Black Holes There are many strange and wonderful phenomenons being discovered throughout our Universe. One of the most intriguing is the concept of a black hole in space. Astronomers have discovered a black hole just 1, 600 light years away from Earth. The National Radio Astronomy Observatory cataloged this black hole in the constellation Sagitta ri on a star called V 4641.
A black hole is one form of a dead star. A star has three choices when it dies, it can: shrink until it is a white dwarf, shrink until it is a neutron star, or keep on shrinking until it is a point in space with an infinite density known as a black hole. A black hole is an extremely dense outer space body that has been theorized to exist in the universe. The gravitational field of a black hole is so strong that, if the body is large enough, nothing, including electromagnetic radiation, can escape from its area.
The body is surrounded by a spherical boundary, called a horizon, through which light can enter but not escape; it therefore appears totally black. The idea of a mass concentration so dense that even light would be trapped goes all the way back to Laplace in the 18 th century. Almost immediately after Einstein developed general relativity, Karl Schwarzschild discovered a mathematical solution to the equations of the theory that described such an object. The radius of the horizon of a Schwarzschild black hole depends only on the mass of the body, being 2. 95 km (1.
The Term Paper on Black Holes Star Hole Light
... become a black hole. If though a star with an equivalent mass to the Earth were to collapse into a black hole, the space that all ... an example of the Schwarzchild black hole in nature. An Australian mathematician named Roy P. Kerr only discovered the relative equations to this ... there were also distinct differences. In this new type of black hole, a body that enters it would be forced to move in ...
83 mi) times the mass of the body in solar units (the mass of the body divided by the mass of the sun).
If a body is electrically charged or rotating, Schwarzschild’s results are modified. According to general relativity, gravitation severely modifies space and time near a black hole. As the horizon is approached from outside, time slows down relative to that of distant observers, stopping completely on the horizon.
Once a body has contracted within its Schwarzschild radius (radius of the horizon), it would theoretically collapse to a dimensionless object of infinite density. Although Schwarzschild discovered black holes, it wasn’t until much later with the work of people such as Oppenheimer, Volk off, and Snyder in the 1930’s, that people thought seriously about the possibility that such objects might actually exist in the Universe. These researchers showed that when a sufficiently massive star runs out of fuel, it is unable to support itself against its own gravitational pull, and it should collapse into a black hole. In general relativity, gravity is a manifestation of the curvature of spacetime. Massive objects distort space and time, so that the usual rules of geometry don’t apply anymore. Near a black hole, this distortion of space is extremely severe and causes black holes to have some very strange properties.
In particular, a black hole has something called an ‘event horizon.’ This is a spherical surface that marks the boundary of the black hole. You can pass in through the horizon, but you can’t get back out. In fact, once you ” ve crossed the horizon, you ” re doomed to move inexorably closer and closer to the ‘singularity’ at the center of the black hole. You can think of the horizon as the place where the escape velocity equals the velocity of light.
Outside of the horizon, the escape velocity is less than the speed of light, so if you fire your rockets hard enough, you can give yourself enough energy to get away. But if you find yourself inside the horizon, then no matter how powerful your rockets are, you can’t escape. The horizon has some very strange geometrical properties. To an observer who is sitting still somewhere far away from the black hole, the horizon seems to be a nice, static, unmoving spherical surface. But once you get close to the horizon, you realize that it has a very large velocity. In fact, it is moving outward at the speed of light! That explains why it is easy to cross the horizon in the inward direction, but impossible to get back out.
The Essay on Black Hole Holes Intro Star
One of the few remaining mysteries of science is the black hole. When a star runs out of fuel to keep it burning, it explodes into a supernova (Intro. to Black Holes 1) After a supernova, some of the matter that was blown off leaves in pockets to different places in space. These pockets contract to from a pulsar, or new born star. The rest of the matter left from the massive explosion of the ...
Since the horizon is moving out at the speed of light, in order to escape back across it, you would have to travel faster than light. You can’t go faster than light, and so you can’t escape from the black hole. Scientists had no proof that black holes existed until 1994, when the Hubble Space Telescope uncovered the first convincing evidence that black holes exist in Galaxy M 87. Second and third black holes were discovered in 1995 in Galaxy NGC 4258 and NGC 4261. Incidentally, the name ‘black hole’ was invented by John Archibald Wheeler, and seems to have stuck because it was much catchier than previous names. Before Wheeler came along, these objects were often referred to as ‘frozen stars.’.
