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No. 40. the System of Lunar Craters, Quadrant Ii Alice P
NO. 40. THE SYSTEM OF LUNAR CRATERS, QUADRANT II by D. W. G. ARTHUR, ALICE P. AGNIERAY, RUTH A. HORVATH ,tl l C.A. WOOD AND C. R. CHAPMAN \_9 (_ /_) March 14, 1964 ABSTRACT The designation, diameter, position, central-peak information, and state of completeness arc listed for each discernible crater in the second lunar quadrant with a diameter exceeding 3.5 km. The catalog contains more than 2,000 items and is illustrated by a map in 11 sections. his Communication is the second part of The However, since we also have suppressed many Greek System of Lunar Craters, which is a catalog in letters used by these authorities, there was need for four parts of all craters recognizable with reasonable some care in the incorporation of new letters to certainty on photographs and having diameters avoid confusion. Accordingly, the Greek letters greater than 3.5 kilometers. Thus it is a continua- added by us are always different from those that tion of Comm. LPL No. 30 of September 1963. The have been suppressed. Observers who wish may use format is the same except for some minor changes the omitted symbols of Blagg and Miiller without to improve clarity and legibility. The information in fear of ambiguity. the text of Comm. LPL No. 30 therefore applies to The photographic coverage of the second quad- this Communication also. rant is by no means uniform in quality, and certain Some of the minor changes mentioned above phases are not well represented. Thus for small cra- have been introduced because of the particular ters in certain longitudes there are no good determi- nature of the second lunar quadrant, most of which nations of the diameters, and our values are little is covered by the dark areas Mare Imbrium and better than rough estimates. -
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. -
Preparation of Barium Strontium Titanate Powder from Citrate
APPLIED ORGANOMETALLIC CHEMISTRY Appl. Organometal. Chem. 13, 383–397 (1999) Preparation of Barium Strontium Titanate Powder from Citrate Precursor Chen-Feng Kao* and Wein-Duo Yang Department of Chemical Engineering, National Cheng Kung University, Tainan, 70101, Taiwan TiCl4 or titanium isopropoxide reacted with INTRODUCTION citric acid to form a titanyl citrate precipitate. Barium strontium citrate solutions were then BaTiO3 is ferroelectric and piezoelectric and has added to the titanyl citrate reaction to form gels. extensive applications as an electronic material. It These gels were dried and calcined to (Ba,Sr)- can be used as a capacitor, thermistor, transducer, TiO3 powders. The gels and powders were accelerometer or degausser of colour television. characterized by DSC/TGA, IR, SEM and BaTiO3 doped with strontium retains its original XRD analyses. These results showed that, at characteristics but has a lower Curie temperature 500 °C, the gels decomposed to Ba,Sr carbonate for positive temperature coefficient devices under and TiO2, followed by the formation of (Ba,Sr)- various conditions. TiO3. The onset of perovskite formation oc- Besides solid-state reactions, chemical reactions curred at 600 °C, and was nearly complete at have also been used to prepare BaTiO3 powder. 1 1000 °C. Traces of SrCO3 were still present. Among them the hydrolysis of metal alkoxide , The cation ratios of the titanate powder oxalate precipitation in ethanol2, and alcoholic prepared in the pH range 5–6 were closest to dehydration of citrate solution3 are among the more the original stoichiometry. Only 0.1 mol% of the attractive methods. In 1956 Clabaugh et al.4 free cations remained in solution. -
General Disclaimer One Or More of the Following Statements May Affect
https://ntrs.nasa.gov/search.jsp?R=19710025504 2020-03-11T22:36:49+00:00Z View metadata, citation and similar papers at core.ac.uk brought to you by CORE provided by NASA Technical Reports Server General Disclaimer One or more of the Following Statements may affect this Document This document has been reproduced from the best copy furnished by the organizational source. It is being released in the interest of making available as much information as possible. This document may contain data, which exceeds the sheet parameters. It was furnished in this condition by the organizational source and is the best copy available. This document may contain tone-on-tone or color graphs, charts and/or pictures, which have been reproduced in black and white. This document is paginated as submitted by the original source. Portions of this document are not fully legible due to the historical nature of some of the material. However, it is the best reproduction available from the original submission. Produced by the NASA Center for Aerospace Information (CASI) 6 X t B ICC"m date: July 16, 1971 955 L'Enfant Plaza North, S. W Washington, D. C. 20024 to Distribution B71 07023 from. J. W. Head suhiecf Derivation of Topographic Feature Names in the Apollo 15 Landing Region - Case 340 ABSTRACT The topographic features in the region of the Apollo 15 landing site (Figure 1) are named for a number of philosophers, explorers and scientists (astronomers in particular) representing periods throughout recorded history. It is of particular interest that several of the individuals were responsible for specific discoveries, observations, or inventions which considerably advanced the study and under- standing of the moon (for instance, Hadley designed the first large reflecting telescope; Beer published classic maps and explanations of the moon's surface). -
Aldrich Organometallic, Inorganic, Silanes, Boranes, and Deuterated Compounds
Aldrich Organometallic, Inorganic, Silanes, Boranes, and Deuterated Compounds Library Listing – 1,523 spectra Subset of Aldrich FT-IR Library related to organometallic, inorganic, boron and deueterium compounds. The Aldrich Material-Specific FT-IR Library collection represents a wide variety of the Aldrich Handbook of Fine Chemicals' most common chemicals divided by similar functional groups. These spectra were assembled from the Aldrich Collections of FT-IR Spectra Editions I or II, and the data has been carefully examined and processed by Thermo Fisher Scientific. Aldrich Organometallic, Inorganic, Silanes, Boranes, and Deuterated Compounds Index Compound Name Index Compound Name 1066 ((R)-(+)-2,2'- 1193 (1,2- BIS(DIPHENYLPHOSPHINO)-1,1'- BIS(DIPHENYLPHOSPHINO)ETHAN BINAPH)(1,5-CYCLOOCTADIENE) E)TUNGSTEN TETRACARBONYL, 1068 ((R)-(+)-2,2'- 97% BIS(DIPHENYLPHOSPHINO)-1,1'- 1062 (1,3- BINAPHTHYL)PALLADIUM(II) CH BIS(DIPHENYLPHOSPHINO)PROPA 1067 ((S)-(-)-2,2'- NE)DICHLORONICKEL(II) BIS(DIPHENYLPHOSPHINO)-1,1'- 598 (1,3-DIOXAN-2- BINAPH)(1,5-CYCLOOCTADIENE) YLETHYNYL)TRIMETHYLSILANE, 1140 (+)-(S)-1-((R)-2- 96% (DIPHENYLPHOSPHINO)FERROCE 1063 (1,4- NYL)ETHYL METHYL ETHER, 98 BIS(DIPHENYLPHOSPHINO)BUTAN 1146 (+)-(S)-N,N-DIMETHYL-1-((R)-1',2- E)(1,5- BIS(DI- CYCLOOCTADIENE)RHODIUM(I) PHENYLPHOSPHINO)FERROCENY TET L)E 951 (1,5-CYCLOOCTADIENE)(2,4- 1142 (+)-(S)-N,N-DIMETHYL-1-((R)-2- PENTANEDIONATO)RHODIUM(I), (DIPHENYLPHOSPHINO)FERROCE 99% NYL)ETHYLAMIN 1033 (1,5- 407 (+)-3',5'-O-(1,1,3,3- CYCLOOCTADIENE)BIS(METHYLD TETRAISOPROPYL-1,3- IPHENYLPHOSPHINE)IRIDIUM(I) -
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. -
Annual Report 2008 – 2009
O L D S T U R B R I D G E Summer 2009 Special Annual VILLAGE Report Edition Visitor 2008-2009 2008--2009 Momentum and More The History of Fireworks Farms, Families, and Change Cooking with OSV Summer Events a member magazine that keeps you coming back Old Sturbridge Village, a museum and learning resource of 2008-2009 Building Momentum New England life, invites each visitor to find meaning, pleasure, a letter from President Jim Donahue relevance, and inspiration through the exploration of history. to our newly designed V I S I T O R magazine. We hope that you will learn new things and come to visit t is no secret around the Village that I like to keep my eye on the “dashboard” – a set of key the Village soon. There is always something fun to do at indicators that I am consistently checking to make sure we are steering OSV in the right direction. In fact, Welcome O l d S T u R b ri d g E V I l l a g E . I take a lot of good-natured kidding about how often I peek at the attendance figures each day, eager to see if we beat last year’s number. And I have to admit that I get energized when the daily mail brings in new donations, when the sun is shining, the parking lot is full, when I can hear happy children touring the Village, and the visitor comments are upbeat and favorable. Volume XlIX, No. 2 Summer 2009 Special Annual Report Edition I am happy to report these indicators have been overwhelmingly positive during the past year – solid proof that Old Sturbridge Village is building on last year’s successes and is poised to finish this decade much stronger There is nothing quite like learning about history from than when it started. -
List of Targets for the Lunar II Observing Program (PDF File)
Task or Task Description or Target Name Wood's Rükl Target LUNAR # 100 Atlas Catalog (chart) Create a sketch/map of the visible lunar surface: 1 Observe a Full Moon and sketch a large-scale (prominent features) L-1 map depicting the nearside; disk of visible surface should be drawn 2 at L-1 3 least 5-inches in diameter. Sketch itself should be created only by L-1 observing the Moon, but maps or guidebooks may be used when labeling sketched features. Label all maria, prominent craters, and major rays by the crater name they originated from. (Counts as 3 observations (OBSV): #1, #2 & #3) Observe these targets; provide brief descriptions: 4 Alpetragius 55 5 Arago 35 6 Arago Alpha & Arago Beta L-32 35 7 Aristarchus Plateau L-18 18 8 Baco L-55 74 9 Bailly L-37 71 10 Beer, Beer Catena & Feuillée 21 11 Bullialdus, Bullialdus A & Bullialdus B 53 12 Cassini, Cassini A & Cassini B 12 13 Cauchy, Cauchy Omega & Cauchy Tau L-48 36 14 Censorinus 47 15 Crüger 50 16 Dorsae Lister & Smirnov (A.K.A. Serpentine Ridge) L-33 24 17 Grimaldi Basin outer and inner rings L-36 39, etc. 18 Hainzel, Hainzel A & Hainzel C 63 19 Hercules, Hercules G, Hercules E 14 20 Hesiodus A L-81 54, 64 21 Hortensius dome field L-65 30 22 Julius Caesar 34 23 Kies 53 24 Kies Pi L-60 53 25 Lacus Mortis 14 26 Linne 23 27 Lamont L-53 35 28 Mairan 9 29 Mare Australe L-56 76 30 Mare Cognitum 42, etc. -
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 -
Hydrothermal Synthesis of Titanate Nanotubes Followed by Electrodeposition Process
Korean J. Chem. Eng., 23(6), 1037-1045 (2006) SHORT COMMUNICATION Hydrothermal synthesis of titanate nanotubes followed by electrodeposition process Gil-Sung Kim, Young-Soon Kim, Hyung-Kee Seo and Hyung-Shik Shin† Thin Film Technology Laboratory, School of Chemical Engineering, Chonbuk National University, Jeonju 561-756, Korea (Received 27 January 2006 • accepted 4 July 2006) Abstract−Titanate nanotubes were synthesized by hydrothermal process using commercial titania nanoparticles. The experiments were carried out as a function of reaction time, temperature, and NaOH concentration. Furthermore, the titanate nanotube film was fabricated on the Si substrate using electrodeposition method with 60 V and at room tem- perature. The specimens were investigated by using various techniques such as field-emission scanning electron micro- scopy (FESEM), transmission electron microscopy (TEM), X-ray diffraction (XRD), Raman Spectroscopy, and X- ray photoelectron spectroscopy (XPS). The formation of sodium titanate nanotubes was affected strongly by the varia- tion in all parameters. The best conditions for the titanate nanotubes were found to be a reaction temperature of 150 oC, 10 M NaOH concentration, and reaction time of 48 hr. Under the best conditions, the resulting titanate nanotubes did not contain any remains of starting material, namely P25 nanoparticles, and also the resulting nanotubes had very smooth morphology with a diameter of ~10 nm and length extending up to several micrometers without presence of any bundle- like structures. The washing of sodium titanate nanotubes with HCl solution leads to conversion into protonic titanate nanotubes via ion exchange reaction. The subsequent sintering of the titanate nanotubes renders dehydration of inter- layered OH groups, thereby leading to precipitation of anatase phase. -
Chemical Substances Exempt from Notification of Manufacturing/Import Amount
Chemical Substances Exempt from Notification of Manufacturing/Import Amount A list under Chemical Substance Control Law (Japan) 2014-3-24 Official issuance: Joint Notice No.1 of MHLW, METI and MOE English source: Chemical Risk Information Platform (CHRIP) Edited by: https://ChemLinked.com ChemLinked Team, REACH24H Consulting Group| http://chemlinked.com 6 Floor, Building 2, Hesheng Trade Centre, No.327 Tianmu Mountain Road, Hangzhou, China. PC: 310023 Tel: +86 571 8700 7545 Fax: +86 571 8700 7566 Email: [email protected] 1 / 1 Specification: In Japan, all existing chemical substances and notified substances are given register numbers by Ministry of International Trade and Industry (MITI Number) as a chemical identifier. The Japanese Chemical Management Center continuously works on confirming the mapping relationships between MITI Numbers and CAS Registry Numbers. Please enter CHRIP to find if there are corresponding CAS Numbers by searching the substances’ names or MITI Numbers. The first digit of a MITI number is a category code. Those adopted in this List are as follows: 1: Inorganic compounds 2: Chained organic low-molecular-weight compounds 3: Mono-carbocyclic organic low-molecular-weight compounds 5: Heterocyclic organic low-molecular-weight compounds 6: Organic compounds of addition polymerization 7: Organic compounds of condensation polymerization 8: Organic compounds of modified starch, and processed fats and oils 9: Compounds of pharmaceutical active ingredients, etc. This document is provided by ChemLinked, a division of REACH24H Consulting Group. ChemLinked is a unique portal to must-know EHS issues in China, and essential regulatory database to keep all EHS & Regulatory Affairs managers well-equipped. You may subscribe and download this document from ChemLinked.com. -
Pilot-Scale Demonstration of Ilmenite Processing Technology UMD NRRI
Pilot-Scale Demonstration of Ilmenite Processing Technology Submitted by: Matthew Mlinar, Program Manager, Mineral Processing Shashi Rao, Metallurgical Engineer Tom Petersen, Technical Manager, Mineral Processing May 2017 May Date: May 24, 2017 – Collaborator: Process Research Ortech (PRO) Mississauga, Ontario, Canada Funders: Iron Range Resources and Rehabilitation Board (IRRRB) University of Minnesota Duluth Vice Chancellor for Academic Affairs (UMD EVCAA) University of Minnesota Office of the Vice President for Research (UM OVPR) Technical Report Report Technical NRRI Duluth Laboratories & Administration 5013 Miller Trunk Highway Duluth, Minnesota 55811 Coleraine Laboratories One Gayley Avenue P.O. Box 188 Coleraine, Minnesota 55722 Pilot-Scale Demonstration of Ilmenite Processing Technology UMD NRRI By: ________________________________________________________________ Matthew Mlinar – UMD NRRI Program Manager, Mineral Processing By: ________________________________________________________________ Shashi Rao – UMD NRRI Metallurgical Engineer By: ________________________________________________________________ Tom Petersen – UMD NRRI Technical Manager, Mineral Processing Approved By: ________________________________________________________________ Richard Kiesel – UMD NRRI Asst. Director Minerals, Metallurgy, and Mining Approved By: ________________________________________________________________ George Hudak, Ph. D. – UMD NRRI Director Minerals, Metallurgy, and Mining Peer Reviewed By: Harvey Thorleifson Ph.D., P.Geo., D.Sc., Director,