Using data from NASA’s Transiting Exoplanet Survey Satellite (TESS), astronomers at MIT have discovered a rocky exoplanet orbiting the bright K-dwarf star BD+05 4868A and observed variable transit depths that are characteristic of comet-like tails formed by dusty effluents emanating from a disintegrating planet. Unique to this exoplanet is the presence of prominent dust tails in both the trailing and leading directions that contribute to the extinction...
