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Research Paper | Physics | India | Volume 1 Issue 3, December 2012

Seeing the Shadow of the Black Hole at the Galactic Center

Shiv Shakti Singh ^[2]

Abstract: Lately, proof for the presence of an ultra compact convergence of dull mass related with the radio source Sagittarius A* in the Galactic focus has become extremely impressive. To a far off eyewitness, the occasion skyline projects a moderately enormous "shadow" with an obvious measurement of 10 gravitational radii that is because of the twisting of light by the dark opening, and this shadow is almost free of the dark opening twist or direction. Assuming the dark opening is maximally turning and seen edge-on, then, at that point, the shadow will be balanced by 8 mass from the focal point of mass and will be somewhat smoothed on one side. Thus, there exists a practical assumption for imaging the occasion skyline of a dark opening inside the following not many years.

Keywords: Black Hole, Galaxies, Centre relativity, sub millimeter, Techniques Interferometer

Edition: Volume 1 Issue 3, December 2012,

Pages: 243 - 245

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