orbitálokon

Orbitalons are hypothetical, ultra-compact celestial bodies theorized to exist in the extreme gravitational environment near a black hole. They are not considered to be stars or planets in the conventional sense but rather dense concentrations of matter that somehow maintain a stable orbit. The concept of orbitalons arises from attempts to reconcile the physics of black holes with the potential for matter to survive and form structures under such immense gravitational stress.

The precise nature and composition of orbitalons remain speculative. Some theories suggest they might be composed of exotic matter or possess unique quantum properties that allow them to resist tidal forces which would otherwise tear apart ordinary objects. Their existence would challenge current astrophysical models and could provide insights into the behavior of matter under conditions that cannot be replicated on Earth.

The search for orbitalons is primarily observational, relying on the detection of subtle gravitational effects or electromagnetic signatures that might betray their presence. However, their small size and proximity to black holes make them exceptionally difficult to detect directly. If confirmed, orbitalons would represent a significant discovery in astrophysics, expanding our understanding of the universe's most extreme environments.