Black hole naked

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By Leah Crane. There is a black hole in our backyard. Astronomers have found the closest black hole yet at just light years from Earth, close enough to see the stars that orbit it without a telescope. Marianne Heida at the European Southern Observatory in Germany, and her colleagues spotted this black hole completely by accident. It is part of a system called HR that also contains two stars.
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You can 'see' the closest known black hole to Earth with the naked eye

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[] Black holes and naked singularities from Anton-Schmidt's fluids

A black hole horizon brings the added benefit of hiding an embarrassment of the theory that predicts it. Fortunately, our inability to determine the whereabouts of infalling matter as its density diverges near this singularity has no influence on the outside world, which remains protected by the horizon. If such regions of spacetime affect us, we would not be able to predict our future using general relativity. To avoid such a crisis, the physicist Roger Penrose postulated in the cosmic censorship hypothesis , which conjectures that there might be constraints prohibiting naked singularities in nature. If so, general relativity has a way of maintaining determinism by capping the influence of regions whose future behavior cannot be forecasted. But is there really a need for cosmic censorship? A complete theory of quantum gravity, which we currently do not have, might cure singularities and allow the usual determinism to manifest itself throughout the entirety of spacetime.
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Black hole and naked singularity geometries supported by three-form fields

Black holes are regions of infinite density, known as a singularity. And according to mainstream physics, each of these cosmic matter munchers is fringed by an event horizon —- a boundary where once you fall in, you never come out. But what if some black holes are naked — completely lacking such frontiers? As far as we can tell, singularities are always wrapped in event horizons, but a more detailed look at the math of general relativity suggests that doesn't have to be the case. If such naked black holes dot the universe, new research reveals how we might be able to detect one: by looking at the ring of light surrounding it.
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The field equations are obtained explicitly for a static and spherically symmetric geometry in vacuum. For a vanishing three-form field potential the gravitational field equations can be solved exactly. For arbitrary potentials numerical approaches are adopted in studying the behavior of the metric functions and of the three-form field.
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