Black holes form when massive stars (20 times the Sun's mass) collapse under gravity, compressing their core from Earth-sized to smaller than an atom; the event horizon is the point of no return where space curves so dramatically that outward movement becomes impossible; supermassive black holes like Sagittarius A* (4 million solar masses) sit at galaxy centers and are detected through orbiting stars; contrary to popular belief, black holes emit Hawking radiation from virtual particles at the event horizon, causing them to slowly evaporate over 10^100 years, far exceeding the universe's 13.8 billion year age.
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What They Don't Tell You About How Do Black Holes Actually Work #shortsAdded:
Black holes are the ultimate cosmic mystery. Here's how they actually work.
When a massive star dies, we're talking 20 times the mass of our sun, it collapses under its own gravity.
The core shrinks from the size of Earth to the size of a city.
All that mass packed into a point smaller than an atom. That's a stellar black hole.
The event horizon is the point of no return. Cross it and you can never come back.
Not because a force pushes you in, but because every direction you could possibly move leads inward.
Space itself has curved so dramatically that outward simply doesn't exist anymore.
Supermassive black holes sit at the center of every large galaxy.
Our Milky Way has one called Sagittarius A* 4 million times the mass of the sun.
It's 26,000 light-years away and completely invisible.
We only know it's there because stars orbited at impossible speeds.
Here's the wildest part. Black holes aren't actually black.
They glow with Hawking radiation.
Virtual particles that pop into existence at the event horizon.
One particle falls in, the other escapes. Over an unimaginable time, the black hole slowly evaporates. The largest ones will take 10 to the 100 years to disappear. That's a Google years.
The universe is 13.8 billion years old.
Black holes will outlast it by a factor of 10 to the 90.
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