Bipolar nebula
Encyclopedia
A bipolar nebula is a distinctive nebular formation characterized by an axially symmetric bi-lobed appearance.
Many, but not all, planetary nebula
e exhibit an observed bipolar structure. It may be that the two types of nebulae are directly related, one preceding or superseding the other in the evolution of the nebula.
in which a star ejects highly energetic streams of outflow along both poles. One theory states that these outflows collide with material surrounding the star (either stellar dust, or shells of matter sloughed off in a prior Supernova
event).
Many, but not all, planetary nebula
Planetary nebula
A planetary nebula is an emission nebula consisting of an expanding glowing shell of ionized gas ejected during the asymptotic giant branch phase of certain types of stars late in their life...
e exhibit an observed bipolar structure. It may be that the two types of nebulae are directly related, one preceding or superseding the other in the evolution of the nebula.
Formation
Though the exact causes of this nebular structure are not known, it may be related to the physical process known as bipolar outflowBipolar outflow
A bipolar outflow represents two continuous flows of gas from the poles of a star. Bipolar outflows may be associated with protostars , or with evolved post-AGB stars ....
in which a star ejects highly energetic streams of outflow along both poles. One theory states that these outflows collide with material surrounding the star (either stellar dust, or shells of matter sloughed off in a prior Supernova
Supernova
A supernova is a stellar explosion that is more energetic than a nova. It is pronounced with the plural supernovae or supernovas. Supernovae are extremely luminous and cause a burst of radiation that often briefly outshines an entire galaxy, before fading from view over several weeks or months...
event).
Examples
- Homunculus NebulaHomunculus NebulaThe Homunculus Nebula is an emission nebula surrounding the massive star system Eta Carinae. The nebula is embedded within a much larger ionized hydrogen region, the Eta Carinae Nebula....
around Eta Carinae - Hubble 5
- M2-9 – The Wings of a Butterfly NebulaPlanetary Nebula M2-9Minkowski 2-9, abbreviated M2-9, is a planetary nebula that was discovered by Rudolph Minkowski in 1947. It is located about 2,100 light-years away from Earth in the direction of the constellation Ophiuchus...
- OH231.8+4.2 – The Calabash NebulaCalabash NebulaThe Calabash Nebula, also known as the Rotten Egg Nebula or by its technical name OH 231.84 +4.22, is a protoplanetary nebula 1.4 light years long and located some 5,000 light years from Earth in the constellation Puppis....
or Rotten Egg Nebula - Mz3 (or Menzel 3) – The Ant NebulaMz3Mz 3 is a young bipolar planetary nebula in the constellation Norma that is composed of a bright core and four distinct high-velocity outflows that have been named lobes, columns, rays, and chakram...
- CRL 2688 – The Egg NebulaEgg NebulaThe Egg Nebula is a bipolar protoplanetary nebula approximately 3,000 light-years away from Earth. It was discovered by Raghvendra Sahai and John Trauger of NASA's Jet Propulsion Laboratory in Pasadena, California...
- HD 44179 – The Red Rectangle NebulaRed Rectangle nebulaThe Red Rectangle Nebula, so called because of its red color and unique rectangular shape, is a protoplanetary nebula in the Monoceros constellation. Also known as HD 44179, the nebula was discovered in 1973 during a rocket flight associated with the AFCRL Infrared Sky Survey called Hi Star...
- MyCn18 – The Hourglass NebulaHourglass NebulaThe Engraved Hourglass Nebula is a young planetary nebula situated in the southern constellation Musca about 8,000 light-years away from Earth. It was discovered by Annie Jump Cannon and Margaret W. Mayall during their work on an extended Henry Draper Catalogue...
- He2-104 – The Southern Crab NebulaSouthern Crab NebulaThe Southern Crab Nebula or Hen2-104 is a nebula located, as seen from Earth, in the constellation Centaurus, but it is actually several thousand light years from our planet. Its central star is a symbiotic Mira variable - white dwarf pair....
- The Boomerang NebulaBoomerang NebulaThe Boomerang Nebula is a protoplanetary nebula located 5,000 light-years away from Earth in the constellation Centaurus. The nebula is measured at , the naturally coldest place currently known in the Universe. The Boomerang Nebula was formed from the outflow of gas from a star at its core...
- NGC 2346NGC 2346NGC 2346 is a planetary nebula near the celestial equator in the Monoceros constellation. It is bright and conspicuous and has been extensively studied...
– Also known as Butterfly NGC 2346
See also
- Bipolar outflowBipolar outflowA bipolar outflow represents two continuous flows of gas from the poles of a star. Bipolar outflows may be associated with protostars , or with evolved post-AGB stars ....
- Stellar evolutionStellar evolutionStellar evolution is the process by which a star undergoes a sequence of radical changes during its lifetime. Depending on the mass of the star, this lifetime ranges from only a few million years to trillions of years .Stellar evolution is not studied by observing the life of a single...