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Everything about Planetar Astronomy totally explained

Planetar is a term used in astronomy that refers to one of two things:* Brown dwarfs - objects intermediate in size between planets and stars.
  • Interstellar planets - planetars that are cold masses smaller than brown dwarfs and don't orbit a star, but are free-floating in space.
Both definitions have been proposed, but neither has achieved wide usage in the astronomical and planetary science communities.

Brown dwarf planetars

Planetars are planet-like objects that are more massive than the low-mass cut-off for brown dwarfs. These generally are referred to as brown dwarfs. However, a planetar is formed in the manner of planets, through accretion or core collapse from a circumstellar disc, and not through the collapse of a gas cloud. The distinction between a planetar and a brown dwarf is unclear, astronomers are divided into two camps as whether to consider the formation process of a planet as part of its division in classification. Such a planet might also be referred to as a hypergiant planet.

Red dwarf planetars

Hypothetically an ultra-giant planet may result from planetary formation large enough to become a red dwarf. Perhaps even larger stars may form from discs of gas of Population III protostars.

Unbound planet planetars

Interstellar planetary mass objects, also known as planetars, are called such, because a portion of the astronomy community defines a planet as something that must orbit a star. Any planetary-mass object which doesn't orbit a star, can't according to that rule be called a planet. As it exists alone like a star, it's called a planet-star, or shorter planetar. In 2003, the IAU Extrasolar Planet Working Group recommended that these objects be called sub-brown dwarfs.
   Some of these planemo harbour debris discs akin to proplyds. The planemo 2M1207b has been discovered to harbour a disc.

Further Information

Get more info on 'Planetar Astronomy'.


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