Supermassive black holes in large galaxies enter active galactic nucleus (AGN) phase, emitting high-energy light like UV radiation that can affect nearby planets.
A recent study in The Astrophysical Journal explores how AGN radiation could potentially help life thrive under certain conditions.
AGN radiation may not be entirely destructive as previously thought, with findings suggesting it could benefit planets with oxygenated atmospheres.
Black holes, like Sagittarius A* in the Milky Way, have likely gone through AGN phases, evidenced by phenomena like Fermi bubbles.
The study utilized computer simulations to show how AGN light interacting with a planet's atmosphere, particularly in the presence of oxygen, could aid in producing ozone.
Oxygen presence can lead to a protective ozone layer forming in the atmosphere, shielding the planet from harmful radiation and supporting life.
Without oxygen, planets are at risk from AGN radiation, potentially hindering the emergence of life.
Research suggests planets in compact galaxies with closer stars to the central black hole are more exposed to lethal radiation compared to galaxies like the Milky Way.
Feedback loops in planetary habitability play a crucial role, where AGN radiation may either help sustain existing life or prevent its emergence.
This study reshapes the view of black holes, suggesting they can act as both threats and aids to life depending on a planet's atmospheric conditions and stage of development.