'Decameter-Scale Rimmed Depressions' in Utopia Planitia" (2018)
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PDF (Chapter5 Doubleside.Pdf)
202 Chapter 5 FUTURE WORK There is more work is planned for these projects. Some of the proposed future work fell out of the questions and problems that arise while first attempting to solve a problem. Some of it was originally intended to be encompassed in the thesis work, but work at an earlier stage grew to dominate the project as a result of the sheer volume of data available. Many questions were left unanswered in the work described in Chapter 4. It is not clear why the MM5 does not predict the secondary winds that clearly must exist in the current wind regime. These winds do not appear in GFDL GCM model runs, and they may not exist in any current atmospheric model. It is possible that they are produced by rare storms (i.e., storms that occur once a decade or century), and I would like to look into the possibility of observing or predicting these storms. The MM5 also does not predict winds strong enough to lift basaltic grains into saltation. This may simply be a problem of model resolution, and it is not a difficult prospect to run the model at a higher resolution and/or to output the strongest hourly winds at each grid point rather than the winds at the top of each hour. There is also the problem that the MM5 is meant to hold subgrids that are no more than three times smaller than their parent grids – and yet our model runs at a scale of 10 km were more than an order of magnitude higher resolution than the parent grid. -
Imaginative Geographies of Mars: the Science and Significance of the Red Planet, 1877 - 1910
Copyright by Kristina Maria Doyle Lane 2006 The Dissertation Committee for Kristina Maria Doyle Lane Certifies that this is the approved version of the following dissertation: IMAGINATIVE GEOGRAPHIES OF MARS: THE SCIENCE AND SIGNIFICANCE OF THE RED PLANET, 1877 - 1910 Committee: Ian R. Manners, Supervisor Kelley A. Crews-Meyer Diana K. Davis Roger Hart Steven D. Hoelscher Imaginative Geographies of Mars: The Science and Significance of the Red Planet, 1877 - 1910 by Kristina Maria Doyle Lane, B.A.; M.S.C.R.P. Dissertation Presented to the Faculty of the Graduate School of The University of Texas at Austin in Partial Fulfillment of the Requirements for the Degree of Doctor of Philosophy The University of Texas at Austin August 2006 Dedication This dissertation is dedicated to Magdalena Maria Kost, who probably never would have understood why it had to be written and certainly would not have wanted to read it, but who would have been very proud nonetheless. Acknowledgments This dissertation would have been impossible without the assistance of many extremely capable and accommodating professionals. For patiently guiding me in the early research phases and then responding to countless followup email messages, I would like to thank Antoinette Beiser and Marty Hecht of the Lowell Observatory Library and Archives at Flagstaff. For introducing me to the many treasures held deep underground in our nation’s capital, I would like to thank Pam VanEe and Ed Redmond of the Geography and Map Division of the Library of Congress in Washington, D.C. For welcoming me during two brief but productive visits to the most beautiful library I have seen, I thank Brenda Corbin and Gregory Shelton of the U.S. -
MID-LATITUDE MARTIAN ICE AS a TARGET for HUMAN EXPLORATION, ASTROBIOLOGY, and IN-SITU RESOURCE UTILIZATION. D. Viola1 ([email protected]), A
First Landing Site/Exploration Zone Workshop for Human Missions to the Surface of Mars (2015) 1011.pdf MID-LATITUDE MARTIAN ICE AS A TARGET FOR HUMAN EXPLORATION, ASTROBIOLOGY, AND IN-SITU RESOURCE UTILIZATION. D. Viola1 ([email protected]), A. S. McEwen1, and C. M. Dundas2. 1University of Arizona, Department of Planetary Sciences, 2USGS, Astrogeology Science Center. Introduction: Future human missions to Mars will region of late Noachian highlands terrain, and is com- need to rely on resources available near the Martian prised of a series of grabens and ridges surrounded by surface. Water is of primary importance, and is known later Hesperian/Amazonian lava flows from the Thar- to be abundant on Mars in multiple forms, including sis region [7]. The proposed landing site is within these hydrated minerals [1] and pore-filling and excess ice lava flows (HAv), and provides access to a region of deposits [2]. Of these sources, excess ice (or ice which late Hesperian lowlands in the western region of the exceeds the available regolith pore space) may be the EZ. There is evidence for Amazonian glacial and peri- most promising for in-situ resource utilization (ISRU). glacial activity [e.g., HiRISE images Since Martian excess ice is thought to contain a low PSP_008671_2210 and ESP_017374_2210], and the fraction of dust and other contaminants (~<10% by Gamma Ray Spectrometer water map suggests that volume, [3]) only a modest deposit of excess ice will there is abundant subsurface ice in the uppermost me- be sufficient to support a human presence. ter within this region [10]. Meandering channel-like Subsurface water ice may also be of astrobiological features have been identified in HiRISE images (e.g., interest as a potential current habitat or as a preserva- PSP_003529_2195 in close proximity to apparent ice tion medium for biosignatures. -
Mars Reconnaissance Orbiter
Chapter 6 Mars Reconnaissance Orbiter Jim Taylor, Dennis K. Lee, and Shervin Shambayati 6.1 Mission Overview The Mars Reconnaissance Orbiter (MRO) [1, 2] has a suite of instruments making observations at Mars, and it provides data-relay services for Mars landers and rovers. MRO was launched on August 12, 2005. The orbiter successfully went into orbit around Mars on March 10, 2006 and began reducing its orbit altitude and circularizing the orbit in preparation for the science mission. The orbit changing was accomplished through a process called aerobraking, in preparation for the “science mission” starting in November 2006, followed by the “relay mission” starting in November 2008. MRO participated in the Mars Science Laboratory touchdown and surface mission that began in August 2012 (Chapter 7). MRO communications has operated in three different frequency bands: 1) Most telecom in both directions has been with the Deep Space Network (DSN) at X-band (~8 GHz), and this band will continue to provide operational commanding, telemetry transmission, and radiometric tracking. 2) During cruise, the functional characteristics of a separate Ka-band (~32 GHz) downlink system were verified in preparation for an operational demonstration during orbit operations. After a Ka-band hardware anomaly in cruise, the project has elected not to initiate the originally planned operational demonstration (with yet-to-be used redundant Ka-band hardware). 201 202 Chapter 6 3) A new-generation ultra-high frequency (UHF) (~400 MHz) system was verified with the Mars Exploration Rovers in preparation for the successful relay communications with the Phoenix lander in 2008 and the later Mars Science Laboratory relay operations. -
Quantitative High-Resolution Reexamination of a Hypothesized
RESEARCH ARTICLE Quantitative High‐Resolution Reexamination of a 10.1029/2018JE005837 Hypothesized Ocean Shoreline in Cydonia Key Points: • We apply a proposed Mensae on Mars ‐ fi paleoshoreline identi cation toolkit Steven F. Sholes1,2 , David R. Montgomery1, and David C. Catling1,2 to newer high‐resolution data of an exemplar site for paleoshorelines on 1Department of Earth and Space Sciences, University of Washington, Seattle, WA, USA, 2Astrobiology Program, Mars • Any wave‐generated University of Washington, Seattle, WA, USA paleoshorelines should exhibit expressions identifiable in the residual topography from an Abstract Primary support for ancient Martian oceans has relied on qualitative interpretations of idealized slope hypothesized shorelines on relatively low‐resolution images and data. We present a toolkit for • Our analysis of these curvilinear features does not support a quantitatively identifying paleoshorelines using topographic, morphological, and spectroscopic paleoshoreline interpretation and is evaluations. In particular, we apply the validated topographic expression analysis of Hare et al. (2001, more consistent with eroded https://doi.org/10.1029/2001JB000344) for the first time beyond Earth, focusing on a test case of putative lithologies shoreline features along the Arabia level in northeast Cydonia Mensae, as first described by Clifford and Supporting Information: Parker (2001, https://doi.org/10.1006/icar.2001.6671). Our results show these curvilinear features are • Supporting Information S1 inconsistent with a wave‐generated shoreline interpretation. The topographic expression analysis identifies a few potential shoreline terraces along the historically proposed contacts, but these tilt in different directions, do not follow an equipotential surface (even accounting for regional tilting), and are Correspondence to: not laterally continuous. -
Mapping the Senses/ Charting Experience
Christian Nold Suzan Shutan Eve Ingalls Chip Lord Susan Sharp Pat Steir Sharon Horvath Denis Wood John Cage Sarah Amos Josephine Napurrula Heidi Whitman Leila Daw Adriana Lara Ree Morton Merce Cunningham Christo & Jean Claude GR UND TRUTH: Mapping the Senses/ Charting Experience Curated by Robbin Zella and Susan Sharp January 13 - February 10, 2012 The Map Land lies in water; it is a shadowed green, Shadows, or are they shallows, at its edges showing the line of long sea-weeded ledges where weeds hang to the simple blue from green. Ground Truth: Mapping the Senses/ Or does the land lean down to lift the sea from under, Charting Experience Drawing it unperturbed around itself? Along the fine tan sandy shelf Looking out into the wider-world requires us to first develop black and white and arrange them so that the larger pattern, the 2 Is the land tugging at the sea from under? a method of finding our way -- signs and symbols that lead pattern of the neighborhood itself, can emerge.” us to new destinations; and second, to rely on memory—an But neighborhoods, and the activities that happen there, can also The shadow of Newfoundland lies flat and still. internalized map. The first way situates us within a space as it relates to the cardinal points on a compass—north, south, change over time. Suzan Shutan’s installation, Sex in the Suburbs, Labrador’s yellow, where the moony Eskimo east, and west; and the second, is in relation to our own home- maps the growing sex-for-hire industry that is slowly taking root. -
Eskers Associated with Extant Glaciers in Mid-Latitude Graben on Mars: Evidence for Geothermal Controls Upon Recent Basal Melting
Lunar and Planetary Science XLVIII (2017) 1234.pdf ESKERS ASSOCIATED WITH EXTANT GLACIERS IN MID-LATITUDE GRABEN ON MARS: EVIDENCE FOR GEOTHERMAL CONTROLS UPON RECENT BASAL MELTING. F.E.G. Butcher1, C. Gallagher2,3, N.S. Arnold4, M.R. Balme1, S.J. Conway5, S.R. Lewis1, A. Hagermann1. 1School of Physical Sciences, The Open University, UK ([email protected]), 2UCD School of Geography, University College Dublin, Ireland, 3UCD Earth Institute, University College Dublin, Ireland 4Scott Polar Research Institute, University of Cambridge, UK, 5CNRS, LPG Nantes, France. Introduction: Diagnostic evidence for past melting of putative debris-covered glaciers (DCGs) in Mars’ mid-latitudes [e.g. 1-2] is extremely rare. As such, it is widely believed that these DCGs have been perennially frozen to their beds in cold-based thermal regimes [e.g. 3] since their formation ~40 Ma to 1 Ga [4-8]. Here, we present a landsystem model that challenges this paradigm. We identify a sinuous ridge emerging from a DCG in the broad rift zone NE of the Tharsis volcanic province. We interpret this ridge as an esker formed by deposition of sediment within a subglacial meltwater conduit. This is only the second esker-like ridge to be identified in association with a mid-latitude DCG. Re- cent work [9] identified a complex of esker-like ridges on the foreland of an extant DCG in Phlegra Montes, for which high-resolution analysis is ongoing [10]. Significantly, both candidate eskers are located within graben. Graben are topographic troughs formed by crustal extension and are commonly associated with elevated geothermal heat (GH) flux [e.g. -
Eskers in a Complete, Wet-Based Glacial System in the Phlegra
Earth and Planetary Science Letters 431 (2015) 96–109 Contents lists available at ScienceDirect Earth and Planetary Science Letters www.elsevier.com/locate/epsl Eskers in a complete, wet-based glacial system in the Phlegra Montes region, Mars ∗ Colman Gallagher a,b, , Matthew Balme c,d a UCD School of Geography, University College Dublin, Belfield, Dublin 4, Ireland b UCD Earth Institute, University College Dublin, Belfield, Dublin 4, Ireland c Dept. of Physical Sciences, Open University, Walton Hall, Milton Keynes MK7 6AA, UK d Planetary Science Institute Tucson, 1700 E. Fort Lowell, Suite 106, Tucson, AZ 85719, United States a r t i c l e i n f o a b s t r a c t Article history: Although glacial landsystems produced under warm/wet based conditions are very common on Earth, Received 30 April 2015 even here, observations of subglacial landforms such as eskers emerging from extant glaciers are rare. Received in revised form 9 September 2015 This paper describes a system of sinuous ridges emerging from the in situ but now degraded piedmont Accepted 14 September 2015 terminus of a Late Amazonian-aged (∼150 Ma) glacier-like form in the southern Phlegra Montes region Available online 29 September 2015 of Mars. We believe this to be the first identification of martian eskers that can be directly linked to their Editor: C. Sotin parent glacier. Together with their contextual landform assemblage, the eskers are indicative of significant Keywords: glacial meltwater production and subglacial routing. However, although the eskers are evidence of a Mars wet-based regime, the confinement of the glacial system to a well-defined, regionally significant graben, glacier and the absence of eskers elsewhere in the region, is interpreted as evidence of sub-glacial melting eskers as a response to locally enhanced geothermal heat flux rather than climate-induced warming. -
THE BUOYS Race Day on US Bellingham Bay, P.14 SOFTLY INSIDE Roberta Flack's Superstar Success, P.08 out Dinner with a View, P.34 the Art of Modulation: 7:30Pm, St
The Gristle, 3.Ɇ * Summer School, 3.ɁɆ * Film Shorts, 3.ɂɆ c a s c a d i a REPORTING FROM THE HEART OF CASCADIA WHATCOM *SKAGIT*ISLAND COUNTIES {06.17.15}{#24}{V.10}{FREE} THE SECOND PAYCHECK What's it worth to live here?, P.08 Between KILLING THE BUOYS Race day on US Bellingham Bay, P.14 SOFTLY INSIDE Roberta Flack's superstar success, P.08 OUT Dinner with a view, P.34 The Art of Modulation: 7:30pm, St. Paul’s Episcopal cascadia Church 34 Week This FILM FOOD FOOD A glance at this Grease: Dusk, Fairhaven Village Green COMMUNITY 27 week’s happenings Antique Fair: 9am-5pm, Christianson’s Nursery, Mount Vernon Family Activity Day: 10am-4pm, Whatcom Museum’s B-BOARD B-BOARD Lightcatcher Building Berry Dairy Days: Through Sunday, throughout Burlington 24 GET OUT FILM Feed the Need 5K: 9am, Hovander Homestead Park, Ferndale 20 Boat Show & Swap Meet: 9am-4pm, La Conner Marina Pet Parade: 11am, Maritime Heritage Park MUSIC Fairy Day: 11am-2pm, Garden Spot Nursery Sin & Gin Tour: 7pm, downtown Bellingham 18 ART FOOD Pancake Breakfast: 8-11am, Ferndale Senior Center Mount Vernon Farmers Market: 9am-2pm, Water- 16 front Plaza Anacortes Farmers Market: 9am-2pm, Depot Arts STAGE Center Bellingham Farmers Market: 10am-3pm, Depot Market Square 14 Farm Fiesta: 11am-7pm, Viva Farmers, Burlington Bring your four-legged, feathered, finned and furry friends to Bellingham Parks VISUAL ARTS GET OUT and Rec’s inaugural Pet Parade Sat., June 20 at Maritime Heritage Park Art Auction: 4-9pm, Museum of Northwest Art SUNDAY 21 12 [06. -
Case Fil Copy
NASA TECHNICAL NASA TM X-3511 MEMORANDUM CO >< CASE FIL COPY REPORTS OF PLANETARY GEOLOGY PROGRAM, 1976-1977 Compiled by Raymond Arvidson and Russell Wahmann Office of Space Science NASA Headquarters NATIONAL AERONAUTICS AND SPACE ADMINISTRATION • WASHINGTON, D. C. • MAY 1977 1. Report No. 2. Government Accession No. 3. Recipient's Catalog No. TMX3511 4. Title and Subtitle 5. Report Date May 1977 6. Performing Organization Code REPORTS OF PLANETARY GEOLOGY PROGRAM, 1976-1977 SL 7. Author(s) 8. Performing Organization Report No. Compiled by Raymond Arvidson and Russell Wahmann 10. Work Unit No. 9. Performing Organization Name and Address Office of Space Science 11. Contract or Grant No. Lunar and Planetary Programs Planetary Geology Program 13. Type of Report and Period Covered 12. Sponsoring Agency Name and Address Technical Memorandum National Aeronautics and Space Administration 14. Sponsoring Agency Code Washington, D.C. 20546 15. Supplementary Notes 16. Abstract A compilation of abstracts of reports which summarizes work conducted by Principal Investigators. Full reports of these abstracts were presented to the annual meeting of Planetary Geology Principal Investigators and their associates at Washington University, St. Louis, Missouri, May 23-26, 1977. 17. Key Words (Suggested by Author(s)) 18. Distribution Statement Planetary geology Solar system evolution Unclassified—Unlimited Planetary geological mapping Instrument development 19. Security Qassif. (of this report) 20. Security Classif. (of this page) 21. No. of Pages 22. Price* Unclassified Unclassified 294 $9.25 * For sale by the National Technical Information Service, Springfield, Virginia 22161 FOREWORD This is a compilation of abstracts of reports from Principal Investigators of NASA's Office of Space Science, Division of Lunar and Planetary Programs Planetary Geology Program. -
March 21–25, 2016
FORTY-SEVENTH LUNAR AND PLANETARY SCIENCE CONFERENCE PROGRAM OF TECHNICAL SESSIONS MARCH 21–25, 2016 The Woodlands Waterway Marriott Hotel and Convention Center The Woodlands, Texas INSTITUTIONAL SUPPORT Universities Space Research Association Lunar and Planetary Institute National Aeronautics and Space Administration CONFERENCE CO-CHAIRS Stephen Mackwell, Lunar and Planetary Institute Eileen Stansbery, NASA Johnson Space Center PROGRAM COMMITTEE CHAIRS David Draper, NASA Johnson Space Center Walter Kiefer, Lunar and Planetary Institute PROGRAM COMMITTEE P. Doug Archer, NASA Johnson Space Center Nicolas LeCorvec, Lunar and Planetary Institute Katherine Bermingham, University of Maryland Yo Matsubara, Smithsonian Institute Janice Bishop, SETI and NASA Ames Research Center Francis McCubbin, NASA Johnson Space Center Jeremy Boyce, University of California, Los Angeles Andrew Needham, Carnegie Institution of Washington Lisa Danielson, NASA Johnson Space Center Lan-Anh Nguyen, NASA Johnson Space Center Deepak Dhingra, University of Idaho Paul Niles, NASA Johnson Space Center Stephen Elardo, Carnegie Institution of Washington Dorothy Oehler, NASA Johnson Space Center Marc Fries, NASA Johnson Space Center D. Alex Patthoff, Jet Propulsion Laboratory Cyrena Goodrich, Lunar and Planetary Institute Elizabeth Rampe, Aerodyne Industries, Jacobs JETS at John Gruener, NASA Johnson Space Center NASA Johnson Space Center Justin Hagerty, U.S. Geological Survey Carol Raymond, Jet Propulsion Laboratory Lindsay Hays, Jet Propulsion Laboratory Paul Schenk, -
The Periglacial Landscape of Utopia Planitia; Geologic Evidence for Recent Climate Change on Mars
Western University Scholarship@Western Electronic Thesis and Dissertation Repository 1-23-2013 12:00 AM The Periglacial Landscape Of Utopia Planitia; Geologic Evidence For Recent Climate Change On Mars. Mary C. Kerrigan The University of Western Ontario Supervisor Dr. Marco Van De Wiel The University of Western Ontario Joint Supervisor Dr. Gordon R Osinski The University of Western Ontario Graduate Program in Geography A thesis submitted in partial fulfillment of the equirr ements for the degree in Master of Science © Mary C. Kerrigan 2013 Follow this and additional works at: https://ir.lib.uwo.ca/etd Part of the Climate Commons, Geology Commons, Geomorphology Commons, and the Physical and Environmental Geography Commons Recommended Citation Kerrigan, Mary C., "The Periglacial Landscape Of Utopia Planitia; Geologic Evidence For Recent Climate Change On Mars." (2013). Electronic Thesis and Dissertation Repository. 1101. https://ir.lib.uwo.ca/etd/1101 This Dissertation/Thesis is brought to you for free and open access by Scholarship@Western. It has been accepted for inclusion in Electronic Thesis and Dissertation Repository by an authorized administrator of Scholarship@Western. For more information, please contact [email protected]. THE PERIGLACIAL LANDSCAPE OF UTOPIA PLANITIA; GEOLOGIC EVIDENCE FOR RECENT CLIMATE CHANGE ON MARS by Mary C. Kerrigan Graduate Program in Geography A thesis submitted in partial fulfillment of the requirements for the degree of Master of Science The School of Graduate and Postdoctoral Studies The University of Western Ontario London, Ontario, Canada © Mary C. Kerrigan 2013 ii THE UNIVERSITY OF WESTERN ONTARIO School of Graduate and Postdoctoral Studies CERTIFICATE OF EXAMINATION Joint Supervisor Examiners ______________________________ Dr.