A neutron star is a compact astronomical object formed from the remnants of a supernova explosion, consisting mostly of tightly packed neutrons and exhibiting extreme density and gravity.
Overview
Magnetic Fields
Physical Properties
Observational Methods
Pulsars And Magnetars
Types Of Neutron Stars
Formation And Evolution
The Role In Astrophysics
Future Research Directions
Jocelyn Bell Burnell
Magnetic Field
Information
Supernova
Mountain
Universe
Pressure
Gravity
Neutron
๐ Neutron stars are remnants of supernova explosions and are incredibly dense, packing more mass than the Sun into a sphere just about 20 kilometers in diameter.
๐ง A neutron star can have a surface temperature of over a million degrees Celsius when it forms, rapidly cooling down over millions of years.
โก Neutron stars can rotate at incredibly high speeds, with some rotating more than 700 times per second.
๐ฅ The gravity on the surface of a neutron star is about 2 billion times stronger than that of Earth.
๐ Some neutron stars emit beams of radiation, making them detectable as pulsars when the beam is oriented towards Earth.
โข๏ธ Neutron stars are primarily composed of neutrons, and the matter inside them is believed to be in a superfluid state.
๐ช The mass of a neutron star typically ranges from 1.4 to about 2.16 solar masses, beyond which it may collapse into a black hole.
๐ญ Neutron stars can generate strong magnetic fields, typically around 1 trillion times stronger than Earth's magnetic field.
๐ When two neutron stars collide, they can create gravitational waves and are thought to be the source of heavy elements like gold.
๐ Neutron stars are among the smallest and densest objects in the universe, making them a key subject of study in astrophysics.
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