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  2. The Black Hole (2016 film) - Wikipedia

    en.wikipedia.org/wiki/The_Black_Hole_(2016_film)

    The Black Hole is an American science-fiction film directed by Mark Grove and released on December 2, 2016. The film was originally titled Mind's Eye , and was also released internationally under the name Quantum Voyage .

  3. The Black Hole (1979 film) - Wikipedia

    en.wikipedia.org/wiki/The_Black_Hole_(1979_film)

    The Black Hole is a 1979 American science fiction film directed by Gary Nelson and produced by Walt Disney Productions.The film stars Maximilian Schell, Robert Forster, Joseph Bottoms, Yvette Mimieux, Anthony Perkins and Ernest Borgnine, while the voices of the main robot characters are provided by Roddy McDowall and Slim Pickens (both uncredited).

  4. Sagittarius A* - Wikipedia

    en.wikipedia.org/wiki/Sagittarius_A*

    Sagittarius A*, abbreviated as Sgr A* (/ ˈ s æ dʒ ˈ eɪ s t ɑːr / SADGE-AY-star [3]), is the supermassive black hole [4] [5] [6] at the Galactic Center of the Milky Way.Viewed from Earth, it is located near the border of the constellations Sagittarius and Scorpius, about 5.6° south of the ecliptic, [7] visually close to the Butterfly Cluster (M6) and Lambda Scorpii.

  5. Black hole - Wikipedia

    en.wikipedia.org/wiki/Black_hole

    A black hole with the mass of a car would have a diameter of about 10 −24 m and take a nanosecond to evaporate, during which time it would briefly have a luminosity of more than 200 times that of the Sun. Lower-mass black holes are expected to evaporate even faster; for example, a black hole of mass 1 TeV/c 2 would take less than 10 −88 ...

  6. The Black Hole (2006 film) - Wikipedia

    en.wikipedia.org/wiki/The_Black_Hole_(2006_film)

    The Black Hole is a 2006 American television film produced for the Sci Fi channel, directed by Tibor Takács and starring Judd Nelson and Kristy Swanson. [1] [2] [3]

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  8. No-hair theorem - Wikipedia

    en.wikipedia.org/wiki/No-hair_theorem

    The no-hair theorem (which is a hypothesis) states that all stationary black hole solutions of the Einstein–Maxwell equations of gravitation and electromagnetism in general relativity can be completely characterized by only three independent externally observable classical parameters: mass, angular momentum, and electric charge.

  9. Hayden–Preskill thought experiment - Wikipedia

    en.wikipedia.org/wiki/Hayden–Preskill_thought...

    Outside of the black hole's event horizon, semi-classical field equations remain valid. A black hole is a quantum system with discrete energy levels, as viewed by a distant observer. A free falling observer encounters nothing unique or strange; passing the event horizon is not marked by observable phenomena intrinsic to the horizon itself.