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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 .
A map of Pluto showing the names officially approved by the IAU as of 12 February 2025, along with many informal names in bold and italics. This is a list of named geological features on Pluto, identified by scientists working with data from the New Horizons spacecraft.
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.
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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]
Baret Montes is a chain of mountains on the surface of the dwarf planet Pluto. It is located near the western border of Sputnik Planitia in Tombaugh Regio. These mountains were first viewed by the New Horizons spacecraft. It features large ridges that are formed by the compression of methane and water ice. [1]
Pluto's far side as imaged by the New Horizons spacecraft on approach to Pluto. Luna Linea extends across the lower right. As Luna Linea was located on the opposite hemisphere (referred to as the far side or anti-encounter hemisphere) of Pluto when New Horizons was at closest approach, it was not imaged in detail.
Pages in category "Geography of Pluto" The following 16 pages are in this category, out of 16 total. This list may not reflect recent changes. ...
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