A blanet is a member of a hypothetical class of exoplanets that directly orbit black holes. [1]
Blanets are fundamentally similar to other planets; they have enough mass to be rounded by their own gravity, but are not massive enough to start thermonuclear fusion and become stars. In 2019, a team of astronomers and exoplanetologists showed that there is a safe zone around a supermassive black hole that could harbor thousands of blanets in orbit around it. [2] [3]
The team led by Keiichi Wada of Kagoshima University in Japan has given this name to black hole planets. [4] The word is a portmanteau of black hole and planet.
Blanets are suspected to form in the accretion disk that orbits a sufficiently large black hole, provided the disk is relatively dim. [3] [5] [6] Radiation feedback from the black hole could rotationally disrupt large dust grains in its accretion disk, causing them to break apart and preventing the formation of blanets. [6]
Blanets around supermassive black holes formed by the hole's accretion disk are likely to be at least 20 Earth masses and may have very long orbital periods to the order of hundreds of thousands of years. Despite their large mass relative to Earth, it would be difficult for blanets to gain a sufficient atmosphere in order to become gas giants due to Bondi accretion by the black hole. [3]
Blanets may be heated by the black hole's accretion disk, or, if sufficiently close to the black hole, may be heated by blueshifted cosmic microwave background radiation. [7]
Blanets sufficiently close to their host black hole may also be tidally locked or even tidally deformed. [7]
