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  2. Blanet - Wikipedia

    en.wikipedia.org/wiki/Blanet

    A blanet is a member of a hypothetical class of exoplanets that directly orbit black holes. [1]Blanets are fundamentally similar to other planets; they have enough mass to be rounded by their own gravity, but are not massive enough to start thermonuclear fusion and become stars.

  3. Are tiny black holes zipping through our solar system ...

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    Scientists say microscopic black holes could explain the elusive "dark matter" that makes up a quarter of all matter in the universe. But can it be proven?

  4. List of most massive black holes - Wikipedia

    en.wikipedia.org/wiki/List_of_most_massive_black...

    The supermassive black hole at the core of Messier 87, here shown by an image by the Event Horizon Telescope, is among the black holes in this list. This is an ordered list of the most massive black holes so far discovered (and probable candidates), measured in units of solar masses ( M ☉ ), approximately 2 × 10 30 kilograms .

  5. Black hole - Wikipedia

    en.wikipedia.org/wiki/Black_hole

    If black holes evaporate via Hawking radiation, a solar mass black hole will evaporate (beginning once the temperature of the cosmic microwave background drops below that of the black hole) over a period of 10 64 years. [149] A supermassive black hole with a mass of 10 11 M ☉ will evaporate in around 2×10 100 years. [150]

  6. Researchers find binary stars orbiting near Milky Way's ... - AOL

    www.aol.com/researchers-binary-stars-orbiting...

    The precise nature of many of the other objects – and, perhaps, even planets – orbiting Sagittarius A*, as well as how they could have formed so close to the supermassive black hole, remain a ...

  7. There could be planets around the supermassive black hole at ...

    www.aol.com/news/could-planets-around-super...

    A disk of hot gas swirls around a black hole in this illustration. The stream of gas stretching to the right is what remains of a star that was pulled apart by the black hole.

  8. Gaia BH1 - Wikipedia

    en.wikipedia.org/wiki/Gaia_BH1

    Gaia BH1 (Gaia DR3 4373465352415301632) is a binary system consisting of a G-type main-sequence star and a likely stellar-mass black hole, located about 1,560 light-years (478 pc) away from the Solar System in the constellation of Ophiuchus. [4]

  9. M33 X-7 - Wikipedia

    en.wikipedia.org/wiki/M33_X-7

    M33 X-7 is a black hole binary system in the Triangulum Galaxy.The system is made up of a stellar-mass black hole and a companion star. The black hole in M33 X-7 has an estimated mass of 15.65 times that of the Sun (M ☉) [3] [4] (formerly the largest known stellar black hole, though this has now been superseded amongst electromagnetically-observed black holes by an increased mass estimate ...