Neutroncsillagokat

Neutroncsillagokat are the incredibly dense remnants of massive stars that have undergone a supernova explosion. When a star much more massive than our Sun exhausts its nuclear fuel, its core collapses under its own gravity. This catastrophic implosion forces protons and electrons to combine, forming neutrons. The resulting object is predominantly composed of neutrons, packed together with immense force.

Neutroncsillagokat are extraordinarily small, typically only about 20 kilometers (12 miles) in diameter, yet they contain more mass than our Sun. This extreme density means that a teaspoonful of neutroncsillag material would weigh billions of tons. Their gravitational pull is also incredibly powerful.

Many neutroncsillagokat rotate very rapidly and possess intense magnetic fields. If their magnetic poles are aligned in such a way that they sweep across our line of sight as they rotate, we observe them as pulsars. These pulsars emit beams of electromagnetic radiation, like radio waves, which are detected as regular pulses. Neutroncsillagokat are among the most extreme objects in the universe, providing valuable insights into the physics of matter under conditions not achievable on Earth.