Gargantura black hole in the film Interstellar and how about this according to Science?

In the film Interstellar, Cooper, played by Matthew McConaughey, plunges into the black hole Gargantura. As Cooper’s ship breaks apart in the force. What is black hole? Here are some scientific explanation about this.

Black holes are space objects that have a very powerful gravity effect so that there are no objects – even particles and electromagnetic radiation such as light – that can escape from these objects. The theory of general relativity predicts objects that have a large enough mass can damage spacetime objects and create black holes. Boundary of the area where there is no way out called the horizon. Although the horizon has a very large effect on fate and state of the objects that cross into it, no object can be found and can be seen. In many ways, black holes are like ideal black bodies, because they don’t reflect light. In addition, the curved quantum field theory predicts that the horizon emits Hawking radiation, with the same spectrum as black matter with a temperature inversely proportional to its mass. This temperature depends on the hole for the blackhole mass, so that at the time specified to be chosen.

Black Holes Theory

Objects that have a release field are too strong for light to escape first introduced in the 18th century by John Michell and Pierre-Simon Laplace. The first modern solution of general relativity that would characterize black holes was invented by Karl Schwarzschild in 1916, while the interpretation of the space area could be escape released by David Finkelstein in 1958. Black holes have long been mathematically curiosity; between 1960s the theory showed that this was the initial prediction of general relativity. Discovery of neutron stars by Jocelyn Bell Burnell in 1967.

Black holes from stellar masses are thought to form when very massive stars collapse at the end of space cycle of space objects. After a black hole is formed, it can continue to grow by absorbing the mass from its surroundings. By absorbing other stars and joining other black holes, supermassive black holes can form millions of solar masses. There is a general theory that supermassive black holes are at the center of most large galaxies.

Black Holes Binary Systems

Although the inside of black hole is not visible, the presence of a black hole can be inferred through its interaction with other matter and with electromagnetic radiation such as visible light. Material that falls into a black hole can form an external accretion disk heated by friction, forming some of the brightest objects in the universe. If there are other stars that orbit the black hole, the orbit can be used to determine the mass and location of the black hole. Such observations can be used to exclude alternatives that might occur like neutron stars. In this way, however astronomers have identified many black hole candidates in binary systems, and determined that the radio source known as Sagittarius A, in the core of the Milky Way galaxy, contains supermassive black holes of around 4.3 million solar masses.

On February 11, 2016, the LIGO consortium announced the first direct detection of gravitational waves, which was also the first observation of a merger of black holes. In December 2018, eleven gravitational wave events have been observed which originated from ten black holes that joined (by combining binary neutron stars). On April 10, 2019, therefore direct images of the first and surrounding black holes have been published, after observations made by the Event Horizon Telescope in 2017 about supermassive black holes at the center of the galaxy Messier 87.

Credit for: