Rine and the Apennine Mountains. INSTITUTION National Aeronautics and Space Administration, Washington, D.C
Total Page:16
File Type:pdf, Size:1020Kb
Load more
Recommended publications
-
Report Resumes
REPORT RESUMES ED 019 218 88 SE 004 494 A RESOURCE BOOK OF AEROSPACE ACTIVITIES, K-6. LINCOLN PUBLIC SCHOOLS, NEBR. PUB DATE 67 EDRS PRICEMF.41.00 HC-S10.48 260P. DESCRIPTORS- *ELEMENTARY SCHOOL SCIENCE, *PHYSICAL SCIENCES, *TEACHING GUIDES, *SECONDARY SCHOOL SCIENCE, *SCIENCE ACTIVITIES, ASTRONOMY, BIOGRAPHIES, BIBLIOGRAPHIES, FILMS, FILMSTRIPS, FIELD TRIPS, SCIENCE HISTORY, VOCABULARY, THIS RESOURCE BOOK OF ACTIVITIES WAS WRITTEN FOR TEACHERS OF GRADES K-6, TO HELP THEM INTEGRATE AEROSPACE SCIENCE WITH THE REGULAR LEARNING EXPERIENCES OF THE CLASSROOM. SUGGESTIONS ARE MADE FOR INTRODUCING AEROSPACE CONCEPTS INTO THE VARIOUS SUBJECT FIELDS SUCH AS LANGUAGE ARTS, MATHEMATICS, PHYSICAL EDUCATION, SOCIAL STUDIES, AND OTHERS. SUBJECT CATEGORIES ARE (1) DEVELOPMENT OF FLIGHT, (2) PIONEERS OF THE AIR (BIOGRAPHY),(3) ARTIFICIAL SATELLITES AND SPACE PROBES,(4) MANNED SPACE FLIGHT,(5) THE VASTNESS OF SPACE, AND (6) FUTURE SPACE VENTURES. SUGGESTIONS ARE MADE THROUGHOUT FOR USING THE MATERIAL AND THEMES FOR DEVELOPING INTEREST IN THE REGULAR LEARNING EXPERIENCES BY INVOLVING STUDENTS IN AEROSPACE ACTIVITIES. INCLUDED ARE LISTS OF SOURCES OF INFORMATION SUCH AS (1) BOOKS,(2) PAMPHLETS, (3) FILMS,(4) FILMSTRIPS,(5) MAGAZINE ARTICLES,(6) CHARTS, AND (7) MODELS. GRADE LEVEL APPROPRIATENESS OF THESE MATERIALSIS INDICATED. (DH) 4:14.1,-) 1783 1490 ,r- 6e tt*.___.Vhf 1842 1869 LINCOLN PUBLICSCHOOLS A RESOURCEBOOK OF AEROSPACEACTIVITIES U.S. DEPARTMENT OF HEALTH, EDUCATION & WELFARE OFFICE OF EDUCATION K-6) THIS DOCUMENT HAS BEEN REPRODUCED EXACTLY AS RECEIVED FROM THE PERSON OR ORGANIZATION ORIGINATING IT.POINTS OF VIEW OR OPINIONS STATED DO NOT NECESSARILY REPRESENT OFFICIAL OFFICE OF EDUCATION POSITION OR POLICY. 1919 O O Vj A PROJECT FUNDED UNDER TITLE HIELEMENTARY AND SECONDARY EDUCATION ACT A RESOURCE BOOK OF AEROSPACE ACTIVITIES (K-6) The work presentedor reported herein was performed pursuant to a Grant from the U. -
S·O:3::~:~T~!E~~ W!~1~;Dmi~E Te~~- ~~:C:#R.:~~ I~Rt~:Rh~4I!I~Ts · ~Perin,~Ne 'R~9.Ioh ·± ~ .~I.G,Ll.T · I;>E J5est Aqhi'ev~Q:J
... , .~ ~70 10029 ~~. '' .. M ·]\.l;la~y~;:~,i·s o.f · th~ Sqi~:ntiiib D~TE: O<::tdbe.r 13, · 1970 ob:j e'¢.tive$· · and J?.:i;-OJ?ps~d +,.an~iin<J . s:i.. tes irt the. aadley.:.Ap,ennine Re:gion FROM: J . w. lie ad case:34o .) The possible scientiEic objectives at the Hadley~ Ap~nnine region a·re out:~ined: CI;J:ld incl,~de. tlle Ap.el}n:~ne Mo,un;t;;tins 1 H~dley. R.±l:le, mar.e mai;.erial~· lladleyf] c qr~·teri yol·can·ic ra:.Pd'"" :~;s·o:3::~:~t~!e~~ w!~1~;dmi~e te~~- ~~:C:#R.:~~ i~rt~:rH~4i!i~ts · ~perin,~ne 'r~9.ioh ·± ~ .~i.g,ll.t · i;>e J5est aqhi'ev~q:j . ·ba$¢d: on cli;ff.e;temt .irit¢]tpret:a~ions of t:h~. origin {Jf :J:hese va,r$.o\lS fe~tures. Five la'ii~i:hg po;iri·ts are evcl;:l:U.atea: in terms of· t:J:ie, ..$:1;:1,3, ty to acnlev¢ the 'sq;lentific o_bjectfves bo~ on a rover .and a walkil19 mii.s;.. sion. ·c .0 ,.... :.. ..,... .. ··ti:]9::ijii11·-·· uncla:s 12811' .B"'E~I¥-:t,;.;CPM~M • .INC. • ss5· ~;ENFAt4T' P~~~~~I~~::s:y;1 . ~As~IW~ro~~ o:.C: -~01)2~.· .. SUBJECT! oAT£: octo.b~r 1:3~ · 1970 .FROMi j.· W. Head t. GEN:E!M:4 li'~cii~yt~Ap~ni1.ine · 'l'h.~ ~pepf!irie Mol;tn-ta.in!3 rise. up to -~' km· above th.e. -
Bombardment History of the Moon: What We Think We Know and What We Don’T Know Donald Bogard, ARES-KR, NASA-JSC, Houston, TX 77058 ([email protected])
Planetary Chronology Workshop 2006 6001.pdf Bombardment History of the Moon: What We Think We Know and What We Don’t Know Donald Bogard, ARES-KR, NASA-JSC, Houston, TX 77058 ([email protected]) Summary. The absolute impact history of and 14 soils show a decrease in the number of the moon and inner solar system can in principle beads with age from ~4 Gyr ago to ~0.4 Gyr ago, be derived from the statistics of radiometric ages followed by a significant increase in beads with of shock-heated planetary samples (lunar or age <0.4 Gyr (2). These authors concluded that meteoritic), from the formation ages of specific the projectile flux had decreased over time, impact craters on the moon or Earth; and from followed by a significant flux increase more age-dating samples representing geologic surface recently. However, this data set has also been units on the moon (or Mars) for which crater interpreted to represent variable rates of impact densities have been determined. This impact melt production as a function of regolith maturity history, however, is still poorly defined. (3). In another study, measured ages of 21 small The heavily cratered surface of the moon is a impact melt clasts in four lunar meteorites from testimony to the importance of impact events in the lunar highlands suggested four to six impact the evolution of terrestrial planets and satellites. events over the period ~2.5-4.0 Gyr ago (4). Lunar impacts range in scale from an early Clearly considerable uncertainty exists in the intense flux of large objects that defined the projectile flux over the past ~3.5 Gyr and whether surface geology of the moon, down to recent, this flux has been approximately constant or smaller impacts that continually generate and exhibited appreciable shorter-term variations. -
Exploring the Bombardment History of the Moon
EXPLORING THE BOMBARDMENT HISTORY OF THE MOON Community White Paper to the Planetary Decadal Survey, 2011-2020 September 15, 2009 Primary Author: William F. Bottke Center for Lunar Origin and Evolution (CLOE) NASA Lunar Science Institute at the Southwest Research Institute 1050 Walnut St., Suite 300 Boulder, CO 80302 Tel: (303) 546-6066 [email protected] Co-Authors/Endorsers: Carlton Allen (NASA JSC) Mahesh Anand (Open U., UK) Nadine Barlow (NAU) Donald Bogard (NASA JSC) Gwen Barnes (U. Idaho) Clark Chapman (SwRI) Barbara A. Cohen (NASA MSFC) Ian A. Crawford (Birkbeck College London, UK) Andrew Daga (U. North Dakota) Luke Dones (SwRI) Dean Eppler (NASA JSC) Vera Assis Fernandes (Berkeley Geochronlogy Center and U. Manchester) Bernard H. Foing (SMART-1, ESA RSSD; Dir., Int. Lunar Expl. Work. Group) Lisa R. Gaddis (US Geological Survey) 1 Jim N. Head (Raytheon) Fredrick P. Horz (LZ Technology/ESCG) Brad Jolliff (Washington U., St Louis) Christian Koeberl (U. Vienna, Austria) Michelle Kirchoff (SwRI) David Kring (LPI) Harold F. (Hal) Levison (SwRI) Simone Marchi (U. Padova, Italy) Charles Meyer (NASA JSC) David A. Minton (U. Arizona) Stephen J. Mojzsis (U. Colorado) Clive Neal (U. Notre Dame) Laurence E. Nyquist (NASA JSC) David Nesvorny (SWRI) Anne Peslier (NASA JSC) Noah Petro (GSFC) Carle Pieters (Brown U.) Jeff Plescia (Johns Hopkins U.) Mark Robinson (Arizona State U.) Greg Schmidt (NASA Lunar Science Institute, NASA Ames) Sen. Harrison H. Schmitt (Apollo 17 Astronaut; U. Wisconsin-Madison) John Spray (U. New Brunswick, Canada) Sarah Stewart-Mukhopadhyay (Harvard U.) Timothy Swindle (U. Arizona) Lawrence Taylor (U. Tennessee-Knoxville) Ross Taylor (Australian National U., Australia) Mark Wieczorek (Institut de Physique du Globe de Paris, France) Nicolle Zellner (Albion College) Maria Zuber (MIT) 2 The Moon is unique. -
Italy's Abruzzo National Park - Wildlife Festival
The Apennines: Italy's Abruzzo National Park - Wildlife Festival Naturetrek Tour Itinerary Outline itinerary Day 1 Fly Rome and transfer to Pescasseroli Day 2/7 A programme of wildlife walks in the Abruzzo National Park from Pescasseroli Day 8 Transfer to Rome and fly London Departs May 2019 Focus Mammals, plants, birds, and butterflies Grading Day walks only with different options offered daily Prices See website (tour code ITA06) or brochure Highlights Look for Marsican Brown Bear, Wolf and Apennine Chamois. Enjoy a myriad of plants, butterflies and birds in the Apennines. Enjoy daily walks in this stunning National Park. Look for Great Sooty Satyr, Blue-spot Hairstreak and numerous other butterflies. Birds may include Golden Eagle, Wryneck, Red- backed Shrike and Rock Thrush. Led by multiple expert Naturetrek leaders. Abruzzo Chamois, Lady Slipper Orchid (Lee Morgan) Marsican Brown Bear (Paolo Iannicca). Naturetrek Mingledown Barn Wolf’s Lane Chawton Alton Hampshire GU34 3HJ UK T: +44 (0)1962 733051 E: [email protected] W: www.naturetrek.co.uk The Apennines: Italy's Abruzzo National Park – Wildlife Festival Introduction Stretching the length of Italy, the Apennine Mountains provide a refuge for much of Italy’s most interesting natural history. This is very much a working rural landscape of rolling hills and traditional sheep farming, made special by its wealth of atmospheric mediaeval villages, traditional cuisine and aromatic local wines, all of which combine to make this holiday a well-rounded and enjoyable Italian experience. Set in the heart of the Apennines is the Abruzzo National Park, established by royal decree in 1923 and today protecting an area of 400 square kilometres. -
January 2019 Cardanus & Krafft
A PUBLICATION OF THE LUNAR SECTION OF THE A.L.P.O. EDITED BY: Wayne Bailey [email protected] 17 Autumn Lane, Sewell, NJ 08080 RECENT BACK ISSUES: http://moon.scopesandscapes.com/tlo_back.html FEATURE OF THE MONTH – JANUARY 2019 CARDANUS & KRAFFT Sketch and text by Robert H. Hays, Jr. - Worth, Illinois, USA September 24, 2018 04:40-05:04 UT, 15 cm refl, 170x, seeing 7/10, transparence 6/6. I drew these craters and vicinity on the night of Sept. 23/24, 2018. The moon was about 22 hours before full. This area is in far western Oceanus Procellarum, and was favorably placed for observation that night. Cardanus is the southern one of this pair and is of moderate depth. Krafft to the north is practically identical in size, and is perhaps slightly deeper. Neither crater has a central peak. Several small craters are near and within Krafft. The crater just outside the southeast rim of Krafft is Krafft E, and Krafft C is nearby within Krafft. The small pit to the west is Krafft K, and Krafft D is between Krafft and Cardanus. Krafft C, D and E are similar sized, but K is smaller than these. A triangular-shaped swelling protrudes from the north side of Krafft. The tiny pit, even smaller than Krafft K, east of Cardanus is Cardanus E. There is a dusky area along the southwest side of Cardanus. Two short dark strips in this area may be part of the broken ring Cardanus R as shown on the. Lunar Quadrant map. -
TRANSIENT LUNAR PHENOMENA: REGULARITY and REALITY Arlin P
The Astrophysical Journal, 697:1–15, 2009 May 20 doi:10.1088/0004-637X/697/1/1 C 2009. The American Astronomical Society. All rights reserved. Printed in the U.S.A. TRANSIENT LUNAR PHENOMENA: REGULARITY AND REALITY Arlin P. S. Crotts Department of Astronomy, Columbia University, Columbia Astrophysics Laboratory, 550 West 120th Street, New York, NY 10027, USA Received 2007 June 27; accepted 2009 February 20; published 2009 April 30 ABSTRACT Transient lunar phenomena (TLPs) have been reported for centuries, but their nature is largely unsettled, and even their existence as a coherent phenomenon is controversial. Nonetheless, TLP data show regularities in the observations; a key question is whether this structure is imposed by processes tied to the lunar surface, or by terrestrial atmospheric or human observer effects. I interrogate an extensive catalog of TLPs to gauge how human factors determine the distribution of TLP reports. The sample is grouped according to variables which should produce differing results if determining factors involve humans, and not reflecting phenomena tied to the lunar surface. Features dependent on human factors can then be excluded. Regardless of how the sample is split, the results are similar: ∼50% of reports originate from near Aristarchus, ∼16% from Plato, ∼6% from recent, major impacts (Copernicus, Kepler, Tycho, and Aristarchus), plus several at Grimaldi. Mare Crisium produces a robust signal in some cases (however, Crisium is too large for a “feature” as defined). TLP count consistency for these features indicates that ∼80% of these may be real. Some commonly reported sites disappear from the robust averages, including Alphonsus, Ross D, and Gassendi. -
A Comparative Analysis of the Geology Tools Used During the Apollo Lunar Program and Their Suitability for Future Missions to the Om on Lindsay Kathleen Anderson
University of North Dakota UND Scholarly Commons Theses and Dissertations Theses, Dissertations, and Senior Projects January 2016 A Comparative Analysis Of The Geology Tools Used During The Apollo Lunar Program And Their Suitability For Future Missions To The oM on Lindsay Kathleen Anderson Follow this and additional works at: https://commons.und.edu/theses Recommended Citation Anderson, Lindsay Kathleen, "A Comparative Analysis Of The Geology Tools Used During The Apollo Lunar Program And Their Suitability For Future Missions To The oonM " (2016). Theses and Dissertations. 1860. https://commons.und.edu/theses/1860 This Thesis is brought to you for free and open access by the Theses, Dissertations, and Senior Projects at UND Scholarly Commons. It has been accepted for inclusion in Theses and Dissertations by an authorized administrator of UND Scholarly Commons. For more information, please contact [email protected]. A COMPARATIVE ANALYSIS OF THE GEOLOGY TOOLS USED DURING THE APOLLO LUNAR PROGRAM AND THEIR SUITABILITY FOR FUTURE MISSIONS TO THE MOON by Lindsay Kathleen Anderson Bachelor of Science, University of North Dakota, 2009 A Thesis Submitted to the Graduate Faculty of the University of North Dakota in partial fulfillment of the requirements for the degree of Master of Science Grand Forks, North Dakota May 2016 Copyright 2016 Lindsay Anderson ii iii PERMISSION Title A Comparative Analysis of the Geology Tools Used During the Apollo Lunar Program and Their Suitability for Future Missions to the Moon Department Space Studies Degree Master of Science In presenting this thesis in partial fulfillment of the requirements for a graduate degree from the University of North Dakota, I agree that the library of this University shall make it freely available for inspection. -
Discovery Marche.Pdf
the MARCHE region Discovering VADEMECUM FOR THE TOURIST OF THE THIRD MILLENNIUM Discovering THE MARCHE REGION MARCHE Italy’s Land of Infinite Discovery the MARCHE region “...For me the Marche is the East, the Orient, the sun that comes at dawn, the light in Urbino in Summer...” Discovering Mario Luzi (Poet, 1914-2005) Overlooking the Adriatic Sea in the centre of Italy, with slightly more than a million and a half inhabitants spread among its five provinces of Ancona, the regional seat, Pesaro and Urbino, Macerata, Fermo and Ascoli Piceno, with just one in four of its municipalities containing more than five thousand residents, the Marche, which has always been Italyʼs “Gateway to the East”, is the countryʼs only region with a plural name. Featuring the mountains of the Apennine chain, which gently slope towards the sea along parallel val- leys, the region is set apart by its rare beauty and noteworthy figures such as Giacomo Leopardi, Raphael, Giovan Battista Pergolesi, Gioachino Rossini, Gaspare Spontini, Father Matteo Ricci and Frederick II, all of whom were born here. This guidebook is meant to acquaint tourists of the third millennium with the most important features of our terri- tory, convincing them to come and visit Marche. Discovering the Marche means taking a path in search of beauty; discovering the Marche means getting to know a land of excellence, close at hand and just waiting to be enjoyed. Discovering the Marche means discovering a region where both culture and the environment are very much a part of the Made in Marche brand. 3 GEOGRAPHY On one side the Apen nines, THE CLIMATE od for beach tourism is July on the other the Adriatic The regionʼs climate is as and August. -
Why NASA Consistently Fails at Congress
W&M ScholarWorks Undergraduate Honors Theses Theses, Dissertations, & Master Projects 6-2013 The Wrong Right Stuff: Why NASA Consistently Fails at Congress Andrew Follett College of William and Mary Follow this and additional works at: https://scholarworks.wm.edu/honorstheses Part of the Political Science Commons Recommended Citation Follett, Andrew, "The Wrong Right Stuff: Why NASA Consistently Fails at Congress" (2013). Undergraduate Honors Theses. Paper 584. https://scholarworks.wm.edu/honorstheses/584 This Honors Thesis is brought to you for free and open access by the Theses, Dissertations, & Master Projects at W&M ScholarWorks. It has been accepted for inclusion in Undergraduate Honors Theses by an authorized administrator of W&M ScholarWorks. For more information, please contact [email protected]. The Wrong Right Stuff: Why NASA Consistently Fails at Congress A thesis submitted in partial fulfillment of the requirement for the degree of Bachelors of Arts in Government from The College of William and Mary by Andrew Follett Accepted for . John Gilmour, Director . Sophia Hart . Rowan Lockwood Williamsburg, VA May 3, 2013 1 Table of Contents: Acknowledgements 3 Part 1: Introduction and Background 4 Pre Soviet Collapse: Early American Failures in Space 13 Pre Soviet Collapse: The Successful Mercury, Gemini, and Apollo Programs 17 Pre Soviet Collapse: The Quasi-Successful Shuttle Program 22 Part 2: The Thin Years, Repeated Failure in NASA in the Post-Soviet Era 27 The Failure of the Space Exploration Initiative 28 The Failed Vision for Space Exploration 30 The Success of Unmanned Space Flight 32 Part 3: Why NASA Fails 37 Part 4: Putting this to the Test 87 Part 5: Changing the Method. -
Modification of the Lunar Surface Composition by Micro-Meteorite Impact Vaporization and Sputtering
EPSC Abstracts Vol. 13, EPSC-DPS2019-705-1, 2019 EPSC-DPS Joint Meeting 2019 c Author(s) 2019 Modification of the lunar surface composition by micro-meteorite impact vaporization and sputtering Audrey Vorburger (1), Peter Wurz (1), André Galli (1), Manuel Scherf (2), and Helmut Lammer (2) (1) Physikalisches Institut, University of Bern, Bern, Switzerland ([email protected]), (2) Space Research Institute, Austrian Academy of Sciences, Graz, Austria Abstract Late Heavy Bombardment model with a half-life time of 100 Myr. Time steps vary between 25 Myr (at the Over the past 4.5 billion years the Moon has been un- beginning) and 560 Myr (today). der constant bombardment by solar wind particles and The only required inputs for this study are the orig- micro-meteorites. These impactors liberate surface inal surface composition, the solar wind particle flux, material into space, and, over time, result in a modi- the solar UV flux, and the micro-meteorite impact rate. fication of the surface composition due to the species’ For the surface composition we implement at t=0 (at different loss rates. Here we model the loss of the the beginning) the BSE composition according to [3]. 7 major lunar surface elements over the past 4.5 bil- We run the simulations for O, Mg, Si, Fe, Al, Ca, and lion years and show how the lunar surface composition K, which together make up more than 99% of today’s changed over time. lunar soil [4]. After each time step we compute for each species the fraction lost from the lunar regolith, 1. -
Mannville Group of Saskatchewan
Saskatchewan Report 223 Industry and Resources Saskatchewan Geological Survey Jura-Cretaceous Success Formation and Lower Cretaceous Mannville Group of Saskatchewan J.E. Christopher 2003 19 48 Printed under the authority of the Minister of Industry and Resources Although the Department of Industry and Resources has exercised all reasonable care in the compilation, interpretation, and production of this report, it is not possible to ensure total accuracy, and all persons who rely on the information contained herein do so at their own risk. The Department of Industry and Resources and the Government of Saskatchewan do not accept liability for any errors, omissions or inaccuracies that may be included in, or derived from, this report. Cover: Clearwater River Valley at Contact Rapids (1.5 km south of latitude 56º45'; latitude 109º30'), Saskatchewan. View towards the north. Scarp of Middle Devonian Methy dolomite at right. Dolomite underlies the Lower Cretaceous McMurray Formation outcrops recessed in the valley walls. Photo by J.E. Christopher. Additional copies of this digital report may be obtained by contacting: Saskatchewan Industry and Resources Publications 2101 Scarth Street, 3rd floor Regina, SK S4P 3V7 (306) 787-2528 FAX: (306) 787-2527 E-mail: [email protected] Recommended Citation: Christopher, J.E. (2003): Jura-Cretaceous Success Formation and Lower Cretaceous Mannville Group of Saskatchewan; Sask. Industry and Resources, Report 223, CD-ROM. Editors: C.F. Gilboy C.T. Harper D.F. Paterson RnD Technical Production: E.H. Nickel M.E. Opseth Production Editor: C.L. Brown Saskatchewan Industry and Resources ii Report 223 Foreword This report, the first on CD to be released by the Petroleum Geology Branch, describes the geology of the Success Formation and the Mannville Group wherever these units are present in Saskatchewan.