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  2. 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.

  3. 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 ...

  4. Katie Bouman - Wikipedia

    en.wikipedia.org/wiki/Katie_Bouman

    Katherine Louise Bouman (/ ˈ b aʊ m ə n /; [1] born 1989) is an American engineer and computer scientist working in the field of computational imaging.She led the development of an algorithm for imaging black holes, known as Continuous High-resolution Image Reconstruction using Patch priors (CHIRP), and was a member of the Event Horizon Telescope team that captured the first image of a ...

  5. List of black holes - Wikipedia

    en.wikipedia.org/wiki/List_of_black_holes

    IGR J17091-3624 (candidate smallest known stellar black hole) [14] [15] LB-1 (name of both a galactic B-type star and a very closely associated over-massive stellar-mass black hole) [16] [17] M33 X-7 (stellar black hole with the most massive stellar companion, located in the Triangulum Galaxy) [18]

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  7. Supermassive black hole - Wikipedia

    en.wikipedia.org/wiki/Supermassive_black_hole

    Formation of black holes from the deaths of the first stars has been extensively studied and corroborated by observations. The other models for black hole formation listed above are theoretical. The formation of a supermassive black hole requires a relatively small volume of highly dense matter having small angular momentum. Normally, the ...

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  9. Outline of black holes - Wikipedia

    en.wikipedia.org/wiki/Outline_of_black_holes

    The LIGO Scientific Collaboration announces the first detection of a black hole merger via gravitational wave observations on February 11, 2016. The Event Horizon Telescope observes the supermassive black hole in Messier 87's galactic center in 2017, leading to the first direct image of a black hole being published on April 10, 2019.