The Sedimentary Record of Mars
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A Comparative Study of the Mississippian Barnett Shale, Fort Worth Basin, and Devonian Marcellus Shale, Appalachian Basin
DOE/NETL-2011/1478 A Comparative Study of the Mississippian Barnett Shale, Fort Worth Basin, and Devonian Marcellus Shale, Appalachian Basin U.S. DEPARTMENT OF ENERGY DISCLAIMER This report was prepared as an account of work sponsored by an agency of the United States Government. Neither the United States Government nor any agency thereof, nor any of their employees, makes any warranty, expressed or implied, or assumes any legal liability or responsibility for the accuracy, completeness, or usefulness of any information, apparatus, product, or process disclosed, or represents that its use would not infringe upon privately owned rights. Reference herein to any specific commercial product, process, or service by trade name, trademark, manufacturer, or otherwise does not necessarily constitute or imply its endorsement, recommendation, or favoring by the United States Government or any agency thereof. The views and opinions of authors expressed herein do not necessarily state or reflect those of the United States Government or any agency thereof. ACKNOWLEDGMENTS The authors greatly thank Daniel J. Soeder (U.S. Department of Energy) who kindly reviewed the manuscript. His criticisms, suggestions, and support significantly improved the content, and we are deeply grateful. Cover. Top left: The Barnett Shale exposed on the Llano uplift near San Saba, Texas. Top right: The Marcellus Shale exposed in the Valley and Ridge Province near Keyser, West Virginia. Photographs by Kathy R. Bruner, U.S. Department of Energy (USDOE), National Energy Technology Laboratory (NETL). Bottom: Horizontal Marcellus Shale well in Greene County, Pennsylvania producing gas at 10 million cubic feet per day at about 3,000 pounds per square inch. -
EGU2015-6247, 2015 EGU General Assembly 2015 © Author(S) 2015
Geophysical Research Abstracts Vol. 17, EGU2015-6247, 2015 EGU General Assembly 2015 © Author(s) 2015. CC Attribution 3.0 License. From Kimberley to Pahrump_Hills: toward a working sedimentary model for Curiosity’s exploration of strata from Aeolis Palus to lower Mount Sharp in Gale crater Sanjeev Gupta (1), David Rubin (2), Katie Stack (3), John Grotzinger (4), Rebecca Williams (5), Lauren Edgar (6), Dawn Sumner (7), Melissa Rice (8), Kevin Lewis (9), Michelle Minitti (5), Juergen Schieber (10), Ken Edgett (11), Ashwin Vasawada (3), Marie McBride (11), Mike Malin (11), and the MSL Science Team (1) Imperial College London, London, United Kingdom ([email protected]), (2) UC, Santa Cruz, CA, USA, (3) Jet Propulsion Laboratory, Pasadena, CA, USA, (4) California Institute of Technology, Pasadena, CA, USA, (5) Planetary Science INstitute, Tucson, AZ, USA, (6) USGS, Flagstaff, AZ, USA, (7) UC, Davis, CA, USA, (8) Western Washington University, Bellingham, WA, USA, (9) Johns Hopkins University, Baltimore, Maryland, USA, (10) Indiana University, Bloomington, Indiana, USA, (11) Malin Space Science Systems, San Diego, CA, USA In September 2014, NASA’s Curiosity rover crossed the transition from sedimentary rocks of Aeolis Palus to those interpreted to be basal sedimentary rocks of lower Aeolis Mons (Mount Sharp) at the Pahrump Hills outcrop. This transition records a change from strata dominated by coarse clastic deposits comprising sandstones and conglomerate facies to a succession at Pahrump Hills that is dominantly fine-grained mudstones and siltstones with interstratified sandstone beds. Here we explore the sedimentary characteristics of the deposits, develop depositional models in the light of observed physical characteristics and develop a working stratigraphic model to explain stratal relationships. -
The Geology of the Lyndonville Area, Vermont
THE GEOLOGY OF THE LYNDONVILLE AREA, VERMONT By JOHN G. DENNIS VERMONT GEOLOGICAL SURVEY CHARLES G. DOLL, Stale Geologist Published by VERMONT DEVELOPMENT COMMISSION MONTPELIER, VERMONT BULLETIN NO. 8 1956 Lake Willoughby, seen from its north shore. TABLE OF CONTENTS ABSTRACT ......................... 7 INTRODUCTION 8 Location 8 Geologic Setting ..................... 8 Previous Work ...................... 8 Purpose of Study ..................... 9 Method of Study 10 Acknowledgments . 11 Physiography ...................... 11 STRATIGRAPHY ....................... 16 Lithologic Descriptions .................. 16 Waits River Formation ................. 16 General Statement .................. 16 Distribution ..................... 16 Age 17 Lithological Detail .................. 17 Gile Mountain Formation ................ 19 General Statement .................. 19 Distribution ..................... 20 Lithologic Detail ................... 20 The Waits River /Gile Mountain Contact ........ 22 Age........................... 23 Preliminary Remarks .................. 23 Early Work ...................... 23 Richardson's Work in Eastern Vermont .......... 25 Recent Detailed Mapping in the Waits River Formation. 26 Detailed Work in Canada ................ 28 Relationships in the Connecticut River Valley, Vermont and New Hampshire ................... 30 Summary of Presently Held Opinions ........... 32 Discussion ....................... 32 Conclusions ...................... 33 STRUCTURE 34 Introduction and Structural Setting 34 Terminology ...................... -
Outcrop Lithostratigraphy and Petrophysics of the Middle Devonian Marcellus Shale in West Virginia and Adjacent States
Graduate Theses, Dissertations, and Problem Reports 2011 Outcrop Lithostratigraphy and Petrophysics of the Middle Devonian Marcellus Shale in West Virginia and Adjacent States Margaret E. Walker-Milani West Virginia University Follow this and additional works at: https://researchrepository.wvu.edu/etd Recommended Citation Walker-Milani, Margaret E., "Outcrop Lithostratigraphy and Petrophysics of the Middle Devonian Marcellus Shale in West Virginia and Adjacent States" (2011). Graduate Theses, Dissertations, and Problem Reports. 3327. https://researchrepository.wvu.edu/etd/3327 This Thesis is protected by copyright and/or related rights. It has been brought to you by the The Research Repository @ WVU with permission from the rights-holder(s). You are free to use this Thesis in any way that is permitted by the copyright and related rights legislation that applies to your use. For other uses you must obtain permission from the rights-holder(s) directly, unless additional rights are indicated by a Creative Commons license in the record and/ or on the work itself. This Thesis has been accepted for inclusion in WVU Graduate Theses, Dissertations, and Problem Reports collection by an authorized administrator of The Research Repository @ WVU. For more information, please contact [email protected]. Outcrop Lithostratigraphy and Petrophysics of the Middle Devonian Marcellus Shale in West Virginia and Adjacent States Margaret E. Walker-Milani THESIS submitted to the College of Arts and Sciences at West Virginia University in partial fulfillment of the requirements for the degree of Master of Science in Geology Richard Smosna, Ph.D., Chair Timothy Carr, Ph.D. John Renton, Ph.D. Kathy Bruner, Ph.D. -
Assessment of the NASA Planetary Science Division's Mission
ASSESSMENT OF THE NASA PLANETARY SCIENCE DIVISION’S MISSION-ENABLING ACTIVITIES By Planetary Sciences Subcommittee of the NASA Advisory Council Science Committee 29 August 2011 i Planetary Science Subcommittee (PSS) Ronald Greeley, Chair Arizona State University Jim Bell Arizona State University Julie Castillo-Rogez Jet Propulsion Laboratory Thomas Cravens University of Kansas David Des Marais Ames Research Center John Grant Smithsonian NASM William Grundy Lowell Observatory Greg Herzog Rutgers University Jeffrey R. Johnson JHU Applied Physics Laboratory Sanjay Limaye University of Wisconsin William McKinnon Washington University Louise Prockter JHU Applied Physics Laboratory Anna-Louise Reysenbach Portland State University Jessica Sunshine University of Maryland Chip Shearer University of New Mexico James Slavin Goddard Space Flight Center Paul Steffes Georgia Institute of Technology Dawn Sumner University of California, Davis Mark Sykes Planetary Science Institute Meenakshi Wadhwa Arizona State University Michael New (through 2010) NASA Headquarters Executive Secretary Jonathan Rall (beginning 2011) NASA Headquarters Executive Secretary Sarah Noble (beginning 2011) Goddard Space Flight Center, Assistant Executive Secretary NASA Headquarters James Green, ex officio NASA Headquarters PSS Working Group for the assessment Mark Sykes, Co-Chair Sarah Noble Ronald Greeley, Co-Chair Jonathan Rall Jim Bell Dawn Sumner Julie Castillo-Rogez Meenakshi Wadhwa Thomas Cravens John Grant James Green, ex officio Sanjay Limaye ii Table of Contents Executive -
Plate Tectonics, Volcanic Petrology, and Ore Formation in the Santa Rosalia Area, Baja California, Mexico
Plate tectonics, volcanic petrology, and ore formation in the Santa Rosalia area, Baja California, Mexico Item Type text; Thesis-Reproduction (electronic) Authors Schmidt, Eugene Karl, 1947- Publisher The University of Arizona. Rights Copyright © is held by the author. Digital access to this material is made possible by the University Libraries, University of Arizona. Further transmission, reproduction or presentation (such as public display or performance) of protected items is prohibited except with permission of the author. Download date 01/10/2021 01:50:58 Link to Item http://hdl.handle.net/10150/555057 PLATE TECTONICS, VOLCANIC PETROLOGY, AND ORE FORMATION IN THE SANTA ROSALIA AREA, BAJA CALIFORNIA, MEXICO by Eugene Karl Schmidt A Thesis Submitted to the Faculty of the DEPARTMENT OF GEOSCIENCES In Partial Fulfillment of the Requirements For the Degree of MASTER OF SCIENCE In the Graduate College THE UNIVERSITY OF ARIZONA 1 9 7 5 z- STATEMENT BY AUTHOR This thesis has been submitted in partial ful fillment of requirements for an advanced degree at The University of Arizona and is deposited in the University Library to be made available to borrowers under rules of the Library. Brief quotations from this thesis are allowable without special permission, provided that accurate ac knowledgment of source is made. Requests for permission for extended quotation from or reproduction of this manu script in whole or in part may be granted by the head of the major department or the Dean of the Graduate College when in his judgment the proposed use of the material is in the interests of scholarship. In all other instances, however, permission must be obtained from the author. -
Sedimentology, Petrography, and Depositional Environment of Dore
SEDIMENTOLOGY, PETROGRAPHY, AND DEPOSITIONAL ENVIRONMENT OF DORE SEDIMENTS ABOVE THE HELEN-ELEANOR IRON RANGE, WAHA, ONTARIO ' SEDIMENTOLOGY, PETROGRAPHY, AND DEPOSITIONAL ENVIRONMENT OF DORE SEDIMENTS AHOVE THE HELEN-ELEANOR IRON RANGE, WAWA, ONTARIO By KATHRYN L. NEALE Submitted to the Department of Geology in Partial Fulfilment of the Requirements for the Degree Bachelor of Science McMaster University April, 1981 BACHELOR OF SCIENCE (1981) McMASTER UNIVERSITY (Geology) Hamilton, Ontario TITLE: Sedimentology, Petrography, and Depositional Environment of Dore Sediments above the Helen Eleanor Iron Range, Wawa, Ontario AUTHOR: Kathryn L. Neale SUPERVISOR: Dr. R. G. Walker NUMBER OF PAGES: ix, 54 ii ABSTRACT Archean sediments of the Dare group, located in the 1-Jawa green stone belt, were studied. The sediments are stratigraphically above the carbonate facies Helen-Eleanor secti on of the Michipicoten Iron Forma tion. A mafic volcanic unit, 90 m thick, lies between the iron range and the sediments. Four main facies have been i dentified in the first cycle of clastic sedimentation above the maf i c flow rocks. A 170 ro break in stratigraphy separates the volcanics from the first facies. The basal sedimentary facies is an unstratified and poorly sorted granule-cobble conglomerate, 200m thick, interpreted as an alluvial mass flow deposit. Above the conglomerate, there is a 20 m break in the stratigraphic column. The second facies, 220m to 415 m thick, consists of laminated (0.1- 2 em) argillites and siltstones, together with massive, thick bedded (8-10 m) greywackes. The argillites and siltstones are interpre ted as interchannel deposits on an upper submarine fan, and the grey wackes are explained as in-channel turbidity current deposition. -
The Stratigraphy and Evolution of Lower Mount Sharp from Spectral
PUBLICATIONS Journal of Geophysical Research: Planets RESEARCH ARTICLE The stratigraphy and evolution of lower Mount Sharp 10.1002/2016JE005095 from spectral, morphological, and thermophysical Key Points: orbital data sets • We have developed a stratigraphy for lower Mount Sharp using analyses of A. A. Fraeman1, B. L. Ehlmann1,2, R. E. Arvidson3, C. S. Edwards4,5, J. P. Grotzinger2, R. E. Milliken6, new spectral, thermophysical, and 2 7 morphologic orbital data products D. P. Quinn , and M. S. Rice • Siccar Point group records a period of 1 2 deposition and exhumation that Jet Propulsion Laboratory, California Institute of Technology, Pasadena, California, USA, Division of Geological and followed the deposition and Planetary Sciences, California Institute of Technology, Pasadena, California, USA, 3Department of Earth and Planetary exhumation of the Mount Sharp Sciences, Washington University in St. Louis, St. Louis, Missouri, USA, 4United States Geological Survey, Flagstaff, Arizona, group USA, 5Department of Physics and Astronomy, Northern Arizona University, Flagstaff, Arizona, USA, 6Department of Earth, • Late state silica enrichment and redox 7 interfaces within lower Mount Sharp Environmental and Planetary Sciences, Brown University, Providence, Rhode Island, USA, Geology Department, Physics were pervasive and widespread in and Astronomy Department, Western Washington University, Bellingham, Washington, USA space and/or in time Abstract We have developed a refined geologic map and stratigraphy for lower Mount Sharp using coordinated analyses of new spectral, thermophysical, and morphologic orbital data products. The Mount Correspondence to: A. A. Fraeman, Sharp group consists of seven relatively planar units delineated by differences in texture, mineralogy, and [email protected] thermophysical properties. -
Grain Size Variations in the Murray Formation
Grain Size Variations in the Murray Formation: Stratigraphic Evidence for Changing Depositional Environments in Gale Crater, Mars Frances Rivera-hernández, Dawn Sumner, Nicolas Mangold, Steven Banham, Kenneth Edgett, Christopher Fedo, Sanjeev Gupta, Samantha Gwizd, Ezat Heydari, Sylvestre Maurice, et al. To cite this version: Frances Rivera-hernández, Dawn Sumner, Nicolas Mangold, Steven Banham, Kenneth Edgett, et al.. Grain Size Variations in the Murray Formation: Stratigraphic Evidence for Changing Depositional Environments in Gale Crater, Mars. Journal of Geophysical Research. Planets, Wiley-Blackwell, 2020, 125 (2), pp.e2019JE006230. 10.1029/2019JE006230. hal-02933725 HAL Id: hal-02933725 https://hal.archives-ouvertes.fr/hal-02933725 Submitted on 14 Sep 2020 HAL is a multi-disciplinary open access L’archive ouverte pluridisciplinaire HAL, est archive for the deposit and dissemination of sci- destinée au dépôt et à la diffusion de documents entific research documents, whether they are pub- scientifiques de niveau recherche, publiés ou non, lished or not. The documents may come from émanant des établissements d’enseignement et de teaching and research institutions in France or recherche français ou étrangers, des laboratoires abroad, or from public or private research centers. publics ou privés. Rivera-Hernández Frances (Orcid ID: 0000-0003-1401-2259) Sumner Dawn, Y (Orcid ID: 0000-0002-7343-2061) Mangold Nicolas (Orcid ID: 0000-0002-0022-0631) Banham Steven (Orcid ID: 0000-0003-1206-1639) Edgett Kenneth, S. (Orcid ID: 0000-0001-7197-5751) Nachon Marion (Orcid ID: 0000-0003-0417-7076) Newsom Horton E., E (Orcid ID: 0000-0002-4358-8161) Stein Nathan (Orcid ID: 0000-0003-3385-9957) Wiens Roger, C. -
Sediment Transport in Distributary Channels and Its Export to the Pro-Deltaic Environment in a Tidally Dominated Delta: Fly River, Papua New Guinea
ARTICLE IN PRESS Continental Shelf Research 24 (2004) 2431–2454 www.elsevier.com/locate/csr Sediment transport in distributary channels and its export to the pro-deltaic environment in a tidally dominated delta: Fly River, Papua New Guinea Peter T. Harrisa,Ã, Michael G. Hughesb, Elaine K. Bakerb, Robert W. Dalrymplec, Jock B. Keeneb aMarine and Coastal Environment Group Geoscience Australia, GPO Box 378, Canberra, ACT 2601, Australia bSchool of Geosciences, University of Sydney, Sydney, NSW 2006, Australia cDepartment of Geological Sciences and Geological Engineering, Queens University, Kingston, Ontario, Canada K7L 3N6 Available online 11 November 2004 Abstract Current metre deployments, suspended sediment measurements and surface sediment samples were collected from three locations within distributary channels of the tidally dominated Fly River delta in southern Papua New Guinea. Net bedload transport vectors and the occurrence of elongate tidal bars indicate that mutually evasive ebb-and flood- dominant transport zones occur in each of the distributary channels. Suspended sediment experiments at two locations show a phase relationship between tidal velocity and sediment concentration such that the net suspended sediment flux is directed seaward. Processes that control the export of fluid muds with concentrations up to 10 g lÀ1 from the distributary channels across the delta front and onto the pro-delta are assessed in relation to the available data. Peak spring tidal current speeds (measured at 100 cm above the bed) drop off from around 100 cm sÀ1 within the distributary channels to o50 cm sÀ1 on the delta front. Gravity-driven, 2-m thick, fluid mud layers generated in the distributary channels are estimated to require at least 35 h to traverse the 20-km-wide, low-gradient (2 Â 10À3 degrees) delta front. -
Chapter 3 Sedimentary Rocks
Chapter 3 Sedimentary Rocks Rivers that flow into the Gulf of Mexico through Alabama and other Gulf Coast states are typically brown, yellow-orange or red in color due to the presence of fine particulate material suspended within the water column. This particulate material is called sediment, and it was produced through the erosion and weathering of rocks exposed far inland from the coast (including the Appalachian Mountains). Sediment transported by rivers eventually finds its way into a standing body of water. Sometimes this is a lake or an inland sea, but for those of us that reside in southern Alabama, it is almost always the Gulf of Mexico. When rivers enter standing bodies of water (e.g., the Gulf), the sediment load that they are carrying is dropped and deposition occurs. Usually deposition forms more or less parallel layers called strata. Given time, and the processes of compaction and cementation, the sediment may be lithified into sedimentary rock. It is important to note that deposition of sediment is not restricted to river mouths. It also occurs on floodplains surrounding rivers, on tidal flats, adjacent to mountains in alluvial fans, and in the deepest portions of the oceans. Sedimentation occurs everywhere and this is one of the reasons why your humble author finds sedimentary geology so fascinating. Sedimentary rocks comprise approximately 30% of all of the rocks exposed at the Earth's surface. Those that are composed of broken rock fragments formed during erosion of bedrock are termed siliciclastic sedimentary rocks (or clastic for short). Sedimentary rocks can also be produced through chemical and biochemical deposition. -
Regional Mapping and Reservoir Analysis of the Middle Devonian Marcellus Shale in the Appalachian Basin
Graduate Theses, Dissertations, and Problem Reports 2014 Regional Mapping and Reservoir Analysis of the Middle Devonian Marcellus Shale in the Appalachian Basin Jared VanMeter West Virginia University Follow this and additional works at: https://researchrepository.wvu.edu/etd Recommended Citation VanMeter, Jared, "Regional Mapping and Reservoir Analysis of the Middle Devonian Marcellus Shale in the Appalachian Basin" (2014). Graduate Theses, Dissertations, and Problem Reports. 634. https://researchrepository.wvu.edu/etd/634 This Thesis is protected by copyright and/or related rights. It has been brought to you by the The Research Repository @ WVU with permission from the rights-holder(s). You are free to use this Thesis in any way that is permitted by the copyright and related rights legislation that applies to your use. For other uses you must obtain permission from the rights-holder(s) directly, unless additional rights are indicated by a Creative Commons license in the record and/ or on the work itself. This Thesis has been accepted for inclusion in WVU Graduate Theses, Dissertations, and Problem Reports collection by an authorized administrator of The Research Repository @ WVU. For more information, please contact [email protected]. Regional Mapping and Reservoir Analysis of the Middle Devonian Marcellus Shale in the Appalachian Basin Jared VanMeter Thesis submitted to the Eberly College of Arts and Sciences at West Virginia University in partial fulfillment of the requirements for the degree of Master of Science in Geology Richard Smosna, Ph.D., Chair Kathy Bruner, Ph.D. Tim Carr, Ph.D. Department of Geology and Geography Morgantown, West Virginia 2013 Keywords: Marcellus, Petroleum, Sequence Stratigraphy Copyright 2014 Jared VanMeter ABSTRACT Regional Mapping and Reservoir Analysis of the Middle Devonian Marcellus Shale in the Appalachian Basin Jared VanMeter The main purpose of this investigation is to define the distribution of organic-rich facies of the Middle Devonian Marcellus Shale in New York, Ohio, Pennsylvania, and West Virginia.