Editing Black Holes (section)

== <span style="color: #FFFFFF;">Remembering</span> ==
* '''Black Hole''' — A region of space with a gravitational pull so strong that nothing can escape.
* '''Singularity''' — The center of a black hole, a point of infinite density where the laws of physics break down.
* '''Event Horizon''' — The "Point of No Return"; the boundary around a black hole beyond which nothing can escape.
* '''Schwarzschild Radius''' — The radius of the event horizon for a non-rotating black hole.
* '''Spaghettification''' — The process by which an object would be stretched vertically and compressed horizontally as it falls into a black hole.
* '''Stellar Black Hole''' — A black hole formed by the collapse of a massive star (up to 20x the mass of the Sun).
* '''Supermassive Black Hole (SMBH)''' — A black hole millions or billions of times the mass of the Sun, found at the centers of galaxies.
* '''Accretion Disk''' — A disk of gas and dust spiraling into a black hole, heating up and emitting intense light/X-rays.
* '''Quasar''' — An extremely bright galactic center powered by a supermassive black hole.
* '''Hawking Radiation''' — The theoretical radiation emitted by black holes due to quantum effects near the event horizon.
* '''Time Dilation''' — The slowing down of time near a massive object (as predicted by General Relativity).
* '''Gravitational Waves''' — Ripples in spacetime caused by the collision of massive objects like black holes.
* '''Gravitational Lensing''' — The bending of light from distant stars as it passes near a black hole.
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