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The PEBBLES project investigates the properties and evolution of dust in young star systems, focusing on how dust forms and evolves in proto-planetary disks. By utilizing advanced observational and numerical methods, it aims to enhance our understanding of planet formation conditions around stars.
The formation and properties of exoplanetary systems is a fascinating question, which has been at the heart of our quest to define mankind and the conditions for life to develop in a broader context.Recent astronomical observations have deeply modified our paradigm of planet formation, as they suggest the so-called ""proto-planetary” disks surrounding T-Tauri stars may actually already host planets.
Moreover, we have obtained some of the first observational clues that the dust particles containe…
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