Primary centers and secondary concentrations of tectonic activity through time in the western hemisphere of Mars

Five main stages of radial and concentric structures formed around Tharsis from the Noachian through the Amazonian as determined by geologic mapping of 24,452 structures within the stratigraphic framework of Mars and by testing their radial and concentric orientations. Tectonic activity peaked in the Noachian (stage 1) around the largest center, Claritas, an elongate center extending more than 20° in latitude and defined by about half of the total grabens which are concentrated in the Syria Planum, Thaumasia, and Tempe Terra regions. During the Late Noachian and Early Hesperian (stage 2), extensional structures formed along the length of present-day Valles Marineris and in Thaumasia (with a secondary concentration near Warrego Vallis) radial to a region just to the south of the central margin of Valles Marineris. Early Hesperian (stage 3) radial grabens in Pavonis, Syria, Ulysses, and Tempe Terra and somewhat concentric wrinkle ridges in Lunae and Solis Plana and in Thaumasia, Sirenum, Memnonia, and Amazonis are centered northwest of Syria with secondary centers at Thaumasia, Tempe Terra, Ulysses Fossae, and western Valles Marineris. Late Hesperian/Early Amazonian (stage 4) structures around Alba Patera, the northeast trending alignment of Tharsis Montes, and Olympus Mons appears centered on Alba Patera. Stage 5 structures (Middle-Late Amazonian) represent the last pulse of Tharsis-related activity and are found around the large shield volcanoes and are centered near Pavonis Mons. Tectonic activity around Tharsis began in the Noachian and generally decreased through geologic time to the Amazonian. Statistically significant radial distributions of structures formed during each stage, centered at different locations within the higher elevations of Tharsis. Secondary centers of radial structures during many of the stages appear related to previously identified local magmatic centers that formed at different times and locations throughout Tharsis.

[1]  Kenneth L. Tanaka,et al.  Reconciliation of stress and structural histories of the Tharsis region of Mars , 1991 .

[2]  Matthew P. Golombek,et al.  Tharsis province of Mars: Geologic sequence, geometry, and a deformation mechanism , 1979 .

[3]  J. Plescia,et al.  Tectonic history of the Tharsis Region, Mars , 1982 .

[4]  Kenneth L. Tanaka Tectonic history of the Alba Patera - Ceraunius Fossae region of Mars. , 1990 .

[5]  A. J. Beasley A computer program for printing geometrically accurate structural fabric diagrams , 1981 .

[6]  M. Golombek,et al.  Origin of planetary wrinkle ridges based on the study of terrestrial analogs , 1986 .

[7]  D. H. Scott,et al.  Faults and ridges - Historical development in Tempe Terra and Ulysses Patera regions of Mars , 1990 .

[8]  M. Davies The control net of Mars: May 1977 , 1978 .

[9]  J. Dohm,et al.  Magmatic-Tectonic Evolution of Tharsis , 2000 .

[10]  H. Frey Thaumasia: A fossilized early forming tharsis uplift , 1979 .

[11]  A. McEwen,et al.  The canyon system on Mars , 1992 .

[12]  S. Schumm Structural origin of large Martian channels , 1974 .

[13]  R. Schultz Multiple-process origin of Valles Marineris basins and troughs, Mars , 1998 .

[14]  Kenneth L. Tanaka,et al.  Geology of the Thaumasia region, Mars: plateau development, valley origins, and magmatic evolution , 1999 .

[15]  Kenneth L. Tanaka,et al.  Geologic maps of the Olympus Mons region of Mars , 1994 .

[16]  David E. Smith,et al.  The global topography of Mars and implications for surface evolution. , 1999, Science.

[17]  M. Carr Tectonism and volcanism of the Tharsis region of Mars , 1974 .

[18]  D. H. Scott,et al.  Tectonic Setting of Martian Volcanoes and Deep-seated Intrusives , 1991 .

[19]  W. B. Kamb,et al.  Ice petrofabric observations from Blue Glacier, Washington, in relation to theory and experiment , 1959 .

[20]  Richard M. Dudley,et al.  Statistical Tests for Preferred Orientation , 1975, The Journal of Geology.

[21]  Richard A. Schultz,et al.  Localization of bedding plane slip and backthrust faults above blind thrust faults: Keys to wrinkle ridge structure , 2000 .

[22]  E. Jowett,et al.  Statistical Significance of Clustered Orientation Data on the Sphere: An Empirical Derivation , 1988, The Journal of Geology.

[23]  M. Golombek,et al.  Martian tension fractures and the formation of grabens and collapse features at Valles Marineris , 1989 .

[24]  Pierre-Yves F. Robin,et al.  COMPUTERIZED DENSITY CONTOURING AND STATISTICAL EVALUATION OF ORIENTATION DATA USING COUNTING CIRCLES AND CONTINUOUS WEIGHTING FUNCTIONS , 1986 .

[25]  J. Pechmann,et al.  The origin of polygonal troughs on the northern plains of Mars , 1980 .

[26]  T. Watters Compressional tectonism on Mars , 1993 .

[27]  G. Mcgill The giant polygons of Utopia, northern Martian Plains , 1986 .

[28]  Thomas R. Watters,et al.  Orientation, relative age, and extent of the Tharsis Plateau ridge system. [volcanic and tectonic regions on Mars] , 1986 .

[29]  Daniel Mège,et al.  A plume tectonics model for the Tharsis province, Mars , 1996 .

[30]  Kenneth L. Tanaka,et al.  Topography of Closed Depressions, Scarps, and Grabens in the North Tharsis Region of Mars: Implications for Shallow Crustal Discontinuities and Graben Formation , 1995 .

[31]  F. Nimmo,et al.  The generation of martian floods by the melting of ground ice above dykes , 1999, Nature.

[32]  T. Watters Wrinkle ridge assemblages on the terrestrial planets , 1988 .

[33]  Daniel Mège,et al.  Amounts of crustal stretching in Valles Marineris, Mars , 1996 .

[34]  Kenneth L. Tanaka,et al.  Tectonic history of the Syria Planum province of Mars , 1988 .

[35]  Kenneth L. Tanaka The stratigraphy of Mars , 1986 .

[36]  A. Chicarro,et al.  Global and regional ridge patterns on Mars , 1984 .

[37]  D. H. Scott,et al.  Chronology and global distribution of fault and ridge systems on Mars , 1990 .

[38]  D. H. Scott,et al.  Geologic map of the Valles Marineris region, Mars , 1991 .

[39]  R. Anderson,et al.  Digital structural mapping of Mars , 1998 .

[40]  H. Masursky,et al.  Geology of the Valles Marineris: First analysis of imaging from the Viking 1 Orbiter Primary Mission , 1977 .