Geomorphologic mapping of titan's polar terrains: Constraining surface processes and landscape evolution

被引:56
作者
Birch, S. P. D. [1 ]
Hayes, A. G. [1 ,2 ]
Dietrich, W. E. [3 ]
Howard, A. D. [4 ]
Bristow, C. S. [5 ]
Malaska, M. J. [6 ]
Moore, J. M. [7 ]
Mastrogiuseppe, M. [2 ]
Hofgartner, J. D. [2 ,6 ]
Williams, D. A. [8 ]
White, O. L.
Soderblom, J. M. [9 ]
Barnes, J. W. [10 ]
Turtle, E. P. [11 ]
Lunine, J. I. [2 ]
Wood, C. A. [12 ]
Neish, C. D. [13 ]
Kirk, R. L. [14 ]
Stofan, E. R. [15 ]
Lorenz, R. D. [11 ]
Lopes, R. M. C. [6 ]
机构
[1] Cornell Univ, Dept Earth & Atmospher Sci, Ithaca, NY 14853 USA
[2] Cornell Univ, Dept Astron, Ithaca, NY 14853 USA
[3] Univ Calif Berkeley, Dept Earth & Planetary Sci, Berkeley, CA 94720 USA
[4] Univ Virginia, Dept Environm Sci, Clark Hall, Charlottesville, VA 22903 USA
[5] Birkbeck Univ London, Dept Earth & Planetary Sci, London, England
[6] CALTECH, Jet Prop Lab, Pasadena, CA USA
[7] NASA Ames Res Facil, Div Space Sci, Moffett Field, CA USA
[8] Arizona State Univ, Sch Earth & Space Explorat, Tempe, AZ USA
[9] MIT, Dept Earth Atmospher & Planetary Sci, Boston, MA USA
[10] Univ Idaho, Dept Phys, Moscow, ID USA
[11] Johns Hopkins Univ, Appl Phys Lab, Laurel, MD USA
[12] Planetary Sci Inst Tucson, Tucson, AZ USA
[13] Univ Western Ontario, London, ON, Canada
[14] US Geol Survey, Astrogeol Div, Flagstaff, AZ 86001 USA
[15] UCL, Dept Earth & Planetary Sci, London WC1E 6BT, England
关键词
Titan; Geological processes; Titan hydrology; Titan surface; CASSINI RADAR; FLUVIAL EROSION; SALINITY CRISIS; SEAS; TOPOGRAPHY; LAKES; SHORELINES; EVAPORITES; MORPHOLOGY; FEATURES;
D O I
10.1016/j.icarus.2016.08.003
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We present a geomorphologic map of Titan's polar terrains. The map was generated from a combination of Cassini Synthetic Aperture Radar (SAR) and Imaging Science Subsystem imaging products, as well as altimetry, SARTopo and radargrammetry topographic datasets. In combining imagery with topographic data, our geomorphologic map reveals a stratigraphic sequence from which we infer process interactions between units. In mapping both polar regions with the same geomorphologic units, we conclude that processes that formed the terrains of the north polar region also acted to form the landscape we observe at the south. Uniform, SAR-dark plains are interpreted as sedimentary deposits, and are bounded by moderately dissected uplands. These plains contain the highest density of filled and empty lake depressions, and canyons. These units unconformably overlay a basement rock that outcrops as mountains and SARbright dissected terrains at various elevations across both poles. All these units are then superposed by surficial units that slope towards the seas, suggestive of subsequent overland transport of sediment. From estimates of the depths of the embedded empty depressions and canyons that drain into the seas, the SAR-dark plains must be >600 m thick in places, though the thickness may vary across the poles. At the lowest elevations of each polar region, there are large seas, which are currently liquid methane/ethane filled at the north and empty at the south. The large plains deposits and the surrounding hillslopes may represent remnant landforms that are a result of previously vast polar oceans, where larger liquid bodies may have allowed for a sustained accumulation of soluble and insoluble sediments, potentially forming layered sedimentary deposits. Coupled with vertical crustal movements, the resulting layers would be of varying solubilities and erosional resistances, allowing formation of the complex landscape that we observe today. (C) 2016 Elsevier Inc. All rights reserved.
引用
收藏
页码:214 / 236
页数:23
相关论文
共 94 条
[1]   An asymmetric distribution of lakes on Titan as a possible consequence of orbital forcing [J].
Aharonson, O. ;
Hayes, A. G. ;
Lunine, J. I. ;
Lorenz, R. D. ;
Allison, M. D. ;
Elachi, C. .
NATURE GEOSCIENCE, 2009, 2 (12) :851-854
[2]  
Aharonson O., 2013, CAMBRIDGE PLANETARY, P646
[3]   Titan's methane cycle [J].
Atreya, Sushil K. ;
Adams, Elena Y. ;
Niemann, Hasso B. ;
Demick-Montelara, Jaime E. ;
Owen, Tobias C. ;
Fulchignoni, Marcello ;
Ferri, Francesca ;
Wilson, Eric H. .
PLANETARY AND SPACE SCIENCE, 2006, 54 (12) :1177-1187
[4]   Near-infrared spectral mapping of Titan's mountains and channels [J].
Barnes, Jason W. ;
Radebaugh, Jani ;
Brown, Robert H. ;
Wall, Steve ;
Soderblom, Laurence ;
Lunine, Jonathan ;
Burr, Devon ;
Sotin, Christophe ;
Le Mouelic, Stephane ;
Rodriguez, Sebastien ;
Buratti, Bonnie J. ;
Clark, Roger ;
Baines, Kevin H. ;
Jaumann, Ralf ;
Nicholson, Phillip D. ;
Kirk, Randolph L. ;
Lopes, Rosaly ;
Lorenz, Ralph D. ;
Mitchell, Karl ;
Wood, Charles A. .
JOURNAL OF GEOPHYSICAL RESEARCH-PLANETS, 2007, 112 (E11)
[5]   Organic sedimentary deposits in Titan's dry lakebeds: Probable evaporite [J].
Barnes, Jason W. ;
Bow, Jacob ;
Schwartz, Jacob ;
Brown, Robert H. ;
Soderblom, Jason M. ;
Hayes, Alexander G. ;
Vixie, Graham ;
Le Mouelic, Stephane ;
Rodriguez, Sebastien ;
Sotin, Christophe ;
Jaumann, Ralf ;
Stephan, Katrin ;
Soderblom, Laurence A. ;
Clark, Roger N. ;
Buratti, Bonnie J. ;
Baines, Kevin H. ;
Nicholson, Philip D. .
ICARUS, 2011, 216 (01) :136-140
[6]   Alluvial Fan Morphology, distribution and formation on Titan [J].
Birch, S. P. D. ;
Hayes, A. G. ;
Howard, A. D. ;
Moore, J. M. ;
Radebaugh, J. .
ICARUS, 2016, 270 :238-247
[7]   Estimating erosional exhumation on Titan from drainage network morphology [J].
Black, Benjamin A. ;
Perron, J. Taylor ;
Burr, Devon M. ;
Drummond, Sarah A. .
JOURNAL OF GEOPHYSICAL RESEARCH-PLANETS, 2012, 117
[8]  
BLOOM AL, 1991, GEOMORPHOLOGY SYSTEM
[9]   The identification of liquid ethane in Titan's Ontario Lacus [J].
Brown, R. H. ;
Soderblom, L. A. ;
Soderblom, J. M. ;
Clark, R. N. ;
Jaumann, R. ;
Barnes, J. W. ;
Sotin, C. ;
Buratti, B. ;
Baines, K. H. ;
Nicholson, P. D. .
NATURE, 2008, 454 (7204) :607-610
[10]  
Brown R. H., 2006, EUR PLAN SCI C 2006, P602