Definition
A type of landscape similar to karst.
Interpretation
The presence of exo-, endo-, and paleokarst indicates that liquid water, as solvent, and carbonate or evaporite rocks, as solutes, were available in the geologic past of the area where these karst landforms occur. If dissolution in the presence of liquid water does not seem plausible (such as in the case of Saturn’s moon, Titan), the presence of karst-like features may indicate dissolution chemistries involving other types of solutes and solvents.
Composition
On Mars, karst landforms have been proposed to occur in evaporite outcrops on the eastern Tithonium dome (ETD) and in other regions of the Valles Marineris (Baioni and Wezel 2008; Baioni et al. 2009; Wezel and Baioni 2010a, b; Baioni and Sgavetti 2012). The presence of kieserite deposits (magnesium sulfate) in these regions was confirmed by data supplied by the OMEGA spectrometer aboard the Mars Express and the Mars Exploration Rovers (Gendrin et al. 2005). Several...
References
Baioni D, Sgavetti M (2012) Karst terrains as possible lithologic and stratigraphic markers in northern Sinus Meridiani, Mars. Planet Space Sci. doi:10.1016/j.pss.2012.08.011
Baioni D, Wezel FC (2008) Similarities of a Martian dome with terrestrial salt domes. Boll Soc Geol It (Ital J Geosci) 127(3):453–465
Baioni D, Hajna NZ, Wezel FC (2009) Karst landforms in a Martian evaporitic dome Kraške oblike površja na marsovi evaporitni domi. Acta Carsologica 1(10):38
Cornet T, Bourgeois O, Le Mouelic S, Rodriguez S, Sotin C, Lefevre A, Barnes JW, Brown RH, Baines KH, Buratti BJ, Clark RN, Nicholson PD (2012) Shaping Titan’s landscapes by dissolution and evaporation: the case of Ontario Lacus, a high-latitude semi-arid karst-playa land system. 43rd Lunar Planet Sci Conf, Houston
Gendrin A, Mangold N, Bibring J-P, Langevin Y, Gondet B, Poulet F, Bonello G, Quantin C, Mustard J, Arvidson R, LeMouélic S (2005) Sulfates in Martian Layered Terrains: The OMEGA/Mars Express View. Science 307:1587–1591
Ford DC, Williams PW (2007) Karst hydrogeology and geomorphology. John Wiley & Sons, Ltd
Graves SDB, McKay CP, Griffith CA, Ferri F, Fulchignoni M (2008) Rain and hail can reach the surface of Titan. Planet Space Sci 56:346–357
Grotzinger JP, Hayes AG, Lamb MP, McLennan SM (2014) Sedimentary processes on Earth, Mars, Titan, and Venus. In: Mackwell SJ et al (eds) Comparative climatology of terrestrial planets. University of Arizona, Tucson, pp 439–472
Harrison KP (2012) Thermokarst processes in Titan’s lakes: comparison with terrestrial data. Presented at the 43rd Lunar Planet Sci Conf, abstract #2271, Houston
Hayes AG, Aharonson O, Callahan P, Elachi C, Gim Y, Kirk R, Lewis K, Lopes R, Lorenz R, Lunine J, Mitchell K, Mitri G, Stofan E, S. Wall (2008) Hydrocarbon lakes on Titan: Distribution and interaction with an isotropic porous regolith. Geophys Res Lett 35:L09204
Hayes AG, Dietrich WE, Kirk RL, Turtle EP, Barnes JW, Lucas A, Aharonson O, Mitchell KL (2013) Morphologic analysis of Polar landscape evolution on Titan. LPI Contrib 1719:2000
Kargel JS, Furfaro R, Hays CC, Lopes RMC, Lunine JI, Mitchell KL, Wall SD, Cassini RADAR Team (2007) Titan’s GOO-sphere: glacial, permafrost, evaporite, and other familiar processes involving exotic materials. Lunar Planet Inst Sci Conf Abstr 38:1992
Lorenz RD, Lunine JI (1996) Erosion on Titan: past and present. Icarus 122:79–91
Lorenz RD, Lunine JI (2005) Titan’s surface before Cassini. Planet Space Sci 53:557–576
Lunine JI, Atreya S (2008) The methane cycle on Titan. Nat Geosci 1:159–164
Malaska M, Radebaugh J, Lorenz R, Mitchell K, Farr T, Stofan E (2010) Identification of karst-like terrain on Titan from valley analysis. Lunar Planet Inst Sci Conf Abstr 41:1544
Malaska M, Radebaugh J, Mitchell KL, Lopes R, Wall S, Lorenz R (2011). Surface dissolution model for Titan Karst. First international planetary cave research workshop, #8018. LPI Contributions, 1640, p 15
Mitchell KL, Malaska M (2011) Karst on Titan. In: First international planetary caves workshop: implications for astrobiology, climate, detection, and exploration. LPI Contribution No. 1640. Lunar and Planetary Institute, Houston, p 15
Mitchell KL, Kargel JS, Wood CA, Radebaugh J, Lopes RMC, Lunine JI, Stofan ER, Kirk RL, Cassini Radar Team (2007) Titan’s crater lakes: Caldera vs. Karst. Lunar Planet Inst Sci Conf Abstr 38:2064
Stafford KW, Boston PJ (2005) Theoretical evaporite karst development on Mars. Lunar Planet Sci 36:2291
Stofan ER, Elachi C, Lunine JI, Lorenz RD, Stiles B, Mitchell KL et al (2007) The lakes of Titan. Nature 445(7123):61–64
Wezel FC, Baioni D (2010a) Morphology and origin of an evaporitic dome in the Eastern Tithonium Chasma, Mars. Planet Space Sci 58(5):847–857
Wezel FC, Baioni D (2010b) Evidence for subaqueously resedimented sulphate evaporites on Mars. Planet Space Sci 58(11):1500–1505
Wood CA, Mitchell KL, Lopes RMC, Radebaugh J, Stoffan E, Lunine J (2007) Volcanic calderas in the north polar region of Titan. Lunar Planet Inst Sci Conf Abstr 38:1454
Wood CA, Lorenz R, Kirk R, Lopes R, Mitchell K, Stofan E (2010) Impact craters on Titan. Icarus 206(1):334–344
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Chirienco, M. (2014). Karst-Like Landforms. In: Encyclopedia of Planetary Landforms. Springer, New York, NY. https://doi.org/10.1007/978-1-4614-9213-9_630-1
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DOI: https://doi.org/10.1007/978-1-4614-9213-9_630-1
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