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  2. Geology of Pluto - Wikipedia

    en.wikipedia.org/wiki/Geology_of_Pluto

    The geology of Pluto consists of the characteristics of the surface, crust, and interior of Pluto. Because of Pluto's distance from Earth, in-depth study from Earth is difficult. Many details about Pluto remained unknown until 14 July 2015, when New Horizons flew through the Pluto system and began transmitting data back to Earth. [1]

  3. Pluto - Wikipedia

    en.wikipedia.org/wiki/Pluto

    Pluto (minor-planet designation: 134340 Pluto) is a dwarf planet in the Kuiper belt, a ring of bodies beyond the orbit of Neptune. It is the ninth-largest and tenth-most-massive known object to directly orbit the Sun. It is the largest known trans-Neptunian object by volume, by a small margin, but is less massive than Eris.

  4. List of geological features on Pluto - Wikipedia

    en.wikipedia.org/wiki/List_of_geological...

    A map of Pluto showing the names officially approved by the IAU as of 3 February 2021.. This is a list of named geological features on Pluto, identified by scientists working with data from the New Horizons spacecraft.

  5. Geography of Pluto - Wikipedia

    en.wikipedia.org/wiki/Geography_of_Pluto

    The geography of Pluto refers to the study and mapping of physical features across the dwarf planet Pluto. On 14 July 2015, the New Horizons spacecraft became the first spacecraft to fly by Pluto. [ 1 ] [ 2 ] During its brief flyby, New Horizons made detailed geographical measurements and observations of Pluto and its moons .

  6. Wright Mons - Wikipedia

    en.wikipedia.org/wiki/Wright_Mons

    An enhanced-color view of Pluto with Wright Mons's location marked. Wright Mons is located in Pluto's southern hemisphere [1] within the roughly 400 by 700 kilometer-wide (250 by 435 miles-wide) Hyecho Palus, a walled low-lying plain and one of the lowest-altitude regions on Pluto.

  7. Plutonism - Wikipedia

    en.wikipedia.org/wiki/Plutonism

    Plutonism is the geologic theory that the igneous rocks forming the Earth originated from intrusive magmatic activity, with a continuing gradual process of weathering and erosion wearing away rocks, which were then deposited on the sea bed, re-formed into layers of sedimentary rock by heat and pressure, and raised again.

  8. Tombaugh Regio - Wikipedia

    en.wikipedia.org/wiki/Tombaugh_Regio

    Tombaugh Regio (/ ˈ t ɒ m b aʊ ˈ r ɛ dʒ i oʊ /), sometimes nicknamed "Pluto's heart" after its shape, [2] is the largest bright surface feature of the dwarf planet Pluto. [ 3 ] [ 4 ] [ 5 ] It lies just north of Pluto's equator, to the northeast of Belton Regio and to the northwest of Safronov Regio , which are both dark features. [ 6 ]

  9. Moons of Pluto - Wikipedia

    en.wikipedia.org/wiki/Moons_of_Pluto

    Pluto's four small circumbinary moons orbit Pluto at two to four times the distance of Charon, ranging from Styx at 42,700 kilometres to Hydra at 64,800 kilometres from the barycenter of the system. They have nearly circular prograde orbits in the same orbital plane as Charon. All are much smaller than Charon.