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Journal Pre-proof A statistical review of light curves and the prevalence of contact binaries in the Kuiper Belt Mark R. Showalter, Susan D. Benecchi, Marc W. Buie, William M. Grundy, James T. Keane, Carey M. Lisse, Cathy B. Olkin, Simon B. Porter, Stuart J. Robbins, Kelsi N. Singer, Anne J. Verbiscer, Harold A. Weaver, Amanda M. Zangari, Douglas P. Hamilton, David E. Kaufmann, Tod R. Lauer, D.S. Mehoke, T.S. Mehoke, J.R. Spencer, H.B. Throop, J.W. Parker, S. Alan Stern, the New Horizons Geology, Geophysics, and Imaging Team PII: S0019-1035(20)30444-9 DOI: https://doi.org/10.1016/j.icarus.2020.114098 Reference: YICAR 114098 To appear in: Icarus Received date: 25 November 2019 Revised date: 30 August 2020 Accepted date: 1 September 2020 Please cite this article as: M.R. Showalter, S.D. Benecchi, M.W. Buie, et al., A statistical review of light curves and the prevalence of contact binaries in the Kuiper Belt, Icarus (2020), https://doi.org/10.1016/j.icarus.2020.114098 This is a PDF file of an article that has undergone enhancements after acceptance, such as the addition of a cover page and metadata, and formatting for readability, but it is not yet the definitive version of record. This version will undergo additional copyediting, typesetting and review before it is published in its final form, but we are providing this version to give early visibility of the article. Please note that, during the production process, errors may be discovered which could affect the content, and all legal disclaimers that apply to the journal pertain. -
Your Guide to the Transit of Mercury of 9Th May 2016
!1 ! Your guide to the Transit of Mercury of 9th May 2016 a publication of the Public Outreach & Education Committee of the Astronomical Society of India Your guide to the Transit of Mercury 2016 !2 ! This work is licensed under a Creative Commons (Attribution - Non Commercial - ShareAlike) License. Please share/print/ photocopy/distribute this work widely, with attribution to the Public Outreach and Education Committee (POEC) of the Astronomical Society of India (ASI) under this same license. This license is granted for non-commercial use only. Contact details of the Public Outreach and Education Committee of the ASI : URL : http://astron-soc.in/outreach Email : [email protected] Facebook : asi poec Twitter : www.twitter.com/asipoec Download from : The pdf of this documents is available for free download from : http://astron-soc.in/outreach/activities/sky-event-related/transit- of-mercury-2016/ (also http://bit.ly/tom-india) Acknowledgement : We thank all those who made images available online either under the Creative Commons License or by a copyleft through image credits. Compiled by Niruj Ramanujam with contributions from Samir Dhurde, B.S. Shylaja and N. Rathnasree, for the POEC of the ASI April 2016 Your guide to the Transit of Mercury 2016 !3 1. Transit of Mercury ! Transit of Mercury, 8 Nov 2006, Transit of Venus, 6 Jun 2012, photographed by Eric Kounce, from Hungary Texas, USA DID YOU KNOW? The planets, with their moons, steadily revolve around the The next transit Sun, with Mercury taking 88 days and Neptune taking as of Mercury will much as 165 years to make one revolution! We barely occur on 9 May notice any of this, unless something spectacular happens to 2016 but it will not be visible remind us how fast this motion actually is. -
ÉRIS Thèmes De Sa Découverte
Carmela Di Martine – Juin 2020 ÉRIS Thèmes de sa découverte Astronomie La première prise de cliché de l’astre date du 3 septembre 1954 au Mont Palomar en Californie. Éris a été ensuite photographiée lors d’observations effectuées le 21 octobre 2003, avec le télescope Oschin du Mont Palomar par l’équipe de Mike Brown, Chadwick Trujillo et David Rabinowitz. Mais ce n’est en fait que le 5 janvier 2005 qu’elle fut vraiment découverte, lorsque des photographies du même pan de ciel révélèrent son déplacement. Éris et Dysnomie Sous la désignation provisoire 2003 UB313 est officiellement classé « planète naine » le 24 août 2006 par l’Union astronomique internationale. Après avoir été désignée sous différents noms (Xena, Lila, Perséphone, Érèbe...), le « choix » final de la dénomination d’Éris par l’UAI, le 13 septembre 2006, évoque aussi d’une part les discussions et controverses acharnées entre scientifiques sur la remise en cause de la définition du mot « planète » du fait de sa découverte, et d’autre part, l’apparente diversité des orbites des objets épars de cette zone du Système solaire (au-delà de la ceinture de Kuiper) par rapport aux orbites régulières des planètes plus proches du Soleil (jusqu’à Neptune). Sa désignation scientifique officielle complète est (136199) Éris. Pour les principales caractéristiques d’Éris, lire aussi mon article : « Les planètes » (p. 25-27). Astrologie N’aurait-on pas une vision "patriarcale" d’Éris ? Éris la "semeuse de Discordes"… Éris, "l’Emmerdeuse"… Expressions très, trop facilement accordées aussi aux femmes par les hommes… Car des questions se posent tout de même… Pourquoi n’est-ce pas Thétis la « plus Belle » en ce jour de son mariage ? Pourquoi le choix d’Aphrodite embarrasse tant toute l’Assemblé divine qui n’en est pourtant pas habituellement à une guerre près ? Contre toute attente, les thèmes de découvertes d’Éris vont nous dévoiler en effet une toute autre vérité…. -
1 Sednan Day = 10.273 Earth Hours (French)
Welcome to a scale model of our solar system. Sedna In the model, this circle shows Sedna is a trans-Neptunian object (an object that on average orbits the relative size of the Sun. The farther from the Sun than Neptune) discovered on November 14, distances between panels show the 2003 by Michael Brown, Chad Trujillo and David Rabinowitz. relative distances between solar system Sedna has a very elongated orbit, more like a comet than a planet, French translation of text in Sun at upper left corner of panel. objects. The panels for the Sun, Earth and takes over twelve thousand years just to orbit the Sun once. and other planets are located on the It is composed mostly of ices which for unknown reasons are Keele campus. The object Sedna is so far from the Sun that almost as red as the surface of Mars. The temperature on Sedna it is located at Glendon never gets warmer than -240 C (33 degrees above absolute zero). in this scale model. Because it is the coldest, most distant place known in the solar NASA / JPL - system, Sedna was named after the Inuit goddess of the sea, who Caltech / R. Hurt The false-color image to the right, our The four panels above (moving clockwise from the upper left) repeatedly zoom out to best photo of Sedna to date, was taken is thought to live at the bottom of the frigid arctic ocean. with the Hubble Space Telescope. place Sedna in context. The first panel shows the orbits of the inner planets and Jupiter. -
Relatório De Conferência De Produção Intelectual
Relatório de Conferência de Produção Intelectual Dados Gerais Instituição de Ensino: OBSERVATÓRIO NACIONAL (ON) Programa: ASTRONOMIA (31013015001P9) Ano de Referência: 2017 Produções Intelectuais Produção: A GRAVITATIONAL-WAVE STANDARD SIREN MEASUREMENT OF THE HUBBLE CONSTANT AUTHORS: Instituição de Ensino: OBSERVATÓRIO NACIONAL (ON) Programa: ASTRONOMIA (31013015001P9) Ano da Publicação: 2017 A Produção é vinculada a Trabalho de Conclusão concluído: Não É um dos 5 trabalhos mais relevantes do seu programa: Não Autores Ordem Nome Categoria 1 B. P Abbott Sem Categoria 2 MARCIO ANTONIO GEIMBA MAIA DOCENTE 3 RICARDO LOURENCO CORREIA DOCENTE OGANDO 4 LUIZ ALBERTO NICOLACI DA COSTA PARTICIPANTE EXTERNO Detalhamento Tipo: BIBLIOGRÁFICA Subtipo: ARTIGO EM PERIÓDICO ISSN: 1476-4687 Estrato: - Natureza: Completo ISSN / Título do periódico: (1476-4687) NATURE (ONLINE) Nome da editora: Cidade: Volume: 551 Fascículo: Série: Número da página inicial: Número da página final: Idioma: inglês Divulgação: VÁRIOS URL: Observação: Trata-se de um artigo com mais de 30 autores. Apenas os autores vinculados ao Observatório Nacional foram listados. Este artigo é fruto de uma grande colaboração. 10/01/2019 14:14:50 1 Relatório de Conferência de Produção Intelectual DOI: 10.1038/nature24471 Contexto Área de Concentração: ASTROFISICA Linha de Pesquisa: ASTROFÍSICA EXTRAGALÁCTICA Projeto de Pesquisa: Produção: A MODIFIED COROT DETREND ALGORITHM AND THE DISCOVERY OF A NEW PLANETARY COMPANION Instituição de Ensino: OBSERVATÓRIO NACIONAL (ON) Programa: ASTRONOMIA (31013015001P9) Ano da Publicação: 2017 A Produção é vinculada a Trabalho de Conclusão concluído: Sim É um dos 5 trabalhos mais relevantes do seu programa: Sim Autores Ordem Nome Categoria 1 RODRIGO CARLOS BOUFLEUR DISCENTE 2 MARCELO EMILIO DOCENTE 3 EDUARDO JANOT PACHECO PARTICIPANTE EXTERNO 4 LAERTE BRANDAO PAES DE ANDRADE PARTICIPANTE EXTERNO 5 SYLVIO FERRAZ DE MELLO PARTICIPANTE EXTERNO 6 José Dias do Nascimento Jr. -
Spitzer to Size up Newly Found Planet
I n s i d e August 12, 2005 Volume 35 Number 16 News Briefs . 2 The story behind ‘JPL Stories’ . 3 Special Events Calendar . 2 Passings . 4 MRO launch postponed . 2 Letters, Classifieds . 4 Jet Propulsion Laborator y However, the object was so far away Spitzer that its motion was not detected until they reanalyzed the data in January of this year. In the last seven months, to size up the scientists have been studying the planet to better estimate its size and newly its motions. “It's definitely bigger than Pluto,” said found Brown, a professor of planetary astrono- my at Caltech. Scientists can infer the size of a solar planet system object by its brightness, just as one can infer the size of a faraway light bulb if one knows its wattage. The re- Artist’s concept of the flectance of the planet is not yet known. planet catalogued as Scientists cannot yet tell how much 2003UB313 at the light from the Sun is reflected away, lonely outer fringes of but the amount of light the planet re- our solar system. Later this month, the Spitzer Space Telescope flects puts a lower limit on its size. “Even if it reflected 100 percent of the light reaching it, it would Our Sun can be seen will look toward the recently discovered planet in the outlying regions of the solar system. The observation will still be as big as Pluto,” says Brown. “I'd say it’s probably one and a in the distance. bring new information on the size of the 10th planet, which lies half times the size of Pluto, but we’re not sure yet of the final size. -
Asteroid Regolith Weathering: a Large-Scale Observational Investigation
University of Tennessee, Knoxville TRACE: Tennessee Research and Creative Exchange Doctoral Dissertations Graduate School 5-2019 Asteroid Regolith Weathering: A Large-Scale Observational Investigation Eric Michael MacLennan University of Tennessee, [email protected] Follow this and additional works at: https://trace.tennessee.edu/utk_graddiss Recommended Citation MacLennan, Eric Michael, "Asteroid Regolith Weathering: A Large-Scale Observational Investigation. " PhD diss., University of Tennessee, 2019. https://trace.tennessee.edu/utk_graddiss/5467 This Dissertation is brought to you for free and open access by the Graduate School at TRACE: Tennessee Research and Creative Exchange. It has been accepted for inclusion in Doctoral Dissertations by an authorized administrator of TRACE: Tennessee Research and Creative Exchange. For more information, please contact [email protected]. To the Graduate Council: I am submitting herewith a dissertation written by Eric Michael MacLennan entitled "Asteroid Regolith Weathering: A Large-Scale Observational Investigation." I have examined the final electronic copy of this dissertation for form and content and recommend that it be accepted in partial fulfillment of the equirr ements for the degree of Doctor of Philosophy, with a major in Geology. Joshua P. Emery, Major Professor We have read this dissertation and recommend its acceptance: Jeffrey E. Moersch, Harry Y. McSween Jr., Liem T. Tran Accepted for the Council: Dixie L. Thompson Vice Provost and Dean of the Graduate School (Original signatures are on file with official studentecor r ds.) Asteroid Regolith Weathering: A Large-Scale Observational Investigation A Dissertation Presented for the Doctor of Philosophy Degree The University of Tennessee, Knoxville Eric Michael MacLennan May 2019 © by Eric Michael MacLennan, 2019 All Rights Reserved. -
WHERE WAS MEAN SOLAR TIME FIRST ADOPTED? Simone Bianchi INAF-Osservatorio Astrofisico Di Arcetri, Largo E. Fermi, 5, 50125, Flor
WHERE WAS MEAN SOLAR TIME FIRST ADOPTED? Simone Bianchi INAF-Osservatorio Astrofisico di Arcetri, Largo E. Fermi, 5, 50125, Florence, Italy [email protected] Abstract: It is usually stated in the literature that Geneva was the first city to adopt mean solar time, in 1780, followed by London (or the whole of England) in 1792, Berlin in 1810 and Paris in 1816. In this short paper I will partially revise this statement, using primary references when available, and provide dates for a few other European cities. Although no exact date was found for the first public use of mean time, the primacy seems to belong to England, followed by Geneva in 1778–1779 (for horologists), Berlin in 1810, Geneva in 1821 (for public clocks), Vienna in 1823, Paris in 1826, Rome in 1847, Turin in 1849, and Milan, Bologna and Florence in 1860. Keywords: mean solar time 1 INTRODUCTION The inclination of the Earth’s axis with respect to the orbital plane and its non-uniform revolution around the Sun are reflected in the irregularity of the length of the day, when measured from two consecutive passages of the Sun on the meridian. Though known since ancient times, the uneven length of true solar days became of practical interest only after Christiaan Huygens (1629 –1695) invented the high-accuracy pendulum clock in the 1650s. For proper registration of regularly-paced clocks, it then became necessary to convert true solar time into mean solar time, obtained from the position of a fictitious mean Sun; mean solar days all having the same duration over the course of the year. -
Detecting the Yarkovsky Effect Among Near-Earth Asteroids From
Detecting the Yarkovsky effect among near-Earth asteroids from astrometric data Alessio Del Vignaa,b, Laura Faggiolid, Andrea Milania, Federica Spotoc, Davide Farnocchiae, Benoit Carryf aDipartimento di Matematica, Universit`adi Pisa, Largo Bruno Pontecorvo 5, Pisa, Italy bSpace Dynamics Services s.r.l., via Mario Giuntini, Navacchio di Cascina, Pisa, Italy cIMCCE, Observatoire de Paris, PSL Research University, CNRS, Sorbonne Universits, UPMC Univ. Paris 06, Univ. Lille, 77 av. Denfert-Rochereau F-75014 Paris, France dESA SSA-NEO Coordination Centre, Largo Galileo Galilei, 1, 00044 Frascati (RM), Italy eJet Propulsion Laboratory/California Institute of Technology, 4800 Oak Grove Drive, Pasadena, 91109 CA, USA fUniversit´eCˆote d’Azur, Observatoire de la Cˆote d’Azur, CNRS, Laboratoire Lagrange, Boulevard de l’Observatoire, Nice, France Abstract We present an updated set of near-Earth asteroids with a Yarkovsky-related semi- major axis drift detected from the orbital fit to the astrometry. We find 87 reliable detections after filtering for the signal-to-noise ratio of the Yarkovsky drift esti- mate and making sure the estimate is compatible with the physical properties of the analyzed object. Furthermore, we find a list of 24 marginally significant detec- tions, for which future astrometry could result in a Yarkovsky detection. A further outcome of the filtering procedure is a list of detections that we consider spurious because unrealistic or not explicable with the Yarkovsky effect. Among the smallest asteroids of our sample, we determined four detections of solar radiation pressure, in addition to the Yarkovsky effect. As the data volume increases in the near fu- ture, our goal is to develop methods to generate very long lists of asteroids with reliably detected Yarkovsky effect, with limited amounts of case by case specific adjustments. -
Spectrum May June 2016.Pub
Inside this issue: The Spectrum The Calendar 2 The Newsletter for the Buffalo Astronomical Obs report 3 Association Wilson Star Search 7 Randy B. Article 9 Astro Events 11 Eyes on the Earth 12 Star Chart 13 14 Mars Viewing 15 May/June Volume 18, Issue 3 Map 17 ….In This Issue: Did you miss Astro Day? Phil Newman didn’t! Here are some of his slides. hps://db./U8GFuAgM (more pic next issue). Dark Maer And The Demise Of The Dinosaurs. Randy Boswell does it again with another fascinang arcle. Usual charts, calendars. And obs report Don’t forget the 2016 BAA elecons are almost here. You will be deciding on who will serve on the board and guide the associaon into the next few years. There will be more informaon in upcoming meengs and posts, so stay tuned. 1 BAA Schedule of Astronomy Fun for 2016 Public Nights and Events Public Nights ‐ First Saturday of the Month March through October. 2016 Tentave Schedule of Events: May 7 Public Night at BMO May 9 Mercury Transit visible from Buffalo ‐ trip to clear skies anyone?? May 13 BAA meeng May 14 Wilson Star Search June 4 Public Night BMO June 10 BAA meeng‐ Elecons/party June 11 Wilson Star Search July 2 Public Night BMO July 9 Wilson Star Search July 30 BAA annual star party at BMO Aug 6 Public Night BMO Aug 13 Wilson Star Search‐ think meteors! Sep 2/3/4 Black Forest (Rain Fest) Star Party Cherry Springs Pa. Sep 3 Public Night BMO Sep 9 BAA Meeng Sept 10 Wilson Star Search Oct 1 Public Night BMO Oct 8 Wilson Star Search Oct 14 BAA meeng Nov 11 BAA meeng Dec 9 BAA Holiday party 2 Observatory Report The refrigerator is full again (thanks to Dennis B), so I will connue to hold "Tues at the Observatory" The Snow season is over, and the rainy season has started (never stopped), I will be holding Tues night on the clearest night Mon/Tue/or Wed. -
Lunar Distances Final
A (NOT SO) BRIEF HISTORY OF LUNAR DISTANCES: LUNAR LONGITUDE DETERMINATION AT SEA BEFORE THE CHRONOMETER Richard de Grijs Department of Physics and Astronomy, Macquarie University, Balaclava Road, Sydney, NSW 2109, Australia Email: [email protected] Abstract: Longitude determination at sea gained increasing commercial importance in the late Middle Ages, spawned by a commensurate increase in long-distance merchant shipping activity. Prior to the successful development of an accurate marine timepiece in the late-eighteenth century, marine navigators relied predominantly on the Moon for their time and longitude determinations. Lunar eclipses had been used for relative position determinations since Antiquity, but their rare occurrences precludes their routine use as reliable way markers. Measuring lunar distances, using the projected positions on the sky of the Moon and bright reference objects—the Sun or one or more bright stars—became the method of choice. It gained in profile and importance through the British Board of Longitude’s endorsement in 1765 of the establishment of a Nautical Almanac. Numerous ‘projectors’ jumped onto the bandwagon, leading to a proliferation of lunar ephemeris tables. Chronometers became both more affordable and more commonplace by the mid-nineteenth century, signaling the beginning of the end for the lunar distance method as a means to determine one’s longitude at sea. Keywords: lunar eclipses, lunar distance method, longitude determination, almanacs, ephemeris tables 1 THE MOON AS A RELIABLE GUIDE FOR NAVIGATION As European nations increasingly ventured beyond their home waters from the late Middle Ages onwards, developing the means to determine one’s position at sea, out of view of familiar shorelines, became an increasingly pressing problem. -
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.