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Black Holes Black holes are composed of condensed matter or antimatter and can have the mass of billion suns but still be smaller than the size of the sun. The existence of black holes has be know for centuries. In 1784, John Michell realized that gravity could attract light and form "dark stars". Michell ideas were published by Pierre Simon Laplace in first editions of an astronomy guide. In 1795, Laplace defined the requirements for a black hole. According to "Hubble Space Telescope News", massive black holes have been shown to dwell in the center of most galaxies. The massive black holes are so common, nearly every large galaxy has them. The University of Michigan News Release entitled Galaxies and Black Holes: You can't Have One Without the Other provides colored images, that can be electronically downloaded for galaxies. Computer simulations demonstrate how the Einstein-Rosen Bridge keeps the matter and antimatter black holes separated and the oscillations between the black holes at opposite ends of the wormhole force the black holes to become white holes that eject matter and antimatter in opposite directions forming the spiral arms of stars within the galactic disk. The white holes are ejecting matter and antimatter from opposite directions into space. The galaxy are slowly spinning as they eject matter and antimatter into spiral arms of stars. The article on Stringy Black Holes by Martijn Derix & Jan Pieter van der Schaar has extensive discussions and solutions on black holes. |
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Matter
Opportunities
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Space:
The Final Frontier *
Dangers
AntiMatter |