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Planet-Forming Disks Around Very Low-Mass Stars Are Different

Planet-Forming Disks Around Very Low-Mass Stars Are Different
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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.

Webb Detects Abundant Hydrocarbons in Protoplanetary Disk around Very-Low-Mass Star

astronomers used the NASA/ESA/CSA James Webb Space Telescope to investigate the chemical composition of the planet-forming disk around ISO-ChaI 147, a red dwarf star weighing just one-tenth as much as our Sun.

Rocky, carbon-rich exoplanets more likely around tiny stars, James Webb Space Telescope reveals

Rocky, carbon-rich exoplanets more likely around tiny stars, James Webb Space Telescope reveals
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NASA s James Webb Space Telescope Finds Abundance of Carbon Molecules Around Young Star

NASA s James Webb Space Telescope Finds Abundance of Carbon Molecules Around Young Star
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