Neutron Stars

Unravel the mysteries of the cosmos with our comprehensive look into Neutron Stars. Astonishingly dense and shrouded in mystery, Neutron Stars are some of the most intriguing celestial objects in the universe. They are the remnants of massive stars that have gone supernova, compacted into a dense core only about 20 kilometers (12.4 miles) in diameter.

Created from the most violent of cosmic events, Neutron Stars are stars that have collapsed under their own gravity, resulting in an incredibly dense object primarily made up of compressed neutrons. Despite their small size, they have a mass up to three times that of our Sun. Their extreme density gives them a gravitational pull two billion times stronger than Earth's gravity.

The rapid rotation and strong magnetic fields of Neutron Stars generate intense electromagnetic radiation, making them detectable as pulsars and sources of powerful X-rays and gamma rays. Despite their tremendous power and density, because of their small size, neutron stars were only discovered fairly recently in the grand scheme of astronomy — the discovery of pulsars in 1967 confirmed their existence.

A close study of Neutron Stars serves as a key to understanding many forceful events and fundamental laws of the universe. They shed light on the workings of supernovae, neutron matter, gravitational waves, and more. Explore our collection of articles, videos, and interactive materials to delve deeper into the captivating world of Neutron Stars.