretion, migration--how raw material becomes mature planets.
Detections and beyond: Transmission spectroscopy, direct imaging, and demographics turn detections into physical understanding.
The up-to-date scientific programme — including the full list of speakers, talk titles, session times, and the online access link — is maintained in the programme PDF and updated as details are finalized.
Programme (PDF)