DOCSLIB.ORG

Guidelines for the Development of Community Park and Recreation Plans

Total Page：16

File Type：pdf, Size：1020Kb

Download full-text PDF Read full-text
Guidelines for the Development of Community Park and Recreation Plans Michigan Department of Natural Resources www.michigan.gov/dnr GUIDELINES FOR THE DEVELOPMENT OF COMMUNITY PARK AND RECREATION PLANS Grants Management IC1924 (Rev. 01/19/2021) MICHIGAN DEPARTMENT OF NATURAL RESOURCES MISSION STATEMENT "The Michigan Department of Natural Resources is committed to the conservation, protection, management, use and enjoyment of the State's natural resources for current and future generations." NATURAL RESOURCES COMMISSION STATEMENT The Natural Resources Commission (NRC), as the governing body for the Michigan Department of Natural Resources, provides a strategic framework for the DNR to effectively manage your resources. The NRC holds monthly, public meetings throughout Michigan, working closely with its constituencies in establishing and improving natural resources management policy. The Michigan Department of Natural Resources (DNR) provides equal opportunities for employment and access to Michigan's natural resources. Both state and Federal laws prohibit discrimination on the basis of race, color, national origin, religion, disability, age, sex, height, weight, or marital status under the U.S. Civil Rights Acts of 1964 as amended, 1976 MI PA 453, 1976 MI PA 220, Title V of the Rehabilitation Act of 1973 as amended, and the 1990 Americans with Disabilities Act, as amended. If you believe that you have been discriminated against in any program, activity, or facility, or if you desire additional information, please write: Human Resources, Michigan Department of Natural Resources, PO Box 30028, Lansing MI 48909-7528 or Michigan Department of Civil Rights, Cadillac Place, Suite 3-600, 3054 W. Grand Blvd, Detroit, MI 48202, or Division of Federal Assistance, U.S. Fish and Wildlife Service, 4401 North Fairfax Drive, Mail Stop MBSP-4020, Arlington, VA 22203. For information or assistance on this publication, contact Grants Management, Michigan Department of Natural Resources, PO Box 30425, Lansing, MI 48909-7925. This publication is available in alternative formats upon request. IC1924 (Rev. 01/19/2021) Grants Management staff is available to provide additional guidance to you as you prepare your recreation plan. We can be reached at the following address and telephone number: GRANTS MANAGEMENT MICHIGAN DEPARTMENT OF NATURAL RESOURCES PO BOX 30425 LANSING, MI 48909-7925 On the web at: www.michigan.gov/dnr-grants MiRecGrants Online Application Website: www.midnr.intelligrants.com Telephone: 517-284-7268 FAX: 517-241-0013 IC1924 (Rev. 01/19/2021) TABLE OF CONTENTS Introduction ........................................................................................................................................................ 1 Establishing Eligibility to Apply for Recreation Grants ........................................................................................ 1 Coordination of Planning ................................................................................................................................... 2 Preparing the Plan and Plan Content ................................................................................................................. 5 Community Description .................................................................................................................................. 5 Administrative Structure ................................................................................................................................. 6 Inventory of Existing Parks, Natural Areas and Recreation Facilities .............................................................. 6 Inventory of Existing Recreational Boating Facilities ...................................................................................... 8 Natural Resource Inventory (Optional) ........................................................................................................... 8 Description of the Planning and Public Input Process .................................................................................... 9 Goals and Objectives ................................................................................................................................... 11 Action Program ............................................................................................................................................ 12 Local Adoption and DNR Approval of Recreation Plans ................................................................................... 12 Planning Deadline ........................................................................................................................................... 13 Plan Amendments ........................................................................................................................................... 13 Submitting Documents for MiRecGrants .......................................................................................................... 14 General MiGrants Information.......................................................................................................................... 16 Bibliography ..................................................................................................................................................... 17 Appendix A: Michigan Enabling Legislation for Providing Public Recreation and Parks .................................. 19 Appendix B: Recommended Classification System for Local and Regional recreation Open Space and Trails 20 Appendix C: Suggested Facility Development Standards ................................................................................ 22 Appendix D: Barrier Free Accessibility Requirements for Parks ....................................................................... 25 Appendix E: ..................................................................................................................................................... 26 Appendix F: Government Agencies and Non-Profit Organizations that may be of Assistance in Preparing a Plan ................................................................................................................................................................. 27 Appendix G: Sources of Information on Accessibility for People with Disabilities ............................................. 28 Appendix H: Resources for Park Design Considerations ................................................................................. 29 Appendix I: Community Park and Recreation Plan Certification Checklist ....................................................... 30 Appendix J: Community Park and Recreation Plan Amendment Certification Checklist ................................... 32 Appendix K: Sample Resolution for Adopting a Plan and Plan Amendment ..................................................... 34 Appendix L: Post Completion Self-Inspection Report ....................................................................................... 35 Appendix M: Recreational Boating Facilities .................................................................................................... 37 Appendix N: Example of Existing Boating Inventory ........................................................................................ 38 IC1924 (Rev. 01/19/2021) INTRODUCTION The intent of a Community Park and Recreation Plan is to create an inventory of existing facilities and resources, identify community recreation and open space needs and set a plan of action for a 5-year period. The Michigan Department of Natural Resources (DNR) provides financial assistance to communities through its grant programs. A current DNR approved Community Park and Recreation Plan is required to be eligible for Land and Water Conservation Fund (LWCF), Michigan Natural Resources Trust Fund (MNRTF) and Waterways grants. For the Recreation Passport grant program either an approved Community Park and Recreation Plan or approved Capital Improvement Plan may be used for eligibility to this grant program. LWCF, MNRTF and RP grants can be used for the development of public outdoor recreation facilities including support facilities. RP can be used for indoor public recreation facilities. MNRTF is the only program that can be used for the acquisition of land for public recreation and for protection of land for environmental importance or scenic beauty. A Community Park and Recreation Waterways Grants can be used for development of marinas and recreational boating facilities. Questions regarding the Community Park and Recreation Plan requirements must be addressed with Grants Management at 517-284-7268. Questions specific to the Waterways Programs requirements must be addressed with the DNR Waterways Program at 517-284-6122. Ultimately approval of your Community Park and Recreation Plan will come from DNR Grants Management. Information on grant programs is available on the DNR website, www.Michigan.gov/DNR-Grants. A Community Park and Recreation Plan is also be referred to as a “5-Year Recreation Plan”. The 5-Year Plan must be submitted in MiRecGrants by February 1 of the year an applicant intends to apply for grants. This booklet describes the information that is required if the plan is to be approved by Grants Management. Information contained in the plan will be used by Grants Management staff in scoring applications. ESTABLISHING ELIGIBILITY TO APPLY FOR RECREATION GRANTS Local units of government are eligible to apply for recreation grants from the MDNR. Local units of government are defined according to Part 19 of The Natural Resources
Load more

Recommended publications
  • The Evolution of a Heterogeneous Martian Mantle: Clues from K, P, Ti, Cr, and Ni Variations in Gusev Basalts and Shergottite Meteorites
    Earth and Planetary Science Letters 296 (2010) 67–77 Contents lists available at ScienceDirect Earth and Planetary Science Letters journal homepage: www.elsevier.com/locate/epsl The evolution of a heterogeneous Martian mantle: Clues from K, P, Ti, Cr, and Ni variations in Gusev basalts and shergottite meteorites Mariek E. Schmidt a,⁎, Timothy J. McCoy b a Dept. of Earth Sciences, Brock University, St. Catharines, ON, Canada L2S 3A1 b Dept. of Mineral Sciences, National Museum of Natural History, Smithsonian Institution, Washington, DC 20560-0119, USA article info abstract Article history: Martian basalts represent samples of the interior of the planet, and their composition reflects their source at Received 10 December 2009 the time of extraction as well as later igneous processes that affected them. To better understand the Received in revised form 16 April 2010 composition and evolution of Mars, we compare whole rock compositions of basaltic shergottitic meteorites Accepted 21 April 2010 and basaltic lavas examined by the Spirit Mars Exploration Rover in Gusev Crater. Concentrations range from Available online 2 June 2010 K-poor (as low as 0.02 wt.% K2O) in the shergottites to K-rich (up to 1.2 wt.% K2O) in basalts from the Editor: R.W. Carlson Columbia Hills (CH) of Gusev Crater; the Adirondack basalts from the Gusev Plains have more intermediate concentrations of K2O (0.16 wt.% to below detection limit). The compositional dataset for the Gusev basalts is Keywords: more limited than for the shergottites, but it includes the minor elements K, P, Ti, Cr, and Ni, whose behavior Mars igneous processes during mantle melting varies from very incompatible (prefers melt) to very compatible (remains in the shergottites residuum).
    [Show full text]
  • Hirise Camera Views the Mars Rover 'Spirit' at 'Home Plate' 26 November 2007
    HiRISE Camera Views the Mars Rover 'Spirit' at 'Home Plate' 26 November 2007 Herkenhoff said. At the time, the camera was flying about 270 kilometers, or about 168 miles, over the surface. At that distance, the camera could resolve objects about 81 centimeters, or about 32 inches, across. The sun was about 56 degrees above the horizon in the winter afternoon sky. The HiRISE image of Home Plate and others are on the HiRISE Website, hirise.lpl.arizona.edu . HiRISE operations are based at The University of Arizona in Tucson. Professor Alfred S. McEwen of the Lunar and Planetary Laboratory is principal investigator for the experiment. The Mars rover "Spirit" is indicated by a circle on "Home Plate" in this new image of Gusev Crater on Mars. This The HiRISE camera is the most powerful camera detail is part of a much larger image the HiRISE camera ever to orbit another planet. It has taken thousands took on Sept. 27, 2007. The rover has since driven of black-and-white images, and hundreds of color north. (Photo: NASA/JPL/University of Arizona) images, since it began science operations in 2006. A single HiRISE image will often be a multigigabyte image that measures 20,000 pixels by 50,000 The High Resolution Imaging Science Experiment, pixels, which includes a 4,000-by-50,000 pixel or HiRISE, camera onboard NASA's Mars region in three colors. It can take a computer up to Reconnaissance Orbiter has taken a new color three hours to process such an image. image of the feature dubbed "Home Plate" in Gusev Crater on Mars.
    [Show full text]
  • 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,
    [Show full text]
  • Mars Exploration Rovers: 4 Years on Mars
    https://ntrs.nasa.gov/search.jsp?R=20080047431 2019-10-28T16:17:34+00:00Z Mars Exploration Rovers: 4 Years on Mars Geoffrey A. Landis This January, the Mars Exploration Rovers "Spirit" and "Opportunity" are starting their fifth year of exploring the surface of Mars, well over ten times their nominal 90-day design lifetime. This lecture discusses the Mars Exploration Rovers, presents the current mission status for the extended mission, some of the most results from the mission and how it is affecting our current view of Mars, and briefly presents the plans for the coming NASA missions to the surface of Mars and concepts for exploration with robots and humans into the next decade, and beyond. Four Years on Mars: the Mars Exploration Rovers Geoffrey A. Landis NASA John Glenn Research Center http://www.sff.net/people/geoffrey.landis Presentation at MIT Department of Aeronautics and Astronautics, January 18, 2008 Exploration - Landis Mars viewed from the Hubble Space Telescope Exploration - Landis Views of Mars in the early 20th century Lowell 1908 Sciaparelli 1888 Burroughs 1912 (cover painting by Frazetta) Tales of Outer Space ed. Donald A. Wollheim, Ace D-73, 1954 (From Winchell Chung's web page projectrho.com) Exploration - Landis Past Missions to Mars: first close up images of Mars from Mariner 4 Mariner 4 discovered Mars was a barren, moon-like desert Exploration - Landis Viking 1976 Signs of past water on Mars? orbiter Photo from orbit by the 1976 Viking orbiter Exploration - Landis Pathfinder and Sojourner Rover: a solar-powered mission
    [Show full text]
  • CONVENIENCE SUMMARY REPORT NATIONAL HIGH SCHOOL SPORTS-RELATED INJURY SURVEILLANCE STUDY 2009-2010 School Year Compiled By
    CONVENIENCE SUMMARY REPORT NATIONAL HIGH SCHOOL SPORTS-RELATED INJURY SURVEILLANCE STUDY 2009-2010 School Year Compiled by: R. Dawn Comstock, PhD Christy L. Collins, MA Natalie M. McIlvain, BS Acknowledgements We thank the certified athletic trainers (ATCs) for their hard work and dedication in providing us with complete and accurate data. Without their efforts, this study would not have been possible. We would like to thank the National Federation of State High School Associations (NFHS) for their support of this project. The content of this report was funded in part by the Centers for Disease Control and Prevention (CDC) grants #R49/CE000674-01 and #R49/CE001172-01. The content of this report is solely the responsibility of the authors and does not necessarily represent the official views of the CDC. We would also like to acknowledge the generous research funding contributions of the National Federation of State High School Associations (NFHS), National Operating Committee on Standards for Athletic Equipment (NOCSAE), and DonJoy Orthotics. Note The analyses presented here provide only a brief summary of collected data, with the feasibility of a more detailed presentation limited by the extensive breadth and detail contained in the dataset. The principal investigator, Dr. R. Dawn Comstock, is happy to provide further information or to discuss research partnership opportunities upon request. For reprints/further information contact: R. Dawn Comstock, PhD Center for Injury Research and Policy The Research Institute at Nationwide Children’s Hospital 700 Children’s Drive Columbus, OH 43205 (614) 722-2400 [email protected] 2 Chapter Page 1. Introduction and Methodology 14 1.1 Project Overview 15 1.2 Background and Significance 15 1.3 Specific Aims 16 1.4 Project Design 17 1.5 Sample Recruitment 18 1.6 Data Collection 20 1.7 Data Management 21 1.8 Data Analysis 21 2.
    [Show full text]
  • MARS ORBITAL DATA — METHODS and INTERPRETATION 6:30 P.M
    Lunar and Planetary Science XXXIX (2008) sess614.pdf Thursday, March 13, 2008 POSTER SESSION II: MARS ORBITAL DATA — METHODS AND INTERPRETATION 6:30 p.m. Fitness Center Farrand W. H. Johnson J. R. Schmidt M. E. Bell J. F. III VNIR Spectral Differences on Natural and Brushed/Wind-abraded Surfaces on Home Plate, Gusev Crater, Mars: Spirit Pancam and HiRISE Color Observations [#1774] Color differences between the eastern and western rims of Home Plate are examined using Spirit Pancam and HiRISE color observations. Differences between near-field and remote observations are considered. Rice M. S. Bell J. F. III Wang A. Cloutis E. A. Vis-NIR Spectral Characterization of Si-rich Deposits at Gusev Crater, Mars [#2138] The Spirit rover has discovered high concentrations of silica at Gusev Crater, and a distinct spectral feature near 1000 nm appears to be diagnostic of these materials. We hypothesize that the presence of H2O or OH may be responsible for this feature. Combe J.-Ph. McCord T. B. Mars-Express/HRSC Spectral Data of MER Landing Sites Analyzed by a Multiple-Endmember Linear Spectral Linear Unmixing Model (MELSUM) [#2381] HRSC multispectral data are analyzed for mapping the main surface spectral components and photometric properties of Mars. The unique geometry of observation of this dataset is investigated. Results will be compared to field observations from the MERs. Hauber E. Gwinner K. Gendrin A. Fueten F. Stesky R. Pelkey S. Reiss D. Zegers T. E. MacKinnon P. Jaumann R. Bibring J.-P. Neukum G. Hebes Chasma, Mars: Slopes and Stratigraphy of Interior Layered Deposits [#2375] We present new data from HRSC and CTX on the topography, stratigraphy, and structure of Interior Layered Deposits in Hebes Chasma, Valles Marineris, Mars.
    [Show full text]
  • Pyroclastic Activity at Home Plate in Gusev Crater, Mars
    REPORTS 5. R. T. T. Forman, R. D. Deblinger, Conserv. Biol. 14,36 14. H. John Heinz III Center for Science, Economics, and the 20. The movie of RV change for the Colorado Front Range is (2000). Environment, The State of the Nation's Ecosystems: available as supporting material on Science Online. 6. K. H. Riitters, J. D. Wickham, Front. Ecol. Environ. 1, 125 Measuring the Lands, Waters, and Living Resources of the 21. W. R. Tobler, Econ. Geogr. 46, 234 (1970). (2003). United States (Cambridge Univ. Press, Cambridge, 2002). 22. We thank the Southern Rockies Ecosystem Project for 7. R. T. T. Forman, L. E. Alexander, Annu. Rev. Ecol. Syst. 15. C. Homer, M. Coan, C. Huang, L. Yang, B. Wylie, introducing us to large-area DTR maps nearly a decade 29, 207 (1998). Photogramm. Eng. Remote Sens. 70, 829 (2004). ago. Support for the development and analysis of 8. J. L. Gelbard, J. Belnap, Conserv. Biol. 17, 420 (2003). 16. Materials and methods, including a table of county values national DTR data was provided by the USGS Geographic 9. R. L. DeVelice, J. R. Martin, Ecol. Appl. 11,1008 of mean DTR and RV, are available as supporting Analysis and Monitoring Program. (2001). material on Science Online. 10. I. F. Spellerberg, Ecological Effects of Roads, Land 17. Because calculations were done with a 30-m grid, the Supporting Online Material Reconstruction and Management (Science Publishers, accuracy of the calculations is low where roads are dense. www.sciencemag.org/cgi/content/full/316/5825/736/DC1 Materials and Methods Enfield, NH, 2002).
    [Show full text]
  • Columbia Hills, Gusev Crater: Mission Overview and Selected Results from the Cumberland Ridge to Home Plate, J
    Columbia Hills, Location 14.5478 S, 175.6255 E (lat,lon): MOLA128: -1.932 km Gusev Crater Summary of observations and interpreted history, including unknowns: Gusev crater formed around 3.9–4.1 billion years ago (Werner et al., 2008). The Columbia Hills may represent peak ring hills, intersecting rims of multiple craters, or eroded, possibly lacustrine fill. Subsequent geologic processes emplaced successive volcanics and possibly evaporites, draping over the Hills at dips of 7–30 degrees (McSween et al., 2008; McCoy et al., 2008; Ruff et al., 2014). Basaltic plains dated to 3.65 Ga onlap the Columbia Hills (Greeley et al., 2005). Multiple igneous rock units are present in the Columbia Hills, including high-alkali and high olivine materials and some tuffs or ashes (McSween et al., 2008). Several types of evidence of aqueous processes are preserved in rocks that have possible Al-phyllosilicates (Clark et al., 2007), Mg-Fe carbonates (Morris et al., 2010), and opaline silica (Squyres et al., 2008; Ruff et al., 2011). Near surface soil crusts have ferric sulfates, calcium sulfates, and silica (Arvidson et al., 2010). The silica-enriched rocks and ferric sulfate-bearing soils occur in and around the 80 m-diameter “Home Plate” volcaniclastic deposit. The presence of the Spirit rover represents a long duration exposure facility experiment, of potential value in human exploration. Key units are: the "Comanche" carbonate-bearing outcrops (~15-30 wt% Mg-Fe carbonate, plus olivine and an amorphous silicate), which has been interpreted to result from (a) hydrothermal alteration (Morris et al., 2010) or (b) evaporation of an ephemeral lake (Ruff et al., 2014).
    [Show full text]
  • Tuesday February Through
    Amended Agenda St Clair Shores City Council Meeting Tuesday February pm City Hall Jefferson Circle Drive St Clair Shores MI Call to Order Roll Call and Pledge of Allegiance Proclamations Presentations Audience Participation on agenda items minute time limit Submit form to City Clerk prior to start of meeting Request to hold ShoresPointes Adventure Triathlon on Saturday July from am am at Blossom Heath ParkBeach zfrwrn nr rescheduled to Request approval for sale of Evergreen Recommendations from the Communications Commission for Modifications to the Citys Facebook Policy BidslContractsPurchase Orders a Award bid for the Purchase of Natural Gas for City Owned Municipal Buildings bid opened rescheduled to c Award bid for the Request for Proposal RFP for Food and Beverage Concessions in Parks bid opened d Award Bids from the Energy Efficiency Grants i Award bid for Civic Center Pump Motor and Water Heater Replacement bid opened Request from the Fire Department for Ordinance Adoption and Amendments a Adopt new sections to Ordinance Regarding Ambulance Service fees on transporting confined patients b Amend Ordinance to update the language to reflect our current practices Consent Agenda Items shall be considered without debate by motion and vote ofCouncil unless a member of Council specifically requests action taken separately on said item a Bills b Fees c Progress Payments d Approval of Minutes e Receive File Boards Commissions Committee Minutes f Request to set Public Hearings for vacation of Public Alleys on April as follows i Public Alley
    [Show full text]
  • Gale Crater: the Mars Science Laboratory/ Curiosity Rover Landing Site
    International Journal of Astrobiology 12 (1): 25–38 (2013) doi:10.1017/S1473550412000328 © Cambridge University Press 2012. The online version of this article is published within an Open Access environment subject to the conditions of the Creative Commons Attribution-NonCommercial-ShareAlike licence <http://creativecommons.org/licenses/by-nc-sa/2.5/>. The written permission of Cambridge University Press must be obtained for commercial re-use. Gale crater: the Mars Science Laboratory/ Curiosity Rover Landing Site James J. Wray School of Earth and Atmospheric Sciences, Georgia Institute of Technology, 311 Ferst Drive, Atlanta, GA 30332-0340, USA e-mail: [email protected] Abstract: Gale crater formed from an impact on Mars *3.6 billion years ago. It hosts a central mound nearly 100 km wide and *5 km high, consisting of layered rocks with a variety of textures and spectral properties. The oldest exposed layers contain variably hydrated sulphates and smectite clay minerals, implying an aqueous origin, whereas the younger layers higher on the mound are covered by a mantle of dust. Fluvial channels carved into the crater walls and the lower mound indicate that surface liquids were present during and after deposition of the mound material. Numerous hypotheses have been advocated for the origin of some or all minerals and layers in the mound, ranging from deep lakes to playas to mostly dry dune fields to airfall dust or ash subjected to only minor alteration driven by snowmelt. The complexity of the mound suggests that multiple depositional and diagenetic processes are represented in the materials exposed today. Beginning in August 2012, the Mars Science Laboratory rover Curiosity will explore Gale crater by ascending the mound’s northwestern flank, providing unprecedented new detail on the evolution of environmental conditions and habitability over many millions of years during which the mound strata accumulated.
    [Show full text]
  • Volcanically Driven Hydrothermal Systems in Post-Noachian Mars
    Volcanically Driven Hydrothermal Systems on Post‐Noachian Mars: Hotspots of Habitability on a Changing Planet J.R. Skok and J.F. Mustard Brown University with B. Ehlmann, R. Milliken, S. Murchie Exploring Mars Habitability Lisbon, Portugal June 13, 2011 Detailed View of Terrestrial Volcanic Hydrothermal System • System driven by heat from magmatic chamber. • Increased thermal gradient heats ground water and may contain magmatic sourced waters. • Dissolution of mafic minerals would create silica saturated fluids. • Deposition of silica, sulfates, travertines and oxides occur Pirajno and Kranendonk 2005 nears vents and hot springs. Proposed Sites of Hydrothermal Systems on Mars Apollinaris Mons Lava‐Rock Home Plate, Gusev interaction to create rootless Crater. Squyres et al 2007 cones. South of Elysium HiRISE PSP_002622_1820 Syrtis Major Volcanic Complex Nili Fossae Isidis Basin Syrtis Major Nili Patera Nili Patera Caldera Nili 400 m elevation Fossae Isidis Basin Syrtis Major Nili Patera 30km CTX:P04_002427_1888_XI_08N292W High Silica THEMIS:I09472026: 9,7,5 DCS Detection Nili Fossae Isidis Basin Syrtis Major Nili Patera 30km 10 km CTX:P04_002427_1888_XI_08N292W THEMIS:I09472026: 9,7,5 DCS Nili Patera Cone Nili Fossae Isidis Basin Syrtis Major Nili Patera 10 km CTX:P04_002427_1888_XI_08N292W THEMIS:I09472026: 9,7,5 DCS Light‐toned Deposits 10 km Calibrated CRISM Spectra 10 km FRT000010628 Ratioed Spectra 2.212.21 µm µm Hawaiian Volcanic Silica 2.21µm Position and shape of 2.21 µm FRT000010628 are consistent with Si‐OH. Spectral Reproduction with Super resolution CRISM Super resolution ~10m/pixel 150m CRISM 18m/pixel Super Resolution 80 pixels FRT000010628 160 pixels FRT0001DE11 Nili Patera Volcanic Cone CTX‐CRISM Composite on CTX Stereo DEM 5x Nili Patera Volcanic Cone CTX‐CRISM Composite on CTX Stereo DEM 5x HiRISE:ESP_013582_1895 Fan Deposit 400m HiRISE:ESP_013582_1895 South Deposit HiRISE:ESP_013582_1895 200m Review of Nili Patera Hydrothermal System Model • Complex Syrtis Major caldera Nili Patera Cone indicated several eruptive episodes.
    [Show full text]
  • Martian Rock Types Analysis of Surface Composition
    Martian rock types Analysis of surface composition • Most of the knowledge from the surface compostion of Mars comes from: • Orbital spacecraft’s spectroscopic data • Analysis by rovers on the surface • Analysis of meteroites Southern Highlands • Mainly Basalts – Consists primarily of Olivine, Feldspars and Pyroxenes Northern Lowlands • Mainly Andesite – More evolved forms of magma – Highly volatile – Constitutes the majority of the crust Intermediate Felsic Types • High Silica Rocks • Exposed on the surface near Syrtis Major • Uncommon but include: • Dacites and Granitoids • Suggest diverse crustal composition Sedimentary Rocks • Widespread on the surface • Makes up the majority of the Northern lowlands deposists – May have formed from sea/lake deposits – Some show cross‐bedding in their layers – Hold the best chance to find fossilized life Carbonate Rocks • Formed through hydrothermal precipitation Tracks from rover unveil different soil types • Most soil consists of finely ground basaltic rock fragments • Contains iron oxide which gives Mars its red color • Also contains large amounts of sulfur and chlorine Tracks from rover unveil different soil types • Light colored soil is silica rich • High concentrations suggest water must have been involved to help concentrate the silica Blueberries • Iron rich spherules Meteorites on Mars What is a Martian meteorite? • Martian meteorites are achondritic meteorites with strong linear correlations of gases in the Martian atmosphere. Therefore, the gas trapped in each meteorite matches those that the Viking Lander found in Mar’s atmosphere. The graph below explains this correlation. • Image: http://www.imca.cc/mars/martian‐meteorites.htm Types of Martian Meteorites • 34 meteorites have been found that are Martian and they can be separated into 4 major categories with sub‐categories.
    [Show full text]