Orbitaalins

Orbitaalins are hypothetical, naturally occurring celestial bodies that are not planets, moons, or comets. The concept of an orbitaalin was first proposed as a theoretical object that could exist within a solar system, occupying a stable orbit but not fitting the established definitions of other astronomical bodies. They are characterized by their size and composition, which would typically be smaller than a planet but larger than an asteroid, and could potentially possess a significant gravitational influence.

The existence of orbitaalins remains speculative, as no definitive observations have been made. However, their theoretical framework allows for a broader classification of objects within planetary systems. Such bodies could represent a transitional stage in planetary formation or remnants of collisions between larger celestial bodies. The term itself is derived from the concept of an orbit, highlighting their primary characteristic of revolving around a star. Further research and advancements in astronomical observation technology might provide evidence to support or refute the existence of orbitaalins.