TOI-3757b is the lowest-density transiting exoplanet known to orbit an M-dwarf (red dwarf) star. An artist’s impression of TOI-3757b and its parent star. Image credit: NOIRLab / NSF / AURA / J. da Silva / Spaceengine / M. Zamani. “Giant planets around red dwarf stars have traditionally been thought to be hard to form,” said Dr. Shubham Kanodia, an astronomer at Carnegie Institution for Science. “So far this has only been looked at with small...
 