Analysis of Stellar Occultation from the Observation of 2011 WG57, 2005 RM45 and 38628 Huya KBO Targets in Algiers Observatory
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Surface Characteristics of Transneptunian Objects and Centaurs from Photometry and Spectroscopy
Barucci et al.: Surface Characteristics of TNOs and Centaurs 647 Surface Characteristics of Transneptunian Objects and Centaurs from Photometry and Spectroscopy M. A. Barucci and A. Doressoundiram Observatoire de Paris D. P. Cruikshank NASA Ames Research Center The external region of the solar system contains a vast population of small icy bodies, be- lieved to be remnants from the accretion of the planets. The transneptunian objects (TNOs) and Centaurs (located between Jupiter and Neptune) are probably made of the most primitive and thermally unprocessed materials of the known solar system. Although the study of these objects has rapidly evolved in the past few years, especially from dynamical and theoretical points of view, studies of the physical and chemical properties of the TNO population are still limited by the faintness of these objects. The basic properties of these objects, including infor- mation on their dimensions and rotation periods, are presented, with emphasis on their diver- sity and the possible characteristics of their surfaces. 1. INTRODUCTION cally with even the largest telescopes. The physical char- acteristics of Centaurs and TNOs are still in a rather early Transneptunian objects (TNOs), also known as Kuiper stage of investigation. Advances in instrumentation on tele- belt objects (KBOs) and Edgeworth-Kuiper belt objects scopes of 6- to 10-m aperture have enabled spectroscopic (EKBOs), are presumed to be remnants of the solar nebula studies of an increasing number of these objects, and signifi- that have survived over the age of the solar system. The cant progress is slowly being made. connection of the short-period comets (P < 200 yr) of low We describe here photometric and spectroscopic studies orbital inclination and the transneptunian population of pri- of TNOs and the emerging results. -
Exploration of the Kuiper Belt by High-Precision Photometric Stellar Occultations: First Results F
Exploration of the Kuiper Belt by High-Precision Photometric Stellar Occultations: First Results F. Roques, A. Doressoundiram, V. Dhillon, T. Marsh, S. Bickerton, J. J. Kavelaars, M. Moncuquet, M. Auvergne, I. Belskaya, M. Chevreton, et al. To cite this version: F. Roques, A. Doressoundiram, V. Dhillon, T. Marsh, S. Bickerton, et al.. Exploration of the Kuiper Belt by High-Precision Photometric Stellar Occultations: First Results. Astronomical Journal, Amer- ican Astronomical Society, 2006, 132, pp.819-822. 10.1086/505623. hal-00640050 HAL Id: hal-00640050 https://hal.archives-ouvertes.fr/hal-00640050 Submitted on 10 Nov 2011 HAL is a multi-disciplinary open access L’archive ouverte pluridisciplinaire HAL, est archive for the deposit and dissemination of sci- destinée au dépôt et à la diffusion de documents entific research documents, whether they are pub- scientifiques de niveau recherche, publiés ou non, lished or not. The documents may come from émanant des établissements d’enseignement et de teaching and research institutions in France or recherche français ou étrangers, des laboratoires abroad, or from public or private research centers. publics ou privés. The Astronomical Journal, 132:819Y822, 2006 August # 2006. The American Astronomical Society. All rights reserved. Printed in U.S.A. EXPLORATION OF THE KUIPER BELT BY HIGH-PRECISION PHOTOMETRIC STELLAR OCCULTATIONS: FIRST RESULTS F. Roques,1,2 A. Doressoundiram,1 V. Dhillon,3 T. Marsh,4 S. Bickerton,5,6 J. J. Kavelaars,5 M. Moncuquet,1 M. Auvergne,1 I. Belskaya,7 M. Chevreton,1 F. Colas,1 A. Fernandez,1 A. Fitzsimmons,8 J. Lecacheux,1 O. Mousis,9 S. -
Réhabilitation Des Villes À Secteurs Sauvegardé, En Europe Et Au Maghreb
Réhabilitation des villes à secteurs sauvegardé, en Europe et au Maghreb Barcelone, 16 Mai 2011 M. Ballalou Zouhir: Directeur de la culture de la Wilaya de Ghardaïa MEDITERRANEE Alger Constantine Dans le paysage historique et culturel national, la vallée du Oran M’Zab, berceau d’une civilisation ksourienne DJERBA AIN MADI TUNISIE millénaire, constitue de nos Laghouat jour une référence dans la MAROC parfaite harmonie entre La vallée du M’Zab Ghardaïa l’organisation sociale, le SADRATA système d’urbanisation, la Ouargla typologie architecturale, la BECHAR AL-MENIAA maîtrise des ressources hydriques et l’équilibre Tindouf A L G E R I E LIBYE écologique. ADRAR L’ingéniosité du système Ilizi d’urbanisation dans la MAURITANIE maîtrise de la structuration territoriale et le savoir faire architecturale lui ont valu Tamanrasset son classement comme patrimoine national en 1971 MALI et patrimoine de l’humanité par l’UNESCO en 1982. NIGER TOMBOUCTOU Selon la loi 98-04, sont considérés comme patrimoine culturel de la nation, d’une part, les biens culturels immobiliers tels que les monuments historiques, les sites archéologiques et les ensembles urbains ou ruraux; et, d’autres part, les biens culturel mobiliers comme les vestiges préhistoriques, les divers objets de l’antiquité, le matériel anthropologiques et les manuscrits et les archives; légués par les différentes civilisations qui se sont succédés de la préhistoire à nos jours. Font également partie du patrimoine culturel de la nation, les biens culturels immatériels considérés comme des produits de manifestations sociales et de création individuelles et collectives qui s’expriment depuis des temps immémoriaux à nos jours. -
March 21–25, 2016
FORTY-SEVENTH LUNAR AND PLANETARY SCIENCE CONFERENCE PROGRAM OF TECHNICAL SESSIONS MARCH 21–25, 2016 The Woodlands Waterway Marriott Hotel and Convention Center The Woodlands, Texas INSTITUTIONAL SUPPORT Universities Space Research Association Lunar and Planetary Institute National Aeronautics and Space Administration CONFERENCE CO-CHAIRS Stephen Mackwell, Lunar and Planetary Institute Eileen Stansbery, NASA Johnson Space Center PROGRAM COMMITTEE CHAIRS David Draper, NASA Johnson Space Center Walter Kiefer, Lunar and Planetary Institute PROGRAM COMMITTEE P. Doug Archer, NASA Johnson Space Center Nicolas LeCorvec, Lunar and Planetary Institute Katherine Bermingham, University of Maryland Yo Matsubara, Smithsonian Institute Janice Bishop, SETI and NASA Ames Research Center Francis McCubbin, NASA Johnson Space Center Jeremy Boyce, University of California, Los Angeles Andrew Needham, Carnegie Institution of Washington Lisa Danielson, NASA Johnson Space Center Lan-Anh Nguyen, NASA Johnson Space Center Deepak Dhingra, University of Idaho Paul Niles, NASA Johnson Space Center Stephen Elardo, Carnegie Institution of Washington Dorothy Oehler, NASA Johnson Space Center Marc Fries, NASA Johnson Space Center D. Alex Patthoff, Jet Propulsion Laboratory Cyrena Goodrich, Lunar and Planetary Institute Elizabeth Rampe, Aerodyne Industries, Jacobs JETS at John Gruener, NASA Johnson Space Center NASA Johnson Space Center Justin Hagerty, U.S. Geological Survey Carol Raymond, Jet Propulsion Laboratory Lindsay Hays, Jet Propulsion Laboratory Paul Schenk, -
Abstracts of the 50Th DDA Meeting (Boulder, CO)
Abstracts of the 50th DDA Meeting (Boulder, CO) American Astronomical Society June, 2019 100 — Dynamics on Asteroids break-up event around a Lagrange point. 100.01 — Simulations of a Synthetic Eurybates 100.02 — High-Fidelity Testing of Binary Asteroid Collisional Family Formation with Applications to 1999 KW4 Timothy Holt1; David Nesvorny2; Jonathan Horner1; Alex B. Davis1; Daniel Scheeres1 Rachel King1; Brad Carter1; Leigh Brookshaw1 1 Aerospace Engineering Sciences, University of Colorado Boulder 1 Centre for Astrophysics, University of Southern Queensland (Boulder, Colorado, United States) (Longmont, Colorado, United States) 2 Southwest Research Institute (Boulder, Connecticut, United The commonly accepted formation process for asym- States) metric binary asteroids is the spin up and eventual fission of rubble pile asteroids as proposed by Walsh, Of the six recognized collisional families in the Jo- Richardson and Michel (Walsh et al., Nature 2008) vian Trojan swarms, the Eurybates family is the and Scheeres (Scheeres, Icarus 2007). In this theory largest, with over 200 recognized members. Located a rubble pile asteroid is spun up by YORP until it around the Jovian L4 Lagrange point, librations of reaches a critical spin rate and experiences a mass the members make this family an interesting study shedding event forming a close, low-eccentricity in orbital dynamics. The Jovian Trojans are thought satellite. Further work by Jacobson and Scheeres to have been captured during an early period of in- used a planar, two-ellipsoid model to analyze the stability in the Solar system. The parent body of the evolutionary pathways of such a formation event family, 3548 Eurybates is one of the targets for the from the moment the bodies initially fission (Jacob- LUCY spacecraft, and our work will provide a dy- son and Scheeres, Icarus 2011). -
Appulses of Jupiter and Saturn
IN ORIGINAL FORM PUBLISHED IN: arXiv:(side label) [physics.pop-ph] Sternzeit 46, No. 1+2 / 2021 (ISSN: 0721-8168) Date: 6th May 2021 Appulses of Jupiter and Saturn Joachim Gripp, Emil Khalisi Sternzeit e.V., Kiel and Heidelberg, Germany e-mail: gripp or khalisi ...[at]sternzeit-online[dot]de Abstract. The latest conjunction of Jupiter and Saturn occurred at an optical distance of 6 arc minutes on 21 December 2020. We re-analysed all encounters of these two planets between -1000 and +3000 CE, as the extraordinary ones (< 10′) take place near the line of nodes every 400 years. An occultation of their discs did not and will not happen within the historical time span of ±5,000 years around now. When viewed from Neptune though, there will be an occultation in 2046. Keywords: Jupiter-Saturn conjunction, Appulse, Trigon, Occultation. Introduction reason is due to Earth’s orbit: while Jupiter and Saturn are locked in a 5:2-mean motion resonance, the Earth does not The slowest naked-eye planets Jupiter and Saturn made an join in. For very long periods there could be some period- impressive encounter in December 2020. Their approaches icity, however, secular effects destroy a cycle, e.g. rotation have been termed “Great Conjunctions” in former times of the apsides and changes in eccentricity such that we are and they happen regularly every ≈20 years. Before the left with some kind of “semi-periodicity”. discovery of the outer ice giants these classical planets rendered the longest known cycle. The separation at the instant of conjunction varies up to 1 degree of arc, but the Close Encounters latest meeting was particularly tight since the planets stood Most pass-bys of Jupiter and Saturn are not very spectac- closer than at any other occasion for as long as 400 years. -
ASTEROID OCCULTATIONOCCULTATION OBSERVINGOBSERVING (And Recording) ~ a Basic Introduction ~
ASTEROIDASTEROID OCCULTATIONOCCULTATION OBSERVINGOBSERVING (and recording) ~ A basic introduction ~ Most amateur astronomers look forward to observing eclipses – a nice lunar eclipse, and the all-too- rare solar variety. Some travel for hundreds of miles to “catch the shadow”. ...But did you know there are potential eclipses to observe nearly every clear night? There are ---- Asteroid Occultations. What's an asteroid occultation? Assuming you know what an asteroid is.... There are now just over 1 MILLION asteroids that have published orbits. Over 500,000 of them have orbits that are established well enough that they have been “numbered” (in general, the lower the number, the more refined the orbit). There are also billions of stars visible thru a telescope in the night sky. It's only inevitable that at times the alignment will be just right for these chunks of rock in space to pass in front of the absolute pinpoint light from stars. If you are in just the right place on Earth, the asteroid will “eclipse” the star, blocking out its light for anywhere from a fraction of a second, to up to 10's of seconds. As the star is essentially infinitely far away – as compared to the distance to the asteroid – the “shadow” the asteroid casts on Earth is basically the size of the asteroid. This shadow moves across the surface of the Earth in a narrow band (the width of which is the diameter of the asteroid), often crossing thousands of miles of the Earth's surface. If you are located somewhere in this narrow band, and it's clear out, you can see the star “blink out”, and then back - an asteroid occultation. -
Taxonomy of Trans-Neptunian Objects and Centaurs As Seen from Spectroscopy? F
A&A 604, A86 (2017) Astronomy DOI: 10.1051/0004-6361/201730933 & c ESO 2017 Astrophysics Taxonomy of trans-Neptunian objects and Centaurs as seen from spectroscopy? F. Merlin1, T. Hromakina2, D. Perna1, M. J. Hong1, and A. Alvarez-Candal3 1 LESIA – Observatoire de Paris, PSL Research University, CNRS, Sorbonne Universités, UPMC Univ. Paris 06, Univ. Paris Diderot, Sorbonne Paris Cité, 5 place Jules Janssen, 92195 Meudon, France e-mail: [email protected] 2 Institute of Astronomy, Kharkiv V. N. Karin National University, Sumska Str. 35, 61022 Kharkiv, Ukraine 3 Observatorio Nacional, R. Gal. Jose Cristino 77, 20921-400 Rio de Janeiro, Brazil Received 4 April 2017 / Accepted 19 May 2017 ABSTRACT Context. Taxonomy of trans-Neptunian objects (TNOs) and Centaurs has been made in previous works using broadband filters in the visible and near infrared ranges. This initial investigation led to the establishment of four groups with the aim to provide the mean colors of the different classes with possible links with any physical or chemical properties. However, this taxonomy was only made with the Johnson-Cousins filter system and the ESO J, H, Ks filters combination, and any association with other filter system is not yet available. Aims. We aim to edit complete visible to near infrared taxonomy and extend this work to any possible filters system. To do this, we generate mean spectra for each individual group, from a data set of 43 spectra. This work also presents new spectra of the TNO (38628) Huya, on which aqueous alteration has been suspected, and the Centaur 2007 VH305. -
Near-Infrared Mapping and Physical Properties of the Dwarf-Planet Ceres
A&A 478, 235–244 (2008) Astronomy DOI: 10.1051/0004-6361:20078166 & c ESO 2008 Astrophysics Near-infrared mapping and physical properties of the dwarf-planet Ceres B. Carry1,2,C.Dumas1,3,, M. Fulchignoni2, W. J. Merline4, J. Berthier5, D. Hestroffer5,T.Fusco6,andP.Tamblyn4 1 ESO, Alonso de Córdova 3107, Vitacura, Santiago de Chile, Chile e-mail: [email protected] 2 LESIA, Observatoire de Paris-Meudon, 5 place Jules Janssen, 92190 Meudon Cedex, France 3 NASA/JPL, MS 183-501, 4800 Oak Grove Drive, Pasadena, CA 91109-8099, USA 4 SwRI, 1050 Walnut St. # 300, Boulder, CO 80302, USA 5 IMCCE, Observatoire de Paris, CNRS, 77 Av. Denfert Rochereau, 75014 Paris, France 6 ONERA, BP 72, 923222 Châtillon Cedex, France Received 26 June 2007 / Accepted 6 November 2007 ABSTRACT Aims. We study the physical characteristics (shape, dimensions, spin axis direction, albedo maps, mineralogy) of the dwarf-planet Ceres based on high angular-resolution near-infrared observations. Methods. We analyze adaptive optics J/H/K imaging observations of Ceres performed at Keck II Observatory in September 2002 with an equivalent spatial resolution of ∼50 km. The spectral behavior of the main geological features present on Ceres is compared with laboratory samples. Results. Ceres’ shape can be described by an oblate spheroid (a = b = 479.7 ± 2.3km,c = 444.4 ± 2.1 km) with EQJ2000.0 spin α = ◦ ± ◦ δ =+ ◦ ± ◦ . +0.000 10 vector coordinates 0 288 5 and 0 66 5 . Ceres sidereal period is measured to be 9 074 10−0.000 14 h. We image surface features with diameters in the 50–180 km range and an albedo contrast of ∼6% with respect to the average Ceres albedo. -
Vapor Liquid
U.P.B. Sci. Bull., Series B, Vol. 82, Iss. 3, 2020 ISSN 1454-2331 ÉVALUATION DE LA QUALITÉ DES EAUX USÉES TRAITÉES PAR LE SYSTÈME DE LAGUNAGE NATUREL D'EL ATTEUF ET PAR L'ARGILE NATURELLE D'EL MENIA Meriem DJAANI1, Zohra BABA AMER2 Notre étude s’intéresse au traitement des eaux usées urbaines par lagunage naturel d’El atteuf et par l’argile brute d’El menia. Nos résultats montre que les eaux traitées par lagunage naturel ne répondent pas aux normes d’irrigation notamment la DCO, la DBO et la MES (la valeur de l’entrée supérieure à celle de la sortie à cause des algues). En revanche le traitement par l’argile brute permet de résoudre les problèmes obtenus dans le traitement par lagunage naturel et la qualité d’eau traitée utilisable à l’irrigation confortablement. Keywords: Eaux usées urbaines, lagunage naturel d’El atteuf, l’argile brute d’El menia, eaux traitées, irrigation 1. Introduction L'homme à besoin de l'eau pour ses activités et son développement. En revanche l’eau douce ne représente que 2.53 % de toute l’eau de la planète et seule l’eau douce soutien la vie terrestre [1]. D'autre part les accroissements démographiques, économiques et urbains sont à l’origine de différentes sources de pollution environnementale (pollution atmosphérique, pollution des eaux de surfaces et profondes, pollution du sol…), en particulier dans les pays en développement moins préoccupés et moins sensibilisés par les risques sanitaires concomitants [2] et les déversements des eaux usées brutes ou mal épurées sont générateurs de pollution des eaux souterraines et de surface [3]. -
Colours of Minor Bodies in the Outer Solar System II - a Statistical Analysis, Revisited
Astronomy & Astrophysics manuscript no. MBOSS2 c ESO 2012 April 26, 2012 Colours of Minor Bodies in the Outer Solar System II - A Statistical Analysis, Revisited O. R. Hainaut1, H. Boehnhardt2, and S. Protopapa3 1 European Southern Observatory (ESO), Karl Schwarzschild Straße, 85 748 Garching bei M¨unchen, Germany e-mail: [email protected] 2 Max-Planck-Institut f¨ur Sonnensystemforschung, Max-Planck Straße 2, 37 191 Katlenburg- Lindau, Germany 3 Department of Astronomy, University of Maryland, College Park, MD 20 742-2421, USA Received —; accepted — ABSTRACT We present an update of the visible and near-infrared colour database of Minor Bodies in the outer Solar System (MBOSSes), now including over 2000 measurement epochs of 555 objects, extracted from 100 articles. The list is fairly complete as of December 2011. The database is now large enough that dataset with a high dispersion can be safely identified and rejected from the analysis. The method used is safe for individual outliers. Most of the rejected papers were from the early days of MBOSS photometry. The individual measurements were combined so not to include possible rotational artefacts. The spectral gradient over the visible range is derived from the colours, as well as the R absolute magnitude M(1, 1). The average colours, absolute magnitude, spectral gradient are listed for each object, as well as their physico-dynamical classes using a classification adapted from Gladman et al., 2008. Colour-colour diagrams, histograms and various other plots are presented to illustrate and in- vestigate class characteristics and trends with other parameters, whose significance are evaluated using standard statistical tests. -
Jjmonl 1805.Pmd
alactic Observer John J. McCarthy Observatory G Volume 11, No. 5 May 2018 As its fire burns and Cauldron Bubbles, Kilauea’s Secrets are revealed from space Probes the Depths Details on page 16 The John J. McCarthy Observatory Galactic Observer New Milford High School Editorial Committee 388 Danbury Road Managing Editor New Milford, CT 06776 Bill Cloutier Phone/Voice: (860) 210-4117 Production & Design Phone/Fax: (860) 354-1595 www.mccarthyobservatory.org Allan Ostergren Website Development JJMO Staff Marc Polansky Technical Support It is through their efforts that the McCarthy Observatory Bob Lambert has established itself as a significant educational and recreational resource within the western Connecticut Dr. Parker Moreland community. Steve Barone Jim Johnstone Colin Campbell Carly KleinStern Dennis Cartolano Bob Lambert Route Mike Chiarella Roger Moore Jeff Chodak Parker Moreland, PhD Bill Cloutier Allan Ostergren Doug Delisle Marc Polansky Cecilia Detrich Joe Privitera Dirk Feather Monty Robson Randy Fender Don Ross Louise Gagnon Gene Schilling John Gebauer Katie Shusdock Elaine Green Paul Woodell Tina Hartzell Amy Ziffer In This Issue "OUT THE WINDOW ON YOUR LEFT" ............................... 4 ASTRONOMICAL AND HISTORICAL EVENTS ......................... 12 MONS RÜMKER ............................................................. 4 COMMONLY USED TERMS ............................................... 15 JUPITER AT OPPOSITION ................................................... 5 REFERENCES ON DISTANCES ...........................................