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Planet-forming disks around very low-mass stars are different

Using the James Webb Space Telescope, a team of astronomers studied the properties of a planet-forming disk around a young and very low-mass star. The results reveal the richest hydrocarbon composition seen to date in a protoplanetary disk, including the first extrasolar detection of ethane and a relatively low abundance of oxygen-bearing species. By including previous similar detections, this finding confirms a trend of disks around very low-mass stars to be chemically distinct from those around more massive stars like the Sun, influencing the atmospheres of planets forming there. ....

United Kingdom , Baden Wüberg , France General , Jeroen Bouwman , Inga Kamp Groningen , Giulia Perotti , Inga Kamp , Silvia Scheithauer , Carl Zeiss Optronics , Thomas Henning , Agnes Perrin Laboratoire , Aditya Arabhavi , Riccardo Franceschi , Matthias Samland , Kamber Schwartz , German Aerospace Center , European Space Agency , Ewine Van Dishoeck Leiden University , Aditya Arabhavi University Of Groningen , Canadian Space Agency , University Of Cologne , Max Planck Institute For Extraterrestrial Physics , University Of Groningen , Valentin Christiaens University Of Liege , Max Planck Society , Max Planck Institute For Astronomy ,