JPL Will Build Mars Rover to Fly In
Total Page:16
File Type:pdf, Size:1020Kb
Load more
Recommended publications
-
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. -
Martian Crater Morphology
ANALYSIS OF THE DEPTH-DIAMETER RELATIONSHIP OF MARTIAN CRATERS A Capstone Experience Thesis Presented by Jared Howenstine Completion Date: May 2006 Approved By: Professor M. Darby Dyar, Astronomy Professor Christopher Condit, Geology Professor Judith Young, Astronomy Abstract Title: Analysis of the Depth-Diameter Relationship of Martian Craters Author: Jared Howenstine, Astronomy Approved By: Judith Young, Astronomy Approved By: M. Darby Dyar, Astronomy Approved By: Christopher Condit, Geology CE Type: Departmental Honors Project Using a gridded version of maritan topography with the computer program Gridview, this project studied the depth-diameter relationship of martian impact craters. The work encompasses 361 profiles of impacts with diameters larger than 15 kilometers and is a continuation of work that was started at the Lunar and Planetary Institute in Houston, Texas under the guidance of Dr. Walter S. Keifer. Using the most ‘pristine,’ or deepest craters in the data a depth-diameter relationship was determined: d = 0.610D 0.327 , where d is the depth of the crater and D is the diameter of the crater, both in kilometers. This relationship can then be used to estimate the theoretical depth of any impact radius, and therefore can be used to estimate the pristine shape of the crater. With a depth-diameter ratio for a particular crater, the measured depth can then be compared to this theoretical value and an estimate of the amount of material within the crater, or fill, can then be calculated. The data includes 140 named impact craters, 3 basins, and 218 other impacts. The named data encompasses all named impact structures of greater than 100 kilometers in diameter. -
Appendix I Lunar and Martian Nomenclature
APPENDIX I LUNAR AND MARTIAN NOMENCLATURE LUNAR AND MARTIAN NOMENCLATURE A large number of names of craters and other features on the Moon and Mars, were accepted by the IAU General Assemblies X (Moscow, 1958), XI (Berkeley, 1961), XII (Hamburg, 1964), XIV (Brighton, 1970), and XV (Sydney, 1973). The names were suggested by the appropriate IAU Commissions (16 and 17). In particular the Lunar names accepted at the XIVth and XVth General Assemblies were recommended by the 'Working Group on Lunar Nomenclature' under the Chairmanship of Dr D. H. Menzel. The Martian names were suggested by the 'Working Group on Martian Nomenclature' under the Chairmanship of Dr G. de Vaucouleurs. At the XVth General Assembly a new 'Working Group on Planetary System Nomenclature' was formed (Chairman: Dr P. M. Millman) comprising various Task Groups, one for each particular subject. For further references see: [AU Trans. X, 259-263, 1960; XIB, 236-238, 1962; Xlffi, 203-204, 1966; xnffi, 99-105, 1968; XIVB, 63, 129, 139, 1971; Space Sci. Rev. 12, 136-186, 1971. Because at the recent General Assemblies some small changes, or corrections, were made, the complete list of Lunar and Martian Topographic Features is published here. Table 1 Lunar Craters Abbe 58S,174E Balboa 19N,83W Abbot 6N,55E Baldet 54S, 151W Abel 34S,85E Balmer 20S,70E Abul Wafa 2N,ll7E Banachiewicz 5N,80E Adams 32S,69E Banting 26N,16E Aitken 17S,173E Barbier 248, 158E AI-Biruni 18N,93E Barnard 30S,86E Alden 24S, lllE Barringer 29S,151W Aldrin I.4N,22.1E Bartels 24N,90W Alekhin 68S,131W Becquerei -
In Pdf Format
lós 1877 Mik 88 ge N 18 e N i h 80° 80° 80° ll T 80° re ly a o ndae ma p k Pl m os U has ia n anum Boreu bal e C h o A al m re u c K e o re S O a B Bo l y m p i a U n d Planum Es co e ria a l H y n d s p e U 60° e 60° 60° r b o r e a e 60° l l o C MARS · Korolev a i PHOTOMAP d n a c S Lomono a sov i T a t n M 1:320 000 000 i t V s a Per V s n a s l i l epe a s l i t i t a s B o r e a R u 1 cm = 320 km lkin t i t a s B o r e a a A a A l v s l i F e c b a P u o ss i North a s North s Fo d V s a a F s i e i c a a t ssa l vi o l eo Fo i p l ko R e e r e a o an u s a p t il b s em Stokes M ic s T M T P l Kunowski U 40° on a a 40° 40° a n T 40° e n i O Va a t i a LY VI 19 ll ic KI 76 es a As N M curi N G– ra ras- s Planum Acidalia Colles ier 2 + te . -
Australian and New Zealand Guidelines for the Management of Chronic Obstructive Pulmonary Disease 2017
The COPD-X Plan: Australian and New Zealand Guidelines for the management of Chronic Obstructive Pulmonary Disease 2017 Current COPD Guidelines Committee Professor Ian Yang, MBBS(Hons), PhD, FRACP, Grad Dip Clin Epid, FAPSR, FThorSoc, Thoracic Physician, The Prince Charles Hospital and The University of Queensland, Brisbane, QLD (Chair) Dr Eli Dabscheck, MBBS, M Clin Epi, FRACP, Staff Specialist, Department of Allergy, Immunology and Respiratory Medicine, The Alfred Hospital, Melbourne, VIC (Deputy Chair) Dr Johnson George, BPharm, MPharm, PhD, Grad Cert Higher Education, Senior Lecturer, Faculty of Pharmacy and Pharmaceutical Sciences, Monash University, Melbourne, VIC Dr Sue Jenkins, GradDipPhys, PhD, Institute for Respiratory Health; Physiotherapy Department, Sir Charles Gairdner Hospital; Adjunct Professor, School of Physiotherapy and Exercise Science, Curtin University, Perth, WA Professor Christine McDonald, FAHMS, MBBS(Hons), PhD, FRACP, FThorSoc, Director, Department of Respiratory and Sleep Medicine, Austin Hospital, Melbourne, VIC Professor Vanessa McDonald DipHlthScien (Nurs), BNurs, PhD, Professor of Chronic Disease Nursing, Centre for Healthy Lungs, School of Nursing and Midwifery, The University of Newcastle; Academic Clinician, Department of Respiratory and Sleep Medicine, John Hunter Hospital, Newcastle, NSW Professor Brian Smith, MBBS, Dip Clin Ep & Biostats, PhD, FRACP, Thoracic Physician, The Queen Elizabeth Hospital, Adelaide, SA Professor Nick Zwar, MBBS, MPH, PhD, FRACGP, Professor of General Practice, School Public -
Horizons 27 Winter 2011 Volume 35 Number 3 We're Forty Years Strong! Special(Anniversary(Issue
Horizons 27 Winter 2011 Volume 35 Number 3 We're forty years strong! Special(Anniversary(Issue Travel program reinstated Visit New York City Members receive variety of awards Choir and bridge start another season District 27 President chosen for Board of RTO/ ERO Charitable Foundation RTO/ERO District 27 Ottawa-Carleton Communications Committee A word from the Co-Editors Chair Carol Barazzuol This issue of Horizons 27 includes anniversary news and Magazine Carol Barazzuol, Stuart Fraser, Lyndi McDonald pictures. As well, we have a special supplement highlighting Translation Samir Khordoc, Lise Renault our history throughout the years. As members of Ottawa-Carleton Website Stuart Fraser RTO/ERO, we should all be proud of our members and their Editing Committee Stuart Fraser and Carol participation in both local and Samir Khordoc, Murray Kitts, Barazzuol work on this edition. provincial activities. John Knobel, Roger Lalonde Editorial Policies HORIZONS 27 is published three times a year – spring , fall and winter. Its purpose is to provide information to members on matters of current interest, both within District 27 and at the provincial level. It is your magazine. Human interest stories, reports of travels or literary efforts of interest to members, by members and about members are always welcomed. No magazine? The editorial committee reserves the right to modify any Changed address or e-mail? submission to determine the appropriateness of the submission New to the area? and to fit the space available in a particular issue. The views Moving away? expressed by the authors do not necessarily reflect those of RTO/ ERO. Contact Janet Booren 613-256-4031 [email protected] If you do not want your photograph included in the Horizons 27 or magazine or on our district website, please indicate so to the Contact Toronto at 1-800-361-9888 photographers at the various social events. -
The Social Significance of Artistic Representations of Former Coal and Steel Communities
THE SOCIAL SIGNIFICANCE OF ARTISTIC REPRESENTATIONS OF FORMER COAL AND STEEL COMMUNITIES PETER HENRY DAVIES THIS THESIS IS SUBMITTED IN CANDIDATURE FOR THE DEGREE OF DOCTOR OF PHILOSOPHY DECEMBER 2018 SCHOOL OF SOCIAL SCIENCES CARDIFF UNIVERSITY Declaration This work has not been submitted in substance for any other degree or award at this or any other university or place of learning, nor is being submitted concurrently in candidature for any degree or other award. Signed ……………………………………… (candidate) Date…09/05/2019…………….… STATEMENT 1 This thesis is being submitted in partial fulfilment of the requirements for the degree of PhD. Signed ……………………………………..... .(candidate) Date …09/05/2019…………….. STATEMENT 2 This thesis is the result of my own independent work/investigation, except where otherwise stated, and the thesis has not been edited by a third party beyond what is permitted by Cardiff University’s Policy on the Use of Third Party Editors by Research Degree Students. Other sources are acknowledged by explicit references. The views expressed are my own. Signed ……………………………………… (candidate) Date …09/05/2019…………… STATEMENT 3 I hereby give consent for my thesis, if accepted, to be available online in the University’s Open Access repository and for inter-library loan, and for the title and summary to be made available to outside organisations. Signed …………………….………………... (candidate) Date …09/05/2019…………… i Acknowledgements Completing a PhD thesis has been likened to climbing a mountain and there have certainly been some uphill moments along this journey, made immeasurably easier by the help and inspiration provided by my supervisors Eva Elliott, Kate Pahl and Valerie Walkerdine. -
Mineralogy and Fluvial History of the Watersheds of Gale, Knobel
PUBLICATIONS Geophysical Research Letters RESEARCH LETTER Mineralogy and fluvial history of the watersheds 10.1002/2014GL062553 of Gale, Knobel, and Sharp craters: A regional Key Points: context for the Mars Science Laboratory • Olivine- and Fe/Mg phyllosilicate-bearing bedrock throughout the watersheds Curiosity’s exploration • Watershed Fe/Mg phyllosilicates different from Mount Sharp Bethany L. Ehlmann1,2 and Jennifer Buz1 • Intermittent, increasingly localized fl Hesperian/Amazonian uvial activity 1Division of Geological and Planetary Sciences, California Institute of Technology, Pasadena, California, USA, 2Jet Propulsion Laboratory, California Institute of Technology, Pasadena, California, USA Supporting Information: • Figure S1 Abstract A 500 km long network of valleys extends from Herschel crater to Gale, Knobel, and Sharp craters. Correspondence to: The mineralogy and timing of fluvial activity in these watersheds provide a regional framework for deciphering B. L. Ehlmann, the origin of sediments of Gale crater’s Mount Sharp, an exploration target for the Curiosity rover. Olivine-bearing [email protected] bedrock is exposed throughout the region, and its erosion contributed to widespread olivine-bearing sand dunes. Fe/Mg phyllosilicates are found in both bedrock and sediments, implying that materials deposited in Citation: Gale crater may have inherited clay minerals, transported from the watershed. While some topographic lows Ehlmann, B. L., and J. Buz (2015), Mineralogy and fluvial history of the watersheds of of the Sharp-Knobel watershed host chloride salts, the only salts detected in the Gale watershed are sulfates Gale, Knobel, and Sharp craters: A regional within Mount Sharp, implying regional or temporal differences in water chemistry. Crater counts indicate context for the Mars Science Laboratory progressively more spatially localized aqueous activity: large-scale valley network activity ceased by the early ’ Curiositysexploration,Geophys. -
Evidence for Late Alluvial Activity in Gale Crater, Mars
Evidence for late alluvial activity in Gale crater, Mars John A. Grant 1, and Sharon A. Wilson 1 1Center for Earth and Planetary Studies, National Air and Space Museum, Smithsonian Institution, Washington, DC, USA. Corresponding author: John A. Grant ([email protected]). Key Points: Local alluvial deposits in Gale crater were likely emplaced less than 2 Ga, post-dating more widespread water-related deposits in Gale. Water associated with the younger alluvial deposits may be related to late-occurring diagenetic activity. Alluvial deposits formed when Aeolis Mons achieved its present expression, suggesting late-occurring habitable conditions within Gale. 1 Abstract The occurrence of past habitable conditions in Gale crater is generally associated with lacustrine and alluvial environments present >3 Ga ago, during the Hesperian Period on Mars. However, later-occurring aqueous activity is consistent with superposition relations between some alluvial deposits and bounding materials on the crater walls, preservation of fine-scale morphology on these alluvial deposits, and their superposing crater densities. The alluvial deposits include some not previously considered, and collectively lend confidence to the interpretation that local aqueous activity persisted in Gale crater into the Amazonian, or <2 Ga ago. Our conclusions are generally in accordance with late aqueous activity inferred from geochronology data (Martin et al., 2017), in addition to late alluvial activity elsewhere. Interpreted late aqueous activity points to possible habitable settings in Gale later than previously recognized. Plain Language Summary Several fan-shaped deposits on the walls and floor of Gale crater formed via deposition of water transported sediment. Overall, the fan deposits are fairly well preserved, and the number of impact craters on their surfaces indicate they are much younger (~2 billion years old or less) relative to the older, more widespread water-related deposits that formed in the crater over 3 billion years ago. -
Transactions of the APST for the Year 1894
TRANSACTIONS OF THE Astronomical and Physical Society of Toronto, FOR THE YEAR 1894, INCLUDING FIFTH ANNUAL REPORT. PRICE ONE DOLLAR. TORONTO: ROWSELL & HUTCHISON, Printers to the Society. 1895. CHARLES CARPMAEL, M. A. (CANTAB.) TRANSACTIONS OF THE Astronomical and Physical Society of Toronto, FOR THE YEAR 1894, INCLUDING FIFTH ANNUAL REPORT. PRICE ONE DOLLAR. TORONTO: ROWSELL & HUTCHISON, Printers to the Society. 1895. CORRIGENDA. Transactions, 1S90, page 29, line S from bottom, for “ Jupiter ” read “ Neptune.” Transactions, 1891, page 5, line 11 from top, for “ B.C. 380 ” read “ B.C. 310.” Transactions, 1893, page 59, line 9 from top, for “ 7 p.m. ” read “ 11.15 p.m.” Transactions, 1893, page 67, line 3 from bottom, value of comp, log n' should be “ 2.2132633.” Transactions, 1894, page 16, line 3 from top, for “ 1.500th ” read “ l - 500th.” “ “ “ line 5, for “ 1.250th ” read “ l-250th.” Transactions, 1894, page 31, line 14 from top, for “ two angles” read “ three angles. ” TABLE OF CONTENTS. PAGE. Officers ............................................. .......................................... V Council ............................................. .......................................... V Life Members..................................... .......................................... V Honourary Members ...................... .......................................... VI Corresponding Members................... .......................................... VI Active Members and their Addresses .................................... VII Associate -
The Antiquarian Astronomer
The Antiquarian Astronomer Journal of the Society for the History of Astronomy Issue 9 August 2015 ISSN 1740–3677 The Antiquarian Astronomer Journal of the Society for the History of Astronomy On the cover: Conjuring with Mars Two giants of Mars observation stand side-by-side on our cover: Giovanni Virginio Schiaparelli (1835–1910), who at the close opposition of Mars in 1877 saw linear markings on the planet’s red surface that he termed canali; and on the right Percival Lowell (1855–1916), who transformed Schiaparelli’s enigmatic lines into what he regarded as a global network of canals dug by intelligent beings to irrigate a parched planet. They were illusions – really, delusions – that danced in the eyepiece at the hazy limit where imagination supplanted perception. Percival Lowell’s vivid vision of an inhabited Mars, colourfully articulated in popular books and lectures, was one of the most romantic, yet hopelessly flawed, notions of 20th-century astronomy. Firmly entrenched in public consciousness long after it had been rejected by planetary scientists, the fanciful fiction of life on Mars foreshadowed the widespread belief in alien life today. Its social impact was expressed most famously in the public panic sparked by the famous War of the Worlds radio broadcast by Orson Welles in 1938, staged so convincingly that some listeners were persuaded that the Earth was indeed under attack from hostile Martians. See Mars: The History of a Master Illusionist by William Sheehan, on page 12 of this issue. Top right: Giovanni Virginio Schiaparelli, as he looked in 1880. Painting by Maestro G. -
Topographic Map of Mars
U.S. DEPARTMENT OF THE INTERIOR OPEN-FILE REPORT 02-282 U.S. GEOLOGICAL SURVEY Prepared for the NATIONAL AERONAUTICS AND SPACE ADMINISTRATION 180° 0° 55° –55° Russell Stokes 150°E NOACHIS 30°E 210°W 330°W 210°E NOTES ON BASE smooth global color look-up table. Note that the chosen color scheme simply 330°E Darwin 150°W This map is based on data from the Mars Orbiter Laser Altimeter (MOLA) 30°W — 60° represents elevation changes and is not intended to imply anything about –60° Chalcoporous v (Smith and others 2001), an instrument on NASA’s Mars Global Surveyor Milankovic surface characteristics (e.g. past or current presence of water or ice). These two (MGS) spacecraft (Albee and others 2001). The image used for the base of this files were then merged and scaled to 1:25 million for the Mercator portion and Rupes map represents more than 600 million measurements gathered between 1999 1:15,196,708 for the two Polar Stereographic portions, with a resolution of 300 and 2001, adjusted for consistency (Neumann and others 2001 and 2002) and S dots per inch. The projections have a common scale of 1:13,923,113 at ±56° TIA E T converted to planetary radii. These have been converted to elevations above the latitude. N S B LANI O A O areoid as determined from a martian gravity field solution GMM2 (Lemoine Wegener a R M S s T u and others 2001), truncated to degree and order 50, and oriented according to IS s NOMENCLATURE y I E t e M i current standards (see below).