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Until the invention of the telescopeastronomers believed that the universe consisted of a few planetsand the 6000 or so stars they could see with the naked eye. When the telescopebecame available tothem they were amazedto see thatthere were millions of stars in the heavens. In 1785 the German-born English astronomer William Herschel came to the conclusion that our solar system was at the centre of a vast conglomeration of stars which were arranged in the shape of a lens. He estimated that the diameter of the universe was 7,500 light - years. Over the next few centuries European and American astronomers worked doggedly to advance man's knowledge of the universe and by 1920 we knew this much : we were located not at the centre but at the edge of a disc- shaped galaxy. We had two star systems -- the Large Magellanic Cloud and the Small Magellanic Cloud -- as neighbours. This 'universe' was less than 20,000 light-years in diameter. Scientists wondered if that was all there was to the universe. In 1924 the American astronomer, Edwin Hubble found that there was much, much more to it. He discovered that we were not alone,that there were other galaxies besides our own. In 1929 he made the astonishing suggestion that the galaxies were flying away from each other at tremendous speeds. The farthera galaxy, the fasterit moved. Today we know that some of the galaxies are flying away at speeds comparable to the speed of light! So this is the picture we have of the universe now -- a universe thatis perhaps hundreds of millions of light-years in diameter -- and expanding all the while

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