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  2. Spaghettification - Wikipedia

    en.wikipedia.org/wiki/Spaghettification

    The point at which tidal forces destroy an object or kill a person will depend on the black hole's size. For a supermassive black hole, such as those found at a galaxy's center, this point lies within the event horizon, so an astronaut may cross the event horizon without noticing any squashing and pulling, although it remains only a matter of ...

  3. Gravitational singularity - Wikipedia

    en.wikipedia.org/wiki/Gravitational_singularity

    While in a non-rotating black hole the singularity occurs at a single point in the model coordinates, called a "point singularity", in a rotating black hole, also known as a Kerr black hole, the singularity occurs on a ring (a circular line), known as a "ring singularity". Such a singularity may also theoretically become a wormhole. [18]

  4. Black hole - Wikipedia

    en.wikipedia.org/wiki/Black_hole

    The term "black hole" was used in print by Life and Science News magazines in 1963, and by science journalist Ann Ewing in her article " 'Black Holes' in Space", dated 18 January 1964, which was a report on a meeting of the American Association for the Advancement of Science held in Cleveland, Ohio.

  5. Stephen Hawking's famous prediction about black holes was ...

    www.aol.com/article/2016/08/15/stephen-hawking-s...

    In 1974, Hawking predicted that black holes might not be the bottomless pits we imagine them to be -- and now, there may be evidence to support that theory.

  6. Scientists witness a dormant supermassive black hole roar to life

    www.aol.com/news/scientists-witness-dormant...

    Supermassive black holes sometimes shoot vast jets of high-energy particles into space, but no such jet has been detected in this instance, according to astrophysicist and study co-author Lorena ...

  7. Future of an expanding universe - Wikipedia

    en.wikipedia.org/wiki/Future_of_an_expanding...

    A black hole with a mass of around 1 M ☉ will vanish in around 2 × 10 64 years. As the lifetime of a black hole is proportional to the cube of its mass, more massive black holes take longer to decay. A supermassive black hole with a mass of 10 11 (100 billion) M ☉ will evaporate in around 2 × 10 93 years. [45]

  8. Event horizon - Wikipedia

    en.wikipedia.org/wiki/Event_horizon

    For black holes, this manifests as Hawking radiation, and the larger question of how the black hole possesses a temperature is part of the topic of black hole thermodynamics. For accelerating particles, this manifests as the Unruh effect , which causes space around the particle to appear to be filled with matter and radiation.

  9. Oldest black hole discovered dating back to 470 million years ...

    www.aol.com/news/oldest-black-hole-discovered...

    NASA’s James Webb Space Telescope and Chandra X-Ray Observatory teamed up over the past year to make the observations. Scientists have discovered the oldest black hole yet, a cosmic beast formed ...