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  2. Oppenheimer–Snyder model - Wikipedia

    en.wikipedia.org/wiki/Oppenheimer–Snyder_model

    This paper predicted the existence of what are today known as black holes. [1] [7] The term "black hole" was coined decades later, in the fall of 1967, by John Archibald Wheeler at a conference held by the Goddard Institute for Space Studies in New York City; [7] it appeared for the first time in print the following year. [8]

  3. Black hole - Wikipedia

    en.wikipedia.org/wiki/Black_hole

    A black hole is a massive, compact astronomical object so dense that its gravity prevents prevents anything from escaping, even light. Albert Einstein's theory of general relativity predicts that a sufficiently compact mass can deform spacetime to form a black hole. [2] [3] The boundary of no escape is called the event horizon.

  4. Schwarzschild geodesics - Wikipedia

    en.wikipedia.org/wiki/Schwarzschild_geodesics

    Other tachyonic solutions can enter a black hole and re-exit into the parallel exterior region. The constant t {\textstyle t} solution inside the event horizon ( r s {\textstyle r_{\text{s}}} ) is continued by a constant t {\textstyle t} solution in a white hole .

  5. 30-year-old black hole mystery has finally been solved

    www.aol.com/news/2016-08-01-30-year-old-black...

    A 30-year-long question about black holes has finally been resolved. Apparently, black holes twist space time like taffy. This finding is based off a principle put forward by renowned scientist ...

  6. Outline of black holes - Wikipedia

    en.wikipedia.org/wiki/Outline_of_black_holes

    Extremal black hole – black hole with the minimal possible mass that can be compatible with a given charge and angular momentum. Black hole electron – if there were a black hole with the same mass and charge as an electron, it would share many of the properties of the electron including the magnetic moment and Compton wavelength.

  7. Alex Filippenko - Wikipedia

    en.wikipedia.org/wiki/Alex_Filippenko

    His other videos courses are Black Holes Explained [8] and Skywatching: Seeing and Understanding Cosmic Wonders. [ 9 ] With co-author Jay M. Pasachoff , Filippenko also wrote the award-winning introductory textbook The Cosmos: Astronomy in the New Millennium , now in its fifth edition (2019).

  8. Innermost stable circular orbit - Wikipedia

    en.wikipedia.org/wiki/Innermost_stable_circular...

    The ISCO plays an important role in black hole accretion disks since it marks the inner edge of the disk. The ISCO should not be confused with the Roche limit, the innermost point where a physical object can orbit before tidal forces break it up. The ISCO is concerned with theoretical test particles, not real objects. In general terms, the ISCO ...

  9. Binary black hole - Wikipedia

    en.wikipedia.org/wiki/Binary_black_hole

    A binary black hole (BBH), or black hole binary, is a system consisting of two black holes in close orbit around each other. Like black holes themselves, binary black holes are often divided into binary stellar black holes , formed either as remnants of high-mass binary star systems or by dynamic processes and mutual capture; and binary ...