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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. -
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. -
August 2017 Posidonius P & Luther
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 – AUGUST 2017 POSIDONIUS P & LUTHER Sketch and text by Robert H. Hays, Jr. - Worth, Illinois, USA March 5, 2017 01:28-01:48; UT, 15 cm refl, 170x, seeing 7-8/10. I drew these craters on the evening of March 4/5, 2017 while the moon was hiding some Hyades stars. This area is in northeast Mare Serenitatis west of Posidonius itself. Posidonius P is the largest crater on this sketch. The smaller crater south of P is Posidonius F and Posidonius G is the tiny pit to the north. There is a halo around Posidonius G, but this crater is noticeably north of the halo's center. A very low round swelling is northeast of Posidonius G. Luther is the crater well to the west of Posidonius P. All four of these craters are crisp, symmetric features, differing only in size. There are an assortment of elevations near Luther. The peak Luther alpha is well to the west of Luther, and showed dark shadowing at this time. All of the other features near Luther are more subtle than Luther alpha. One mound is between Luther and Luther alpha. Two more mounds are north of Luther, and a low ridge is just east of this crater. A pair of very low mounds are south of Luther. These are the vaguest features depicted here, and may be too conspicuous on the sketch. -
Who Got Moseley's Prize?
Chapter 4 Who Got Moseley’s Prize? Virginia Trimble1 and Vera V. Mainz*,2 1Department of Physics and Astronomy, University of California, Irvine, Irvine, California 92697-4575, United States 2Department of Chemistry, University of Illinois at Urbana-Champaign, Urbana, Illinois 61802, United States *E-mail: [email protected]. Henry Gwyn Jeffreys Moseley (1887-1915) made prompt and very skilled use of the then new technique of X-ray scattering by crystals (Bragg scattering) to solve several problems about the periodic table and atoms. He was nominated for both the chemistry and physics Nobel Prizes by Svante Arrhenius in 1915, but was dead at Gallipoli before the committees finished their deliberations. Instead, the 1917 physics prize (announced in 1918 and presented on 6 June 1920) went to Charles Glover Barkla (1877-1944) “for discovery of the Röntgen radiation of the elements.” This, and his discovery of X-ray polarization, were done with earlier techniques that he never gave up. Moseley’s contemporaries and later historians of science have written that he would have gone on to other major achievements and a Nobel Prize if he had lived. In contrast, after about 1916, Barkla moved well outside the scientific mainstream, clinging to upgrades of his older methods, denying the significance of the Bohr atom and quantization, and continuing to report evidence for what he called the J phenomenon. This chapter addresses the lives and scientific endeavors of Moseley and Barkla, something about the context in which they worked and their connections with other scientists, contemporary, earlier, and later. © 2017 American Chemical Society Introduction Henry Moseley’s (Figure 1) academic credentials consisted of a 1910 Oxford BA with first-class honors in Mathematical Moderations and a second in Natural Sciences (physics) and the MA that followed more or less automatically a few years later. -
6 Supplementary References
6 6 SUPPLEMENTARY REFERENCES 6 SUPPLEMENTARY REFERENCES 1203 6.1 GENERAL ENCYCLOPEDIAS Cosmology glossary. Western Washington Univ. Planetarium, Bellingham, WA; http://www.wwu.edu/depts/skywise/a101_cosmologyglossary.html. Bilder-Konversationslexikon. 4 vols., Brockhaus, Leipzig (1834). CXC Glossary of astrophysical terms. Chandra X-ray Center (CXC), operated Brockhaus Enzyklopädie. 20 vols., Brockhaus, Wiesbaden (1966–1974). for NASA by Harvard-Smithsonian Center for Astrophysics, Cambridge, Brockhaus-Konversationslexikon. 16 vols., Brockhaus, Leipzig (1892–1897). MA; http://chandra.harvard.edu/resources/glossaryA.html. Chambers’s encyclopaedia (ed. by M.D. LAW). 15 vols., International Learn- Dictionnaire des sciences naturelles (ed. by F.G. CUVIER). Levrault, Stras- ing Systems Corporation Ltd., London (1963). bourg (1816–1826). Columbia encyclopedia. Columbia University Press, New York (6th edn., Dictionary of medieval Latin from British sources (ed. by R.E. LATHAM and 2001–2005); http://www.bartleby.com/65/. D.R. HOWLETT). Oxford University Press, London; vol. 1 (1975) to vol. 6 Collier’s encyclopedia. 24 vols., Macmillan Education Co, New York (1987). (2003). Der Große Herder. 13 vols., Herder, Freiburg (1932–1935). Dictionary of mining, mineral, and related terms [compiled and edited by the Encyclopaedia Britannica. 29 vols. (11th edn., 1911). LoveToKnow™ free U.S. Bureau of Mines, U.S. Dept. of the Interior]. Am. Geol. Inst., Alex- online Encyclopedia; http://www.1911encyclopedia.org/. andria, VA (1997); http://www.maden.hacettepe.edu.tr/dmmrt/index.html. Encyclopaedia Britannica. 24 vols. (1875–1889), 24 vols. (1929), 24 vols. Dictionary of SDI (ed. by H. WALDMAN). Scholarly Resources Imprint, Wil- (1959); 30 vols. (1974–1984); 32 vols. (1985–2002) mington, DE (1988). -
Main Attributes of Nuclides Presented in This Book
Appendix A Main Attributes of Nuclides Presented in This Book Data given in TableA.1 can be used to determine the various decay energies for the specific radioactive decay examples as well as for the nuclear activation examples presented in this book. M stands for the nuclear rest mass; M stands for the atomic rest mass. The data were obtained from the NIST and are based on CODATA 2010 as follows: 1. Data for atomic masses M are given in atomic mass constants u and were obtained from the NIST at: (http://www.physics.nist.gov/pml/data/comp.cfm). 2. Rest mass of proton mp, neutron mn, electron me, and of the atomic mass constant u are from the NIST (http://www.physics.nist.gov/cuu/constants/index. html) as follows: −27 2 mp = 1.672 621 777×10 kg = 1.007 276 467 u = 938.272 046 MeV/c (A.1) −27 2 mn = 1.674 927 351×10 kg = 1.008 664 916 u = 939.565 379 MeV/c (A.2) −31 −4 2 me = 9.109 382 91×10 kg = 5.485 799 095×10 u = 0.510 998 928 MeV/c (A.3) − 1u= 1.660 538 922×10 27 kg = 931.494 060 MeV/c2 (A.4) 3. For a given nuclide, its nuclear rest energy was determined by subtracting the 2 rest energy of all atomic orbital electrons (Zmec ) from the atomic rest energy M(u)c2 as follows 2 2 2 Mc = M(u)c − Zmec = M(u) × 931.494 060 MeV/u − Z × 0.510 999 MeV. -
Miguel A. Catalán's CXXV Anniversary
Advances in Historical Studies, 2019, 8, 239-251 https://www.scirp.org/journal/ahs ISSN Online: 2327-0446 ISSN Print: 2327-0438 Miguel A. Catalán’s CXXV Anniversary Gabriel Barceló Pedro de Valdivia, Madrid, Spain How to cite this paper: Barceló, G. (2019). Abstract Miguel A. Catalán’s CXXV Anniversary. Advances in Historical Studies, 8, 239-251. We would like to memorialize the CXXV anniversary of the following phy- https://doi.org/10.4236/ahs.2019.85017 sicist: Miguel A. Catalán (1894-1957), who contributed to science advance- ment and to define the atomic model of matter, and quantum theory, hun- Received: November 6, 2019 Accepted: December 7, 2019 dred years ago. The objective of the research was to define the biography of Published: December 10, 2019 Miguel A. Catalán and his contribution to the advancement of science. To this end, this work has been historically documented. Copyright © 2019 by author(s) and Scientific Research Publishing Inc. This work is licensed under the Creative Keywords Commons Attribution International Miguel A. Catalán, Atomic Physics, Atomic Spectroscopy, Spectrum of License (CC BY 4.0). http://creativecommons.org/licenses/by/4.0/ Manganese, Atomic Model Open Access 1. Introduction We would like to remember the 125th birth anniversary of the physicist Miguel A. Catalán (1894-1957), who, one hundred years ago, contributed to the ad- vancement of science and the definition of the atomic model of matter. He was a great teacher and pedagogue as well; he was my professor. Even before becoming a doctor, on February 6 of 1917, he had applied for a fellowship in order to study abroad. -
FEATURE of the MONTH – AUGUST 2016 W Bond B
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 – AUGUST 2016 W Bond B Sketch and text by Robert H. Hays, Jr. - Worth, Illinois, USA March 18, 2016 01:50-02:30 UT, 15 cm refl, 170x, seeing 8/10, transparency 6/6 I drew this crater and vicinity on the evening of March 17/18, 2016 before the moon hid 1 Cancri. This crater is the most conspicuous feature within the large ruined ring W. Bond, north of Mare Frigoris. This is a very crisp crater with much interior shadow and slight exterior shadow at this time. The smaller crater W. Bond C is north of B, and is a miniature version of its neighbor. A wide, slightly curved ridge with dark shadowing is southeast of W. Bond B. It tapers almost to a point at its southern end, and a small peak is just off this tip. A large, blocky peak, also with dark shadowing, is north of this ridge, and a small peak with much lighter shadowing is between this block and W. Bond C. Another ridge is just east of the wide ridge and block. This ridge has two branches, and has relatively light shadowing except at the elbow formed by one of its branches. A low peak is just off this ridge's north end. The crater just east of this ridge is probably Archytas U. -
SPRING2017.Pdf
ACA – Structure Matters www.AmerCrystalAssn.org Table of Contents 2 President’s Column 2-5 RefleXions from Canada 7-9 News from Latin America 9 YSIG Activities in New Orleans From the Editor's Desk Index of Advertisers 10-11 Update on Structural Dynamics Amy Sarjeant 2017 ACA President 12 ACA 2017 New Orleans Preview What's on the Cover 13 Corporate Members Page 14 14 What's on the Cover 15 ACA Council Officers; Appointments & Staff; Canadian Division Officers 16 ACA RefleXions Co-Editors & Staff 22017 ACA Award Winners Nominations for 2018 to Be Honored in New Orleans 17 Standing Committees 18-20 Scientific Interest Group Officers 21 U. S. National Committee for Crystallography 23-24 Net RefleXions 24-26 News & Awards 26-30 Remembering Dick Marsh Christine Dunham 31-32 Highlights from 2016 Fall ACA Coun- Etter Award cil Meeting Zbigniew Dauter 32 Small Grants for Outreach Patterson Award X-ray Equipment for Donation Contributors to this Issue Helen Berman 33 ACA History Project News Rognlie Award 33-34 Space Crystal Prize James O'Brien 34 Promoting Crystallography through Coloring Wood Award 35 2016 U. S. Crystal Growing Competition 37-38 Book Reviews 39 Spotlight on Stamps Manuel Soriano-Garcia 40-45 ACA Living History – Manuel Soriano-García ACA Living History 46 AIP Niels Bohr Library & Archives Announcement 47 Puzzle Corner Nobel Laureate Sir James Fraser Stoddart 48 Future Meetings Plenary Lecturer in New Orleans Contributions to ACA RefleXions may be sent to either of the Editors: Please address matters pertaining to advertisements, membership Judith L. Flippen-Anderson [email protected] inquiries, or use of the ACA mailing list to: Thomas F. -
Biodiversity in Aotearoa
Biodiversity in Aotearoa an overview of state, trends and pressures 2020 Front cover: Homer grasshopper (Sigaus homerensis) occurs in a few small, isolated gullies in Northern Fiordland which are prone to avalanche and rock fall. Predation and the effects of climate change pose the most significant threats for this species. It has a conservation status of ‘Threatened – Nationally Critical’. Photo: Simon Morris Published by: Department of Conservation, PO Box 10420, Wellington 6143 Editing and design: DOC Creative Services August 2020 This work is licensed under the Creative Commons Attribution 4.0 International license unless otherwise stated. In essence, you are free to copy, distribute and adapt the work, as long as you attribute the work to the Crown and abide by the other licence terms. To view a copy of this licence, www.creativecommons.org/licenses/by/4.0. Please note that no departmental or governmental emblem, logo or Coat of Arms may be used in any way that infringes any provision of the Flags, Emblems, and Names Protection Act 1981. Use the wording ‘Department of Conservation’ in your attribution, not the Department of Conservation logo. Biodiversity in Aotearoa Contents Executive summary | Whakarāpopoto matua ����������������������������������������������������������������������������������������5 Foreword | Kupu whakataki ����������������������������������������������������������������������������������������������������������������������7 Introduction | Kupu arataki �����������������������������������������������������������������������������������������������������������������������8 -
Draft Wildlife Conservation Plan for Seabirds
DRAFT WILDLIFE CONSERVATION PLAN FOR SEABIRDS 1 The Species Profile and Threats Database pages linked to this recovery plan is obtainable from: http://www.environment.gov.au/cgi-bin/sprat/public/sprat.pl © Copyright Commonwealth of Australia, 2019. <insert name of report> is licensed by the Commonwealth of Australia for use under a Creative Commons Attribution 4.0 International licence with the exception of the Coat of Arms of the Commonwealth of Australia, the logo of the agency responsible for publishing the report, content supplied by third parties, and any images depicting people. For licence conditions see: https://creativecommons.org/licenses/by/4.0/ This report should be attributed as ‘Draft Wildlife Conservation Plan for Seabirds, Commonwealth of Australia 2019’. The Commonwealth of Australia has made all reasonable efforts to identify content supplied by third parties using the following format ‘© Copyright, [name of third party] ’. Disclaimer While reasonable efforts have been made to ensure that the contents of this publication are factually correct, the Commonwealth does not accept responsibility for the accuracy or completeness of the contents, and shall not be liable for any loss or damage that may be occasioned directly or indirectly through the use of, or reliance on, the contents of this publication. Images credits Cover page: Red-footed Booby (Sula sula) over North Keeling Island © Copyright Department of the Environment and Energy 2 Contents Summary ............................................................................................................................. -
Greene Et Al. 2014.Pdf
154 Notornis, 2014, Vol. 61: 154-161 0029-4470 © The Ornithological Society of New Zealand Inc. Assessing minimum population size of Kermadec parakeets (Cyanoramphus novaezelandiae cyanurus) on Macauley Island, Kermadec Islands TERRY C. GREENE* IAN M. WESTBROOKE DEREK BROWN PETER J. DILKS Science and Technical, Department of Conservation, Private Bag 4715, Christchurch 8140, New Zealand JOHN W. BARKLA Department of Conservation, PO Box 5244, Dunedin 9058, New Zealand RICHARD GRIFFITHS Department of Conservation, PO Box 32026, Devonport 0744, New Zealand Abstract The minimum population size of Kermadec parakeets (Cyanoramphus novaezelandiae cyanurus) is reported for Macauley Island in the southern Kermadec Islands group. To minimise population impacts of any accidental parakeet deaths the confirmed presence of a minimum population of 3,000 parakeets was required prior to the attempted eradication of Pacific rats (Rattus exulans) from Macauley Island. Eight pre-defined vegetation strata were identified and 4 count methods ranging from simple counts to distance sampling were assigned to each strata depending on sampling conditions. As the resultant point estimate of 3,484 parakeets during the 29 June to 1 July 2006 survey period was greater than the minimum threshold the rat eradication was able to proceed. The potential impacts of changes in the vegetation on the population dynamics of Kermadec parakeets and recommendations for future monitoring of this species on Macauley Island are discussed. Greene, T.C.; Westbrooke, I.M; Brown, D.; Dilks, P.J.; Barkla, J.W.; Griffiths, R. 2014. Assessing minimum population size of Kermadec parakeets (Cyanoramphus novaezelandiae cyanurus) on Macauley Island, Kermadec Islands. Notornis 61 (3): 154-161.