Methods and Latest Progress on Planet Detections

As we look up at the night sky, we are surprised by humanity as a huge unknown for the universe. We can see thousands of shining stars and other things, but there are billions of things that we can not see. Many people may think there are billions of stars and planets, and we are the only creatures in this universe. There are many other problems. These answers are not that simple. The only way we can answer the question is to have astronomers and planetary hunters do their work. The research process and research they use to find new planets and research processes is complicated.

Most of today's planetary detection methods are detecting the influence of planets on the movement and light of stars around them; they can not "see" the planet directly. To find the symbol of life, astronomers must take photos from the planets themselves and analyze them. But planets like the earth around other stars are small and weak, so direct imaging requires a large space telescope to block light from the parent's star. This type of life requires complex carbon-based compounds that interact in liquid water. Carbon is unparalleled in its ability to form a strong bond and can form complex molecules that store and transfer large amounts of information. This is one of the outstanding features of life. Many of the characteristics and functions of liquid water are unique and can be executed efficiently. Carbon, hydrogen and oxygen constituting water are abundant in the universe.

For centuries scientists, philosophers, and science fiction writers doubted the existence of extrasolar planets, but how to detect them and to know their frequency and similarity with solar system planets there is no. Astronomers rejected various experiment reports from the 19th century. The first evidence of extrasolar planets was known as early as 1917, but it was not recognized. For the first time, it was suspected that the scientific detection of the outer planet was done in 1988. Shortly thereafter, the first confirmed explorer occurred in 1992 and several land - quality planets orbiting the pulsar PSR B 1257 + 12 orbit were discovered. In 1995, a huge planet was discovered in a four day orbit around the nearby star 51 Pegasi. This is the first confirmation of an outer planet orbiting the main sequence star. Unlike the Earth, most extrasolar planets are not closely related to the stars, so they are actually in the universe or in a loose orbit between the stars.

Since the fraudulent planet is a starless planet, it runs directly around the galaxy. It is difficult to find this because it is not reflecting the star's light or can not be detected by the general extra solar planetary detection method. However, science opened the way to such a planet lurking in the dark beyond 80 light years. The faint red light of the rogue planet PSO J 318.5 - 22 was imaged directly by the Pan - STARRS PS 1 telescope. It is difficult to find such a rogue planet, but it is relatively easy to find because some people think that it is six times bigger than Jupiter.