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  2. Naked singularity - Wikipedia

    en.wikipedia.org/wiki/Naked_singularity

    Ray traced image of a hypothetical naked singularity in front of a Milky Way background. The parameters of the singularity are M=1, a²+Q²=2M². The singularity is viewed from its equatorial plane at θ=90° (edge on). Comparison with an extremal black hole with M=1, a²+Q²=1M²

  3. Gravitational singularity - Wikipedia

    en.wikipedia.org/wiki/Gravitational_singularity

    However, it is hypothesized that light entering a singularity would similarly have its geodesics terminated, thus making the naked singularity look like a black hole. [17] [18] [19] Disappearing event horizons exist in the Kerr metric, which is a spinning black hole in a vacuum, if the angular momentum () is high

  4. Cosmic censorship hypothesis - Wikipedia

    en.wikipedia.org/wiki/Cosmic_censorship_hypothesis

    Failure of the cosmic censorship hypothesis leads to the failure of determinism, because it is yet impossible to predict the behavior of spacetime in the causal future of a singularity. Cosmic censorship is not merely a problem of formal interest; some form of it is assumed whenever black hole event horizons are mentioned. [citation needed]

  5. Over a year ago, a group of researchers made a revolutionary breakthrough when they successfully captured the first-ever image of a celestial phenomenon — a black hole. The short sequence of ...

  6. Scientists capture first-ever image of 'the unseeable' black hole

    www.aol.com/weather/scientists-capture-first...

    This is the first image of Sagittarius A* (or Sgr A* for short), the supermassive black hole at the center of the Milky Way galaxy, 27,000 light-years from Earth. It's the first direct visual ...

  7. Mesmerizing image of black hole reveals magnetic field

    www.aol.com/mesmerizing-image-black-hole-reveals...

    The first image of a black hole just became even more fascinating. At the center of the Messier 87 (M87) galaxy is a supermassive black hole about 38 billion kilometers wide, a behemoth so dense ...

  8. File:Naked.Singularity,Overextremal.Kerr.Newman,Raytracing ...

    en.wikipedia.org/wiki/File:Naked.Singularity...

    English: Gravitational lensing of an overextremal Kerr-Newman naked ring singularity with spin a/M=√2 and charge Q/M=√2, in natural units of G=K=c=1 (so a²+Q²=2M²). The observer is at r=50M and views the naked singularity from the equatorial plane (edge on); its left side is rotating towards the observer.

  9. File:Black hole - Messier 87 crop max res.jpg - Wikipedia

    en.wikipedia.org/wiki/File:Black_hole_-_Messier...

    The black hole’s boundary — the event horizon from which the EHT takes its name — is around 2.5 times smaller than the shadow it casts and measures just under 40 billion km across. While this may sound large, this ring is only about 40 microarcseconds across — equivalent to measuring the length of a credit card on the surface of the Moon.