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http://thetartan.org/2007/2/26/scitech/workHow Things Work: Black Holes<br />Sci/Tech | Sarah Mogin <br /><br /> <br />Courtesy of NASA/JPL-Caltech<br />Black holes exert gravitational forces on objects that bring them to the singularity, or center.<br />More Sci/Tech Stories<br />Pitt develops molecule that fights cancer cell growth <br />Professor makes presentation on carbon control policy <br />SciTech Briefs <br />How Things Work: Black Holes <br />More »<br /><br />Up there with the aliens from War of the Worlds, black holes are probably some of the more terrifying aspects of the universe.<br /><br />Black holes form following the deaths of massive stars.<br /><br />Throughout their lifetimes, stars are subject to their own gravitational fields in space. The gravitational fields create forces on the star.<br /><br />One would expect this force to cause the star to collapse inward. However, there is an equally strong force in opposition to this gravitational force.<br /><br />Elements of a star<br /><br />This latter force is caused by the fusion reactions taking place within the star. For the majority of the star’s lifetime, hydrogen fuses inside its core to create helium.<br /><br />When the star’s supply of hydrogen runs out, it becomes a red giant. The star initially expands and then shrinks to a helium core, at which point the helium atoms begin to fuse with other helium atoms to form carbon and oxygen.<br /><br />In massive stars (those at least nine times as big as the sun) this process of expansion and contraction keeps going; the red giant phase typically lasts between a few hundred thousand to one million years.<br /><br />Following oxygen, the star produces neon, silicon, sulfur, and then iron. The star begins fusing the element that it has just produced after each expansion and contraction.<br /><br />At the end of its life, the star will fuse multiple elements at once in onion-layer shells. The outermost