2012
DOI: 10.1130/b30612.1
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Fluvial features on Titan: Insights from morphology and modeling

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Cited by 105 publications
(80 citation statements)
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References 167 publications
(243 reference statements)
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“…Thus, for fully turbulent and hydraulically rough flows, flow velocity is independent of the Reynolds number and fluid viscosity. This makes laboratory experiments using water flows also applicable to different gravities and rivers of more exotic fluids, such as brines on Mars (Lamb et al, 2012;Grotzinger et al, 2013) or methane rivers on Titan Burr et al, 2013), as long as they are also Reynolds-number independent. Most bedrock erosion experiments to date have been conducted in the turbulent regime (Fig.…”
Section: Accepted Manuscriptmentioning
confidence: 98%
See 1 more Smart Citation
“…Thus, for fully turbulent and hydraulically rough flows, flow velocity is independent of the Reynolds number and fluid viscosity. This makes laboratory experiments using water flows also applicable to different gravities and rivers of more exotic fluids, such as brines on Mars (Lamb et al, 2012;Grotzinger et al, 2013) or methane rivers on Titan Burr et al, 2013), as long as they are also Reynolds-number independent. Most bedrock erosion experiments to date have been conducted in the turbulent regime (Fig.…”
Section: Accepted Manuscriptmentioning
confidence: 98%
“…To investigate the role of flaw size, Beyeler and Sklar (2010) measured crystal and clast size (D c ) in thin sections of disks eroded by Sklar and Dietrich (2001) and found that grain size, together with porosity (p), explained a large fraction of the scatter in the fit between erosion rate and tensile strength present There, where surface temperature is ~90 K, channels may be actively incising into Titan's waterice bedrock by flows of liquid methane carrying water-ice clasts as bedload (Collins, 2005;Perron et al, 2006;Burr et al, 2013). To extend rock erosion resistance scaling to ultracold ice, Litwin et al (2012) volumetric erosion rates of ultracold ice subjected to particle impacts and found that the impact energy required to erode a unit volume of ice was roughly equal to that measured by Sklar and Dietrich (2004) for natural rock of similar tensile strength.…”
Section: Accepted Manuscriptmentioning
confidence: 98%
“…This makes Titan and Earth the only worlds in the Solar System with stable liquids on their surfaces. On Titan's surface, channels and fluvial valley networks have been identified both by Cassini, as well as by the Huygens descent probe (Burr et al, 2013;Langhans et al, 2012;Jaumann et al, 2008). Cassini spacecraft instruments, including both the ISS and VIMS instruments, have observed storms and transient surface albedo changes resulting from precipitation Turtle et al, 2011Turtle et al, , 2009).…”
Section: Introductionmentioning
confidence: 97%
“…In this way, catchment power could help explain how topography mediates the linkage between climate and tectonics. Catchment power could also be used to compare numerical simulations of landscape evolution with real landscapes (Willgoose, 1994;Willgoose et al, 2003) and contrast terrestrial catchments with catchments on Mars or Titan, where the topography reflects differing gravitational accelerations, fluids, and rock properties (Mest et al, 2010;Burr et al, 2012).…”
Section: Future Research Opportunitiesmentioning
confidence: 99%