Black Holes

In 1916, German astronomer Carl Schwarzchild tried to find out how the stars narrowed down to what he called "black hole". Schwarzchild predicts that the sun has to shrink to a radius of 2 miles or less. He also predicts that the sun will not change its weight even if it contracts its weight, which means that the planets will remain unaffected in their orbit. Schwarzchild still asked if the star could become this contract. 1934, W. Baade and F. Zwicky predict that the collapse of the stars removes those electron atoms and makes them a neutron star.

Part 1 of the 4 part series series on black holes. In this section we define what a black hole is and go back to the beginning of the black hole study and show how physicists can agree on the presence of these strange objects. Part 2 explains the role of the black hole in the galaxy and how the invisible object will be the brightest in the universe. In Part 3, we will explain how astronomers use the most complex observatory to observe black holes. Part 4 enters a strange aspect of black hole science: how these objects challenge our basic physics theory

Astrophysicist Jedidah Isler is studying a black hole with excessive mass and overactivity. These objects waste material at a thousand times faster than the average super mass black hole. They draw material through an accretion disk rotating around a black hole and then eject it through an ejector moving at 99.99% light speed. When these jets point to the earth, we call them Super Mass, Overactive Black Hole, which produces their Mars or hot quasars. Isler is trying to understand the direction and location of the highest energy light generated by the injector and how this energy is transmitted through the Milky Way

LIGO's black hole is twelve times the mass of the sun. However, astronomers believe that super mass black holes must also collide. That is how the universe forms the biggest quality black hole. However, the gravitational wave generated by the super mass black hole pair has a wavelength that is too large to be seen in LIGO. I returned to the radio telescope. Astronomers recognize that gravitational waves can affect the very fast rotating core of pulsar pulses. Pulsar is one of the most accurate watches in the universe. Pulsar can deliver radio waves because radio waves that emit radio waves arrive as expected. Using a pulsar pair that separates the light of many years in the Milky Way, radio astronomers can look for signs of gravitational waves that affect pulses.