AIRECLEAN ANTI MOSCAS OPCIONES

AireClean anti moscas Opciones

AireClean anti moscas Opciones

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An animation of how light rays Perro be gravitationally bent The simplest static black holes have mass but neither electric charge nor angular momentum. These black holes are often referred to as Schwarzschild black holes after Karl Schwarzschild who discovered this solution in 1916.[17] According to Birkhoff's theorem, it is the only vacuum solution that is spherically symmetric.

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Closer to the black hole, spacetime starts to deform. There are more paths going towards the black hole than paths moving away.[Note 3]

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However, black holes slowly evaporate by emitting Hawking radiation. This radiation does not appear to carry any additional information about the matter that formed the black hole, meaning that this information appears to be gone forever.[216]

Far away from the black hole, a particle can move in any direction, Ganador illustrated by the set of arrows. It is restricted only by the speed of light.

In 1971, Hawking showed under Caudillo conditions[Note 5] that the total area of the event horizons of any collection of classical black holes can never decrease, even if they collide and merge.[211] This result, now known Triunfador the second law of black hole mechanics, is read more remarkably similar to the second law of thermodynamics, which states that the total entropy of an isolated system Perro never decrease.

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The extreme gravitational lensing associated with black holes produces the illusion of a perspective that sees the accretion disc from above. In reality, most of the ring in the EHT image was created when the light emitted by the far side of the accretion disc bent around the black hole's gravity well and escaped, meaning that most of the possible perspectives on M87* Perro see the entire disc, even that directly behind the "shadow".

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