Analyzing Black Holes

The universe contains many diverse and exotic bodies that we just started to understand. Among the myriad of exotic bodies, the most elusive thing is the black hole. In astronomy there are many theories and problems about black holes. The subjects of these queries are black hole characteristics, processes, effects and functions. Scientists still do not fully understand it because it is difficult to find a black hole. By definition, the black hole is an area within the space, and the collapse of the material causes the gravitational field to be very strong, causing the light not to escape as well.

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.