Serenity Chasma

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Serenity Chasma
PIA20467(1).jpg
The side of Charon viewed by the passing New Horizons spacecraft in July 2015 shows a system of “pull apart” tectonic faults, which look like ridges, scarps and valleys—the latter sometimes reaching more than 4 miles (6.5 kilometers) deep. Courtesy New Horizons mission/JHU/APL
Feature typeTectonic fault
LocationPluto-facing side of Charon
Coordinates 19°N5°W / 19°N 5°W / 19; -5 [1]
Length>200 km
Width40–50 km
Depth5–7 km
Discoverer New Horizons
Eponym Serenity , a spaceship in the Firefly series

Serenity Chasma is the unofficial name given to a large pull-apart fault on Pluto's moon, Charon. [2] It is part of a series of faults that run along the perimeter of Vulcan Planum. It was discovered by the New Horizons mission, and informally named after the fictitious spaceship, Serenity .

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Geology

Serenity Chasma is over 200 km (120 mi) long, about 5–7 km (3.1–4.3 mi) deep, and its typical width is 40–50 km (25–31 mi). [3] The northern wall continues for an additional 200 km as a scarp after exiting the chasma. The chasma is part of a major tectonic belt, which involves a series of canyons, scarps, and troughs that traverse most of Charon's encounter hemisphere. The entire tectonic system, which also includes Mandjet Chasma, is one of the longest-known canyon systems in the Solar System. [2] [4] The morphology of Serenity Chasma resembles that of rift valleys, indicative of extentional tectonics. [3]

Serenity Chasma likely formed as Charon's subsurface ocean froze, leading to the expansion of Charon's interior and the creation of extensional tectonics. The episode of extension may have occurred between 1.7 to 2.5 billion years ago. This expansion pushed the Oz Terra region higher and produced the fault belt across Charon's equatorial region. [5] [2]

Five major landslide sites have been identified within Serenity Chasma, all bound by the largest cliffs of the chasm. In addition to the five most prominent landslides, numerous minor landslides too small for detailed observation have also been observed, primarily within impact craters and a small ridge inside Serenity Chasma. Of the five major landslides, all appear to be long-runout landslides, with the ratios between the landslide runout length (L) and drop height (H) between 3.2 and 6.8; terrestrial landslide typically have L/H ratios of ~2. The runout length of the five landslides varies between 15.7 to 24.6 km, with depositional thickness at the landslide toes in the hundreds of meters. The landslides provide insight into the properties of Charon's surface material; the frictional coefficient of the landslide material is rather low, ranging from 0.15 to 0.31, comparable to terrestrial debris flows, rock avelanches, and pyroclastic flows. [6]

See also

Related Research Articles

<span class="mw-page-title-main">Charon (moon)</span> Largest natural satellite of Pluto

Charon, known as (134340) Pluto I, is the largest of the five known natural satellites of the dwarf planet Pluto. It has a mean radius of 606 km (377 mi). Charon is the sixth-largest known trans-Neptunian object after Pluto, Eris, Haumea, Makemake, and Gonggong. It was discovered in 1978 at the United States Naval Observatory in Washington, D.C., using photographic plates taken at the United States Naval Observatory Flagstaff Station (NOFS).

<span class="mw-page-title-main">Rift valley</span> Linear lowland created by a tectonic rift or fault

A rift valley is a linear shaped lowland between several highlands or mountain ranges produced by the action of a geologic rift. Rifts are formed as a result of the pulling apart of the lithosphere due to extensional tectonics. The linear depression may subsequently be further deepened by the forces of erosion. More generally the valley is likely to be filled with sedimentary deposits derived from the rift flanks and the surrounding areas. In many cases rift lakes are formed. One of the best known examples of this process is the East African Rift. On Earth, rifts can occur at all elevations, from the sea floor to plateaus and mountain ranges in continental crust or in oceanic crust. They are often associated with a number of adjoining subsidiary or co-extensive valleys, which are typically considered part of the principal rift valley geologically.

<span class="mw-page-title-main">Cryovolcano</span> Type of volcano that erupts volatiles such as water, ammonia or methane, instead of molten rock

A cryovolcano is a type of volcano that erupts gases and volatile material such as liquid water, ammonia, and hydrocarbons. The erupted material is collectively referred to as cryolava; it originates from a reservoir of subsurface cryomagma. Cryovolcanic eruptions can take many forms, such as fissure and curtain eruptions, effusive cryolava flows, and large-scale resurfacing, and can vary greatly in output volumes. Immediately after an eruption, cryolava quickly freezes, constructing geological features and altering the surface.

<span class="mw-page-title-main">Moons of Pluto</span> Natural satellites orbiting Pluto

The dwarf planet Pluto has five natural satellites. In order of distance from Pluto, they are Charon, Styx, Nix, Kerberos, and Hydra. Charon, the largest, is mutually tidally locked with Pluto, and is massive enough that Pluto and Charon are sometimes considered a binary dwarf planet.

<span class="mw-page-title-main">Atmosphere of Pluto</span> Layer of gases surrounding the dwarf planet Pluto

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<span class="mw-page-title-main">Coprates Chasma</span> Chasma on Mars

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<span class="mw-page-title-main">Mordor Macula</span> North polar dark region on Charon

Mordor Macula is the informal name for a large dark area about 475 km in diameter near the north pole of Charon, Pluto's largest moon. It is named after the black land called Mordor in J.R.R. Tolkien's The Lord of the Rings.

<span class="mw-page-title-main">Geology of Charon</span> Geologic structure and composition of Charon

The geology of Charon encompasses the characteristics of the surface, crust, and interior of Pluto's moon Charon. Like the geology of Pluto, almost nothing was known of Charon's geology until the New Horizons of the Pluto system on 14 July 2015. Charon's diameter is 1,208 km (751 mi)—just over half that of Pluto. Charon is sufficiently massive to have collapsed into a spheroid under its own gravity.

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 of the Space Shuttle Challenger, which was destroyed with all seven crew lost on January 28, 1986. The name Challenger Colles was officially approved by the International Astronomical Union on May 27, 2022.

<span class="mw-page-title-main">Vulcan Planitia</span> Major plain on Charon

Vulcan Planitia, or Vulcan Planum, is the unofficial name given to a large plain on the southern hemisphere of Pluto's moon Charon. It discovered by New Horizons during its flyby of Pluto in July 2015. It is named after the fictional planet Vulcan in the science-fiction series Star Trek. The name is not approved by International Astronomical Union (IAU) as of 2024.

<span class="mw-page-title-main">Coleta de Dados Colles</span> Range of hills on Pluto

The Coleta de 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 to the west, and appear to be blocks of water ice floating in the denser nitrogen ice of Sputnik Planitia. The hills were informally named on July 28, 2015, by the research team of the New Horizons mission after the first Brazilian satellite, the Satélite de Coleta de Dados. The ridge's name has yet to be recognized officially by the IAU.

<span class="mw-page-title-main">Wright Mons</span> Mountain on Pluto

Wright Mons is a large, roughly circular mountain and likely cryovolcano on the dwarf planet Pluto. Discovered 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. A relatively young geological feature, Wright Mons has attracted attention as one of the most apparent examples of recent geological activity on Pluto and borders numerous other similarly young features. Numerous semi-regular hills surround and partially construct the flanks of Wright Mons. Their nature remains unexplained, with few, if any, direct analogs elsewhere in the Solar System.

<span class="mw-page-title-main">Burney (crater)</span> Multi-ring impact basin on Pluto

Burney, sometimes referred to as the Burney basin, is the second-largest known impact basin on the dwarf planet Pluto. With a diameter of over 290 kilometers and possibly up to 350 kilometers, it is the second-largest known impact basin on Pluto, after the Sputnik Planitia basin. Burney is the only impact basin with visible multiple rings known on Pluto and is thus classified as a multi-ringed impact basin, though its rings have been heavily eroded due to Burney's age.

<span class="mw-page-title-main">Oz Terra</span> Major region on Charon

Oz Terra is the unofficial name given to a major geological region on Charon. The Pluto-facing hemisphere of Charon is divided onto two primary regions; Oz Terra in the north and Vulcan Planum in the south. These regions are separated by a series of scarps near Charon's equator, particularly Serenity Chasma and Mandjet Chasma. The region was discovered by New Horizons during its flyby of Pluto in July 2015.

<span class="mw-page-title-main">Mandjet Chasma</span> Surface feature on the Plutonian moon Charon

Mandjet Chasma is a chasma on Pluto's moon Charon. Mandjet Chasma is 385 km (239 mi) long, and about 5–7 km (3.1–4.3 mi) deep with an average width of 30 km (19 mi). The chasma is part of a global tectonic belt: a series of canyons, scarps, and troughs that traverse the face of Charon along the northern edge of Vulcan Planitia. The feature was discovered using stereoscopic processing of New Horizons images.

<span class="mw-page-title-main">Dorothy (Charonian crater)</span> Largest crater on Charon

Dorothy is the largest known impact basin on Pluto's moon Charon. The crater was discovered by the New Horizons space probe in 2015 during its flyby of Pluto and its moons. It was named after Dorothy Gale from the novel The Wonderful Wizard of Oz. The crater is located near Charon's north pole, and overlaps the edge of Mordor Macula.

<span class="mw-page-title-main">Climate of Pluto</span> Types of climate on the dwarf planet Pluto

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<span class="mw-page-title-main">Caleuche Chasma</span> Major chasm on Charon

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<span class="mw-page-title-main">Leviathan Patera</span> Caldera on Triton

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<span class="mw-page-title-main">Tuonela Planitia</span> Walled plain on Triton

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References

  1. "USGS Astrogeology Science Center". astrogeology.usgs.gov. Retrieved 9 April 2020.
  2. 1 2 3 "Pluto's 'Hulk-like' Moon Charon: A Possible Ancient Ocean?". www.jpl.nasa.gov. 18 February 2016. Retrieved 9 April 2020.
  3. 1 2 Beyer, Ross A.; Nimmo, Francis; McKinnon, William B.; et al. (1 May 2017). "Charon tectonics". Icarus. 287: 161–174. Bibcode:2017Icar..287..161B. doi:10.1016/j.icarus.2016.12.018. PMC   5599803 . PMID   28919640.
  4. Moore, J. M.; McKinnon, W. B.; Spencer, J. R.; et al. (17 March 2016). "The geology of Pluto and Charon through the eyes of New Horizons". Science. 351 (6279): 1284–1293. arXiv: 1604.05702 . Bibcode:2016Sci...351.1284M. doi: 10.1126/science.aad7055 . PMID   26989245.
  5. Desch, S. J.; Neveu, M. (May 2017). "Differentiation and cryovolcanism on Charon: A view before and after New Horizons". Icarus. 287: 175–186. Bibcode:2017Icar..287..175D. doi:10.1016/j.icarus.2016.11.037.
  6. Beddingfield, Chloe B.; et al. (January 2020). "Landslides on Charon". Icarus. 335. Bibcode:2020Icar..33513383B. doi:10.1016/j.icarus.2019.07.017.