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  2. The “Interstellar” Ending Explained, 10 Years Later: What ...

    www.aol.com/interstellar-ending-explained-10...

    Making their way around the third planet, Coop falls into a black hole, which allows him to send the NASA site coordinates to his past self and, subsequently, Murph on Earth.

  3. Interstellar (film) - Wikipedia

    en.wikipedia.org/wiki/Interstellar_(film)

    Interstellar is a 2014 epic science fiction drama film directed by Christopher Nolan, who co-wrote the screenplay with his brother Jonathan.It stars Matthew McConaughey, Anne Hathaway, Jessica Chastain, Bill Irwin, Ellen Burstyn, and Michael Caine.

  4. Gravitational collapse - Wikipedia

    en.wikipedia.org/wiki/Gravitational_collapse

    Over time an initial, relatively smooth distribution of matter, after sufficient accretion, may collapse to form pockets of higher density, such as stars or black holes. Star formation involves a gradual gravitational collapse of interstellar medium into clumps of molecular clouds and potential protostars.

  5. The Science of Interstellar - Wikipedia

    en.wikipedia.org/wiki/The_Science_of_Interstellar

    The Science of Interstellar is a non-fiction book by American theoretical physicist and Nobel laureate Kip Thorne, with a foreword by Christopher Nolan. The book was initially published on November 7, 2014 by W. W. Norton & Company. [1] [2] This is his second full-size book for non-scientists after Black Holes and Time Warps, released in 1994.

  6. Active galactic nucleus - Wikipedia

    en.wikipedia.org/wiki/Active_galactic_nucleus

    Quasar – Active galactic nucleus (AGN) containing a supermassive black hole; Radio galaxy – Type of active galaxy that is very luminous at radio wavelengths; Relativistic jet – Beam of ionized matter flowing along the axis of a rotating astronomical object; Supermassive black hole – Largest type of black hole

  7. Black hole - Wikipedia

    en.wikipedia.org/wiki/Black_hole

    A black hole is a region of spacetime where gravity is so strong that nothing, not even light, can escape it. [2] Albert Einstein's theory of general relativity predicts that a sufficiently compact mass can deform spacetime to form a black hole. [3] [4] The boundary of no escape is called the event horizon.

  8. 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 ...

  9. 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 ...