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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. Stellar collision - Wikipedia

    en.wikipedia.org/wiki/Stellar_collision

    Any stars in the universe can collide, whether they are "alive", meaning fusion is still active in the star, or "dead", with fusion no longer taking place. White dwarf stars, neutron stars , black holes , main sequence stars , giant stars , and supergiants are very different in type, mass, temperature, and radius, and accordingly produce ...

  4. How the Universe Works - Wikipedia

    en.wikipedia.org/wiki/How_the_Universe_Works

    A two-hour episode examines what scientists have learned about M87*, the supermassive black hole in the supergiant elliptical galaxy Messier 87 (also known as Virgo A or NGC 4486). M87* is the first supermassive black hole photographed by the Event Horizon Telescope.

  5. Astronomers theorize what it's like when worlds (and black ...

    www.aol.com/news/2010-08-25-astronomers-theorize...

    Tight binary solar systems are inhabited in science fiction -- remember the Star Wars world of Tatooine -- but humanity might find such planets inhospitable over the long term, and not just ...

  6. Gravitational collapse - Wikipedia

    en.wikipedia.org/wiki/Gravitational_collapse

    Gravitational collapse of a massive star, resulting in a Type II supernova. Gravitational collapse is the contraction of an astronomical object due to the influence of its own gravity, which tends to draw matter inward toward the center of gravity. [1]

  7. Accretion (astrophysics) - Wikipedia

    en.wikipedia.org/wiki/Accretion_(astrophysics)

    Accretion disks are common around smaller stars, stellar remnants in a close binary, or black holes surrounded by material (such as those at the centers of galaxies). Some dynamics in the disk, such as dynamical friction , are necessary to allow orbiting gas to lose angular momentum and fall onto the central massive object.

  8. Neutron star merger - Wikipedia

    en.wikipedia.org/wiki/Neutron_star_merger

    When two neutron stars fall into mutual orbit, they gradually spiral inward due to the loss of energy emitted as gravitational radiation. [1] When they finally meet, their merger leads to the formation of either a more massive neutron star, or—if the mass of the remnant exceeds the Tolman–Oppenheimer–Volkoff limit—a black hole.

  9. Humanity gets peek at what happens inside a black hole

    www.aol.com/humanity-gets-peek-happens-inside...

    Scientists have got a peek at what is happening inside of black holes. A new model – built on gravitational waves that were first detected almost 10 years ago – indicates what is going inside ...