Hubble has observed a new object in Cygnus, initially thought to be a supernova but later identified as a protoplanetary nebula, IRAS 20068+4051. This nebula forms when a star exhausts its lighter fuel, shedding outer layers, and may eventually take on a more spherical shape due to radiation pressure. The discussion highlights the distinction between planetary nebulae and supernova remnants, noting that planetary nebulae are created from stars less than 8 solar masses, while supernovae result from more massive stars. The term "planetary nebula" is misleading, as these nebulae have no relation to planets; they are merely named for their appearance. Understanding these differences is crucial for grasping stellar evolution and the lifecycle of stars.