The formula for the Schwarzchild radius of a black hole is given by
Rs = (M/Mo) x 3km.
Here Mo means the mass of the Sun.
For Earth, M/Mo = 0.000 003, that is, Earth has 0.000 003 x Mo.
Thus Earth's Schwarzchild radius is about 1 cm.
That means that if a giant squeezed Earth into a diameter less than 2cm,
it would be a black hole.
For a 10 solar mass black hole, the Schwarzschild radius would be 2.95x104m.
The Schwarzschild radius is directly proportional to the mass of the black hole. It is about 2.95 km for every solar mass.
This is known as the Schwarzschild radius. It is approximately 2.95 km per solar mass.
The Schwarzchild radius of a black hole is linearly dependent on its mass. The relationship is rs = 2GM / c2 where G is the Newtonian gravitational constant, m is the mass of the black hole, and c is the speed of light. The Schwarzchild radius works out to be 2.95 km per solar mass. There is nothing at all mysterious about this formula. It comes from the standard classical formula for escape velocity ve = sqrt(2Gm / r) by substituting c for the velocity and then solving for r.
The radius of the event horizon of a black hole can be approximated by its Schwarzschild radius which is given by the formula r=2GM/(c^2) where G is Newton's gravitational constant, M is the object's mass, and c is the speed of light. Standard units for mass and speed are kilograms and meters per second respectively, yielding a radius in meters. For a 7 solar mass black hole the Scwarzschild radius would be about 20.67 kilometers. So the event horizon would be about 40.34 kilometers across.
A black hole of 100 solar masses would have an event horizon 185.3 miles in radius.
The Schwarzschild radius is directly proportional to the mass of the black hole. It is about 2.95 km for every solar mass.
This is known as the Schwarzschild radius. It is approximately 2.95 km per solar mass.
The Schwarzchild radius of a black hole is linearly dependent on its mass. The relationship is rs = 2GM / c2 where G is the Newtonian gravitational constant, m is the mass of the black hole, and c is the speed of light. The Schwarzchild radius works out to be 2.95 km per solar mass. There is nothing at all mysterious about this formula. It comes from the standard classical formula for escape velocity ve = sqrt(2Gm / r) by substituting c for the velocity and then solving for r.
The radius of the event horizon of a black hole can be approximated by its Schwarzschild radius which is given by the formula r=2GM/(c^2) where G is Newton's gravitational constant, M is the object's mass, and c is the speed of light. Standard units for mass and speed are kilograms and meters per second respectively, yielding a radius in meters. For a 7 solar mass black hole the Scwarzschild radius would be about 20.67 kilometers. So the event horizon would be about 40.34 kilometers across.
The Schwarzchild radius of a 2 solar mass black hole would be about 5.9 km.
A black hole of 100 solar masses would have an event horizon 185.3 miles in radius.
There is no theoretical limit to the MASS of a black hole. The largest known black holes have a mass in excess of a billion solar masses... so far. In the distant future, you can expect them to continue growing.The DIAMETER or the RADIUS of a black hole is directly proportional to the black hole's mass; the radius would be about 3.0 kilometers for every solar mass. The diameter, of course, is twice as much. Thus, a black hole of 10 billion solar masses would have a radius of 30 billion kilometers... about 200 AU.
The event horizon of a black hole is a spherical area round the center of the black hole; it has a radius proportional to the mass of the black hole - a radius of about 2.95 kilometers for every solar mass.
I don't know the solar radius, but all I know is the radius and that is 25.7 R. you. :)
Anywhere from about 100,000 solar masses (100,000 times the mass of our Sun), to more than 10 billion solar masses (the approximate size of the largest known black holes).
1180 solar radius
The mass of the black hole in Sgr A* is estimated at approximately 4 million solar masses (see related links).Assuming its rate of rotation is sufficiently small, we can estimate its Schwarzschild radius R, i.e. the radius of the event horizon, using the following formula from General Relativity:R = 2GM / c2where G is the gravitational constant and c is the speed of light. M is simply the mass mentioned above.This gives a radius of approximately R = 1010 m, which is very roughly a tenth of the distance between the Earth and the Sun.