Using NASA’s Transiting Exoplanet Survey Satellite (TESS) and several ground-based telescopes, astronomers have discovered and confirmed a warm super-Neptune orbiting the red dwarf TOI-1728. An artist’s impression of the super-Neptune exoplanet TOI-1728b. Image credit: Sci-News.com. TOI-1728 is an inactive M0-type star located 198 light-years away in the large northern constellation of Camelopardalis. Also cataloged as TIC 285048486 and UCAC4...