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Thaumasia Highlands

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Series: Geological Society, London, Special Publications, Geological Society, London, Special Publications
Published: 01 January 2011
DOI: 10.1144/SP356.5
EISBN: 9781862396043
... Abstract Possible periglacial and relict glacial landforms in the ancient mountain range of the Thaumasia Highlands, Mars, are described. The landforms include large-scale mantling, lineated crater and valley-fill materials, debris aprons, protalus lobes and ramparts. The most pristine ice...
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Image
Shaded-relief map of the <b>Thaumasia</b> <b>Highlands</b> (Thermal Emission Imaging Syst...
Published: 01 January 2009
Figure 3. Shaded-relief map of the Thaumasia Highlands (Thermal Emission Imaging System infrared [THEMIS IR] base) showing the distribution of normal faults (yellow) and thrust faults (thin red), trace of frontal anticlinal (thick red), and truncated craters along the southern edge
Journal Article
Journal: GSA Bulletin
Published: 01 January 2009
GSA Bulletin (2009) 121 (1-2): 117–133.
...Figure 3. Shaded-relief map of the Thaumasia Highlands (Thermal Emission Imaging System infrared [THEMIS IR] base) showing the distribution of normal faults (yellow) and thrust faults (thin red), trace of frontal anticlinal (thick red), and truncated craters along the southern edge...
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Image
Longitudinal profiles across <b>Thaumasia</b> Plateau through Solis Planum (locati...
Published: 01 January 2009
Figure 10. Longitudinal profiles across Thaumasia Plateau through Solis Planum (locations shown in Fig. 1 ). Vertical exaggeration is 100:1. Shaded area is the “excess area” of the Coprates Rise–Thaumasia Highlands projecting above the regional elevation trend. Dots mark locations of craters
Journal Article
Journal: Lithosphere
Publisher: GSW
Published: 01 December 2012
Lithosphere (2012) 4 (6): 553–593.
... morphology ( Fig. 2A ). Scott and Tanaka (1986) and Skinner et al. (2006) recognized the following geologic units across the Tharsis rise: (1) heavily cratered and highly fractured Early Noachian basement (Nf) that is exposed at Thaumasia Highlands, Coprates rise, Clarita Fossae, Ceraunius Fossae...
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Image
(A) Detailed topographic relationship between the exposed dichotomy boundar...
Published: 01 December 2012
between the plateau region of the southern highlands and the floor of the northern lowland basin. Note that the area between the Thaumasia Plateau and the Argyre impact structure is much higher that the transitional zone, which was probably created by the oblique (northwestward) Argyre impact. See text
Journal Article
Journal: Geology
Published: 21 December 2020
Geology (2021) 49 (5): 504–509.
.... Fluvial ridges are most common in the lower extents of the southern highlands ( Fig. 3 ). The Argyre region has ridges downslope from the Thaumasia-Warrego valley networks. Fluvial ridges were observed in the Hellas region, though they occur sparsely. Two fluvial ridge systems were found within the Isidis...
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Journal Article
Journal: Lithosphere
Publisher: GSW
Published: 01 August 2012
Lithosphere (2012) 4 (4): 286–330.
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Journal Article
Journal: Geology
Published: 01 February 2010
Geology (2010) 38 (2): 183–186.
... smoothing radii do not affect the outcome of the cluster analysis significantly; see footnote 1 .) Province 1 is relatively low in all five elements, although only Fe is low at the 1σ level. The largest region of it encompasses the southern highlands from Terra Sirenum through Aonia Terra to western...
FIGURES
Journal Article
Journal: GSA Bulletin
Published: 01 May 2004
GSA Bulletin (2004) 116 (5-6): 594–605.
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Journal Article
Journal: GSA Bulletin
Published: 01 July 2011
GSA Bulletin (2011) 123 (7-8): 1596–1627.
... are a strikingly linear set of trenches trending east-southeast along the north rim of the Thaumasia Plateau in equatorial Mars ( Fig. 1A ). Among the northern chasmata is Hebes Chasma, a cavity 315 km long and 126 km wide. The chasma is more than 8 km deep from its rim at +3950 m to its floor at −4530 m...
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Journal Article
Journal: GSA Bulletin
Published: 01 May 2006
GSA Bulletin (2006) 118 (5-6): 557–566.
... evidence supported that interpretation. The evidence included the concave to flat transition of feeder valleys from the highlands to the fan proper, the low declivity of the fan surface versus the steep fanmargin profiles, the multilobate form and avulsive nature of the lobes, and the proximity of the fan...
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Series: Geological Society, London, Special Publications, Geological Society, London, Special Publications
Published: 01 January 2011
DOI: 10.1144/SP356.1
EISBN: 9781862396043
... the evolution of lobate debris aprons in the northern mid-latitude Tempe Terra region. These landforms are thought to have formed by creep of rock–ice mixtures. In Chapter 5 Rossi et al . find evidence for a suite of glacial and periglacial landforms in the southern mid-latitude Thaumasia Highlands...
Journal Article
Journal: GSA Bulletin
Published: 28 November 2018
GSA Bulletin (2019) 131 (5-6): 782–802.
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Series: Geological Society, London, Special Publications, Geological Society, London, Special Publications
Published: 01 January 2015
DOI: 10.1144/SP401.22
EISBN: 9781862396777
..., Pavonis and Ascraeus), steep-sided domes (e.g. Tharsis Tholus) and highland paterae (e.g. Tyrrhenus and Hadriacus Montes) (Fig. 8 ) – the latter being the only large-scale volcanic landforms attesting to explosive volcanism in early Mars history (Fig. 8 ). Extensive volcanic plains associated with large...
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Series: SEPM Special Publication, SEPM Special Publication
Published: 01 January 2012
DOI: 10.2110/pec.12.102.0001
EISBN: 9781565763135
... by physical weathering. As the flux of impactors and volcanism declined, and as the planet’s hydrologic cycle decreased in vigor, the formation of sedimentary rocks also declined. Today the Martian highlands appear to be in a net state of erosion, and outcrops of sedimentary rocks are exposed as a result...
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