The Science Process for Selecting the Landing Site for the 2011 Mars Science Laboratory
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Thermal Studies of Martian Channels and Valleys Using Termoskan Data
JOURNAL OF GEOPHYSICAL RESEARCH, VOL. 99, NO. El, PAGES 1983-1996, JANUARY 25, 1994 Thermal studiesof Martian channelsand valleys using Termoskan data BruceH. Betts andBruce C. Murray Divisionof Geologicaland PlanetarySciences, California Institute of Technology,Pasadena The Tennoskaninstrument on boardthe Phobos '88 spacecraftacquired the highestspatial resolution thermal infraredemission data ever obtained for Mars. Included in thethermal images are 2 km/pixel,midday observations of severalmajor channel and valley systems including significant portions of Shalbatana,Ravi, A1-Qahira,and Ma'adimValles, the channelconnecting Vailes Marineris with HydraotesChaos, and channelmaterial in Eos Chasma.Tennoskan also observed small portions of thesouthern beginnings of Simud,Tiu, andAres Vailes and somechannel material in GangisChasma. Simultaneousbroadband visible reflectance data were obtainedfor all but Ma'adimVallis. We find thatmost of the channelsand valleys have higher thermal inertias than their surroundings,consistent with previousthermal studies. We show for the first time that the thermal inertia boundariesclosely match flat channelfloor boundaries.Also, butteswithin channelshave inertiassimilar to the plainssurrounding the channels,suggesting the buttesare remnants of a contiguousplains surface. Lower bounds ontypical channel thermal inertias range from 8.4 to 12.5(10 -3 cal cm-2 s-1/2 K-I) (352to 523 in SI unitsof J m-2 s-l/2K-l). Lowerbounds on inertia differences with the surrounding heavily cratered plains range from 1.1 to 3.5 (46 to 147 sr). Atmosphericand geometriceffects are not sufficientto causethe observedchannel inertia enhancements.We favornonaeolian explanations of the overall channel inertia enhancements based primarily upon the channelfloors' thermal homogeneity and the strongcorrelation of thermalboundaries with floor boundaries. However,localized, dark regions within some channels are likely aeolian in natureas reported previously. -
Curiosity's Candidate Field Site in Gale Crater, Mars
Curiosity’s Candidate Field Site in Gale Crater, Mars K. S. Edgett – 27 September 2010 Simulated view from Curiosity rover in landing ellipse looking toward the field area in Gale; made using MRO CTX stereopair images; no vertical exaggeration. The mound is ~15 km away 4th MSL Landing Site Workshop, 27–29 September 2010 in this view. Note that one would see Gale’s SW wall in the distant background if this were Edgett, 1 actually taken by the Mastcams on Mars. Gale Presents Perhaps the Thickest and Most Diverse Exposed Stratigraphic Section on Mars • Gale’s Mound appears to present the thickest and most diverse exposed stratigraphic section on Mars that we can hope access in this decade. • Mound has ~5 km of stratified rock. (That’s 3 miles!) • There is no evidence that volcanism ever occurred in Gale. • Mound materials were deposited as sediment. • Diverse materials are present. • Diverse events are recorded. – Episodes of sedimentation and lithification and diagenesis. – Episodes of erosion, transport, and re-deposition of mound materials. 4th MSL Landing Site Workshop, 27–29 September 2010 Edgett, 2 Gale is at ~5°S on the “north-south dichotomy boundary” in the Aeolis and Nepenthes Mensae Region base map made by MSSS for National Geographic (February 2001); from MOC wide angle images and MOLA topography 4th MSL Landing Site Workshop, 27–29 September 2010 Edgett, 3 Proposed MSL Field Site In Gale Crater Landing ellipse - very low elevation (–4.5 km) - shown here as 25 x 20 km - alluvium from crater walls - drive to mound Anderson & Bell -
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). -
The Paleoecology and Fire History from Crater Lake
THE PALEOECOLOGY AND FIRE HISTORY FROM CRATER LAKE, COLORADO: THE LAST 1000 YEARS By Charles T. Mogen A Thesis Submitted in Partial Fulfillment of the Requirements for the Degree of Master of Science in Environmental Science and Policy Northern Arizona University August 2018 Approved: R. Scott Anderson, Ph.D., Chair Nicholas P. McKay, Ph.D. Darrell S. Kaufman, Ph.D. Abstract High-resolution pollen, plant macrofossil, charcoal and pyrogenic Polycyclic Aromatic Hydrocarbon (PAH) records were developed from a 154 cm long sediment core collected from Crater Lake (37.39°N, 106.70°W; 3328 m asl), San Juan Mountains, Colorado. Several studies have explored Holocene paleo-vegetation and fire histories from mixed conifer and subalpine bogs and lakes in the San Juan and southern Rocky Mountains utilizing both palynological and charcoal studies, but most have been at relatively low resolution. In addition to presenting the highest resolution palynological study over the last 1000 years from the southern Rocky Mountains, this thesis also presents the first high-resolution pyrogenic PAH and charcoal paired analysis aimed at understanding both long-term fire history and the unresolved relationship between how each of these proxies depict paleofire events. Pollen assemblages, pollen ratios, and paleofire activity, indicated by charcoal and pyrogenic PAH records, were used to infer past climatic conditions. Although the ecosystem surrounding Crater Lake has remained a largely spruce (Picea) dominated forest, the proxies developed in this thesis suggest there were two distinct climate intervals between ~1035 to ~1350 CE and ~1350 to ~1850 CE in the southern Rocky Mountains, associated with the Medieval Climate Anomaly (MCA) and Little Ice Age (LIA) respectively. -
Portal Valiant Integrated Com My Policy
Portal Valiant Integrated Com My Policy Bejeweled Leonhard usually tickling some Kulturkreis or vacillates soundlessly. Drier and honeycombed Kurtis disunites almost traitorously, though Tann harasses his Mombasa neighbours. Vindictive and unsolicitous Matthiew blast her chirm qualifies or retorts refutably. Where policy and my very great efficiencies and automated sms and handmade gifts for valiant portal has given your supervisor and. WatchGuard has deployed nearly a million integrated multi-function threat management appliances worldwide. Backbase Press & Latest News Backbase. Wholesale Club Holdings Inc. Joint Deployment Energy Planning and Logistics Optimization Initiative J-DEPLOI Video Portal. Active bidding campaigns, my son who killed anyone! Drop your anchor than a better harbor! And relieve want to link my ship to JIRA but I can't fetch an asset. News 'Network of faith' for Hawaii's military DVIDS. Vessel Registration The Texas General society Office. Inkfidel is my name is an integrated resources activity rooms that productivity, integration with policies, and operated business and. Rosalyn. Having something new data integration continues to valiant integrated population to rest of communication provides a recently, texas area to learn best alongside the agglomeration of. We created Exteriors Denver, llc to raise excellent products and services to you. Backbase and Mambu partner to deliver high end-to-end integrated SaaS banking solution. IBSA invites both individuals and businesses to delay more hand our work drop the communities we serve. It was reading much my own idea. Mstxs is the small business men, that she worked together to join forces case studies on the market helped me give us take a specific individuals. -
Grumbles from the Grave
GRUMBLES FROM THE GRAVE Robert A. Heinlein Edited by Virginia Heinlein A Del Rey Book BALLANTINE BOOKS • NEW YORK For Heinlein's Children A Del Rey Book Published by Ballantine Books Copyright © 1989 by the Robert A. and Virginia Heinlein Trust, UDT 20 June 1983 All rights reserved under International and Pan-American Copyright Conventions. Published in the United States by Ballantine Books, a division of Random House, Inc., New York, and simultaneously in Canada by Random House of Canada Limited, Toronto. Grateful acknowledgment is made to the following for permission to reprint the following material: Davis Publications, Inc. Excerpts from ten letters written by John W. Campbell as editor of Astounding Science Fiction. Copyright ® 1989 by Davis Publications, Inc. Putnam Publishing Group: Excerpt from the original manuscript of Podkayne of Mars by Robert A. Heinlein. Copyright ® 1963 by Robert A. Heinlein. Reprinted by permission of the Putnam Publishing Group. Library of Congress Catalog Card Number: 89-6859 ISBN 0-345-36941-6 Manufactured in the United States of America First Hardcover Edition: January 1990 First Mass Market Edition: December 1990 CONTENTS Foreword A Short Biography of Robert A. Heinlein by Virginia Heinlein CHAPTER I In the Beginning CHAPTER II Beginnings CHAPTER III The Slicks and the Scribner's Juveniles CHAPTER IV The Last of the Juveniles CHAPTER V The Best Laid Plans CHAPTER VI About Writing Methods and Cutting CHAPTER VII Building CHAPTER VIII Fan Mail and Other Time Wasters CHAPTER IX Miscellany CHAPTER X Sales and Rejections CHAPTER XI Adult Novels CHAPTER XII Travel CHAPTER XIII Potpourri CHAPTER XIV Stranger CHAPTER XV Echoes from Stranger AFTERWORD APPENDIX A Cuts in Red Planet APPENDIX B Postlude to Podkayne of Mars—Original Version APPENDIX C Heinlein Retrospective, October 6, 1988 Bibliography Index FOREWORD This book does not contain the polished prose one normally associates with the Heinlein stories and articles of later years. -
A La Torre Aaker Aalbers Aaldert Aarmour Aaron
A LA TORRE ABDIE ABLEMAN ABRAMOWITCH AAKER ABE ABLES ABRAMOWITZ AALBERS ABEE ABLETSON ABRAMOWSKY AALDERT ABEEL ABLETT ABRAMS AARMOUR ABEELS ABLEY ABRAMSEN AARON ABEKE ABLI ABRAMSKI AARONS ABEKEN ABLITT ABRAMSON AARONSON ABEKING ABLOTT ABRAMZON AASEN ABEL ABNER ABRASHKIN ABAD ABELA ABNETT ABRELL ABADAM ABELE ABNEY ABREU ABADIE ABELER ABORDEAN ABREY ABALOS ABELES ABORDENE ABRIANI ABARCA ABELI ABOT ABRIL ABATE ABELIN ABOTS ABRLI ABB ABELL ABOTSON ABRUZZO ABBA ABELLA ABOTT ABSALOM ABBARCROMBIE ABELLE ABOTTS ABSALON ABBAS ABELLS ABOTTSON ABSHALON ABBAT ABELMAN ABRAHAM ABSHER ABBATE ABELS ABRAHAMER ABSHIRE ABBATIELLO ABELSON ABRAHAMI ABSOLEM ABBATT ABEMA ABRAHAMIAN ABSOLOM ABBAY ABEN ABRAHAMOF ABSOLON ABBAYE ABENDROTH ABRAHAMOFF ABSON ABBAYS ABER ABRAHAMOV ABSTON ABBDIE ABERCROMBIE ABRAHAMOVITZ ABT ABBE ABERCROMBY ABRAHAMOWICZ ABTS ABBEKE ABERCRUMBIE ABRAHAMS ABURN ABBEL ABERCRUMBY ABRAHAMS ABY ABBELD ABERCRUMMY ABRAHAMSEN ABYRCRUMBIE ABBELL ABERDEAN ABRAHAMSOHN ABYRCRUMBY ABBELLS ABERDEEN ABRAHAMSON AC ABBELS ABERDEIN ABRAHAMSSON ACASTER ABBEMA ABERDENE ABRAHAMY ACCA ABBEN ABERG ABRAHM ACCARDI ABBERCROMBIE ABERLE ABRAHMOV ACCARDO ABBERCROMMIE ABERLI ABRAHMOVICI ACE ABBERCRUMBIE ABERLIN ABRAHMS ACERO ABBERDENE ABERNATHY ABRAHMSON ACESTER ABBERDINE ABERNETHY ABRAM ACETO ABBERLEY ABERT ABRAMCHIK ACEVEDO ABBETT ABEYTA ABRAMCIK ACEVES ABBEY ABHERCROMBIE ABRAMI ACHARD ABBIE ABHIRCROMBIE ABRAMIN ACHENBACH ABBING ABIRCOMBIE ABRAMINO ACHENSON ABBIRCROMBIE ABIRCROMBIE ABRAMO ACHERSON ABBIRCROMBY ABIRCROMBY ABRAMOF ACHESON ABBIRCRUMMY ABIRCROMMBIE ABRAMOFF -
Interior Layered Deposits in the Eastern Valles Marineris and Chaotic Terrains on Mars M
Lunar and Planetary Science XXXVIII (2007) 1568.pdf Interior Layered Deposits in the Eastern Valles Marineris and Chaotic Terrains on Mars M. Sowe1, E. Hauber1, R. Jaumann1,4, K. Gwinner1, F. Fueten2, R. Stesky3, and G. Neukum4 1Institute of Planetary Research, German Aerospace Center (DLR), Berlin, Germany, 2Department of Earth Sciences, Brock University, St. Catharines, Ontario, Canada, 3Pangaea Scientific, Brockville, Ontario, Canada, 4Department of Earth Sciences, Institute of Geosciences, Remote Sensing of the Earth and Planets, Freie Universitaet Berlin, Germany Introduction Interior Layered Deposits (ILDs) are widespread throughout the whole Valles Marineris. They have been known and analysed for many decades but their origin remains uncertain. There are several hypotheses concerning the origin of ILDs (eolian [1] or lacustrine deposition [2], pyroclastic volcanism in subaerial [3,4,5,6] or sub glacial environments [7,8]). They all imply that the ILDs A B are younger than the troughs in which they formed. Contrary ILDs may also be ancient deposits exhumed due to uplift of the basement [9,10]. We concentrate on ILDs in the eastern Valles Marineris and chaotic terrains and analyse their elevation, thickness, stratigraphic position, competence, state of alteration, and mineralogical composition. Overview The ILDs occur at different elevations from -6000 up to -800m but always lie below the surrounding plateau rim. In contrast to ILDs in the Eastern Valles Marineris (e.g. Candor, Hebes and Ophir Chasma) that reach or even overlap the canyon rim with elevations from ~ -5000 up to ~3500 m. ILDs vary in morphology. Mostly they appear as -2800 -3000 light-toned layered outcrops. -
Read Ebook {PDF EPUB} the Moon Maze Game by Larry Niven the Moon Maze Game by Larry Niven
Read Ebook {PDF EPUB} The Moon Maze Game by Larry Niven The Moon Maze Game by Larry Niven. Completing the CAPTCHA proves you are a human and gives you temporary access to the web property. What can I do to prevent this in the future? If you are on a personal connection, like at home, you can run an anti-virus scan on your device to make sure it is not infected with malware. If you are at an office or shared network, you can ask the network administrator to run a scan across the network looking for misconfigured or infected devices. Another way to prevent getting this page in the future is to use Privacy Pass. You may need to download version 2.0 now from the Chrome Web Store. Cloudflare Ray ID: 661a828c784f2c22 • Your IP : 116.202.236.252 • Performance & security by Cloudflare. The Moon Maze Game by Larry Niven. Completing the CAPTCHA proves you are a human and gives you temporary access to the web property. What can I do to prevent this in the future? If you are on a personal connection, like at home, you can run an anti-virus scan on your device to make sure it is not infected with malware. If you are at an office or shared network, you can ask the network administrator to run a scan across the network looking for misconfigured or infected devices. Another way to prevent getting this page in the future is to use Privacy Pass. You may need to download version 2.0 now from the Chrome Web Store. -
Preliminary Mission Analysis and Orbit Design for Next Mars Exploration
Trans. JSASS Aerospace Tech. Japan Vol. 8, No. ists27, pp. Tk_7-Tk_12, 2010 Topics Preliminary Mission Analysis and Orbit Design for Next Mars Exploration By Naoko OGAWA 1), Mutsuko Y. MORIMOTO1), Yuichi TSUDA1,2), Tetsuya YAMADA1,2), Kazuhisa FUJITA1,3), Tomohiro YAMAGUCHI4), Yasuhiro KAWAKATSU1,2), Takashi KUBOTA1,2) and Jun’ichiro KAWAGUCHI1,2) 1)JAXA Space Exploration Center, Japan Aerospace Exploration Agency, Sagamihara, Japan 2)Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency, Sagamihara, Japan 3)Aerospace Research and Development Directorate, Japan Aerospace Exploration Agency, Tokyo, Japan 4)The Graduate University for Advanced Studies, Sagamihara, Japan (Received July 21st, 2009) Japan has launched many interplanetary spacecraft for exploration of solar system bodies including Mars. Now we are planning the next Mars mission in the late 2010’s. This paper describes the preliminary mission analysis and orbit design for this plan. The combined exploration by several spacecraft requires complicated and careful consideration, different from those for single-probe missions. Mission plans to realize required configuration by a single launch and simple simulation results are reported. Key Words: Mars, Mission Analysis, Orbit Design, MELOS 1. Introduction 2.1.1. Meteorological orbiter for martian climate One orbiter of the two, called hereafter as the meteorological In 2008, Japan Aerospace Exploration Agency (JAXA) orbiter, aims understanding of the interaction between the has established a novel working group toward a novel Mars atmosphere and subsurface ice, and atmospheric dynamics. exploration program named MELOS, an acronym for “Mars Global, high-resolution and continuous mapping of water vapor, Exploration with Lander-Orbiter Synergy”1). As its name clouds, dusts and atmospheric temperature will be performed indicates, this is an ambitious mission composed of several with imaging cameras from the apoapsis of its highly elliptic landers and orbiters, schematically illustrated in Fig. -
Mars Mapping, Data Mining, Change Detection, GIS Mapping, Time Series Analysis
ISPRS Technical Commission IV Symposium on Geospatial Databases and Location Based Services, 14 – 16 May 2014, Suzhou, China, MTSTC4-2014-172-2 TEMPORAL ANALYSIS OF ALL AVAILABLE HIGH-RESOLUTION MARS IMAGING PRODUCTS SINCE 1976 Panagiotis Sidiropoulos1 and Jan-Peter Muller Mullard Space Science Laboratory, University College London, Holmbury St Mary, Surrey, RH56NT, UK [email protected], [email protected] Commission KEY WORDS: Mars mapping, data mining, change detection, GIS mapping, time series analysis ABSTRACT: Starting from Viking Orbiter 1, launched in August 1975, several mainly NASA orbiters have been sent to Mars to accomplish the robotic tasks of imaging its surface. Initial analyses of these early images indicated a planet with similar characteristics to the Moon pitted with craters and large volcanic and tectonic features but dead from a geological perspective. Recently, scientific interest has shifted towards high-resolution imaging, which allows the identification of previously undiscovered geological phenomena and surface features as well as the examination of surface composition and geological history. The increasing frequency of Mars orbiters, carrying high-resolution cameras, allows the dynamic analysis of Martian surface, i.e. the analysis of the temporal evolution of certain areas that reveal natural processes that happen over time. The latter can be roughly classified into two major categories; processes that happen periodically each and every Martian season (e.g. seasonal flows in high latitude areas (McEwen et al., 2011) and events that do not follow some iterative pattern but are rather sporadic (e.g. new impact craters (Byrne et al., 2009)). Consequently, it is beneficial to conduct a twin temporal grouping of Mars imaging products, the first examining product distribution through time, so as to point out areas that favor the search for sporadic events, and the second product distribution per season, to identify areas favouring the search for periodic events. -
Salt Triggered Melting of Permafrost in the Chaos Regions of Mars
Lunar and Planetary Science XXXVII (2006) 2218.pdf SALT TRIGGERED MELTING OF PERMAFROST IN THE CHAOS REGIONS OF MARS. Popa I.C., Università degli Studi "G. d'Annunzio" Chieti-Pescara, Pescara, Viale Pindaro 42, Italy. ([email protected]) Introduction: Mars surface bears traces of many landing site (Chryse Planitia) is the place where Ares fluvial-like features, geomorphic identified as outflow outflow channel is depositing its transporting channels, valley networks etc. Among these a particular materials. The following Martian landers Pathfinder one stands above others from the dimensional point of [6] and MER A Spirit [7], and MER B Opportunity [8] view. Outflow channels bear unique water erosion also revealed high soluble salts contents in places characteristics, that led Baker and Milton (1974) [1] to possibly genetically connected. Recently OMEGA believe that are caused by a surface runoff of large aboard Mars Express spacecraft has proven the amounts of water, in short geological time. Water existence of gypsum and other highly soluble salts (e.g origin, necessary for these processes was the topic of kieserite and epsomite) in localized deposits in places around Valles Marineris, and Iani Chaos [9]. many works. Among these theories one generally Freezing point depression of water solutions: accepted idea considers that water is originating from The freezing point of pure water at 1 bar is 0°C melting of permafrost layers positioned in the places of (273K). This melting point can be easily depressed by today chaos’. Here is an investigation that takes into adding impurities or soluble salts to the solvent. In the account the exoergic salt-ice dissolution reaction, along case of halite (NaCl) salt it is known that a 10% NaCl with freezing point depression of formed salty solutions, solution lowers the melting point of about -6°C (267K) as a complentary or a stand-alone process in chaos- and a 20% salt solution lowers it to -16°C (257K).