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  2. 55 Cancri e - Wikipedia

    en.wikipedia.org/wiki/55_Cancri_e

    This is the first time the atmosphere of a super-Earth exoplanet was analyzed successfully. [31] [32] In November 2017, it was announced that infrared observations with the Spitzer Space Telescope indicated the presence of a global lava ocean obscured by an atmosphere with a pressure of about 1.4 bar, slightly thicker than that of Earth.

  3. List of directly imaged exoplanets - Wikipedia

    en.wikipedia.org/wiki/List_of_directly_imaged...

    Motion interpolation of seven images of the HR 8799 system taken from the W. M. Keck Observatory over seven years, featuring four exoplanets. This is a list of extrasolar planets that have been directly observed, sorted by observed separations. This method works best for young planets that emit infrared light and are far from the glare of the star.

  4. PSR J1719−1438 b - Wikipedia

    en.wikipedia.org/wiki/PSR_J1719%E2%88%921438_b

    PSR J1719−1438 b is an extrasolar planet that was discovered on August 25, 2011, in orbit around PSR J1719−1438, a millisecond pulsar.The pulsar planet is most likely composed largely of crystalline carbon but with a density far greater than diamond.

  5. Scientists recreate Neptune's diamond rain using ... - AOL

    www.aol.com/news/2017-08-21-neptune-diamond-rain...

    They recreated Neptune's conditions at Stanford's SLAC Laboratory and successfully observed the formation of diamond rain, thanks to the help of some very powerful lasers. Scientists recreate ...

  6. On Neptune and Uranus, Diamonds Rain Down from the Sky - AOL

    www.aol.com/neptune-uranus-diamonds-rain-down...

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  7. 55 Cancri b - Wikipedia

    en.wikipedia.org/wiki/55_Cancri_b

    55 Cancri b is in a short-period orbit, though not so extreme as that of the previously detected hot Jupiter 51 Pegasi b.The orbital period indicates that the planet is located close to a 1:3 mean motion resonance with 55 Cancri c, however investigations of the planetary parameters in a Newtonian simulation indicate that while the orbital periods are close to this ratio, the planets are not ...

  8. Scientists spot ‘glory effect’ on a world beyond our solar ...

    www.aol.com/rainbow-glory-spotted-hellishly-hot...

    The exoplanet closely orbits its host star, and the intense heat and radiation received from that sun-like star — more than 4,000 times the amount of radiation that Earth gets from our sun ...

  9. Exometeorology - Wikipedia

    en.wikipedia.org/wiki/Exometeorology

    The first exoplanet atmosphere ever observed was that of HD 209458b, a Hot Jupiter orbiting a G-type star similar in size and mass to our sun. Its atmosphere was discovered by spectroscopy; as the planet transited its star, its atmosphere absorbed some of the star's light according to the detectable absorption spectrum of sodium in the planet's atmosphere. [9]