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  2. Discovery of Neptune - Wikipedia

    en.wikipedia.org/wiki/Discovery_of_Neptune

    In 1848, Jacques Babinet raised an objection to Le Verrier's calculations, claiming that Neptune's observed mass was smaller and its orbit larger than Le Verrier had initially predicted. He postulated, based largely on simple subtraction from Le Verrier's calculations, that another planet of roughly 12 Earth masses, which he named "Hyperion ...

  3. John Couch Adams - Wikipedia

    en.wikipedia.org/wiki/John_Couch_Adams

    Only after the discovery of Neptune on 23 September 1846 had been announced in Paris did it become apparent that Neptune had been observed on 8 and 12 August but because Challis lacked an up-to-date star-map it was not recognized as a planet. [1] A keen controversy arose in France and England as to the merits of the two astronomers.

  4. Urbain Le Verrier - Wikipedia

    en.wikipedia.org/wiki/Urbain_Le_Verrier

    Urbain Jean Joseph Le Verrier (French: [yʁbɛ̃ ʒɑ̃ ʒozɛf lə vɛʁje]; 11 March 1811 – 23 September 1877) was a French astronomer and mathematician who specialized in celestial mechanics and is best known for predicting the existence and position of Neptune using only mathematics.

  5. Historical models of the Solar System - Wikipedia

    en.wikipedia.org/wiki/Historical_models_of_the...

    Later, between 1845 and 1846, John Adams and Urbain Le Verrier separately predicted the existence and location of a new planet from irregularities in the orbit of Uranus. [100] This new planet was finally found by Johann Galle and eventually named Neptune, following the predicted position gave to him by Le Verrier. This fact marked the climax ...

  6. Neptune’s clouds have disappeared, and scientists think they ...

    www.aol.com/neptune-disappearing-clouds-may...

    Four years ago, astronomers noticed the abundant clouds on Neptune had largely disappeared. Telescope data may have helped researchers figure out why. Neptune’s clouds have disappeared, and ...

  7. Neptune - Wikipedia

    en.wikipedia.org/wiki/Neptune

    Neptune's mass of 1.0243 × 10 26 kg [8] is intermediate between Earth and the larger gas giants: it is 17 times that of Earth but just 1/19th that of Jupiter. [g] Its gravity at 1 bar is 11.15 m/s 2, 1.14 times the surface gravity of Earth, [71] and surpassed only by Jupiter. [72] Neptune's equatorial radius of 24,764 km [11] is nearly four ...

  8. Scientists Find a 'Forbidden Planet' That Shouldn't Exist - AOL

    www.aol.com/news/scientists-forbidden-planet...

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  9. NASA says this planet is just too damn hot to exist - AOL

    www.aol.com/nasa-says-planet-just-too-140026044.html

    Hot Neptunes are — theoretically — worlds the size of Neptune or slightly larger than Neptune, orbiting close to their parent stars. NASA says this planet is just too damn hot to exist Skip to ...