CORDIS Project
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This project investigates the chemical evolution from protostars to planet-forming disks, focusing on the survival and transformation of prebiotic molecules. It combines observational data with chemical modeling to understand the processes affecting planetary composition.
The emergence of Life relied on the presence of key molecules like water and prebiotic molecules.
The primitive objects of our Solar System (comets, asteroids), which formed in the disk of dust and gas surrounding the young Sun, are thought to have delivered them to Earth during heavy bombardments.
Observations show that the deeply embedded Class 0 protostars also harbour a very rich chemistry in their inner regions.
What occurs to the chemical composition between this early stage of the star fo…
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