A New Method To Measure Black Hole’s Spin

Black holes are incredibly fascinating and mysterious objects in space. They’re regions in space where the gravitational pull is so strong that nothing, not even light, can escape from them once it passes a certain boundary called the event horizon.

They form when massive stars collapse under their own gravity at the end of their life cycle. The gravitational force becomes so intense that it creates a singularity, an infinitely dense point at the center of a black hole. Surrounding this singularity is the event horizon, which marks the point of no return.

Black holes come in different sizes. Stellar black holes are formed from the remnants of massive stars and can be several times more massive than our sun. Supermassive black holes, found at the centers of most galaxies including our Milky Way, are millions to billions of times more massive than the sun.

They continue to intrigue scientists because they challenge our understanding of physics, particularly the laws of gravity and the behavior of matter at extreme densities. Their study has also led to significant advancements in astrophysics and our understanding of the universe.

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