Star count can be an elusive problem. It’s critical to distinguish between the entire cosmos and the universe that can be seen. We can only witness objects up to a certain distance from Earthlight from more distant objects that haven’t had time to reach us yet because the cosmos was […]

A star is formed when light element atoms are crushed under enough pressure for their nuclei to fuse. Gravitational forces compress atoms in the interstellar plasma until fusion reactions begin, resulting in all-stars. And as the fusion processes start, they exert pressure outward. The star will remain stable as long […]