Planetary nebula

A planetary nebula is an astronomical object that usually appears nebulous and disk-like in low-resolution observations.\nBecause of this appearance, similar to the appearance of planets in early observations, the "planetary" adjective was attached and has since been retained for historical consistency. According to current observations and models, planetary nebulae in fact have little to do with planets. Instead, as a small star (less than a few times the mass of the Sun) grows older, it tends to throw off upper layers of stellar material in various episodes of fusion reactions. \nWhile the central progenitor star dwindles to a white dwarf, the thrown-off gases form a cloud of material around it. \nIt is this cloud which is designated as a planetary nebula. \nThe remains of the star which produced the nebula is also responsible for the energy which causes it to glow. The Sun is predicted to become a planetary nebula at least 5 billion years in the future. Some of the more famous examples of this type of object are the Ring Nebula, the Helix nebula, the Eskimo Nebula and the Cat's Eye nebula.

Related topics

• List of planetary nebulas

References and external links:

\n* Press release on Cat's Eye Nebula, including above image: http://chandra.harvard.edu/photo/cycle1/1220/index.html\n* Planetary Nebulae, SEDS Messier Pages \n\n\n