Sunday, 2 February 2014

THE MILKY WAY

ThE MiLKy WaY




THE MILKY WAY IS THE NAME GIVEN TO THE FAINT BAND OF LIGHT that stretches  across the night sky. This light comes from the stars and nebulae in our galaxy, known as the MILKY WAY Galaxy as "the galaxy". The galaxy is shaped like a spiral, with a dense central bulge that is encircled by four arms spiralling  outwards and surrounded by a less dense halo. We can not see the spiral shape because the solar system is in one of the spiral arms, the orion arm ( also called the Local arm ). From our position, the  center of galaxy is completely obscured by dust clouds; as a result, optical maps give only a limited view of galaxy .  However, a more complete picture be obtained  by studying radio, infra-red and other radiations. the central bulge of the galaxy is a relatively small, dense sphere that contains mainly older red and yellow stars. The halo is a less dense region in which the oldest stars are situated; some of these stars may be old as the Galaxy itself ( possibly 15 billion years). The spiral arm contains mainly hot, young, blue stars as well as nebulae (clouds of dust and gas inside which stars are born). The Galaxy is vast, about 100,000 light year across ( a light year is about 9,460 billion km); in comparison, the solar systems seems small st about 12 light hours across ( about 13 billion km). the entire Galaxy is rotating in space, although the inner stars travel faster than those further out. The sun, which is about two-thirds out from the center, completes one lap of the Galaxy about every 220 million years.













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