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• W2160213138 abstract "Research Article| May 01, 2004 Mechanical stratigraphy in the western equatorial region of Mars based on thrust fault–related fold topography and implications for near-surface volatile reservoirs Chris H. Okubo; Chris H. Okubo 1Geomechanics–Rock Fracture Group, Department of Geological Sciences, Mackay School of Earth Sciences and Engineering, University of Nevada, Reno, Nevada 89557-0138, USA Search for other works by this author on: GSW Google Scholar Richard A. Schultz Richard A. Schultz 1Geomechanics–Rock Fracture Group, Department of Geological Sciences, Mackay School of Earth Sciences and Engineering, University of Nevada, Reno, Nevada 89557-0138, USA Search for other works by this author on: GSW Google Scholar Author and Article Information Chris H. Okubo 1Geomechanics–Rock Fracture Group, Department of Geological Sciences, Mackay School of Earth Sciences and Engineering, University of Nevada, Reno, Nevada 89557-0138, USA Richard A. Schultz 1Geomechanics–Rock Fracture Group, Department of Geological Sciences, Mackay School of Earth Sciences and Engineering, University of Nevada, Reno, Nevada 89557-0138, USA Publisher: Geological Society of America Received: 24 Mar 2003 Revision Received: 06 Aug 2003 Accepted: 10 Sep 2003 First Online: 02 Mar 2017 Online ISSN: 1943-2674 Print ISSN: 0016-7606 Geological Society of America GSA Bulletin (2004) 116 (5-6): 594–605. https://doi.org/10.1130/B25361.1 Article history Received: 24 Mar 2003 Revision Received: 06 Aug 2003 Accepted: 10 Sep 2003 First Online: 02 Mar 2017 Cite View This Citation Add to Citation Manager Share Icon Share Facebook Twitter LinkedIn Email Permissions Search Site Citation Chris H. Okubo, Richard A. Schultz; Mechanical stratigraphy in the western equatorial region of Mars based on thrust fault–related fold topography and implications for near-surface volatile reservoirs. GSA Bulletin 2004;; 116 (5-6): 594–605. doi: https://doi.org/10.1130/B25361.1 Download citation file: Ris (Zotero) Refmanager EasyBib Bookends Mendeley Papers EndNote RefWorks BibTex toolbar search Search Dropdown Menu toolbar search search input Search input auto suggest filter your search All ContentBy SocietyGSA Bulletin Search Advanced Search Abstract Variations in lithology and pore-volatile pressure influence the distribution of layer and interface strength (mechanical stratigraphy) within the crust. In this paper, we show how mechanical stratigraphy can be inferred from the topography of thrust fault–related folds. A thrust fault propagating upward through mechanically well- stratified crust induces the nucleation of secondary backthrust faults. Because such backthrusts are not predicted (and do not occur) in mechanically homogeneous crust, the presence of backthrusts can be used to map variations in the mechanical strength of the crust (e.g., bedding planes, volatile- saturated reservoirs). Dip directions of faults indicate the presence of strength discontinuities within thrust-related folds. We show that the slopes of fault-related fold limbs are reliable indicators of fault-dip direction. We then apply this slope- asymmetry approach to thrust-related folds on Mars. We find that thrust-related folds that have secondary backthrusts are spatially correlated with a general lithologic sequence of lava flows overlying older impact ejecta and young lobate ejecta craters on the lava-flow surface—evidence of near- surface volatiles such as water ice. We demonstrate that secondary backthrusts within fault-related folds in the western equatorial region of Mars formed because of volatile- enhanced mechanical stratification of lava- flow and ejecta lithologic sequences. You do not have access to this content, please speak to your institutional administrator if you feel you should have access." @default.
• W2160213138 created "2016-06-24" @default.
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• W2160213138 date "2004-01-01" @default.
• W2160213138 modified "2023-10-13" @default.
• W2160213138 title "Mechanical stratigraphy in the western equatorial region of Mars based on thrust fault–related fold topography and implications for near-surface volatile reservoirs" @default.
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• W2160213138 doi "https://doi.org/10.1130/b25361.1" @default.
• W2160213138 hasPublicationYear "2004" @default.

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