Telescopes in Astronomy

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Telescopes in Astronomy Telescopes in Astronomy Some simple information of telescopes in astronomy will be discussed in this paper. For many years telescopes have been used for observing celestial objects. Telescopes have changed our understanding and knowledge by detecting substances in the universe. New developments have been revealed based on measuring the wavelength omitted from the celestial objects with improved technology creating many kinds of telescopes. Studying different stages of stars in detail can be done by using different telescopes that are used for specific purposes. This paper will touch bases on how the telescope changed our understanding of the universe and our place in it, describe the main designs of telescopes and discuss their strengths and weaknesses, define the best places to build ground-based telescopes and why astronomers choose those places, contrast the strengths and weaknesses between building telescopes on the Earth, in orbit, or even on the Moon, describe how different frequencies of light tell more about the birth, life, and death in the nature and properties of the Sun, the stars, and the universe, and describe how telescopes manage to operate in wavelengths of light that stretch from radio waves to gamma rays. Telescopes have expanded our vision to the universe. Initial telescopes showed that Earth was not the midpoint of the universe, as was formerly believed. Telescopes also indicated mountains and craters on the moon. Future telescopes have discovered geography and weather on the planets in our solar system. Telescopes have also exposed new planets and asteroids. These devices helped us make the first legitimate measurement of the speed of light. Telescopes have also assisted us to comprehend gravity and other vital laws of the physical world. Telescopes have also assisted in recognizing the light that releases from

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