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Les Principaux Astres Du Système Solaire

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seconde 2009-2010 Les principaux astres du système solaire NB : les corps qui suivent n'étaient pas tous connus des astronomes de l'Antiquité, donc les noms latins et grecs ne sont que des transcriptions modernes. Les planètes et planètes naines sont mises en gras. La distance au Soleil n'est que la moyenne (demi-grand axe) entre l'aphélie et la périhélie ; exemple avec l'orbite de Sedna qui passe en 12 000 ans de 76,057 à 935,451 UA (demi-grand axe : 505,754 UA). Étant donné qu'au printemps 2009 l'Union astronomique internationale dénombrait plus de 450 000 astéroïdes dans notre système, tous ne sont pas présents ci-dessous... Sources : IAU ; Names & discoverers ; Minor Planet Center (Smithsonian). Noms Distances Années de Noms Noms systématiques Symboles au Soleil Noms latins Noms grecs découverte français anglais selon l'IAU (en UA) - 0,000 - Soleil Sol Ήλιος Sun Sol I 0,387 - Mercure Mercvrivs Ερμής Mercury - 0,635 2004 2004 JG6 2004 JG6 Sol II 0,723 - Vénus Venvs Αφροδίτη Venus - 0,723 2002 2002 VE68 2002 VE68 163693 - 0,741 2003 Atira Atira - 0,818 2004 2004 FH 2004 FH 2100 - 0,832 1978 Ra-Shalom Ra-Shalom 2340 - 0,844 1976 Hathor Hathor 99942 - 0,922 2004 Apophis Άποφις Apophis 2062 - 0,967 1976 Aten Aten - 0,997 2003 2003 YN107 2003 YN107 3753 - 0,998 1986 Cruithne Cruithne Sol III 1,000 - Terre Tellvs/Terra Γη/Γαῖα Earth Earth I - - Lune Lvna Σελήνη Moon - 1,000 2002 2002 AA29 2002 AA29 54509 - 1,005 2000 YORP YORP 4581 - 1,022 1989 Asclépios Asclepius 4769 - 1,063 1989 Castalia Castalia 1620 - 1,245 1951 Géographos Geographos 25143 - 1,323 1998 Itokawa Itokawa 433 - 1,458 1898 Éros Eros Eros Sol IV 1,523 - Mars Mars Άρης Mars Mars I - - 1877 Hall Phobos Phobos Φόβος Phobos Mars II - - 1877 Hall Déimos Dimos Δείμος Deimos 5261 - 1,523 1990 Eurêka Eureka 69230 - 1,655 1937 Hermès Hermes 951 - 2,209 1916 Gaspra Gaspra 8 2,201 1847 Hind Flore Χλωρίς Flora 18 - 2,296 1852 Hind Melpomène Μελπομένη Melpomene 12 2,334 1850 Hind Victoria Βικτωρία Victoria 4 2,361 1807 Olbers Vesta Vesta Εστία Vesta 7 2,387 1847 Hind Iris Iris Ίρις Iris 9 2,387 1848 Graham Métis Μήτις Metis 192 - 2,402 1879 Palisa Nausicaa Nausikaa 20 - 2,408 1852 Chacornac Massalia Μασσαλία Massalia 6 2,426 1847 Hencke Hébé Ήβη Hebe 21 - 2,435 1852 Goldschmidt Lutèce Λουτητία Lutetia 19 - 2,441 1852 Hind Fortune Φορτούνα Fortuna 11 2,453 1850 Gasparis Parthénope Παρθενόπη Parthenope 17 - 2,470 1852 Luther Thétis Θέτις Thetis 4179 - 2,522 1989 Toutatis Toutatis 5 2,573 1845 Hencke Astrée Astraea Αστραία Astraea 13 - 2,576 1850 Gasparis Égérie Ηγερία Egeria 14 - 2,585 1851 Hind Irène Ειρήνη Irene 23 - 2,628 1852 Hind Thalie Θάλεια Thalia 253 - 2,646 1885 Palisa Mathilde Mathilde 15 2,646 1851 Gasparis Eunomie Ευνομία Eunomia 3 2,670 1804 Harding Junon Ivno Ήρα Juno 324 - 2,683 1892 Bamberga Bamberga 45 - 2,720 1857 Goldschmidt Eugénie Ευγενία Eugenia (45) Eugenia I - - 1999 Petit-Prince Petit-Prince 1 2,765 1801 Piazzi Cérès Ceres Δήμητρα Ceres 88 - 2,768 1866 Peters Thisbé Thisbe Θίσβη Thisbe 2 2,772 1802 Olbers Pallas Pallas Παλλάς Pallas 243 - 2,861 1884 Ida Ida (243) Ida I - - 1993 Dactyl Dactyl 22 - 2,908 1852 Hind Calliope Καλλιόπη Kalliope 16 - 2,921 1852 Gasparis Psyché Ψυχή Psyche 704 - 3,063 1910 Interamnia Interamnia 52 - 3,100 1858 Goldschmidt Europe Ευρώπη Europa 24 - 3,130 1853 Gasparis Thémis Θέμις Themis 10 3,137 1849 Gasparis Hygie Υγιεία Hygiea 31 - 3,150 1854 Ferguson Euphrosyne Ευφροσύνη Euphrosyne 511 - 3,167 1903 Davida Νταβίντα Davida 65 - 3,434 1861 Tempel Cybèle Κυβέλη Cybele 121 - 3,446 1872 Watson Hermione Hermione 87 - 3,490 1866 Pogson Sylvia Sylvia (87) Sylvia I - - 2001 Romulus Romvlvs Ρωμύλος Romulus (87) Sylvia II - - 2005 Rémus Remvs Ρέμος Remus 659 - 5,187 1908 Nestor Nestor Sol V 5,203 - Jupiter Ivppiter Δίας Jupiter Jupiter I - - 1610 Galilée Io Io Ιώ Io Jupiter II - - 1610 Galilée Europe Europa Ευρώπη Europa Jupiter IV - - 1610 Galilée Callisto Callisto Καλλιστώ Callisto Jupiter III - - 1610 Galilée Ganymède Ganymedes Γανυμήδης Ganymede Jupiter V - - 1892 Amalthée Amalthea Αμάλθεια Amalthea Jupiter VI - - 1905 Himalia Himalia Ιμαλία Himalia Jupiter VII - - 1905 Élara Elara Ελάρα Elara Jupiter VIII - - 1908 Pasiphaé Pasiphae Πασιφάη Pasiphaë Jupiter IX - - 1914 Sinopé Sinope Σινώπη Sinope Jupiter X - - 1938 Lysithéa Lysithea Lysithea Jupiter XI - - 1938 Carmé Carme Carme Jupiter XII - - 1951 Ananké Anance Ananke Jupiter XIII - - 1974 Léda Leda Leda Jupiter XVIII - - 1975 Thémisto Themisto Jupiter XV - - 1979 Adrastée Adrastea Adrastea Jupiter XIV - - 1980 Thébé Thebe Thebe Jupiter XVI - - 1980 Métis Metis Metis Jupiter XVII - - 2000 Callirrhoé Callirrhoe Jupiter XVIII - - 2000 Thémisto Themisto Jupiter XXIII - - 2000 Calycé Kalyke Jupiter XXIV - - 2000 Jocaste Iocaste Jupiter XXV - - 2000 Érinomé Erinome Jupiter XXII - - 2000 Harpalycé Harpalyke Jupiter XXVI - - 2000 Isonoé Isonoe Jupiter XXVII - - 2000 Praxidiké Praxidike Jupiter XIX - - 2000 Mégaclité Megaclite Jupiter XX - - 2000 Taygète Taygete Jupiter XXI - - 2000 Chaldèné Chaldene Jupiter - - 2000 S/2000 J 11 S/2000 J 11 Jupiter XXX - - 2002 Hermippé Hermippe Jupiter XXXII - - 2002 Eurydomé Eurydome Jupiter XXXVI - - 2002 Spondé Sponde Jupiter XXXVII - - 2002 Calé Kale Jupiter XXVIII - - 2002 Autonoé Autonoe Jupiter XXIX - - 2002 Thyoné Thyone Jupiter XXXVIII - - 2002 Pasithée Pasithee Jupiter XXXIII - - 2002 Euanthé Euanthe Jupiter XXXV - - 2002 Orthosie Orthosie Jupiter XXXIV - - 2002 Euporie Euporie Jupiter XXXI - - 2002 Aitné Aitne Jupiter XLIII - - 2002 Arché Arche Jupiter XLVII - - 2003 Eukéladé Eukelade Jupiter - - 2003 S/2003 J 2 S/2003 J 2 Jupiter - - 2003 S/2003 J 3 S/2003 J 3 Jupiter - - 2003 S/2003 J 4 S/2003 J 4 Jupiter - - 2003 S/2003 J 5 S/2003 J 5 Jupiter XLV - - 2003 Hélicé Helike Jupiter XLI - - 2003 Aoédé Aoede Jupiter XXXIX - - 2003 Hégémone Hegemone Jupiter - - 2003 S/2003 J 9 S/2003 J 9 Jupiter - - 2003 S/2003 J 10 S/2003 J 10 Jupiter XLIV - - 2003 Callichore Kallichore Jupiter - - 2003 S/2003 J 12 S/2003 J 12 Jupiter XLVIII - - 2003 Cyllèné Cyllene Jupiter XLIX - - 2003 Coré Kore Jupiter - - 2003 S/2003 J 15 S/2003 J 15 Jupiter - - 2003 S/2003 J 16 S/2003 J 16 Jupiter - - 2003 S/2003 J 17 S/2003 J 17 Jupiter - - 2003 S/2003 J 18 S/2003 J 18 Jupiter - - 2003 S/2003 J 19 S/2003 J 19 Jupiter XLVI - - 2003 Carpo Carpo Jupiter XL - - 2003 Mnémé Mneme Jupiter XLII - - 2004 Thelxinoé Thelxinoe Jupiter - - 2004 S/2003 J 23 S/2003 J 23 3317 - 5,212 1984 Paris Paris 624 - 5,222 1907 Hector Έκτωρ Hektor 1143 - 5,258 1930 Odyssée Odysseus 1173 - 5,315 1930 Anchise Anchises Sol VI 9,537 - Saturne Satvrnvs Κρόνος Saturn Saturn VI - - 1655 Huygens Titan Titan Τιτάνας Titan Saturn VIII - - 1671 Cassini Japet Iapetvs Ιαπετός Iapetus Saturn V - - 1672 Cassini Rhéa Rhea Ρέα Rhea Saturn III - - 1684 Cassini Téthys Tethys Τηθύς Tethys Saturn IV - - 1684 Cassini Dioné Dione Διώνη Dione Saturn II - - 1789 Herschel Encelade Enceladvs Εγκέλαδος Enceladus Saturn I - - 1789 Herschel Mimas Mimas Μίμας Mimas Saturn VII - - 1848 Bond Hypérion Hyperion Υπερίων Hyperion Saturn IX - - 1899 Phœbé Phoebe Φοίβη Phoebe Saturn X - - 1966 Janus Ianvs Janus Saturn XI - - 1966 Épiméthée Epimethevs Epimetheus Saturn XII - - 1980 Hélène Helene Helene Saturn XIII - - 1980 Télesto Telesto Telesto Saturn XIV - - 1980 Calypso Calypso Calypso Saturn XVI - - 1980 Prométhée Promethevs Prometheus Saturn XVII - - 1980 Pandore Pandora Pandora Saturn XV - - 1980 Atlas Atlas Atlas Saturn XVIII - - 1990 Pan Pan Pan Saturn XIX - - 2000 Ymir Ymir Ymir Saturn XX - - 2000 Paaliaq Paaliaq Paaliaq Saturn XXIX - - 2000 Siarnaq Siarnaq Siarnaq Saturn XXI - - 2000 Tarvos Tarvos Tarvos Saturn XXIV - - 2000 Kiviuq Kivivq Kiviuq Saturn XXII - - 2000 Ijiraq Iiraq Ijiraq Saturn XXX - - 2000 Thrymr Thrymer Thrymr Saturn XXVII - - 2000 Skathi Scathi Skathi Saturn XXV - - 2000 Mundilfari Mvndilfari Mundilfari Saturn XXVIII - - 2000 Erriapo Erriapo Erriapus Saturn XXVI - - 2000 Albiorix Albiorix Albiorix Saturn XXIII - - 2000 Suttungr Svttvnger Suttungr Saturn XXXI - - 2003 Narvi Narvi Narvi Saturn XXXII - - 2004 Méthone Methone Methone Saturn XXXIII - - 2004 Pallène Pallene Pallene Saturn - - 2004 S/2004 S 3 S/2004 S 3 Saturn - - 2004 S/2004 S 4 S/2004 S 4 Saturn XXXIV - - 2004 Pollux Polydeuces Saturn - - 2004 S/2004 S 6 S/2004 S 6 Saturn - - 2005 S/2004 S 7 S/2004 S 7 Saturn XLII - - 2005 Fornjot Fornjot Saturn XL - - 2005 Farbauti Farbauti Saturn XXXVI - - 2005 Ægir Aegir Saturn XXXVII - - 2005 Bebhionn Bebhionn Saturn - - 2005 S/2004 S 12 S/2004 S 12 Saturn - - 2005 S/2004 S 13 S/2004 S 13 Saturn XLIII - - 2005 Hati Hati Saturn XXXVIII - - 2005 Bergelmir Bergelmir Saturn XLI - - 2005 Fenrir Fenrir Saturn - - 2005 S/2004 S 17 S/2004 S 17 Saturn XXXIX - - 2005 Bestla Bestla Saturn XXXV - - 2005 Daphnis Daphnis Saturn XLIV - - 2006 Hyrrokkin Hyrrokkin Saturn - - 2006 S/2006 S 1 S/2006 S 1 Saturn XLV - - 2006 Kari Kari Saturn - - 2006 S/2006 S 3 S/2006 S 3 Saturn LI - - 2006 Greip Greip Saturn XLVI - - 2006 Loge Loge Saturn L - - 2006 Jarnsaxa Jarnsaxa Saturn XLVIII - - 2006 Surtur Surtur Saturn XLVII - - 2006 Skoll Skoll Saturn LII - - 2007 Tarqeq Tarqeq Saturn - - 2007 S/2007 S 2 S/2007 S 2 Saturn - - 2007 S/2007 S 3 S/2007 S 3 Saturn XLIX - - 2007 Anthée Anthe Saturn LIII - - 2009 Égéon Aegaeon 2060 - 13,65 1977 Chiron Chiron 10199 - 15,86 1997 Chariklo Χαρικλώ Chariklo 54598 - 16,47 2000 Bienor Bienor Sol VII 19,22 1781 Herschel Uranus Vranvs Ουρανός Uranus Uranus III - - 1787 Herschel Titania Titania Τιτάνια Titania Uranus IV - - 1787 Herschel Obéron Oberon Όμπερον Oberon Uranus I - - 1851 Lassell Ariel
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    MNRAS 451, 244–256 (2015) doi:10.1093/mnras/stv997 Dynamical evolution of the Cybele asteroids Downloaded from https://academic.oup.com/mnras/article-abstract/451/1/244/1381346 by Universidade Estadual Paulista J�lio de Mesquita Filho user on 22 April 2019 V. Carruba,1‹ D. Nesvorny,´ 2 S. Aljbaae1 andM.E.Huaman1 1UNESP, Univ. Estadual Paulista, Grupo de dinamicaˆ Orbital e Planetologia, 12516-410 Guaratingueta,´ SP, Brazil 2Department of Space Studies, Southwest Research Institute, Boulder, CO 80302, USA Accepted 2015 May 1. Received 2015 May 1; in original form 2015 April 1 ABSTRACT The Cybele region, located between the 2J:-1A and 5J:-3A mean-motion resonances, is ad- jacent and exterior to the asteroid main belt. An increasing density of three-body resonances makes the region between the Cybele and Hilda populations dynamically unstable, so that the Cybele zone could be considered the last outpost of an extended main belt. The presence of binary asteroids with large primaries and small secondaries suggested that asteroid families should be found in this region, but only relatively recently the first dynamical groups were identified in this area. Among these, the Sylvia group has been proposed to be one of the oldest families in the extended main belt. In this work we identify families in the Cybele region in the context of the local dynamics and non-gravitational forces such as the Yarkovsky and stochastic Yarkovsky–O’Keefe–Radzievskii–Paddack (YORP) effects. We confirm the detec- tion of the new Helga group at 3.65 au, which could extend the outer boundary of the Cybele region up to the 5J:-3A mean-motion resonance.
  • Universidade Estadual Paulista "Júlio De Mesquita Filho" Campus De Guaratinguetá

    Universidade Estadual Paulista "Júlio De Mesquita Filho" Campus De Guaratinguetá

    UNIVERSIDADE ESTADUAL PAULISTA "JÚLIO DE MESQUITA FILHO" CAMPUS DE GUARATINGUETÁ TIAGO FRANCISCO LINS LEAL PINHEIRO Estudo da estabilidade de anéis em exoplanetas Guaratinguetá 2019 Tiago Francisco Lins Leal Pinheiro Estudo da estabilidade de anéis em exoplanetas Trabalho Mestrado apresentado ao Conselho da Pós Graduação em Mestrado em Física da Faculdade de Engenharia do Campus de Guaratinguetá, Univer- sidade Estatual Paulista, como parte dos requisitos para obtenção do diploma de Mestre em Mestrado em Física . Orientador: Profo Dr. Rafael Sfair Guaratinguetá 2019 Pinheiro, Tiago Francisco Lins Leal P654E Estudo da estabilidade de anéis em exoplanetas / Tiago Francisco Lins Leal Pinheiro – Guaratinguetá, 2019. 57 f : il. Bibliografia: f. 54 Dissertação (Mestrado) – Universidade Estadual Paulista, Faculdade de Engenharia de Guaratinguetá, 2019. Orientador: Prof. Dr. Rafael Sfair 1. Exoplanetas. 2. Satélites. 3. Métodos de simulação. I. Título. CDU 523.4(043) Luciana Máximo Bibliotecária/CRB-8 3595 DADOS CURRICULARES TIAGO FRANCISCO LINS LEAL PINHEIRO NASCIMENTO 03/06/1993 - Lorena / SP FILIAÇÃO Roberto Carlos Pinheiro Jurema Lins Leal Pinheiro 2012 / 2016 Bacharelado em Física Universidade Estadual Paulista "Júlio de Mesquita Filho" 2017 / 2019 Mestrado em Física Universidade Estadual Paulista "Júlio de Mesquita Filho" Dedico este trabalho aos meus pais, Roberto e Jurema, aos meus irmãos, Maria Teresa, Daniel, Gabriel e Rafael, a minha sobrinha Giovanna Maria e amigos. AGRADECIMENTOS Em primeiro lugar agradeço a Deus, fonte da vida e da graça. Agradeço pela minha vida, minha inteligência, minha família e meus amigos, ao meu orientador, Prof. Dr. Rafael Sfair que jamais deixou de me incentivar. Sem a sua orientação, dedicação e auxílio, o estudo aqui apresentado seria praticamente impossível.
  • Occultation Newsletter Volume 8, Number 4

    Occultation Newsletter Volume 8, Number 4

    Volume 12, Number 1 January 2005 $5.00 North Am./$6.25 Other International Occultation Timing Association, Inc. (IOTA) In this Issue Article Page The Largest Members Of Our Solar System – 2005 . 4 Resources Page What to Send to Whom . 3 Membership and Subscription Information . 3 IOTA Publications. 3 The Offices and Officers of IOTA . .11 IOTA European Section (IOTA/ES) . .11 IOTA on the World Wide Web. Back Cover ON THE COVER: Steve Preston posted a prediction for the occultation of a 10.8-magnitude star in Orion, about 3° from Betelgeuse, by the asteroid (238) Hypatia, which had an expected diameter of 148 km. The predicted path passed over the San Francisco Bay area, and that turned out to be quite accurate, with only a small shift towards the north, enough to leave Richard Nolthenius, observing visually from the coast northwest of Santa Cruz, to have a miss. But farther north, three other observers video recorded the occultation from their homes, and they were fortuitously located to define three well- spaced chords across the asteroid to accurately measure its shape and location relative to the star, as shown in the figure. The dashed lines show the axes of the fitted ellipse, produced by Dave Herald’s WinOccult program. This demonstrates the good results that can be obtained by a few dedicated observers with a relatively faint star; a bright star and/or many observers are not always necessary to obtain solid useful observations. – David Dunham Publication Date for this issue: July 2005 Please note: The date shown on the cover is for subscription purposes only and does not reflect the actual publication date.
  • Precision Astrometry for Fundamental Physics – Gaia

    Precision Astrometry for Fundamental Physics – Gaia

    Gravitation astrometric tests in the external Solar System: the QVADIS collaboration goals M. Gai, A. Vecchiato Istituto Nazionale di Astrofisica [INAF] Osservatorio Astrofisico di Torino [OATo] WAG 2015 M. Gai - INAF-OATo - QVADIS 1 High precision astrometry as a tool for Fundamental Physics Micro-arcsec astrometry: Current precision goals of astrometric infrastructures: a few 10 µas, down to a few µas 1 arcsec (1) 5 µrad 1 micro-arcsec (1 µas) 5 prad Reference cases: • Gaia – space – visible range • VLTI – ground – near infrared range • VLBI – ground – radio range WAG 2015 M. Gai - INAF-OATo - QVADIS 2 ESA mission – launched Dec. 19th, 2013 Expected precision on individual bright stars: 1030 µas WAG 2015 M. Gai - INAF-OATo - QVADIS 3 Spacetime curvature around massive objects 1.5 G: Newton’s 1".74 at Solar limb 8.4 rad gravitational constant GM 1 cos d: distance Sun- 1 1 observer c2d 1 cos M: solar mass 0.5 c: speed of light Deflection [arcsec] angle : angular distance of the source to the Sun 0 0 1 2 3 4 5 6 Distance from Sun centre [degs] Light deflection Apparent variation of star position, related to the gravitational field of the Sun ASTROMETRY WAG 2015 M. Gai - INAF-OATo - QVADIS 4 Precision astrometry for Fundamental Physics – Gaia WAG 2015 M. Gai - INAF-OATo - QVADIS 5 Precision astrometry for Fundamental Physics – AGP Talk A = Apparent star position measurement AGP: G = Testing gravitation in the solar system Astrometric 1) Light deflection close to the Sun Gravitation 2) High precision dynamics in Solar System Probe P = Medium size space mission - ESA M4 (2014) Design driver: light bending around the Sun @ μas fraction WAG 2015 M.