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  2. Neptune - Wikipedia

    en.wikipedia.org/wiki/Neptune

    Neptune was visited by Voyager 2, which flew by the planet on 25 August 1989; Voyager 2 remains the only spacecraft to have visited it. [ 22 ] [ 23 ] Like the gas giants ( Jupiter and Saturn ), Neptune's atmosphere is composed primarily of hydrogen and helium , along with traces of hydrocarbons and possibly nitrogen , but contains a higher ...

  3. Climate of Triton - Wikipedia

    en.wikipedia.org/wiki/Climate_of_Triton

    The mean surface pressure varies significantly with respect to Triton's seasons; by 1997, Triton's atmospheric surface pressure had risen to approximately 1.9 +0.18 −0.15 Pa [ 2 ] and the surface pressure may have reached a maximum of roughly 4 Pa by 2010 (though there were no direct measurements via occultation between 2007 and 2017).

  4. Geology of Triton - Wikipedia

    en.wikipedia.org/wiki/Geology_of_Triton

    The geology of Triton encompasses the physical characteristics of the surface, internal structure, and geological history of Neptune's largest moon Triton. With a mean density of 2.061 g/cm 3 , [ 1 ] Triton is roughly 15-35% water ice by mass; Triton is a differentiated body, with an icy solid crust atop a probable subsurface ocean and a rocky ...

  5. Mystery of why Neptune’s clouds have disappeared ... - AOL

    www.aol.com/mystery-why-neptune-clouds...

    Neptune has long been known to have white clouds circling it, but images of the furthest planet in the solar system have shown this changing over time - the most recent image, taken by the Hubble ...

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

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

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

  7. Triton (moon) - Wikipedia

    en.wikipedia.org/wiki/Triton_(moon)

    Based on the increase in atmospheric pressure between 1989 and 1997, it is estimated that by 2010 Triton's atmospheric pressure may have increased to as much as 4 Pa. [12] By 2017, however, Triton's atmospheric surface pressure had nearly returned to Voyager 2 levels; the cause for the rapid spike in atmospheric pressure between 1989 and 2017 ...

  8. List of Solar System objects by size - Wikipedia

    en.wikipedia.org/wiki/List_of_Solar_System...

    For the giant planets, the "radius" is defined as the distance from the center at which the atmosphere reaches 1 bar of atmospheric pressure. [11] Because Sedna and 2002 MS 4 have no known moons, directly determining their mass is impossible without sending a probe (estimated to be from 1.7x10 21 to 6.1×10 21 kg for Sedna [12]).

  9. Atmosphere of Triton - Wikipedia

    en.wikipedia.org/wiki/Atmosphere_of_Triton

    The surface pressure in the late 1990s is thought to have increased to at least 19 μbar [3] or, possibly, even to 40 μbar. [39] Other observations have shown an increase in temperature by 5% from 1989 to 1998. [13] One of the scientists involved in investigation of Triton, James L. Elliot, said: [13]