kääpiösferoida

Kääpiösferoida is a term used in astrophysics to describe a hypothetical compact object that is smaller and denser than a neutron star. These objects are theorized to form from the core collapse of very massive stars during a supernova event. Unlike neutron stars, which are primarily composed of neutrons, kääpiösferoida are thought to be made up of a state of matter that is even more exotic and compressed. The extreme density implies that the gravitational forces at their surface would be immense.

The exact composition and properties of kääpiösferoida remain largely speculative, as they have not been directly observed. Theoretical models suggest that if they exist, they would be incredibly difficult to detect due to their small size and low luminosity. Their formation would likely involve conditions far beyond those found in typical stellar evolution scenarios. Research into kääpiösferoida is driven by the desire to understand the ultimate limits of matter under extreme gravitational pressure and to explore the diverse outcomes of stellar death.