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π 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.
π§ A neutron star can have a surface temperature of over a million degrees Celsius when it forms, rapidly cooling down over millions of years.
β‘ Neutron stars can rotate at incredibly high speeds, with some rotating more than 700 times per second.
π₯ The gravity on the surface of a neutron star is about 2 billion times stronger than that of Earth.
π Some neutron stars emit beams of radiation, making them detectable as pulsars when the beam is oriented towards Earth.
β’οΈ Neutron stars are primarily composed of neutrons, and the matter inside them is believed to be in a superfluid state.
πͺ 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.
π Neutron stars can generate strong magnetic fields, typically around 1 trillion times stronger than Earth's magnetic field.
π When two neutron stars collide, they can create gravitational waves and are thought to be the source of heavy elements like gold.
π 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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