Dark hole nude
Eye-to-Eye with a Black Hole
3 Nov Millions of years ago, B3 + was just an ordinary supermassive black hole. Now, starless and alone, it’s screaming through space at 2, kilometers per second—and it may never stop. Normally, when two galaxies collide, the supermassive black holes at their centers start.
Astronomers find a ‘nearly-naked’ supermassive black hole | www.biozdravi.eu
5 Jan Astronomers try to figure out why a supermassive black hole is surrounded by almost no stars.
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Dark Holes
Description:This so-called frame dragging will affect everything in the vicinity of the spinning black hole. But light traveling just outside a black hole will be bent -- similar to what happens in a lens. This means the metric is regular for all positive values of r , or in other words, the singularity has no event horizon. Such mathematical calculations have been done before for stationary black holes, but this is the first time it has been done for spinning black holes, Kornreich told SPACE. But this does not mean astronomers will be able to see themselves through a telescope. While they investigate a strange cosmological phenomenon, their two small space crafts begin to shake, and they are unable to leave the area.
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