NATURE [Dec. 7, 1871
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Former Astronaut Visits Stennis
Volume 7 Issue 8 www.nasa.gov/centers/stennis August 2012 Touchdown! Take it both ways – the Mars Science Laboratory rover, Curiosity, touched Sharp at a height of about 3.4 miles, taller than Mount Whitney in California. down on the surface of Mars early on the morning of Aug. 6 CDT, and the The Curiosity team hopes to drive the rover to the mountain to investigate NASA team scored a very big touchdown for space exploration. This image its lower layers, which scientists think hold clues to past environmental taken by Curiosity shows what lies ahead for the rover – its main science change. This image was captured by a rover camera shortly after it landed. target, Mount Sharp. The rover’s shadow can be seen in the foreground, It has been linearized to remove the distorted appearance that results from and the dark bands beyond are dunes. Rising up in the distance is Mount its fisheye lens. For additional coverage and photos, see pages 4-7. Page 2 LAGNIAPPE August 2012 “NASA is in a unique position to excite and inspire students about STEM education, and to help grow our technical workforce.” From the desk of Katie Wallace Director, Office of Education, Stennis Space Center he Mars Science Laboratory’s successful land- and over 8,000 students and parents. Our workshops ing on Mars early Aug. 6 was a huge engi- have a satisfaction rating of 99 percent. Tneering accomplishment! Years of research, planning, collaboration and dedication came down to In addition, we focus on student activities that enrich seven minutes. -
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. -
Glossary Glossary
Glossary Glossary Albedo A measure of an object’s reflectivity. A pure white reflecting surface has an albedo of 1.0 (100%). A pitch-black, nonreflecting surface has an albedo of 0.0. The Moon is a fairly dark object with a combined albedo of 0.07 (reflecting 7% of the sunlight that falls upon it). The albedo range of the lunar maria is between 0.05 and 0.08. The brighter highlands have an albedo range from 0.09 to 0.15. Anorthosite Rocks rich in the mineral feldspar, making up much of the Moon’s bright highland regions. Aperture The diameter of a telescope’s objective lens or primary mirror. Apogee The point in the Moon’s orbit where it is furthest from the Earth. At apogee, the Moon can reach a maximum distance of 406,700 km from the Earth. Apollo The manned lunar program of the United States. Between July 1969 and December 1972, six Apollo missions landed on the Moon, allowing a total of 12 astronauts to explore its surface. Asteroid A minor planet. A large solid body of rock in orbit around the Sun. Banded crater A crater that displays dusky linear tracts on its inner walls and/or floor. 250 Basalt A dark, fine-grained volcanic rock, low in silicon, with a low viscosity. Basaltic material fills many of the Moon’s major basins, especially on the near side. Glossary Basin A very large circular impact structure (usually comprising multiple concentric rings) that usually displays some degree of flooding with lava. The largest and most conspicuous lava- flooded basins on the Moon are found on the near side, and most are filled to their outer edges with mare basalts. -
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,. 1. I , Har,.-apy (HC) icrofichs (MF) ff 063 July 06 i I BIBLIOGRAPHY OF CHE&CAL PRODUCTS OF VOLCANISM prepared by Paul Pushkar and Paul E. Damon - Prepared for the National Aeronautics and Space Administration (SC - NGR - 03 - 002 - 076) Laboratory of Geochronometry and Geochemistry Geochronology Department University of Arizona IE ie (PAGES) ,g1: Qjf-- 910 73 , (NASX~ROR TMX OR AD NUMBER) i BIBLIOGRAPHY OF CHEMICAL PRODUCTS OF VOLCANISM prepared by Paul Pushkar and Paul E. Damon Prepared for the National Aeronautics and Space Administration (SC - NGR - 03- 002 - 076) Laboratory of Geochronometry and Geochemistry Geochronology Department University of Arizona +. s i i Lunar Orbiter IV, Frame No. 157 THE EjARIUS HILLS: A LUNAR VOLCANIC FIELD? '- sa 3 TABLE OF CONTENTS Page Preface. 8 . i Acknowledgments . * a e . e i I Volcanic Gases and Sublimates, Gases Contained in Rocks, and Related Matters . e . 1 II Nongaseous Chemical Products of Terrestrial Volcanism . III Gas Content of Meteorites, Lunar Volcanfsm, and Related Subjects . 46 IV General References Dealing with Terrestrial Volcanism . 53 PREFACE This bibliography was compiled during a one-year literature search on possible volcanic products on the Moon. The bibliography is divided into four sections: I. Volcanic Gases and Sublimates, Gases Contained in Rocks, and Related Matters The literature in these fields, as emphasized recently by White and Waring (1963) is scanty, and for the most part by fiussian and Japanese scientists arid hence often presents difficulties in access and language to English-specking scientists. This section is believed to be fairly com- prehensive from the present to at least 1935. -
Ensory a Teacher’S Learning Guide to Multi Sensory LEARNING Improving Literacy by Engaging the Senses
Education A Teacher’s Guide to multisensory Guide to Multi A Teacher’s LEARNING Improving Literacy by Engaging the Senses ow can teachers help students develop the literacy skills that are H necessary for learning and retaining information in any subject? Traditional memory tricks, mnemonic devices, graphic organizers, and A Teacher’s Guide to role-playing do little to turn bored or reluctant students into enthusiastic learners. In A Teacher's Guide to Multisensory Learning: Improving Literacy by Engaging the Senses, Lawrence Baines shows teachers how to engage students through hands-on, visual, auditory, and olfactory stimuli and link the activities sensory multisensory to relevant academic objectives. Throughout the book, you’ll find real classroom examples of how teachers use multisensory learning techniques to help students interact with material more intensely and retain what they learn for longer periods of time. Baines provides a wide variety of engaging Learning lesson plans to keep students motivated, such as LEARNING • Scent of my Soul—helps students learn expository writing through a Improving Literacy by Engaging the Senses series of sensory lessons and encourages them to investigate a subject of infinite interest—themselves! • Between the Ears—develops students’ ability to infer and deduce by working with their own drawings • Film Score—teaches the art of persuasive writing through the emotional appeal of music • Adagio Suite—encourages students to expand their critical thinking through sight, sound, and touch Seventeen additional lessons plans from Baines and experts in the field are complemented with practical assessments and strategies for engaging students’ sense of play. Baines For teachers who are ready to energize their classrooms, this book is an invaluable resource for expanding students' capacity to learn and helping them cultivate essential skills that will last a lifetime. -
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 -
Drug-Rich Phases Induced by Amorphous Solid Dispersion: Arbitrary Or Intentional Goal in Oral Drug Delivery?
pharmaceutics Review Drug-Rich Phases Induced by Amorphous Solid Dispersion: Arbitrary or Intentional Goal in Oral Drug Delivery? Kaijie Qian 1 , Lorenzo Stella 2,3 , David S. Jones 1, Gavin P. Andrews 1,4, Huachuan Du 5,6,* and Yiwei Tian 1,* 1 Pharmaceutical Engineering Group, School of Pharmacy, Queen’s University Belfast, 97 Lisburn Road, Belfast BT9 7BL, UK; [email protected] (K.Q.); [email protected] (D.S.J.); [email protected] (G.P.A.) 2 Atomistic Simulation Centre, School of Mathematics and Physics, Queen’s University Belfast, 7–9 College Park E, Belfast BT7 1PS, UK; [email protected] 3 David Keir Building, School of Chemistry and Chemical Engineering, Queen’s University Belfast, Stranmillis Road, Belfast BT9 5AG, UK 4 School of Pharmacy, China Medical University, No.77 Puhe Road, Shenyang North New Area, Shenyang 110122, China 5 Laboratory of Applied Mechanobiology, Department of Health Sciences and Technology, ETH Zurich, Vladimir-Prelog-Weg 4, 8093 Zurich, Switzerland 6 Simpson Querrey Institute, Northwestern University, 303 East Superior Street, 11th Floor, Chicago, IL 60611, USA * Correspondence: [email protected] (H.D.); [email protected] (Y.T.); Tel.: +41-446339049 (H.D.); +44-2890972689 (Y.T.) Abstract: Among many methods to mitigate the solubility limitations of drug compounds, amor- Citation: Qian, K.; Stella, L.; Jones, phous solid dispersion (ASD) is considered to be one of the most promising strategies to enhance D.S.; Andrews, G.P.; Du, H.; Tian, Y. the dissolution and bioavailability of poorly water-soluble drugs. -
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Julie Mitchell1* and Philip Christensen1
#1624 Recurring Slope Lineae and Chlorides in the Southern Hemisphere of Mars Julie Mitchell1* and Philip Christensen1 1Arizona State University, 201 E. Orange Mall, Tempe, AZ, 85281 *[email protected] Introduction Results Conclusions • Recurring Slope Lineae (RSL): candidates for Confirmed RSL were mapped at each location listed in Table 1 and as shown in Figure 3. Palikir Crater was the most The lack of chloride signatures collocated with liquid water on the martian surface [1] distinct locale, showing local evidence of chlorides in areas where RSL were most densely located (Figure 4). This RSL in the Southern hemisphere could be the • RSL peak activity during southern summer [1, 2] locale has also shown periodic evidence of ferric iron in the near-infrared [8]. For all RSL, DCS chloride signatures result of one of three scenarios: • RSL active below H O freezing point → brine 2 did not correlate to the presence of RSL on the regional scale. In some cases, such as Triolet Crater, neither local- nor flow? 1. RSL may not contain chlorides, either because • CaCl , MgCl : most likely compounds in brine [3] regional-scale evidence of chlorides was observed (Figure 5). 2 2 they a) are not aqueous flow features or b) are The purpose of this study is to investigate the not chloride-based brines. likelihood that RSL are formed by chloride Nearest Named HiRISE ID THEMIS ID brines. Crater 2. Several locales are dominated by the distinct Palikir ESP_022267_1380 I34263004 steep-slope signature in THEMIS DCS identified by Bandfield [10]; the fact that the Tivat ESP_013624_1335 I17599005 many RSL occur on the steep crater walls Pickering (SW) ESP_022820_1415 I17966002 supports this scenario (Figure 5, right). -
Infrastructure and Everyday Life in Paris, 1870-1914
The Fragility of Modernity: Infrastructure and Everyday Life in Paris, 1870-1914 by Peter S. Soppelsa A dissertation submitted in partial fulfillment of the requirements for the degree of Doctor of Philosophy (History) in The University of Michigan 2009 Doctoral Committee: Associate Professor Joshua H. Cole, Co-Chair Associate Professor Gabrielle Hecht, Co-Chair Professor Richard Abel Professor Geoffrey H. Eley Associate Professor Dario Gaggio Copyright 2009 Peter S. Soppelsa For Jen, who saw me through the whole project. ii Contents Dedication ii List of Figures iv Introduction: Modernity, Infrastructure and Everyday Life 1 Chapter 1: Paris, Modernity and Haussmann 35 Part One: Circulation, The Flow of Traffic 99 Chapter 2: The Dream Life of the Métropolitain, 1872-1895 107 Chapter 3: Paris Under Construction, 1895-1914 182 Part Two: Hygiene, The Flow of Light, Air, Water and Waste 253 Chapter 4: Opening the City: Housing, Hygiene and Urban Density 265 Chapter 5: Flows of Water and Waste 340 Conclusion: The Fragility of Modernity 409 Bibliography 423 iii List of Figures Figure 1: Morice's Marianne on the Place de la République 74 Figure 2: The departmental commission's 1872 Métro plan 120 Figure 3: A standard CGO horse-powered tram 122 Figure 4: CGO Mékarski system compressed air tram, circa 1900 125 Figure 5: Francq's locomotive sans foyer 127 Figure 6: Albert Robida, L'Embellissement de Paris par le métropolitain (1886) 149 Figure 7: Jules Garnier’s Haussmannized Viaduct, 1884 153 Figure 8: From Louis Heuzé's 1878 Pamphlet 154 Figure 9: From Louis Heuzé's 1878 Pamphlet 154 Figure 10: Le Chatelier's 1889 Métro Plan 156 Figure 11: 1890 Métro plan from Eiffel and the North Railway Company 163 Figure 12: J.B. -
Facts & Features Lunar Surface Elevations Six Apollo Lunar
Greek Mythology Quadrants Maria & Related Features Lunar Surface Elevations Facts & Features Selene is the Moon and 12 234 the goddess of the Moon, 32 Diameter: 2,160 miles which is 27.3% of Earth’s equatorial diameter of 7,926 miles 260 Lacus daughter of the titans 71 13 113 Mare Frigoris Mare Humboldtianum Volume: 2.03% of Earth’s volume; 49 Moons would fit inside Earth 51 103 Mortis Hyperion and Theia. Her 282 44 II I Sinus Iridum 167 125 321 Lacus Somniorum Near Side Mass: 1.62 x 1023 pounds; 1.23% of Earth’s mass sister Eos is the goddess 329 18 299 Sinus Roris Surface Area: 7.4% of Earth’s surface area of dawn and her brother 173 Mare Imbrium Mare Serenitatis 85 279 133 3 3 3 Helios is the Sun. Selene 291 Palus Mare Crisium Average Density: 3.34 gm/cm (water is 1.00 gm/cm ). Earth’s density is 5.52 gm/cm 55 270 112 is often pictured with a 156 Putredinis Color-coded elevation maps Gravity: 0.165 times the gravity of Earth 224 22 237 III IV cresent Moon on her head. 126 Mare Marginis of the Moon. The difference in 41 Mare Undarum Escape Velocity: 1.5 miles/sec; 5,369 miles/hour Selenology, the modern-day 229 Oceanus elevation from the lowest to 62 162 25 Procellarum Mare Smythii Distances from Earth (measured from the centers of both bodies): Average: 238,856 term used for the study 310 116 223 the highest point is 11 miles. -
304 Index Index Index
_full_alt_author_running_head (change var. to _alt_author_rh): 0 _full_alt_articletitle_running_head (change var. to _alt_arttitle_rh): 0 _full_article_language: en 304 Index Index Index Adamson, Robert (1821–1848) 158 Astronomische Gesellschaft 216 Akkasbashi, Reza (1843–1889) viiii, ix, 73, Astrolog 72 75-78, 277 Astronomical unit, the 192-94 Airy, George Biddell (1801–1892) 137, 163, 174 Astrophysics xiv, 7, 41, 57, 118, 119, 139, 144, Albedo 129, 132, 134 199, 216, 219 Aldrin, Edwin Buzz (1930) xii, 244, 245, 248, Atlas Photographique de la Lune x, 15, 126, 251, 261 127, 279 Almagestum Novum viii, 44-46, 274 Autotypes 186 Alpha Particle Spectrometer 263 Alpine mountains of Monte Rosa and BAAS “(British Association for the Advance- the Zugspitze, the 163 ment of Science)” 26, 27, 125, 128, 137, Al-Biruni (973–1048) 61 152, 158, 174, 277 Al-Fath Muhammad Sultan, Abu (n.d.) 64 BAAS Lunar Committee 125, 172 Al-Sufi, Abd al-Rahman (903–986) 61, 62 Bahram Mirza (1806–1882) 72 Al-Tusi, Nasir al-Din (1202–1274) 61 Baillaud, Édouard Benjamin (1848–1934) 119 Amateur astronomer xv, 26, 50, 51, 56, 60, Ball, Sir Robert (1840–1913) 147 145, 151 Barlow Lens 195, 203 Amir Kabir (1807–1852) 71 Barnard, Edward Emerson (1857–1923) 136 Amir Nezam Garusi (1820–1900) 87 Barnard Davis, Joseph (1801–1881) 180 Analysis of the Moon’s environment 239 Beamish, Richard (1789–1873) 178-81 Andromeda nebula xii, 208, 220-22 Becker, Ernst (1843–1912) 81 Antoniadi, Eugène M. (1870–1944) 269 Beer, Wilhelm Wolff (1797–1850) ix, 54, 56, Apollo Missions NASA 32, 231, 237, 239, 240, 60, 123, 124, 126, 130, 139, 142, 144, 157, 258, 261, 272 190 Apollo 8 xii, 32, 239-41 Bell Laboratories 270 Apollo 11 xii, 59, 237, 240, 244-46, 248-52, Beg, Ulugh (1394–1449) 63, 64 261, 280 Bergedorf 207 Apollo 13 254 Bergedorfer Spektraldurchmusterung 216 Apollo 14 240, 253-55 Biancani, Giuseppe (n.d.) 40, 274 Apollo 15 255 Biot, Jean Baptiste (1774–1862) 1,8, 9, 121 Apollo 16 240, 255-57 Birt, William R.