Radial Velocities of Visual Binaries E
Total Page:16
File Type:pdf, Size:1020Kb
Load more
Recommended publications
-
Mathématiques Et Espace
Atelier disciplinaire AD 5 Mathématiques et Espace Anne-Cécile DHERS, Education Nationale (mathématiques) Peggy THILLET, Education Nationale (mathématiques) Yann BARSAMIAN, Education Nationale (mathématiques) Olivier BONNETON, Sciences - U (mathématiques) Cahier d'activités Activité 1 : L'HORIZON TERRESTRE ET SPATIAL Activité 2 : DENOMBREMENT D'ETOILES DANS LE CIEL ET L'UNIVERS Activité 3 : D'HIPPARCOS A BENFORD Activité 4 : OBSERVATION STATISTIQUE DES CRATERES LUNAIRES Activité 5 : DIAMETRE DES CRATERES D'IMPACT Activité 6 : LOI DE TITIUS-BODE Activité 7 : MODELISER UNE CONSTELLATION EN 3D Crédits photo : NASA / CNES L'HORIZON TERRESTRE ET SPATIAL (3 ème / 2 nde ) __________________________________________________ OBJECTIF : Détermination de la ligne d'horizon à une altitude donnée. COMPETENCES : ● Utilisation du théorème de Pythagore ● Utilisation de Google Earth pour évaluer des distances à vol d'oiseau ● Recherche personnelle de données REALISATION : Il s'agit ici de mettre en application le théorème de Pythagore mais avec une vision terrestre dans un premier temps suite à un questionnement de l'élève puis dans un second temps de réutiliser la même démarche dans le cadre spatial de la visibilité d'un satellite. Fiche élève ____________________________________________________________________________ 1. Victor Hugo a écrit dans Les Châtiments : "Les horizons aux horizons succèdent […] : on avance toujours, on n’arrive jamais ". Face à la mer, vous voyez l'horizon à perte de vue. Mais "est-ce loin, l'horizon ?". D'après toi, jusqu'à quelle distance peux-tu voir si le temps est clair ? Réponse 1 : " Sans instrument, je peux voir jusqu'à .................. km " Réponse 2 : " Avec une paire de jumelles, je peux voir jusqu'à ............... km " 2. Nous allons maintenant calculer à l'aide du théorème de Pythagore la ligne d'horizon pour une hauteur H donnée. -
Of Vertebrate Fossils from the Middle Eocene Oil Shale of Messel, Germany: Implications for Their Taphonomy and Palaeoenvironment
Palaeogeography, Palaeoclimatology, Palaeoecology 416 (2014) 92–109 Contents lists available at ScienceDirect Palaeogeography, Palaeoclimatology, Palaeoecology journal homepage: www.elsevier.com/locate/palaeo Isotope compositions (C, O, Sr, Nd) of vertebrate fossils from the Middle Eocene oil shale of Messel, Germany: Implications for their taphonomy and palaeoenvironment Thomas Tütken ⁎ Steinmann-Institut für Geologie, Mineralogie und Paläontologie, Universität Bonn, Poppelsdorfer Schloss, 53115 Bonn, Germany article info abstract Article history: The Middle Eocene oil shale deposits of Messel are famous for their exceptionally well-preserved, articulated 47- Received 15 April 2014 Myr-old vertebrate fossils that often still display soft tissue preservation. The isotopic compositions (O, C, Sr, Nd) Received in revised form 30 July 2014 were analysed from skeletal remains of Messel's terrestrial and aquatic vertebrates to determine the condition of Accepted 5 August 2014 geochemical preservation. Authigenic phosphate minerals and siderite were also analysed to characterise the iso- Available online 17 August 2014 tope compositions of diagenetic phases. In Messel, diagenetic end member values of the volcanically-influenced 12 Keywords: and (due to methanogenesis) C-depleted anoxic bottom water of the meromictic Eocene maar lake are isoto- Strontium isotopes pically very distinct from in vivo bioapatite values of terrestrial vertebrates. This unique taphonomic setting al- Oxygen isotopes lows the assessment of the geochemical preservation of the vertebrate fossils. A combined multi-isotope Diagenesis approach demonstrates that enamel of fossil vertebrates from Messel is geochemically exceptionally well- Enamel preserved and still contains near-in vivo C, O, Sr and possibly even Nd isotope compositions while bone and den- Messel tine are diagenetically altered. -
Geoscience and a Lunar Base
" t N_iSA Conference Pubhcatmn 3070 " i J Geoscience and a Lunar Base A Comprehensive Plan for Lunar Explora, tion unclas HI/VI 02907_4 at ,unar | !' / | .... ._-.;} / [ | -- --_,,,_-_ |,, |, • • |,_nrrr|l , .l -- - -- - ....... = F _: .......... s_ dd]T_- ! JL --_ - - _ '- "_r: °-__.......... / _r NASA Conference Publication 3070 Geoscience and a Lunar Base A Comprehensive Plan for Lunar Exploration Edited by G. Jeffrey Taylor Institute of Meteoritics University of New Mexico Albuquerque, New Mexico Paul D. Spudis U.S. Geological Survey Branch of Astrogeology Flagstaff, Arizona Proceedings of a workshop sponsored by the National Aeronautics and Space Administration, Washington, D.C., and held at the Lunar and Planetary Institute Houston, Texas August 25-26, 1988 IW_A National Aeronautics and Space Administration Office of Management Scientific and Technical Information Division 1990 PREFACE This report was produced at the request of Dr. Michael B. Duke, Director of the Solar System Exploration Division of the NASA Johnson Space Center. At a meeting of the Lunar and Planetary Sample Team (LAPST), Dr. Duke (at the time also Science Director of the Office of Exploration, NASA Headquarters) suggested that future lunar geoscience activities had not been planned systematically and that geoscience goals for the lunar base program were not articulated well. LAPST is a panel that advises NASA on lunar sample allocations and also serves as an advocate for lunar science within the planetary science community. LAPST took it upon itself to organize some formal geoscience planning for a lunar base by creating a document that outlines the types of missions and activities that are needed to understand the Moon and its geologic history. -
The Brightest Stars Seite 1 Von 9
The Brightest Stars Seite 1 von 9 The Brightest Stars This is a list of the 300 brightest stars made using data from the Hipparcos catalogue. The stellar distances are only fairly accurate for stars well within 1000 light years. 1 2 3 4 5 6 7 8 9 10 11 12 13 No. Star Names Equatorial Galactic Spectral Vis Abs Prllx Err Dist Coordinates Coordinates Type Mag Mag ly RA Dec l° b° 1. Alpha Canis Majoris Sirius 06 45 -16.7 227.2 -8.9 A1V -1.44 1.45 379.21 1.58 9 2. Alpha Carinae Canopus 06 24 -52.7 261.2 -25.3 F0Ib -0.62 -5.53 10.43 0.53 310 3. Alpha Centauri Rigil Kentaurus 14 40 -60.8 315.8 -0.7 G2V+K1V -0.27 4.08 742.12 1.40 4 4. Alpha Boötis Arcturus 14 16 +19.2 15.2 +69.0 K2III -0.05 -0.31 88.85 0.74 37 5. Alpha Lyrae Vega 18 37 +38.8 67.5 +19.2 A0V 0.03 0.58 128.93 0.55 25 6. Alpha Aurigae Capella 05 17 +46.0 162.6 +4.6 G5III+G0III 0.08 -0.48 77.29 0.89 42 7. Beta Orionis Rigel 05 15 -8.2 209.3 -25.1 B8Ia 0.18 -6.69 4.22 0.81 770 8. Alpha Canis Minoris Procyon 07 39 +5.2 213.7 +13.0 F5IV-V 0.40 2.68 285.93 0.88 11 9. Alpha Eridani Achernar 01 38 -57.2 290.7 -58.8 B3V 0.45 -2.77 22.68 0.57 144 10. -
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 -
Stars and Their Spectra: an Introduction to the Spectral Sequence Second Edition James B
Cambridge University Press 978-0-521-89954-3 - Stars and Their Spectra: An Introduction to the Spectral Sequence Second Edition James B. Kaler Index More information Star index Stars are arranged by the Latin genitive of their constellation of residence, with other star names interspersed alphabetically. Within a constellation, Bayer Greek letters are given first, followed by Roman letters, Flamsteed numbers, variable stars arranged in traditional order (see Section 1.11), and then other names that take on genitive form. Stellar spectra are indicated by an asterisk. The best-known proper names have priority over their Greek-letter names. Spectra of the Sun and of nebulae are included as well. Abell 21 nucleus, see a Aurigae, see Capella Abell 78 nucleus, 327* ε Aurigae, 178, 186 Achernar, 9, 243, 264, 274 z Aurigae, 177, 186 Acrux, see Alpha Crucis Z Aurigae, 186, 269* Adhara, see Epsilon Canis Majoris AB Aurigae, 255 Albireo, 26 Alcor, 26, 177, 241, 243, 272* Barnard’s Star, 129–130, 131 Aldebaran, 9, 27, 80*, 163, 165 Betelgeuse, 2, 9, 16, 18, 20, 73, 74*, 79, Algol, 20, 26, 176–177, 271*, 333, 366 80*, 88, 104–105, 106*, 110*, 113, Altair, 9, 236, 241, 250 115, 118, 122, 187, 216, 264 a Andromedae, 273, 273* image of, 114 b Andromedae, 164 BDþ284211, 285* g Andromedae, 26 Bl 253* u Andromedae A, 218* a Boo¨tis, see Arcturus u Andromedae B, 109* g Boo¨tis, 243 Z Andromedae, 337 Z Boo¨tis, 185 Antares, 10, 73, 104–105, 113, 115, 118, l Boo¨tis, 254, 280, 314 122, 174* s Boo¨tis, 218* 53 Aquarii A, 195 53 Aquarii B, 195 T Camelopardalis, -
Abstracts from the Fifth European Workshop on Astrobiology EANA
International Journal of Astrobiology 5 (1): 67–88 (2006) Printed in the United Kingdom 67 doi:10.1017/S1473550406002849 f 2006 Cambridge University Press Abstracts from the Fifth European Workshop on Astrobiology EANA – European Astrobiology Network Association 10–12 October 2005 Budapest, Hungary Early Stars and Stellar Environments Oral Presentations The UV radiation environment in the Solar System Setting a scene: before another Earth will be found A. Hanslmeier(1), M. Vazquez(2), H. Lammer(3), M. Khodachenko(3) E. Szuszkiewicz(1,2), J. C. B. Papaloizou(3,4) (1) Institut fu¨r Physik, Geophysik Astrophysik Meteorologie, Univ.- (1) Institute of Physics, University of Szczecin, Poland; (2) Centre for Platz 5, A-8010 Graz, Austria; (2) Instituto de Astrofisica de Canarias, Advanced Studies in Astrobiology and Related Topics, Szczecin, C/Vı´aLa´ctea s/n, E-38200, La Laguna, Tenerife, Spain; (3) Austrian Poland; (3) Astronomy Unit, Queen Mary, University of London, Academy of Science Space Research Institute Schmiedlstraße 6, A-8042 England; (4) Department of Applied Mathematics and Theoretical Graz, Austria Physics, Centre for Mathematical Sciences, Cambridge, England The UV radiation environment in the Solar System is dominated of The increasing number of extrasolar multi-planet systems, their diver- course by the Sun. Since the early Sun radiated more intensely in the sity, and dynamical complexities provide a strong motivation to study short wavelength range, the influence of this radiation to the early the evolution and stability of such systems. One of the most important planets and to the formation of early planetary atmospheres as well as features connected with planetary system evolution is the occurrence of to the evolution of life on Earth and possibly other planets has to be mean motion resonances, which may relate to conditions at the time of considered in detail. -
Apollo 17 Index: 70 Mm, 35 Mm, and 16 Mm Photographs
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) Preparation, Scanning, Editing, and Conversion to Adobe Portable Document Format (PDF) by: Ronald A. Wells University of California Berkeley, CA 94720 May 2000 A P O L L O 1 7 I N D E X 7 0 m m, 3 5 m m, A N D 1 6 m m P H O T O G R A P H S M a p p i n g S c i e n c e s B r a n c h N a t i o n a l A e r o n a u t i c s a n d S p a c e A d m i n i s t r a t i o n J o h n s o n S p a c e C e n t e r H o u s t o n, T e x a s APPROVED: Michael C . -
Floris Heyne Joel Meter Simon Phillipson Delano Steenmeijer
Floris Heyne Joel Meter Simon Phillipson Delano Steenmeijer Edited by Neil Pearson With a special foreword by Apollo 7 astronaut Walt Cunningham “When you get back… you will be a national hero. But your photographs… they will live forever. Your only key to immortality is the quality of your photography.” Richard W. Underwood NASA Chief of Photography for Mercury, Gemini and Apollo 4 Small steps. Giant leaps. The English word ‘photograph’ is made up of the The early exploration of space is one such historical ancient Greek words ‘photos’ and ‘graphos’ which event, unrivaled among humanity’s achievements. literally mean ‘light writing’. At the time of the Apollo Fortunately space travelers were able to bring back program, that meant exposing a chemically-treated beautiful, moving and instantly recognizable images film to patterns of light and it was this process which to depict it. Those images add a new understanding made it possible to seize moments in time and share to what it means to be human, what it means to them with the world. live on a delicate little orb circling the Sun since time immemorial. A single photograph can tell a story to billions of people. It transcends language barriers, physical Not only did Apollo bring us this photographic barriers and requires no prior knowledge of testimony but many major advancements in the subject. This is the beauty of photography: photographic technology date back to the extensive it reaches out to all people and everybody can research and engineering that was part of the hugely intuitively understand its form and content. -
Adams Adkinson Aeschlimann Aisslinger Akkermann
BUSCAPRONTA www.buscapronta.com ARQUIVO 27 DE PESQUISAS GENEALÓGICAS 189 PÁGINAS – MÉDIA DE 60.800 SOBRENOMES/OCORRÊNCIA Para pesquisar, utilize a ferramenta EDITAR/LOCALIZAR do WORD. A cada vez que você clicar ENTER e aparecer o sobrenome pesquisado GRIFADO (FUNDO PRETO) corresponderá um endereço Internet correspondente que foi pesquisado por nossa equipe. Ao solicitar seus endereços de acesso Internet, informe o SOBRENOME PESQUISADO, o número do ARQUIVO BUSCAPRONTA DIV ou BUSCAPRONTA GEN correspondente e o número de vezes em que encontrou o SOBRENOME PESQUISADO. Número eventualmente existente à direita do sobrenome (e na mesma linha) indica número de pessoas com aquele sobrenome cujas informações genealógicas são apresentadas. O valor de cada endereço Internet solicitado está em nosso site www.buscapronta.com . Para dados especificamente de registros gerais pesquise nos arquivos BUSCAPRONTA DIV. ATENÇÃO: Quando pesquisar em nossos arquivos, ao digitar o sobrenome procurado, faça- o, sempre que julgar necessário, COM E SEM os acentos agudo, grave, circunflexo, crase, til e trema. Sobrenomes com (ç) cedilha, digite também somente com (c) ou com dois esses (ss). Sobrenomes com dois esses (ss), digite com somente um esse (s) e com (ç). (ZZ) digite, também (Z) e vice-versa. (LL) digite, também (L) e vice-versa. Van Wolfgang – pesquise Wolfgang (faça o mesmo com outros complementos: Van der, De la etc) Sobrenomes compostos ( Mendes Caldeira) pesquise separadamente: MENDES e depois CALDEIRA. Tendo dificuldade com caracter Ø HAMMERSHØY – pesquise HAMMERSH HØJBJERG – pesquise JBJERG BUSCAPRONTA não reproduz dados genealógicos das pessoas, sendo necessário acessar os documentos Internet correspondentes para obter tais dados e informações. DESEJAMOS PLENO SUCESSO EM SUA PESQUISA. -
Nicholas Murray BUTLER Arranged Correspondence Box Contents Box
Nicholas Murray BUTLER Arranged Correspondence Box contents Box# Box contents 1 Catalogued correspondence 2 A-AB 3 AC - ADAMS, J. 4 ADAMS, K.-AG 5 AH-AI 6 AJ-ALD 7 ALE-ALLEN, E. 8 ALLEN, F.-ALLEN, W. 9 ALLEN, Y. - AMERICAN AC. 10 AMERICAN AR. - AMERICAN K. 11 AMERICAN L.-AMZ 12 ANA-ANG 13 ANH-APZ 14 AR-ARZ 15 AS-AT 16 AU-AZ 17 B-BAC 18 BAD-BAKER, G. 19 BAKER, H. - BALDWIN 20 BALE-BANG 21 BANH-BARD 22 BARD-BARNES, J. 23 BARNES, N.-BARO 24 BARR-BARS 25 BART-BAT 26 BAU-BEAM 27 BEAN-BED 28 BEE-BELL, D. 29 BELL,E.-BENED 30 BENEF-BENZ 31 BER-BERN 32 BERN-BETT 33 BETTS-BIK 34 BIL-BIR 35 BIS-BLACK, J. 36 BLACK, K.-BLAN 37 BLANK-BLOOD 38 BLOOM-BLOS 39 BLOU-BOD 40 BOE-BOL 41 BON-BOOK 42 BOOK-BOOT 43 BOR-BOT 44 BOU-BOWEN 45 BOWER-BOYD 46 BOYER-BRAL 47 BRAM-BREG 48 BREH-BRIC 49 BRID - BRIT 50 BRIT-BRO 51 BROG-BROOKS 52 BROOKS-BROWN 53 BROWN 54 BROWN-BROWNE 55 BROWNE -BRYA 56 BRYC - BUD 57 BUE-BURD 58 BURE-BURL 59 BURL-BURR 60 BURS-BUTC 61 BUTLER, A. - S. 62 BUTLER, W.-BYZ 63 C-CAI 64 CAL-CAMPA 65 CAMP - CANFIELD, JAMES H. (-1904) 66 CANFIELD, JAMES H. (1905-1910) - CANT 67 CAP-CARNA 68 CARNEGIE (1) 69 CARNEGIE (2) ENDOWMENT 70 CARN-CARR 71 CAR-CASTLE 72 CAT-CATH 73 CATL-CE 74 CH-CHAMB 75 CHAMC - CHAP 76 CHAR-CHEP 77 CHER-CHILD, K. -
ADAPTATION of FORESTS and PEOPLE to CLIMATE Change – a Global Assessment Report
International Union of Forest Research Organizations Union Internationale des Instituts de Recherches Forestières Internationaler Verband Forstlicher Forschungsanstalten Unión Internacional de Organizaciones de Investigación Forestal IUFRO World Series Vol. 22 ADAPTATION OF FORESTS AND PEOPLE TO CLIMATE CHANGE – A Global Assessment Report Prepared by the Global Forest Expert Panel on Adaptation of Forests to Climate Change Editors: Risto Seppälä, Panel Chair Alexander Buck, GFEP Coordinator Pia Katila, Content Editor This publication has received funding from the Ministry for Foreign Affairs of Finland, the Swedish International Development Cooperation Agency, the United Kingdom´s Department for International Development, the German Federal Ministry for Economic Cooperation and Development, the Swiss Agency for Development and Cooperation, and the United States Forest Service. The views expressed within this publication do not necessarily reflect official policy of the governments represented by these institutions. Publisher: International Union of Forest Research Organizations (IUFRO) Recommended catalogue entry: Risto Seppälä, Alexander Buck and Pia Katila. (eds.). 2009. Adaptation of Forests and People to Climate Change. A Global Assessment Report. IUFRO World Series Volume 22. Helsinki. 224 p. ISBN 978-3-901347-80-1 ISSN 1016-3263 Published by: International Union of Forest Research Organizations (IUFRO) Available from: IUFRO Headquarters Secretariat c/o Mariabrunn (BFW) Hauptstrasse 7 1140 Vienna Austria Tel: + 43-1-8770151 Fax: + 43-1-8770151-50 E-mail: [email protected] Web site: www.iufro.org/ Cover photographs: Matti Nummelin, John Parrotta and Erkki Oksanen Printed in Finland by Esa-Print Oy, Tampere, 2009 Preface his book is the first product of the Collabora- written so that they can be read independently from Ttive Partnership on Forests’ Global Forest Expert each other.