Do black holes break space-time continuum?

Colliding Black Holes May Disrupt The Space-Time Continuum In 100,000 Years. Talk about a fatal attraction. The black hole duo is located about 3.5 billion light-years away, but the encounter will send out ripples in the space-time continuum that will allow scientists to better study the theory of general relativity.

How do black holes affect space-time?

According to Einstein’s General Theory of Relativity, any massive object actually distorts the space-time around it, including our Sun, Earth, or even us. A black hole is an extreme case in the sense that at its singularity the curvature of space-time becomes infinite, preventing even light to escape.

How does a black hole destroy space?

While black holes are mysterious and exotic, they are also a key consequence of how gravity works: When a lot of mass gets compressed into a small enough space, the resulting object rips the very fabric of space and time, becoming what is called a singularity.

Can you rip a hole in space?

Within the framework of classical General Relativity, black holes contain a singularity which can be said to be a “tear” in spacetime, but that is very informal language, is not used by any serious physicist, and should be avoided because it clouds the exact nature of the singularity.

Do black holes distort space-time?

Black Holes Distort Space-Time According to Einstein’s General Theory of Relativity, any massive object actually distorts the space-time around it, including our Sun, Earth, or even us. A black hole is an extreme case in the sense that at its singularity the curvature of space-time becomes infinite, preventing even light to escape.

How do black holes warp the fabric of time?

NASA/JPL-Caltech Black holes are so massive that they severely warp the fabric of spacetime (the three spatial dimensions and time combined in a four-dimensional continuum). For this reason, an observer inside a black hole experiences the passage of time much differently than an outside observer.

What is the event horizon of a black hole?

A black hole is an extreme case in the sense that at its singularity the curvature of space-time becomes infinite, preventing even light to escape. The boundary beyond which light cannot escape the black hole’s gravity well is known as the event horizon, while its radius is called the Schwarzschild radius.

What does a black hole look like?

From the outside, the region of a black hole looks like the surface of a sphere (in our model with two space dimensions and one time dimension, like the circumference of a circle). But inside that sphere, which has only a finite surface area, you can “hide” objects that are infinitely large – infinitely extended in space. How does this work?