Sixth Microgravity Fluid Physics and Transport Phenomena Conference Abstracts
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No Change in the Recent Lunar Impact Flux Required Based On
Geophysical Research Letters RESEARCH LETTER No Change in the Recent Lunar Impact Flux Required Based 10.1029/2018GL077254 on Modeling of Impact Glass Spherule Age Distributions Key Points: • An excess of young lunar impact glass Ya-Huei Huang1 , David A. Minton1, Nicolle E. B. Zellner2 , Masatoshi Hirabayashi3 , spherules <500 Ma likely results from 4 5 limited sampling depths where lunar James E. Richardson , and Caleb I. Fassett soils were collected • Sampling biases can explain the 1Department of Earth, Atmospheric, and Planetary Science, Purdue University, West Lafayette, IN, USA, 2Department of excess of young spherules, rather than Physics, Albion College, Albion, MI, USA, 3Department of Aerospace Engineering, Auburn University, Auburn, AL, USA, a significant change in the impact flux 4Planetary Science Institute, Tucson, AZ, USA, 5NASA Marshall Space Flight Center, Huntsville, AL, USA in the last 500 Ma • Using lunar impact glass spherule ages to constrain the impact flux may 40 39 be less biased if collected beyond the Abstract The distributions of Ar/ Ar-derived ages of impact glass spherules in lunar regolith uppermost lunar surface samples show an excess at <500 Ma relative to older ages. It has not been well understood whether this excess of young ages reflects an increase in the recent lunar impact flux or is due to a bias in the samples. Supporting Information: We developed a model to simulate the production, transport, destruction, and sampling of lunar glass • Supporting Information S1 spherules. A modeled bias is seen when either (1) the simulated sampling depth is 10 cm, consistent with the typical depth from which Apollo soil samples were taken, or (2) when glass occurrence in the ejecta is > Correspondence to: limited to 10 crater radii from the crater, consistent with terrestrial microtektite observations. -
Physics Department Newsletter February 2015
PHYSICS DEPARTMENT NEWSLETTER FEBRUARY 2015 ON THE MOVE Physics student combines science and dance to teach new concepts Scientific exploration is growing by leaps, in the university’s 2014 SpringDance, and also the molecules — or dancers — reacted in bounds and pirouettes thanks to a Kansas acted as a liaison between the two disciplines. certain ways. “I could see them absorbing it,” State University undergraduate student. “I don’t see either field as deeply as the Phillips said. “I’ve heard them tell each other, Daniel Phillips, senior in physics and nuclear experts, but I know enough about each that ‘we turn this way because,’ and explain the engineering, Kaiser, Oregon, is using his I can guide them toward the middle,” Phillips science correctly. If you can teach people dual interests in physics and dance to help said. The second act was polished before the science in a way that relates to their interests, performers discover scientific concepts. “The 2014 WinterDance performance. Phillips has it’s a powerful tool.” Phillips added that one personality of a performer is not necessarily transitioned from a performer to a rehearsal of the best ways in which to learn is to teach conducive to sitting in a lecture hall and assistant, helping dancers with techniques. the subject to someone else. In his research, getting talked at about physics,” Phillips said. Additionally, Phillips has begun his own it’s twofold — not only is he deepening his “I wanted to see if there was a viable way to research using the ballet as a method to teach physics knowledge by teaching the dancers, teach science through performance art to physics to the dancers. -
BEYOND Alumni Share How the Gordon and Judy Dutile Honors Program Has Prepared Them for a Lifetime of Excellence
A B O V E &BEYOND Alumni share how the Gordon and Judy Dutile Honors Program has prepared them for a lifetime of excellence INSIDE: 2015 PRESIDENT’S REPORT PB SBUlife Winter 2015 www.SBUniv.edu SBUlife 1 >> Be Social Read what students are sharing about SBU. sbu is the best; they brought We had a FANTASTIC visit day to- puppies to the union for us to play day with 90+ on campus! Thanks with #sbuniv for making the time to come! (via @elizaburris on Instagram) #futurebearcats #SBUniv @ SBU_Kim Awesome job @SBUbearcatsWBB!! We are so proud of you girls!! Great win!! #bearcatroar #SBUniv @Dewey_Dogger Love this university. Being sur- rounded by so many people who have a deep desire to serve Jesus is truly incredible. #SBUniv @sward2013 In honor of finals and first semester being over, #tbt to when we first became a family. #woodythird #woodygott #sbuniv (via @mary_rose_18 on Instagram) Good morning, SBU. #sbuniv #jantermsnotsobad #midwestisbest (via @courtney_kliment on Instagram) Check out “The Hub” – Southwest Baptist University’s social media mash-up site showcasing what people are saying about SBU online. Go to social.SBUniv.edu to see Facebook, Twitter, Instagram, YouTube and news release postings all in one place. And be sure to use #SBUniv when you post about SBU on social media and you may see your post featured on “The Hub” as well! Be social with SBU on Twitter, Facebook, 2 SBUlife Google+ and Instagram. #SBUniv Winter 2015 www.SBUniv.edu SBUlife 3 SBUlife Magazine of Southwest Baptist University Winter 2016 10th Anniversary of the Gordon and Judy Dutile Honors Program 2 5 Questions with Diana Gallamore 4 Guess Who? 22 SBU News 23 Keeping in Touch 24 Volume 101 Issue 1 ADDRESS CHANGE SBUlife highlights the University’s mission: to be USPS 507-500 POSTMASTER: Send address changes to a Christ-centered, caring academic community SBU 1600 University Avenue, preparing students to be servant leaders in a global PRESIDENT Bolivar, MO 65613-2597 society. -
DMAAC – February 1973
LUNAR TOPOGRAPHIC ORTHOPHOTOMAP (LTO) AND LUNAR ORTHOPHOTMAP (LO) SERIES (Published by DMATC) Lunar Topographic Orthophotmaps and Lunar Orthophotomaps Scale: 1:250,000 Projection: Transverse Mercator Sheet Size: 25.5”x 26.5” The Lunar Topographic Orthophotmaps and Lunar Orthophotomaps Series are the first comprehensive and continuous mapping to be accomplished from Apollo Mission 15-17 mapping photographs. This series is also the first major effort to apply recent advances in orthophotography to lunar mapping. Presently developed maps of this series were designed to support initial lunar scientific investigations primarily employing results of Apollo Mission 15-17 data. Individual maps of this series cover 4 degrees of lunar latitude and 5 degrees of lunar longitude consisting of 1/16 of the area of a 1:1,000,000 scale Lunar Astronautical Chart (LAC) (Section 4.2.1). Their apha-numeric identification (example – LTO38B1) consists of the designator LTO for topographic orthophoto editions or LO for orthophoto editions followed by the LAC number in which they fall, followed by an A, B, C or D designator defining the pertinent LAC quadrant and a 1, 2, 3, or 4 designator defining the specific sub-quadrant actually covered. The following designation (250) identifies the sheets as being at 1:250,000 scale. The LTO editions display 100-meter contours, 50-meter supplemental contours and spot elevations in a red overprint to the base, which is lithographed in black and white. LO editions are identical except that all relief information is omitted and selenographic graticule is restricted to border ticks, presenting an umencumbered view of lunar features imaged by the photographic base. -
Byzantium and France: the Twelfth Century Renaissance and the Birth of the Medieval Romance
University of Tennessee, Knoxville TRACE: Tennessee Research and Creative Exchange Doctoral Dissertations Graduate School 12-1992 Byzantium and France: the Twelfth Century Renaissance and the Birth of the Medieval Romance Leon Stratikis University of Tennessee - Knoxville Follow this and additional works at: https://trace.tennessee.edu/utk_graddiss Part of the Modern Languages Commons Recommended Citation Stratikis, Leon, "Byzantium and France: the Twelfth Century Renaissance and the Birth of the Medieval Romance. " PhD diss., University of Tennessee, 1992. https://trace.tennessee.edu/utk_graddiss/2521 This Dissertation is brought to you for free and open access by the Graduate School at TRACE: Tennessee Research and Creative Exchange. It has been accepted for inclusion in Doctoral Dissertations by an authorized administrator of TRACE: Tennessee Research and Creative Exchange. For more information, please contact [email protected]. To the Graduate Council: I am submitting herewith a dissertation written by Leon Stratikis entitled "Byzantium and France: the Twelfth Century Renaissance and the Birth of the Medieval Romance." I have examined the final electronic copy of this dissertation for form and content and recommend that it be accepted in partial fulfillment of the equirr ements for the degree of Doctor of Philosophy, with a major in Modern Foreign Languages. Paul Barrette, Major Professor We have read this dissertation and recommend its acceptance: James E. Shelton, Patrick Brady, Bryant Creel, Thomas Heffernan Accepted for the Council: Carolyn R. Hodges Vice Provost and Dean of the Graduate School (Original signatures are on file with official studentecor r ds.) To the Graduate Council: I am submitting herewith a dissertation by Leon Stratikis entitled Byzantium and France: the Twelfth Century Renaissance and the Birth of the Medieval Romance. -
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 -
The Composition of the Lunar Crust: Radiative Transfer Modeling and Analysis of Lunar Visible and Near-Infrared Spectra
THE COMPOSITION OF THE LUNAR CRUST: RADIATIVE TRANSFER MODELING AND ANALYSIS OF LUNAR VISIBLE AND NEAR-INFRARED SPECTRA A DISSERTATION SUBMITTED TO THE GRADUATE DIVISION OF THE UNIVERSITY OF HAWAI‘I IN PARTIAL FULFILLMENT OF THE REQUIREMENTS FOR THE DEGREE OF DOCTOR OF PHILOSOPHY IN GEOLOGY AND GEOPHYSICS DECEMBER 2009 By Joshua T.S. Cahill Dissertation Committee: Paul G. Lucey, Chairperson G. Jeffrey Taylor Patricia Fryer Jeffrey J. Gillis-Davis Trevor Sorensen Student: Joshua T.S. Cahill Student ID#: 1565-1460 Field: Geology and Geophysics Graduation date: December 2009 Title: The Composition of the Lunar Crust: Radiative Transfer Modeling and Analysis of Lunar Visible and Near-Infrared Spectra We certify that we have read this dissertation and that, in our opinion, it is satisfactory in scope and quality as a dissertation for the degree of Doctor of Philosophy in Geology and Geophysics. Dissertation Committee: Names Signatures Paul G. Lucey, Chairperson ____________________________ G. Jeffrey Taylor ____________________________ Jeffrey J. Gillis-Davis ____________________________ Patricia Fryer ____________________________ Trevor Sorensen ____________________________ ACKNOWLEDGEMENTS I must first express my love and appreciation to my family. Thank you to my wife Karen for providing love, support, and perspective. And to our little girl Maggie who only recently became part of our family and has already provided priceless memories in the form of beautiful smiles, belly laughs, and little bear hugs. The two of you provided me with the most meaningful reasons to push towards the "finish line". I would also like to thank my immediate and extended family. Many of them do not fully understand much about what I do, but support the endeavor acknowledging that if it is something I’m willing to put this much effort into, it must be worthwhile. -
User Guide to 1:250,000 Scale Lunar Maps
CORE https://ntrs.nasa.gov/search.jsp?R=19750010068Metadata, citation 2020-03-22T22:26:24+00:00Z and similar papers at core.ac.uk Provided by NASA Technical Reports Server USER GUIDE TO 1:250,000 SCALE LUNAR MAPS (NASA-CF-136753) USE? GJIDE TO l:i>,, :LC h75- lu1+3 SCALE LUNAR YAPS (Lumoalcs Feseclrch Ltu., Ottewa (Ontario) .) 24 p KC 53.25 CSCL ,33 'JIACA~S G3/31 11111 DANNY C, KINSLER Lunar Science Instltute 3303 NASA Road $1 Houston, TX 77058 Telephone: 7131488-5200 Cable Address: LUtiSI USER GUIDE TO 1: 250,000 SCALE LUNAR MAPS GENERAL In 1972 the NASA Lunar Programs Office initiated the Apollo Photographic Data Analysis Program. The principal point of this program was a detailed scientific analysis of the orbital and surface experiments data derived from Apollo missions 15, 16, and 17. One of the requirements of this program was the production of detailed photo base maps at a useable scale. NASA in conjunction with the Defense Mapping Agency (DMA) commenced a mapping program in early 1973 that would lead to the production of the necessary maps based on the need for certain areas. This paper is designed to present in outline form the neces- sary background informatiox or users to become familiar with the program. MAP FORMAT * The scale chosen for the project was 1:250,000 . The re- search being done required a scale that Principal Investigators (PI'S) using orbital photography could use, but would also serve PI'S doing surface photographic investigations. Each map sheet covers an area four degrees north/south by five degrees east/west. -
Volume 64, Number 04 (April 1946) James Francis Cooke
Gardner-Webb University Digital Commons @ Gardner-Webb University The tudeE Magazine: 1883-1957 John R. Dover Memorial Library 4-1-1946 Volume 64, Number 04 (April 1946) James Francis Cooke Follow this and additional works at: https://digitalcommons.gardner-webb.edu/etude Part of the Composition Commons, Music Pedagogy Commons, and the Music Performance Commons Recommended Citation Cooke, James Francis. "Volume 64, Number 04 (April 1946)." , (1946). https://digitalcommons.gardner-webb.edu/etude/196 This Book is brought to you for free and open access by the John R. Dover Memorial Library at Digital Commons @ Gardner-Webb University. It has been accepted for inclusion in The tudeE Magazine: 1883-1957 by an authorized administrator of Digital Commons @ Gardner-Webb University. For more information, please contact [email protected]. PIETRO MASCAGNI LAURITZ MELCHIOR, sensational Wag- nerian tenor of the Metropolitan Opera Company, recently celebrated his twen- tieth anniversary with the organization. To commemorate the occasion a gala concert was arranged, in which a num- ber of his colleagues joined Mr. Melchior in singing excerpts from three of the Wagner operas. Following the concert there was a back-stage ceremony, in which all departments of the Metropol- itan, from the board of directors to the stage hands, joined in paying tribute to the distinguished tenor. AN INTERNATIONAL music festival will take place in Prague, Czechoslovakia, from May 11 to 31, in commemoration of the fiftieth birthday of the Czech Phil- harmonic Orchestra. Leonard Bernstein, composer, conductor; Samuel Barber, composer; and Eugene List, pianist, will attend, representing the U.S. cured free upon request to the National THE RESTORED Co- and Inter-American Music Week Com- lonial city of Williams- BERNARD ROGERS’ mittee, 315 Fourth Avenue, New York 10. -
South Pole-Aitken Basin
Feasibility Assessment of All Science Concepts within South Pole-Aitken Basin INTRODUCTION While most of the NRC 2007 Science Concepts can be investigated across the Moon, this chapter will focus on specifically how they can be addressed in the South Pole-Aitken Basin (SPA). SPA is potentially the largest impact crater in the Solar System (Stuart-Alexander, 1978), and covers most of the central southern farside (see Fig. 8.1). SPA is both topographically and compositionally distinct from the rest of the Moon, as well as potentially being the oldest identifiable structure on the surface (e.g., Jolliff et al., 2003). Determining the age of SPA was explicitly cited by the National Research Council (2007) as their second priority out of 35 goals. A major finding of our study is that nearly all science goals can be addressed within SPA. As the lunar south pole has many engineering advantages over other locations (e.g., areas with enhanced illumination and little temperature variation, hydrogen deposits), it has been proposed as a site for a future human lunar outpost. If this were to be the case, SPA would be the closest major geologic feature, and thus the primary target for long-distance traverses from the outpost. Clark et al. (2008) described four long traverses from the center of SPA going to Olivine Hill (Pieters et al., 2001), Oppenheimer Basin, Mare Ingenii, and Schrödinger Basin, with a stop at the South Pole. This chapter will identify other potential sites for future exploration across SPA, highlighting sites with both great scientific potential and proximity to the lunar South Pole. -
Abstract Volume
T I I II I II I I I rl I Abstract Volume LPI LPI Contribution No. 1097 II I II III I • • WORKSHOP ON MERCURY: SPACE ENVIRONMENT, SURFACE, AND INTERIOR The Field Museum Chicago, Illinois October 4-5, 2001 Conveners Mark Robinbson, Northwestern University G. Jeffrey Taylor, University of Hawai'i Sponsored by Lunar and Planetary Institute The Field Museum National Aeronautics and Space Administration Lunar and Planetary Institute 3600 Bay Area Boulevard Houston TX 77058-1113 LPI Contribution No. 1097 Compiled in 2001 by LUNAR AND PLANETARY INSTITUTE The Institute is operated by the Universities Space Research Association under Contract No. NASW-4574 with the National Aeronautics and Space Administration. Material in this volume may be copied without restraint for library, abstract service, education, or personal research purposes; however, republication of any paper or portion thereof requires the written permission of the authors as well as the appropriate acknowledgment of this publication .... This volume may be cited as Author A. B. (2001)Title of abstract. In Workshop on Mercury: Space Environment, Surface, and Interior, p. xx. LPI Contribution No. 1097, Lunar and Planetary Institute, Houston. This report is distributed by ORDER DEPARTMENT Lunar and Planetary institute 3600 Bay Area Boulevard Houston TX 77058-1113, USA Phone: 281-486-2172 Fax: 281-486-2186 E-mail: order@lpi:usra.edu Please contact the Order Department for ordering information, i,-J_,.,,,-_r ,_,,,,.r pA<.><--.,// ,: Mercury Workshop 2001 iii / jaO/ Preface This volume contains abstracts that have been accepted for presentation at the Workshop on Mercury: Space Environment, Surface, and Interior, October 4-5, 2001. -
The Disintegration of the Wolf Creek Meteorite and the Formation of Pecoraite, the Nickel Analog of Clinochrysotile
The Disintegration of the Wolf Creek Meteorite and the Formation of Pecoraite, the Nickel Analog of Clinochrysotile GEOLOGICAL SURVEY PROFESSIONAL PAPER 384-C 1 mm ^^ 5 -fc;- Jj. -f->^ -J^' ' _." ^P^-Arvx^B^ »""*- 'S y^'ir'*'*'/?' trK* ^-7 A5*^v;'VvVr*'^**s! ^^^^V'^"^"''"X^^i^^?l^"%^ - ! ^ Pecoraite, Wolf Creek meteorite of Australia. Upper, Pecoraite grains separated by hand picking from crack fillings in the meteorite (X 25). Lower, Pecoraite grains lining the walls of some cracks in the meteorite. The extent of disintegration of the original metal lic phases into new phases, chiefly goethite and maghemite, is apparent (X 2.3). THE DISINTEGRATION OF THE WOLF CREEK METEORITE AND THE FORMATION OF PECORAITE, THE NICKEL ANALOG OF CLINOCHRYSOTILE The Disintegration of the Wolf Creek Meteorite and the Formation of Pecoraite, the Nickel Analog of Clinochrysotile By GEORGE T. FAUST, JOSEPH J. FAHEY, BRIAN H. MASON and EDWARD J. DWORNIK STUDIES OF THE NATURAL PHASES IN THE SYSTEM MgO-SiO2 -H2O AND THE SYSTEMS CONTAINING THE CONGENERS OF MAGNESIUM GEOLOGICAL SURVEY PROFESSIONAL PAPER 384-C Origin of pecoraite elucidated through its properties and in terms of the geochemical balance in its desert environment UNITED STATES GOVERNMENT PRINTING OFFICE, WASHINGTON : 1973 UNITED STATES DEPARTMENT OF THE INTERIOR ROGERS C. B. MORTON, Secretary GEOLOGICAL SURVEY V. E. McKelvey, Director Library of Congress catalog-card No. 73-600160 For sale by the Superintendent of Documents, U.S. Government Printing Office Washington, D.C. 20402 - Price $1.30 Stock