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Sputnik Planitia information


Sputnik Planitia
New Horizons mosaic of the Sputnik Planitia basin
Feature typePlanitia, impact basin[1]
LocationTombaugh Regio, Pluto
Coordinates20°N 180°E / 20°N 180°E / 20; 180[2]
Diameter1492 km
~1300 km basin diameter[3]
Surface area~5 278 000 km2[a]
Dimensions1400 km × 1200 km[3][b]
DiscovererNew Horizons
EponymSputnik 1 satellite

Sputnik Planitia /ˈspʌtnɪk pləˈnɪʃiə, ˈspʊt-/ (formerly Sputnik Planum)[4] is a large, partially glaciated basin on Pluto. About 1,400 by 1,200 km (870 by 750 mi) in size,[3] Sputnik Planitia is partially submerged in large, bright glaciers of nitrogen ice. Named after Earth's first artificial satellite, Sputnik 1, it constitutes the western lobe of the heart-shaped Tombaugh Regio. Sputnik Planitia lies mostly in the northern hemisphere, but extends across the equator. Much of it has a surface of irregular polygons separated by troughs, interpreted as convection cells in the relatively soft nitrogen ice. The polygons average about 33 km (21 mi) across.[5] In some cases troughs are populated by blocky mountains or hills, or contain darker material.[6] There appear to be windstreaks on the surface with evidence of sublimation.[7][8] The dark streaks are a few kilometers long and all aligned in the same direction.[6] The planitia also contains pits apparently formed by sublimation.[6] No craters were detectable by New Horizons, implying a surface less than 10 million years old.[9] Modeling sublimation pit formation yields a surface age estimate of 180000+90000
−40000
years.[10] Near the northwest margin is a field of transverse dunes (perpendicular to the windstreaks), spaced about 0.4 to 1 km apart, that are thought to be composed of 200-300 μm diameter particles of methane ice derived from the nearby Al-Idrisi Montes.[11][12]

  1. ^ Cite error: The named reference LPSC2017McKinnon was invoked but never defined (see the help page).
  2. ^ "Sputnik Planitia". Gazetteer of Planetary Nomenclature. USGS Astrogeology Research Program.
  3. ^ a b c d Cite error: The named reference McGovern2021 was invoked but never defined (see the help page).
  4. ^ Cite error: The named reference DPS/EPSC update was invoked but never defined (see the help page).
  5. ^ Cite error: The named reference Pluto updates was invoked but never defined (see the help page).
  6. ^ a b c Cite error: The named reference fp was invoked but never defined (see the help page).
  7. ^ Cite error: The named reference JH-20150718 was invoked but never defined (see the help page).
  8. ^ Cite error: The named reference NASA-20150717-video was invoked but never defined (see the help page).
  9. ^ Cite error: The named reference Marchis2016 was invoked but never defined (see the help page).
  10. ^ Cite error: The named reference LPSC2017Buhler was invoked but never defined (see the help page).
  11. ^ Cite error: The named reference Telfer2018 was invoked but never defined (see the help page).
  12. ^ Cite error: The named reference Hayes2018 was invoked but never defined (see the help page).


Cite error: There are <ref group=lower-alpha> tags or {{efn}} templates on this page, but the references will not show without a {{reflist|group=lower-alpha}} template or {{notelist}} template (see the help page).

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Sputnik Planitia

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Sputnik Planitia /ˈspʌtnɪk pləˈnɪʃiə, ˈspʊt-/ (formerly Sputnik Planum) is a large, partially glaciated basin on Pluto. About 1,400 by 1,200 km (870 by...

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Pluto

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Western parts of Sputnik Planitia there are fields of transverse dunes formed by the winds blowing from the center of Sputnik Planitia in the direction...

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Tombaugh Regio

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the atmosphere from Sputnik Planitia, and then deposited as ice. Some of this nitrogen ice then returns to Sputnik Planitia via glacial flow. The region...

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Geology of Pluto

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activity. Geologic map of Sputnik Planitia and surroundings (context), with convection cell margins outlined in black Sputnik Planitia appears to be composed...

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Geography of Pluto

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of Sputnik Planitia near Al-Idrisi Montes, there are fields of transverse dunes formed by the winds, which blow from the center of Sputnik Planitia in...

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Wright Mons

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by the New Horizons spacecraft in 2015, it is located southwest of Sputnik Planitia within Hyecho Palus, adjacent to the Tenzing Montes and Belton Regio...

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Morgoth Macula

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the surface of Pluto, southwest of the Norgay Montes and adjacent to Sputnik Planitia. It was discovered in 2015 by the spacecraft New Horizons and named...

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Baret Montes

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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...

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List of largest craters in the Solar System

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2021). "Tectonism and Enhanced Cryovolcanic Potential Around a Loaded Sputnik Planitia Basin, Pluto". Journal of Geophysical Research: Planets. 126. Bibcode:2021JGRE...

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Cryovolcano

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eruption. Although Sputnik Planitia represents the youngest surface on Pluto, it is not a cryovolcanic structure; Sputnik Planitia continuously resurfaces...

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Belton Regio

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honoring astronomer Michael J. Belton. The macula lies west of the Sputnik Planitia region of Tombaugh Regio, also known as Pluto's "heart", and to the...

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Hillary Montes

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located northwest of Tenzing Montes in the southwest border area of Sputnik Planitia in the south of Tombaugh Regio (or the part of Tombaugh Regio south...

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Geology of Triton

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extent of Triton's volatile distribution (in strong contrast to Pluto's Sputnik Planitia ice sheet). However, the extent of Triton's polar caps may be significantly...

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Nitrogen

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Solid nitrogen on the plains of Sputnik Planitia (on the bottom-right side of the image) on Pluto next to water ice mountains (on the up-left side of the...

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Carbon monoxide

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"Primordial N2 provides a cosmo chemical explanation for the existence of Sputnik Planitia, Pluto". Icarus. 313: 79–92. arXiv:1805.09285. Bibcode:2018Icar..313...

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Tenzing Montes

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range of icy mountains on Pluto, bordering the southwest region of Sputnik Planitia and the nearby Hillary Montes and Wright Mons. With peaks reaching...

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Solid nitrogen

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Solid nitrogen on the plains of Sputnik Planitia on Pluto next to water ice mountains...

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Adlivun Cavus

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Adlivun Cavus is a small depression on the southern tip of Sputnik Planitia. It was discovered by the New Horizons spacecraft in 2015. The name is from...

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Challenger Colles

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Challenger Colles is a range of hills on Pluto near the eastern edge of Sputnik Planitia. Discovered by the New Horizons team in July 2015, It is named in honor...

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Coleta de Dados Colles

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Dados Colles are a cluster of hills ("colles") on the smooth plains of Sputnik Planitia on Pluto. The hills are over 100 km from the major mountain ranges...

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Percival Lowell

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Coleta de Dados Colles Hillary Montes Tenzing Montes Wright Mons Plains Sputnik Planitia Valleys and depressions Adlivun Cavus Lineae Luna Linea Craters Burney...

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Planetary science

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A geological map of the Sputnik Planitia basin on the dwarf planet Pluto. Analysis of planetary surfaces and surface features is a major component of planetary...

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Extraterrestrial sky

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– Tenzing Montes (left-foreground); Hillary Montes (left-skyline); Sputnik Planitia (right) Near-sunset view includes several layers of atmospheric haze...

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Lowell Observatory

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Coleta de Dados Colles Hillary Montes Tenzing Montes Wright Mons Plains Sputnik Planitia Valleys and depressions Adlivun Cavus Lineae Luna Linea Craters Burney...

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Tholin

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Close-up view of Sputnik Planitia on Pluto as viewed by the New Horizons spacecraft, showing nitrogen ice glaciers and reddish-colored tholins....

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Luna Linea

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impact event which created Sputnik Planitia, as seismic energy from the impact may have concentrated at Sputnik Planitia's antipode, fracturing Pluto's...

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