Matrix Matheo Riclin 17

Total Page:16

File Type:pdf, Size:1020Kb

Matrix Matheo Riclin 17 MATRIX MATHEO RICLIN 17 ans MATRIX Mathéo RICLIN 76 510 SAINT VAAST D’EQUIQUEVILLE 06 22 65 04 35 [email protected] http://l-art-de-peindre-de-matrix.e-monsite.com/ Facebook : l’art de peindre de matrix Numéro SIRET : 814 613 220 00015 Né en 2002 à Dieppe, Matrix décide de s’essayer à la peinture à la bombe en juin 2015. Son thème principal repose sur le cosmique et le futurisme. En premier lieu, il réalise ses œuvres sur feuilles de papier glacé A3 puis sur des toiles de petits formats pour enfin passer à des formats de plus en plus grands. Du haut de son jeune âge, il s’initie à l’alliance des couleurs et des ombres maniant différents outils afin de donner de nouveaux effets à ses toiles, toutes uniques. Certaines de ses toiles s’illuminent par transparence intensifiant ainsi les effets de couleur. Certains verront dans ses toiles un besoin d’évasion, d’autres une invitation au voyage. Matrix laisse à chacun la libre interprétation de ses œuvres et espère simplement qu’elle apportera la joie et le plaisir aux yeux. Pour son plus grand plaisir Matrix a participé à quelques expositions PARIS : ART CAPITAL - Salon des Indépendants au Grand Palais PARIS : 2 participations à la Galerie Thuillier CORBEILLE ESSONE MANTES LA JOLIE : Salon Arbuste ROUEN : Salon des Independants ISLE ADAM Invité d’honneur (Notre Dame d’Aliermont, Assigny, …), Artiste unique pour les journées du patrimoine à l’Eglise de Meulers Présentation des toiles lors des 10 ans de la Margotière (établissement pour adultes handicapés) Quelques prix lui ont été décernés. Depuis janvier 2018, MATRIX s’est vu admis à l’académie Art Sciences et Lettres de Paris et obtient en juin le diplôme de la médaille d’Etain. Parmi ces plus belles rencontres, sa passion a permis à Matrix de croiser le chemin du spationaute Thomas PESQUET lors de sa venue à Dieppe en octobre 2017. Liste des expositions Personnelle Du 11 au 29 mars 2020 : Livry Gargan – Château de la foret 2019 : Yvetot - Mairie 2017 : Dieppe - Club House du tennis club de Puys 2017 : Mortemer (près de Neufchatel en Bray) 2016 : Meulers (76) – 95 oeuvres dans une église 2016 : Neufchatel en Bray (76) Collective 2019 Longueville sur scie - Maison médicale MEDISCIE – 21 décembre au 21 mars Paris – Salon des Indépendants au Grand Palais proche des Champs Elysées Rouen - La Halle aux toiles Saint Arnoult Epreville en Roumois – Invité d'honneur Saint Leger du Bourg Denis Saint Nicolas d’Aliermont : Salon d’Art contemporain Yvetot – Mairie – Exposition personnelle Poix de Picardie Veulettes sur Mer – Prix du Jury Isle Adam – Prix d’encouragement par le Lions Club de l’Isle Adam Longueuil Bonsecours Les Damps 2018 Du 24 février au 11 mars : Rouen - 80ème Salon des Artistes Independants Normands - Prix d'Encouragement Du 3 au 4 mars : Saint Nicolas de Bliquetuit Du 17 au 25 mars : Quincampoix Le 25 mars : Le Neubourg (27) Du 6 au 12 avril : Paris - Galerie THUILLIER - Prix de la galerie Thuillier Du 13 au 15 avril : Roumare Du 21 avril au 6 mai : Bernay - Confluent art - Exposition dans l'abbatiale (27) - parmi les 9 coups de cœur Du 28 au 29 avril : Notre Dame d'Aliermont Du 12 au 20 mai : Favières (80) Du 26 mai au 3 juin : Saint Germain les Corbeil (91) – Prix du Jeune Public 2 juin : Paris – Hotel Intercontinental – Diplôme de la médaille d’Etain de Arts-Sciences-Lettres Du 26 au 27 mai : Esteville Du 9 au 10 juin : Bosc Benard Crecy Le 1er juillet : Pont Audemer (27) – 2ème au Prix de la ville de Pont Audemer Du 7 au 8 juillet : Critot Du 13 au 26 juillet : Paris - Galerie Thuillier - Salon d'été Du 1 au 16 septembre : Yebleron Du 14 au 16 septembre : Longueuil Du 29 septembre au 7 octobre : Mantes la Jolie (78) – 8ème Salon Arbuste – Prix Espoir Du 6 au 7 octobre : Croix Mare Du 13 au 14 octobre : Sainte Marguerite sur Duclair Du 8 au 11 novembre : Touffreville la Cable Du 17 au 25 novembre : La Mailleraye - Prix du public et Prix du jeune public Du 24 au 26 novembre : Longueville sur Scie Du 7 au 10 décembre : Evreux 2017 Saint Nicolas de Blicquetuit - 1er Prix du public adulte - 1er Prix du public enfant Rieux - 27ème Salon exposition - Prix d’encouragement Bosc Mesnil - Salon d'Art - 1er Prix du public Neufchatel en Bray - 1er Prix du public Château De Bertangles – Amiens - Prix Jules Lefebvre Auffay - 3ème Prix du public Sainte Marguerite sur Duclair - 1er Prix du public 2016 Du 30 Avril au 1er Mai : Notre Dame d'Aliermont (76) - Invité d'honneur Du 6 au 20 aout : SEAL - Saint Martin en Campagne (76) - Prix du jeune talent Du 16 au 17 septembre : Meulers (76) - Invité d'honneur - exposition en solo dans une église Du 22 au 23 octobre : Saint Vaast d'Equiqueville (76) - Invité d'honneur Du 28 octobre au 1 novembre : Assigny (76) - Invité d'honneur Diplômes et récompenses Articles de presse N° TABLEAU NOM FORMAT PRIX 1 Genese Amazonienne 116*89 350 € 2 Proxima 116*89 350 € 3 Hélio Génèse 116*89 350 € 4 Rives du lotus 80*80 330 € 5 Kappa Columbae 100*70 300 € 6 Sigma Andromedae 80*80 300 € 7 Volta 90*60 270 € N° TABLEAU NOM FORMAT PRIX 8 Mu Columbae 90*60 270 € 9 Beta Orionis 80*80 250 € 10 Andromede 80*80 250 € 11 Univers Bicolore 5 80*80 250 € 12 Cassiopeiae 60*73 180 € 13 Lambda Columbae 70*50 170 € 14 Epsilon Andromedae 65*55 160 € N° TABLEAU NOM FORMAT PRIX 15 Cepheide 70*50 160 € 16 Aldébaran 70*50 160 € 17 Génèse stellaire 80*100 150 € 18 Univers inversé 90*70 150 € 19 Rigel 60*80 140 € 20 Amazonie Boréale 70*93 140 € 21 Mirach 70*50 140 € N° TABLEAU NOM FORMAT PRIX 22 Alpha Trianguli 3 30*95 140 € 23 Almach 60*50 140 € 24 Univers Bicolore 3 60*80 120 € 25 Dzéta Andromedae 60*50 120 € 26 Eta Andromedae 55*45 120 € 27 Gamma Orionis 54*65 100 € 28 Alpha Ross 248 65*54 100 € N° TABLEAU NOM FORMAT PRIX 29 Kappa Orionis 54*65 90 € 30 Alphirk 55*45 80 € 31 Gamma Columbia 46*38 70 € 32 β Amazonie 41*33 60 € 33 Gamma Andromedae 41*33 60 € .
Recommended publications
  • Naming the Extrasolar Planets
    Naming the extrasolar planets W. Lyra Max Planck Institute for Astronomy, K¨onigstuhl 17, 69177, Heidelberg, Germany [email protected] Abstract and OGLE-TR-182 b, which does not help educators convey the message that these planets are quite similar to Jupiter. Extrasolar planets are not named and are referred to only In stark contrast, the sentence“planet Apollo is a gas giant by their assigned scientific designation. The reason given like Jupiter” is heavily - yet invisibly - coated with Coper- by the IAU to not name the planets is that it is consid- nicanism. ered impractical as planets are expected to be common. I One reason given by the IAU for not considering naming advance some reasons as to why this logic is flawed, and sug- the extrasolar planets is that it is a task deemed impractical. gest names for the 403 extrasolar planet candidates known One source is quoted as having said “if planets are found to as of Oct 2009. The names follow a scheme of association occur very frequently in the Universe, a system of individual with the constellation that the host star pertains to, and names for planets might well rapidly be found equally im- therefore are mostly drawn from Roman-Greek mythology. practicable as it is for stars, as planet discoveries progress.” Other mythologies may also be used given that a suitable 1. This leads to a second argument. It is indeed impractical association is established. to name all stars. But some stars are named nonetheless. In fact, all other classes of astronomical bodies are named.
    [Show full text]
  • Camp Marin Lecture Astro Chatter WASP Deadline
    WASP Warren Astronomical Society Paper Volume 31, Number 6 http://www.eaglequest.com/~bondono/WAS June, 1999 Camp Marin Lecture Astro Chatter by Steve Greene by Larry Kalinowski The Warren Astronomical Society was invited to lec- Not one planet, but three, were found circling Upsilon ture at Camp Narrin to 45 Girl Scouts and 15 adults on Andromedae, a fourth magnitude star that can be seen Saturday April 17. The lecture went very well even with with the naked eye, a third of the way between Almach the intense Michigan Nebulosity looming overhead and and M31. One of the planets is four times heavier than in fact falling on our head in the form of rain drops. The Jupiter, the lightest about .75 times. The innermost WAS members and Scouts in attendance persevered. planet has an orbit that carries it around its sun in 4.6 We initiated plan 'B', to take our presentation indoors. days. Two independent teams confirmed each others The audience of Scouts ranged in ages 7 to 14 and conclusions using completely different equipment. The were captivated by the telescopes, the literature, the planets very nearly occupy the same positions as video film and the discussion about astronomy. The Earth, Mars and Mercury, making present theories, scopes were placed near the windows to allow the about where giant gas planets should be from their Scouts look through at the tree tops and an active sun, obsolete. squirrel's nest high in the branches. This exercise pro- vided a way for the girls to understand how to look through a telescope so that when they have a chance see LARRY on page 2 on a dark clear night, their observa- tion of the heavens will be more fruitful.
    [Show full text]
  • GRANDE OURSE URSA MAJOR La Plus Grande Des Constellations
    CONSTELLATIONS DE PRINTEMPS Club d'astronomie de Breuillet – Guide d'observation GOTO – 1/27 GRANDE OURSE URSA MAJOR La plus grande des constellations. Toutes les étoiles du chariot sont des cousines sauf DUBHE et la dernière. Amas de la Grande Ourse, étoiles bleues, d = 80 al, D = 30 al, V = 14 km/s vers le sagittaire. ALCOR et MIZAR double optique mais MIZAR étoile double, d = 78 al, D = 5 millions km, L = 60 sol. ALIOTH géante bleue, d = 82 al, D = 6 millions km, L = 100 sol. ALULA AUSTRALIS couple type soleil, d = 26 al, D = 3 millions km, T = 60 ans M 81 M 82 couple de galaxie d = 11 m.al, Pont gazeux entre les deux M 81 galaxie de Bode, type spirale Seyfert M 82 galaxie du cigare, irrégulière, flambée d’étoiles. M 97 nébuleuse planétaire du Hibou, peu visible M 101 galaxie spirale intermédiaire M 108 galaxie spirale barrée M 109 galaxie spirale barrée PETITE OURSE URSA MINOR Alpha POLARIS super géante bleue double avec compagnon bleu d = 400 al, D = 200 millions km, L = 200 sol. Béta PolarisKOCHAB géante rouge d = 130 al, D = 80 millions km, L = 190 sol. Eta Polaris PERCHAD géante bleue, fausse double. Club d'astronomie de Breuillet – Guide d'observation GOTO – 2/27 d = 500 al, D = 15 millions km, L = 1000 sol. CHIENS DE CHASSE CANES VENATICI Alpha COR CAROLI étoile double d = 100 al, D = 5 millions km, L = 70 sol. M 51 WHIRLPOOL galaxy, galaxie du tourbillon, type spirale de Seyfert, absorption de NGC 5195. M3 amas globulaire d = 340000 al, D = 220 al, V = 147 km/s M 63 galaxie du tournesol d = 36 millions al, V = 570 km/s éloignement M 94 galaxie spirale M 106 galaxie NGC 4631 galaxie LION LEONIS M 65 M 66 Couple de galaxie d = 35 millions al M 65 galaxie spirale intermédiaire M 66 galaxie spirale de Seyfert Amas du Lion M 95 et M 96 galaxie, d = 30 millions al M 105 galaxie elliptique NGC 2903 NGC 3628 Club d'astronomie de Breuillet – Guide d'observation GOTO – 3/27 VIER GE VIR GO Alpha SPICA, Epi de la Vierge, géante bleu d = 270 al, D = 10 millions km, L = 2000 sol.
    [Show full text]
  • Variable Star Classification and Light Curves Manual
    Variable Star Classification and Light Curves An AAVSO course for the Carolyn Hurless Online Institute for Continuing Education in Astronomy (CHOICE) This is copyrighted material meant only for official enrollees in this online course. Do not share this document with others. Please do not quote from it without prior permission from the AAVSO. Table of Contents Course Description and Requirements for Completion Chapter One- 1. Introduction . What are variable stars? . The first known variable stars 2. Variable Star Names . Constellation names . Greek letters (Bayer letters) . GCVS naming scheme . Other naming conventions . Naming variable star types 3. The Main Types of variability Extrinsic . Eclipsing . Rotating . Microlensing Intrinsic . Pulsating . Eruptive . Cataclysmic . X-Ray 4. The Variability Tree Chapter Two- 1. Rotating Variables . The Sun . BY Dra stars . RS CVn stars . Rotating ellipsoidal variables 2. Eclipsing Variables . EA . EB . EW . EP . Roche Lobes 1 Chapter Three- 1. Pulsating Variables . Classical Cepheids . Type II Cepheids . RV Tau stars . Delta Sct stars . RR Lyr stars . Miras . Semi-regular stars 2. Eruptive Variables . Young Stellar Objects . T Tau stars . FUOrs . EXOrs . UXOrs . UV Cet stars . Gamma Cas stars . S Dor stars . R CrB stars Chapter Four- 1. Cataclysmic Variables . Dwarf Novae . Novae . Recurrent Novae . Magnetic CVs . Symbiotic Variables . Supernovae 2. Other Variables . Gamma-Ray Bursters . Active Galactic Nuclei 2 Course Description and Requirements for Completion This course is an overview of the types of variable stars most commonly observed by AAVSO observers. We discuss the physical processes behind what makes each type variable and how this is demonstrated in their light curves. Variable star names and nomenclature are placed in a historical context to aid in understanding today’s classification scheme.
    [Show full text]
  • Milan Dimitrijevic Avgust.Qxd
    1. M. Platiša, M. Popović, M. Dimitrijević, N. Konjević: 1975, Z. Fur Natur- forsch. 30a, 212 [A 1].* 1. Griem, H. R.: 1975, Stark Broadening, Adv. Atom. Molec. Phys. 11, 331. 2. Platiša, M., Popović, M. V., Konjević, N.: 1975, Stark broadening of O II and O III lines, Astron. Astrophys. 45, 325. 3. Konjević, N., Wiese, W. L.: 1976, Experimental Stark widths and shifts for non-hydrogenic spectral lines of ionized atoms, J. Phys. Chem. Ref. Data 5, 259. 4. Hey, J. D.: 1977, On the Stark broadening of isolated lines of F (II) and Cl (III) by plasmas, JQSRT 18, 649. 5. Hey, J. D.: 1977, Estimates of Stark broadening of some Ar III and Ar IV lines, JQSRT 17, 729. 6. Hey, J. D.: Breger, P.: 1980, Stark broadening of isolated lines emitted by singly - ionized tin, JQSRT 23, 311. 7. Hey, J. D.: Breger, P.: 1981, Stark broadening of isolated ion lines by plas- mas: Application of theory, in Spectral Line Shapes I, ed. B. Wende, W. de Gruyter, 201. 8. Сыркин, М. И.: 1981, Расчеты электронного уширения спектральных линий в теории оптических свойств плазмы, Опт. Спектроск. 51, 778. 9. Wiese, W. L., Konjević, N.: 1982, Regularities and similarities in plasma broadened spectral line widths (Stark widths), JQSRT 28, 185. 10. Konjević, N., Pittman, T. P.: 1986, Stark broadening of spectral lines of ho- mologous, doubly ionized inert gases, JQSRT 35, 473. 11. Konjević, N., Pittman, T. P.: 1987, Stark broadening of spectral lines of ho- mologous, doubly - ionized inert gases, JQSRT 37, 311. 12. Бабин, С.
    [Show full text]
  • FY13 High-Level Deliverables
    National Optical Astronomy Observatory Fiscal Year Annual Report for FY 2013 (1 October 2012 – 30 September 2013) Submitted to the National Science Foundation Pursuant to Cooperative Support Agreement No. AST-0950945 13 December 2013 Revised 18 September 2014 Contents NOAO MISSION PROFILE .................................................................................................... 1 1 EXECUTIVE SUMMARY ................................................................................................ 2 2 NOAO ACCOMPLISHMENTS ....................................................................................... 4 2.1 Achievements ..................................................................................................... 4 2.2 Status of Vision and Goals ................................................................................. 5 2.2.1 Status of FY13 High-Level Deliverables ............................................ 5 2.2.2 FY13 Planned vs. Actual Spending and Revenues .............................. 8 2.3 Challenges and Their Impacts ............................................................................ 9 3 SCIENTIFIC ACTIVITIES AND FINDINGS .............................................................. 11 3.1 Cerro Tololo Inter-American Observatory ....................................................... 11 3.2 Kitt Peak National Observatory ....................................................................... 14 3.3 Gemini Observatory ........................................................................................
    [Show full text]
  • Astronomy Magazine 2011 Index Subject Index
    Astronomy Magazine 2011 Index Subject Index A AAVSO (American Association of Variable Star Observers), 6:18, 44–47, 7:58, 10:11 Abell 35 (Sharpless 2-313) (planetary nebula), 10:70 Abell 85 (supernova remnant), 8:70 Abell 1656 (Coma galaxy cluster), 11:56 Abell 1689 (galaxy cluster), 3:23 Abell 2218 (galaxy cluster), 11:68 Abell 2744 (Pandora's Cluster) (galaxy cluster), 10:20 Abell catalog planetary nebulae, 6:50–53 Acheron Fossae (feature on Mars), 11:36 Adirondack Astronomy Retreat, 5:16 Adobe Photoshop software, 6:64 AKATSUKI orbiter, 4:19 AL (Astronomical League), 7:17, 8:50–51 albedo, 8:12 Alexhelios (moon of 216 Kleopatra), 6:18 Altair (star), 9:15 amateur astronomy change in construction of portable telescopes, 1:70–73 discovery of asteroids, 12:56–60 ten tips for, 1:68–69 American Association of Variable Star Observers (AAVSO), 6:18, 44–47, 7:58, 10:11 American Astronomical Society decadal survey recommendations, 7:16 Lancelot M. Berkeley-New York Community Trust Prize for Meritorious Work in Astronomy, 3:19 Andromeda Galaxy (M31) image of, 11:26 stellar disks, 6:19 Antarctica, astronomical research in, 10:44–48 Antennae galaxies (NGC 4038 and NGC 4039), 11:32, 56 antimatter, 8:24–29 Antu Telescope, 11:37 APM 08279+5255 (quasar), 11:18 arcminutes, 10:51 arcseconds, 10:51 Arp 147 (galaxy pair), 6:19 Arp 188 (Tadpole Galaxy), 11:30 Arp 273 (galaxy pair), 11:65 Arp 299 (NGC 3690) (galaxy pair), 10:55–57 ARTEMIS spacecraft, 11:17 asteroid belt, origin of, 8:55 asteroids See also names of specific asteroids amateur discovery of, 12:62–63
    [Show full text]
  • Macrocosmo Nº33
    HA MAIS DE DOIS ANOS DIFUNDINDO A ASTRONOMIA EM LÍNGUA PORTUGUESA K Y . v HE iniacroCOsmo.com SN 1808-0731 Ano III - Edição n° 33 - Agosto de 2006 * t i •■•'• bSÈlÈWW-'^Sif J fé . ’ ' w s » ws» ■ ' v> í- < • , -N V Í ’\ * ' "fc i 1 7 í l ! - 4 'T\ i V ■ }'- ■t i' ' % r ! ■ 7 ji; ■ 'Í t, ■ ,T $ -f . 3 j i A 'A ! : 1 l 4/ í o dia que o ceu explodiu! t \ Constelação de Andrômeda - Parte II Desnudando a princesa acorrentada £ Dicas Digitais: Softwares e afins, ATM, cursos online e publicações eletrônicas revista macroCOSMO .com Ano III - Edição n° 33 - Agosto de I2006 Editorial Além da órbita de Marte está o cinturão de asteróides, uma região povoada com Redação o material que restou da formação do Sistema Solar. Longe de serem chamados como simples pedras espaciais, os asteróides são objetos rochosos e/ou metálicos, [email protected] sem atmosfera, que estão em órbita do Sol, mas são pequenos demais para serem considerados como planetas. Até agora já foram descobertos mais de 70 Diretor Editor Chefe mil asteróides, a maior parte situados no cinturão de asteróides entre as órbitas Hemerson Brandão de Marte e Júpiter. [email protected] Além desse cinturão podemos encontrar pequenos grupos de asteróides isolados chamados de Troianos que compartilham a mesma órbita de Júpiter. Existem Editora Científica também aqueles que possuem órbitas livres, como é o caso de Hidalgo, Apolo e Walkiria Schulz Ícaro. [email protected] Quando um desses asteróides cruza a nossa órbita temos as crateras de impacto. A maior cratera visível de nosso planeta é a Meteor Crater, com cerca de 1 km de Diagramadores diâmetro e 600 metros de profundidade.
    [Show full text]
  • On the Application of Stark Broadening Data Determined with a Semiclassical Perturbation Approach
    Atoms 2014, 2, 357-377; doi:10.3390/atoms2030357 OPEN ACCESS atoms ISSN 2218-2004 www.mdpi.com/journal/atoms Article On the Application of Stark Broadening Data Determined with a Semiclassical Perturbation Approach Milan S. Dimitrijević 1,2,* and Sylvie Sahal-Bréchot 2 1 Astronomical Observatory, Volgina 7, 11060 Belgrade, Serbia 2 Laboratoire d'Etude du Rayonnement et de la Matière en Astrophysique, Observatoire de Paris, UMR CNRS 8112, UPMC, 5 Place Jules Janssen, 92195 Meudon Cedex, France; E-Mail: [email protected] (S.S.-B.) * Author to whom correspondence should be addressed; E-Mail: [email protected]; Tel.: +381-64-297-8021; Fax: +381-11-2419-553. Received: 5 May 2014; in revised form: 20 June 2014 / Accepted: 16 July 2014 / Published: 7 August 2014 Abstract: The significance of Stark broadening data for problems in astrophysics, physics, as well as for technological plasmas is discussed and applications of Stark broadening parameters calculated using a semiclassical perturbation method are analyzed. Keywords: Stark broadening; isolated lines; impact approximation 1. Introduction Stark broadening parameters of neutral atom and ion lines are of interest for a number of problems in astrophysical, laboratory, laser produced, fusion or technological plasma investigations. Especially the development of space astronomy has enabled the collection of a huge amount of spectroscopic data of all kinds of celestial objects within various spectral ranges. Consequently, the atomic data for trace elements, which had not been
    [Show full text]
  • Astronomy 2009 Index
    Astronomy Magazine 2009 Index Subject Index 1RXS J160929.1-210524 (star), 1:24 4C 60.07 (galaxy pair), 2:24 6dFGS (Six Degree Field Galaxy Survey), 8:18 21-centimeter (neutral hydrogen) tomography, 12:10 93 Minerva (asteroid), 12:18 2008 TC3 (asteroid), 1:24 2009 FH (asteroid), 7:19 A Abell 21 (Medusa Nebula), 3:70 Abell 1656 (Coma galaxy cluster), 3:8–9, 6:16 Allen Telescope Array (ATA) radio telescope, 12:10 ALMA (Atacama Large Millimeter/sub-millimeter Array), 4:21, 9:19 Alpha (α) Canis Majoris (Sirius) (star), 2:68, 10:77 Alpha (α) Orionis (star). See Betelgeuse (Alpha [α] Orionis) (star) Alpha Centauri (star), 2:78 amateur astronomy, 10:18, 11:48–53, 12:19, 56 Andromeda Galaxy (M31) merging with Milky Way, 3:51 midpoint between Milky Way Galaxy and, 1:62–63 ultraviolet images of, 12:22 Antarctic Neumayer Station III, 6:19 Anthe (moon of Saturn), 1:21 Aperture Spherical Telescope (FAST), 4:24 APEX (Atacama Pathfinder Experiment) radio telescope, 3:19 Apollo missions, 8:19 AR11005 (sunspot group), 11:79 Arches Cluster, 10:22 Ares launch system, 1:37, 3:19, 9:19 Ariane 5 rocket, 4:21 Arianespace SA, 4:21 Armstrong, Neil A., 2:20 Arp 147 (galaxy pair), 2:20 Arp 194 (galaxy group), 8:21 art, cosmology-inspired, 5:10 ASPERA (Astroparticle European Research Area), 1:26 asteroids. See also names of specific asteroids binary, 1:32–33 close approach to Earth, 6:22, 7:19 collision with Jupiter, 11:20 collisions with Earth, 1:24 composition of, 10:55 discovery of, 5:21 effect of environment on surface of, 8:22 measuring distant, 6:23 moons orbiting,
    [Show full text]
  • Astrobiology Math
    National Aeronautics andSpace Administration Aeronautics National Astrobiology Math This collection of activities is based on a weekly series of space science problems intended for students looking for additional challenges in the math and physical science curriculum in grades 6 through 12. The problems were created to be authentic glimpses of modern science and engineering issues, often involving actual research data. The problems were designed to be one-pagers with a Teacher’s Guide and Answer Key as a second page. This compact form was deemed very popular by participating teachers. Astrobiology Math Mathematical Problems Featuring Astrobiology Applications Dr. Sten Odenwald NASA / ADNET Corp. [email protected] Astrobiology Math i http://spacemath.gsfc.nasa.gov Acknowledgments: We would like to thank Ms. Daniella Scalice for her boundless enthusiasm in the review and editing of this resource. Ms. Scalice is the Education and Public Outreach Coordinator for the NASA Astrobiology Institute (NAI) at the Ames Research Center in Moffett Field, California. We would also like to thank the team of educators and scientists at NAI who graciously read through the first draft of this book and made numerous suggestions for improving it and making it more generally useful to the astrobiology education community: Dr. Harold Geller (George Mason University), Dr. James Kratzer (Georgia Institute of Technology; Doyle Laboratory) and Ms. Suzi Taylor (Montana State University), For more weekly classroom activities about astronomy and space visit the Space Math@ NASA website, http://spacemath.gsfc.nasa.gov Image Credits: Front Cover: Collage created by Julie Fletcher (NAI), molecule image created by Jenny Mottar, NASA HQ.
    [Show full text]
  • News from the Society for Astronomical Sciences
    News from the Society for Astronomical Sciences January, 2011 30th Anniversary of the Call for Papers 2011 Keynote Speaker: Society for Astronomical Papers are now being accepted for the Dr. Petrus Jenniskens Sciences SAS 2011 Symposium on Telescope Science. Topics on the full range of "The impact and recovery The 2011 Symposium on Telescope th small-telescope science are wel- of 2008 TC3" Science will mark the 30 anniversary comed: pro-am collaboration, science of the Society for Astronomical Sci- education, evaluation of recent profes- On October 7, 2008, a small 3-4 m ences. The enthusiasm of the partici- sional results on relevant targets (e.g. sized asteroid was discovered to be on pants for small-telescope science has small solar system bodies, planets, a collision course with Earth, the first not changed over those three dec- variable stars), and special uses of time an asteroid was seen coming in. ades. The growth in the size and par- astronomical data. Now called "2008 TC3", astronomers ticipation by both amateur and profes- studied the asteroid's lightcurve and sional astronomers bear witness to the Please send the abstract of your pro- reflection properties. Twenty hours important roles that the Symposium posed paper to the Program Commit- later, it crashed in the Nubian desert of plays: tee at [email protected]. Northern Sudan. When satellites saw it explode at an unusually high altitude • An opportunity for non-professional Deadlines are: of 37 km, many thought that was the researchers to present their projects Abstract submission: March 12, 2011 end of the story.
    [Show full text]