Schwarzschild radius

That'll tell them you did go through the Schwarzschild radius.

One Schwarzschild radius is the size of the event horizon.

Astronomers measure this using something known as the Schwarzschild radius.

An example of an object smaller than its Schwarzschild radius is a black hole.

This is half the Schwarzschild radius of a one solar mass black hole.

The Schwarzschild radius of an object is proportional to the mass.

"Gentlemen, we simply do not know what goes on inside the Schwarzschild radius of a black hole.

Meanwhile, the Schwarzschild radius of their immense black hole kept out something they feared even more.

The radius is known as the Schwarzschild radius of the star.

This can be rewritten as where the factor and r is the Schwarzschild radius of the body.

The bigger the mass, the bigger the appropriate Schwarzschild radius.

The observable universe's mass has a Schwarzschild radius of approximately 10 billion light years.

Conversely, a small mass has an extremely small Schwarzschild radius.

The threshold of what the tunnel can handle is determined by the object's Schwarzschild radius.

Into the ergosphere, the elliptical region of spin around the Schwarzschild radius.

Otherwise we could get black holes with so much spin to them that there is no Schwarzschild radius around the singularity.

Therefore any star that shrinks within its Schwarzschild radius becomes invisible and is then described as a black hole.

The black hole was set into a netlike structure that started just outside the Schwarzschild radius and extended kilometers.

Two followed the same path, fired a jet before it reached the Schwarzschild radius, and shot away at just less than lightspeed.

As the object shrinks further, no signals from it can cross the sphere with the Schwarzschild radius, not even light.

Production of a black hole requires concentration of mass or energy within the corresponding Schwarzschild radius.

The Schwarzschild radius (r) of any mass is calculated using the following formula:

For a star of about ten solar masses, the Schwarzschild radius is about thirty kilometers.

Any non-rotating and non-charged mass that is smaller than its Schwarzschild radius forms a black hole.

Theoretically, any amount of matter will become a black hole if compressed into a space that fits within its corresponding Schwarzschild radius.