Planetar (astronomy)

From Wikipedia, the free encyclopedia

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 do not 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.

Contents

[edit] 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.[citation needed]

[edit] 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.[citation needed]

[edit] Unbound planet planetars

The free-floating planet, known as a planetar, is called such, because a portion of the astronomy community defines a planet as something that must orbit a star. Any planetary-mass object which does not orbit a star, cannot thus be called a planet. As it exists alone, it is like a star, so it is called a planet-star, or 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.

[edit] See also

[edit] References

[edit] External links


In other languages