Aug 21, 2024
Astronomers explain Rapid Formation of Organic Macromolecules in Protoplanetary Disks around Young Stars
Posted by Dan Breeden in categories: computing, space
Computer modeling shows how macromolecules form quickly in gas & dust disks around young stars, aiding understanding of exoplanet.
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An international team of researchers led by the University of Bern has used observation-based computer modeling to find an explanation for how macromolecules can form in a short time in disks of gas and dust around young stars. These findings could be crucial for understanding how habitability develops around different types of exoplanets and stars.