Topical Teams in the Life & Physical Sciences Towards New Research
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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. -
Special Catalogue Milestones of Lunar Mapping and Photography Four Centuries of Selenography on the Occasion of the 50Th Anniversary of Apollo 11 Moon Landing
Special Catalogue Milestones of Lunar Mapping and Photography Four Centuries of Selenography On the occasion of the 50th anniversary of Apollo 11 moon landing Please note: A specific item in this catalogue may be sold or is on hold if the provided link to our online inventory (by clicking on the blue-highlighted author name) doesn't work! Milestones of Science Books phone +49 (0) 177 – 2 41 0006 www.milestone-books.de [email protected] Member of ILAB and VDA Catalogue 07-2019 Copyright © 2019 Milestones of Science Books. All rights reserved Page 2 of 71 Authors in Chronological Order Author Year No. Author Year No. BIRT, William 1869 7 SCHEINER, Christoph 1614 72 PROCTOR, Richard 1873 66 WILKINS, John 1640 87 NASMYTH, James 1874 58, 59, 60, 61 SCHYRLEUS DE RHEITA, Anton 1645 77 NEISON, Edmund 1876 62, 63 HEVELIUS, Johannes 1647 29 LOHRMANN, Wilhelm 1878 42, 43, 44 RICCIOLI, Giambattista 1651 67 SCHMIDT, Johann 1878 75 GALILEI, Galileo 1653 22 WEINEK, Ladislaus 1885 84 KIRCHER, Athanasius 1660 31 PRINZ, Wilhelm 1894 65 CHERUBIN D'ORLEANS, Capuchin 1671 8 ELGER, Thomas Gwyn 1895 15 EIMMART, Georg Christoph 1696 14 FAUTH, Philipp 1895 17 KEILL, John 1718 30 KRIEGER, Johann 1898 33 BIANCHINI, Francesco 1728 6 LOEWY, Maurice 1899 39, 40 DOPPELMAYR, Johann Gabriel 1730 11 FRANZ, Julius Heinrich 1901 21 MAUPERTUIS, Pierre Louis 1741 50 PICKERING, William 1904 64 WOLFF, Christian von 1747 88 FAUTH, Philipp 1907 18 CLAIRAUT, Alexis-Claude 1765 9 GOODACRE, Walter 1910 23 MAYER, Johann Tobias 1770 51 KRIEGER, Johann 1912 34 SAVOY, Gaspare 1770 71 LE MORVAN, Charles 1914 37 EULER, Leonhard 1772 16 WEGENER, Alfred 1921 83 MAYER, Johann Tobias 1775 52 GOODACRE, Walter 1931 24 SCHRÖTER, Johann Hieronymus 1791 76 FAUTH, Philipp 1932 19 GRUITHUISEN, Franz von Paula 1825 25 WILKINS, Hugh Percy 1937 86 LOHRMANN, Wilhelm Gotthelf 1824 41 USSR ACADEMY 1959 1 BEER, Wilhelm 1834 4 ARTHUR, David 1960 3 BEER, Wilhelm 1837 5 HACKMAN, Robert 1960 27 MÄDLER, Johann Heinrich 1837 49 KUIPER Gerard P. -
A Ballistics Analysis of the Deep Impact Ejecta Plume: Determining Comet Tempel 1’S Gravity, Mass, and Density
Icarus 190 (2007) 357–390 www.elsevier.com/locate/icarus A ballistics analysis of the Deep Impact ejecta plume: Determining Comet Tempel 1’s gravity, mass, and density James E. Richardson a,∗,H.JayMeloshb, Carey M. Lisse c, Brian Carcich d a Center for Radiophysics and Space Research, Cornell University, Ithaca, NY 14853, USA b Lunar and Planetary Laboratory, University of Arizona, Tucson, AZ 85721-0092, USA c Planetary Exploration Group, Space Department, Johns Hopkins University Applied Physics Laboratory, 11100 Johns Hopkins Road, Laurel, MD 20723, USA d Center for Radiophysics and Space Research, Cornell University, Ithaca, NY 14853, USA Received 31 March 2006; revised 8 August 2007 Available online 15 August 2007 Abstract − In July of 2005, the Deep Impact mission collided a 366 kg impactor with the nucleus of Comet 9P/Tempel 1, at a closing speed of 10.2 km s 1. In this work, we develop a first-order, three-dimensional, forward model of the ejecta plume behavior resulting from this cratering event, and then adjust the model parameters to match the flyby-spacecraft observations of the actual ejecta plume, image by image. This modeling exercise indicates Deep Impact to have been a reasonably “well-behaved” oblique impact, in which the impactor–spacecraft apparently struck a small, westward-facing slope of roughly 1/3–1/2 the size of the final crater produced (determined from initial ejecta plume geometry), and possessing an effective strength of not more than Y¯ = 1–10 kPa. The resulting ejecta plume followed well-established scaling relationships for cratering in a medium-to-high porosity target, consistent with a transient crater of not more than 85–140 m diameter, formed in not more than 250–550 s, for the case of Y¯ = 0 Pa (gravity-dominated cratering); and not less than 22–26 m diameter, formed in not less than 1–3 s, for the case of Y¯ = 10 kPa (strength-dominated cratering). -
The Royal Danish Naval Museu
THE ROYAL DANISH NAVAL MUSEU An introduction to the History of th , Royal Danish Na~ Ole lisberg Jensen Royal Danish Naval Museum Copenhagen 1994 THE ROYAL DANISH NAVAL MUSEUM An introduction to the History of the Royal Danish Navy. Ole Lisberg Jensen Copyright: Ole Lisberg Jensen, 1994 Printed in Denmark by The Royal Danish Naval Museum and Amager Centraltrykkeri ApS Published by the Royal Danish Naval Museum ISBN 87-89322-18-5 Frontispiece: c. Neumann 1859 Danish naval vessel at anchor off the British coast. One of the first naval artists, Neumann sailed with the fleet on a summer expedition. Title: The famous Dutch battle artist, Willem van der Velde (the elder), sailed with the Dutch relief fleet to Copenhagen in October 1658. Here we see one of his sketches, showing 5 Danish naval vessels led by TREFOLDIGHED. Copenhagen is in the background. Photo: archives of the Royal Danish Naval Museum. Back cover: The building housing the Royal Danish Naval Museum at Christianshavns Ksnel was originally a hospital wing of the Sekveesthuset. In 1988-89, the building was converted for the use of the Royal Danish Naval Museum with the aid ofa magnificent donation from »TheA.P. Moller and Mrs. Chastine Meersk. Mckinney Moller's Foundation for General Purposes". The building was constructed in 1780 by master builder Schotmann. When it was handed over to the Royal Danish Naval Museum, the building passed from the responsibility of the Ministry of Defence to that of the Ministry of Culture. PREFACE This catalogue is meant as a contribution to an understan War the models were evacuated to Frederiksborg Slot, and it ding ofthe chronology ofthe exhibits in the Royal Danish Na was not until 1957that the Royal Danish Naval Museum was val Museum. -
October 2006
OCTOBER 2 0 0 6 �������������� http://www.universetoday.com �������������� TAMMY PLOTNER WITH JEFF BARBOUR 283 SUNDAY, OCTOBER 1 In 1897, the world’s largest refractor (40”) debuted at the University of Chica- go’s Yerkes Observatory. Also today in 1958, NASA was established by an act of Congress. More? In 1962, the 300-foot radio telescope of the National Ra- dio Astronomy Observatory (NRAO) went live at Green Bank, West Virginia. It held place as the world’s second largest radio scope until it collapsed in 1988. Tonight let’s visit with an old lunar favorite. Easily seen in binoculars, the hexagonal walled plain of Albategnius ap- pears near the terminator about one-third the way north of the south limb. Look north of Albategnius for even larger and more ancient Hipparchus giving an almost “figure 8” view in binoculars. Between Hipparchus and Albategnius to the east are mid-sized craters Halley and Hind. Note the curious ALBATEGNIUS AND HIPPARCHUS ON THE relationship between impact crater Klein on Albategnius’ southwestern wall and TERMINATOR CREDIT: ROGER WARNER that of crater Horrocks on the northeastern wall of Hipparchus. Now let’s power up and “crater hop”... Just northwest of Hipparchus’ wall are the beginnings of the Sinus Medii area. Look for the deep imprint of Seeliger - named for a Dutch astronomer. Due north of Hipparchus is Rhaeticus, and here’s where things really get interesting. If the terminator has progressed far enough, you might spot tiny Blagg and Bruce to its west, the rough location of the Surveyor 4 and Surveyor 6 landing area. -
Insights from Forested Catchments in South-Central Chile
Institute for Earth and Environmental Science Hydrological and erosion responses to man-made and natural disturbances – Insights from forested catchments in South-central Chile Dissertation submitted to the Faculty of Mathematics and Natural Sciences at the University of Potsdam, Germany for the degree of Doctor of Natural Sciences (Dr. rer. nat.) in Geoecology Christian Heinrich Mohr Potsdam, September 2013 This work is licensed under a Creative Commons License: Attribution - Noncommercial - Share Alike 3.0 Germany To view a copy of this license visit http://creativecommons.org/licenses/by-nc-sa/3.0/de/ Published online at the Institutional Repository of the University of Potsdam: URL http://opus.kobv.de/ubp/volltexte/2014/7014/ URN urn:nbn:de:kobv:517-opus-70146 http://nbn-resolving.de/urn:nbn:de:kobv:517-opus-70146 View from Nahuelbuta National park across the central inner valley towards the Sierra Velluda, close to the study area, Biobío region, Chile. Quien no conoce el bosque chileno, no conoce este planeta... Pablo Neruda The climate is moderate and delightful and if the country were to be cleared of forest, the warmth of ground would dissipate the moisture… The Scot Lord Thomas Cochrane commanding the Chilean navy in a letter to the Chilean independence leader Bernardo O’Higgins about the south of Chile, 1890, cited in [Bathurst, 2013] Preface When I started my PhD studies, my main intention was to contribute new knowledge about the impact of forest management practices on runoff and erosion processes. To this end, together with our Chilean colleagues, we established a network of forested catchments on the eastern slopes of the Chilean Coastal Range with water and sediment monitoring devices to quantify water and sediment fluxes associated with different forest management practices. -
View Responses of Scouts, Scout Leaders, and Scientists Who Were Scouts
ABSTRACT This study of science education in the Boy Scouts of America focused on males with Boy Scout experience. The mixed-methods study topics included: merit badge standards compared with National Science Education Standards, Scout responses to open-ended survey questions, the learning styles of Scouts, a quantitative assessment of science content knowledge acquisition using the Geology merit badge, and a qualitative analysis of interview responses of Scouts, Scout leaders, and scientists who were Scouts. The merit badge requirements of the 121 current merit badges were mapped onto the National Science Education Standards: 103 badges (85.12%) had at least one requirement meeting the National Science Education Standards. In 2007, Scouts earned 1,628,500 merit badges with at least one science requirement, including 72,279 Environmental Science merit badges. ―Camping‖ was the ―favorite thing about Scouts‖ for 54.4% of the boys who completed the survey. When combined with other outdoor activities, what 72.5% of the boys liked best about Boy Scouts involved outdoor activity. The learning styles of Scouts tend to include tactile and/or visual elements. Scouts were more global and integrated than analytical in their thinking patterns; they also had a significant intake element in their learning style. ii Earning a Geology merit badge at any location resulted in a significant gain of content knowledge; the combined treatment groups for all location types had a 9.13% gain in content knowledge. The amount of content knowledge acquired through the merit badge program varied with location; boys earning the Geology merit badge at summer camp or working as a troop with a merit badge counselor tended to acquire more geology content knowledge than boys earning the merit badge at a one-day event. -
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. -
Det Kongelige Bibliotek 130021678611
DET KONGELIGE BIBLIOTEK i 130021678611 TT i ‘ " . " 'V ■•-'- ' •’• :-• '. .. v j|E»<8gp*«arsR ? •'■ *fp■'■:'£'*■ ^ y y ■ • y y s . - -V -vV *■ r. '.- . •&. fy jv T 1 .-*,= +'■ - - & ■ ^ ~ v . ^ - fr V K . - , y - ■ S y y v y y c T /• J r , - i" ■ / \ n - * * ■«: . V“C v ' /« ' .. - ’i / i i - * 1 ^ '%). f : - 4„ ? N É f c — ■ V. c ■',-. £' * ''Vn': f '-' . • A ; ~ ’C ,1 • ' ■ r i - . - . i ”’ v ’ H . , *» *;. ; 1 ;*• ' ■;■. J. ‘I f y - --, . ». • . t v '* V . * • . : ' • • • • - y- =i .-■; .--»vt< ,i' y A f ' ■ y y > w t & - im m i i . ' i f • ? •3 * •' r. .-yty •* • w y *• s & S s ? « - * ; £ ' W v : ' ' p»*. • ■•• . '■ •-" » r- ■ - t & F " •V ? V ; X. ^ ..'_ i * ^ v * '* : ■ •;•:%• • ' - y .:.'V .'•. •' • " ' . : * ~ u .;*rr?i; ... .;• -. - *> ' ». * * ->s. .'*> - i / * f ' ■& ^ \. ■ ; v < * - * *•- v > ' <■■:■*. -• V ... .... .■■ i - - v • • V >■ -•. -v. ■: » . '7. ;•* N ; 7 •'••’ : *? '- f y -V ••* y y ; y i ■?; V ■»• .V V ’ ’ ° f J ’* n ,;?r Sf. Jg ; ■ >> f-r H ' ' • J * ■' ■ J«" r ■' * t?" < ' ' -?&. > *r ' .-U- J4- A ,\< 9 - - - ..;-< . ... v : , - ^ a v ^ v ;,-. y . u ' . V . • - * *■ . ' y - ' - ' -y-'t ~ - . '■ V , z * . !-*V .n. • ; ^ ■*.. - ■ A - -' -•• • i r r ». ‘ - > r > s >. ,• • v. ' - r» — „r- -. ... ;^ v - ■•-. , ".- _ ? f ''v : ry. y - . n>-- -'!{ . ‘ y - ■ • - _ - * y . ' V . i ■ ■■■ \ - "c.-... .,.<■-■ ■ ' - ' ":r r ‘ : ' l . :v t - ' i n ^ -s- • ' •<. "■‘■“-1*7 '-y - s - v « , . „ *r .-' '*<» ^ >' M ^ ' \ T r > ■••• - 1 * * >* - V v ' -.V -f: . s y j C ‘ 4 ; y * - •* • A t . - . y ^-i--■■'..yf -y f . A fy ^ c.-■ '"' f..... » --H * 4 y § : v ; u . > - •> *'■■■ •'* ‘ V- ' #■-•' .7 ry* - 'ps£T •>■.■* *':■*-•{- '.- /-,_' . i « : cm :.?;■ ■ . ^ V - ' y \ ~ y - • " f W >• t ^ " -~rf* ■ .« -*.. -V n f. y • s -. .. •; -7 n'. -
Lunar Distances Final
A (NOT SO) BRIEF HISTORY OF LUNAR DISTANCES: LUNAR LONGITUDE DETERMINATION AT SEA BEFORE THE CHRONOMETER Richard de Grijs Department of Physics and Astronomy, Macquarie University, Balaclava Road, Sydney, NSW 2109, Australia Email: [email protected] Abstract: Longitude determination at sea gained increasing commercial importance in the late Middle Ages, spawned by a commensurate increase in long-distance merchant shipping activity. Prior to the successful development of an accurate marine timepiece in the late-eighteenth century, marine navigators relied predominantly on the Moon for their time and longitude determinations. Lunar eclipses had been used for relative position determinations since Antiquity, but their rare occurrences precludes their routine use as reliable way markers. Measuring lunar distances, using the projected positions on the sky of the Moon and bright reference objects—the Sun or one or more bright stars—became the method of choice. It gained in profile and importance through the British Board of Longitude’s endorsement in 1765 of the establishment of a Nautical Almanac. Numerous ‘projectors’ jumped onto the bandwagon, leading to a proliferation of lunar ephemeris tables. Chronometers became both more affordable and more commonplace by the mid-nineteenth century, signaling the beginning of the end for the lunar distance method as a means to determine one’s longitude at sea. Keywords: lunar eclipses, lunar distance method, longitude determination, almanacs, ephemeris tables 1 THE MOON AS A RELIABLE GUIDE FOR NAVIGATION As European nations increasingly ventured beyond their home waters from the late Middle Ages onwards, developing the means to determine one’s position at sea, out of view of familiar shorelines, became an increasingly pressing problem. -
Sweden in the Seventeenth Century
Sweden in the Seventeenth Century Paul Douglas Lockhart Sweden in the Seventeenth Century European History in Perspective General Editor: Jeremy Black Benjamin Arnold Medieval Germany, 500–1300 Ronald Asch The Thirty Years’ War Christopher Bartlett Peace, War and the European Powers, 1814–1914 Robert Bireley The Refashioning of Catholicism, 1450–1700 Donna Bohanan Crown and Nobility in Early Modern France Arden Bucholz Moltke and the German Wars, 1864–1871 Patricia Clavin The Great Depression, 1929–1939 Paula Sutter Fichtner The Habsburg Monarchy, 1490–1848 Mark Galeotti Gorbachev and his Revolution David Gates Warfare in the Nineteenth Century Alexander Grab Napoleon and the Transformation of Europe Martin P. Johnson The Dreyfus Affair Paul Douglas Lockhart Sweden is the Seventeenth Century Peter Musgrave The Early Modern European Economy J.L. Price The Dutch Republic in the Seventeenth Century A.W. Purdue The Second World War Christopher Read The Making and Breaking of the Soviet System Francisco J. Romero-Salvado Twentieth-Century Spain Matthew S. Seligmann and Roderick R. McLean Germany from Reich to Republic, 1871–1918 Brendan Simms The Struggle for Mastery in Germany, 1779–1850 David Sturdy Louis XIV David J. Sturdy Richelieu and Mazarin Hunt Tooley The Western Front Peter Waldron The End of Imperial Russia, 1855–1917 Peter G. Wallace The Long European Reformation James D. White Lenin Patrick Williams Philip II European History in Perspective Series Standing Order ISBN 0–333–71694–9 hardcover ISBN 0–333–69336–1 paperback (outside North America only) You can receive future titles in this series as they are published by placing a standing order. -
Catalogue of Place Names in Northern East Greenland
Catalogue of place names in northern East Greenland In this section all officially approved, and many Greenlandic names are spelt according to the unapproved, names are listed, together with explana- modern Greenland orthography (spelling reform tions where known. Approved names are listed in 1973), with cross-references from the old-style normal type or bold type, whereas unapproved spelling still to be found on many published maps. names are always given in italics. Names of ships are Prospectors place names used only in confidential given in small CAPITALS. Individual name entries are company reports are not found in this volume. In listed in Danish alphabetical order, such that names general, only selected unapproved names introduced beginning with the Danish letters Æ, Ø and Å come by scientific or climbing expeditions are included. after Z. This means that Danish names beginning Incomplete documentation of climbing activities with Å or Aa (e.g. Aage Bertelsen Gletscher, Aage de by expeditions claiming ‘first ascents’ on Milne Land Lemos Dal, Åkerblom Ø, Ålborg Fjord etc) are found and in nunatak regions such as Dronning Louise towards the end of this catalogue. Å replaced aa in Land, has led to a decision to exclude them. Many Danish spelling for most purposes in 1948, but aa is recent expeditions to Dronning Louise Land, and commonly retained in personal names, and is option- other nunatak areas, have gained access to their al in some Danish town names (e.g. Ålborg or Aalborg region of interest using Twin Otter aircraft, such that are both correct). However, Greenlandic names be - the remaining ‘climb’ to the summits of some peaks ginning with aa following the spelling reform dating may be as little as a few hundred metres; this raises from 1973 (a long vowel sound rather than short) are the question of what constitutes an ‘ascent’? treated as two consecutive ‘a’s.