Planets Could Be Orbiting Black Holes, Calculations Show Possibility of Bizarre Worlds
Theoreticians in two fields defied the received wisdom that planets only orbit stars like the sun. They proposed the possibility of thousands of planets around a supermassive black hole.
“With the right conditions, planets could be formed even in harsh environments, such as around a black hole,” says Keiichi Wada, a professor at Kagoshima University researching active galactic nuclei, luminous objects energized by black holes.
According to the latest theories, planets are formed from fluffy dust aggregates in a protoplanetary disk around a young star. But young stars are not the only objects that possess dust disks. In a novel approach, the researchers focused on heavy disks around supermassive black holes in the nuclei of galaxies.
“Our calculations show that tens of thousands of planets with 10 times the mass of the Earth could be formed around 10 light-years from a black hole,” says Eiichiro Kokubo, a professor at the National Astronomical Observatory of Japan who studies planet formation. “Around black holes, there might exist planetary systems of astonishing scale.”
Some supermassive black holes have large amounts of matter around them in the form of a heavy, dense disk. A disk can contain as much dust as 100,000 times the mass of the sun. This is 1 billion times the dust mass of a protoplanetary disk.
In a low temperature region of a protoplanetary disk, dust grains with ice mantles stick together and evolve into fluffy aggregates. A dust disk around a black hole is so dense that the intense radiation from the central region is blocked and low temperature regions are formed. The researchers applied the planet formation theory to circumnuclear disks and found that planets could form over several hundred million years.
Currently, there are no techniques to detect these planets around black holes. However, the researchers expect this study to open a new field of astronomy.
More information: Keiichi Wada, et al. Planet Formation around Super Massive Black Holes in the Active Galactic Nuclei. Astrophysical Journal. arxiv.org/abs/1909.06748
Journal information: Astrophysical Journal