Spitzer to Size up Newly Found Planet
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Unique Sky Survey Brings New Objects Into Focus 15 June 2009
Unique sky survey brings new objects into focus 15 June 2009 human intervention. The Palomar Transient Factory is a collaboration of scientists and engineers from institutions around the world, including the California Institute of Technology (Caltech); the University of California, Berkeley, and the Lawrence Berkeley National Laboratory (LBNL); Columbia University; Las Cumbres Observatory; the Weizmann Institute of Science in Israel; and Oxford University. During the PTF process, the automated wide-angle 48-inch Samuel Oschin Telescope at Caltech's Palomar Observatory scans the skies using a 100-megapixel camera. The flood of images, more than 100 gigabytes This is the Andromeda galaxy, as seen with the new every night, is then beamed off of the mountain via PTF camera on the Samuel Oschin Telescope at the High Performance Wireless Research and Palomar Observatory. This image covers 3 square Education Network¬-a high-speed microwave data degrees of sky, more than 15 times the size of the full connection to the Internet-and then to the LBNL's moon. Credit: Nugent & Poznanski (LBNL), PTF National Energy Scientific Computing Center. collaboration There, computers analyze the data and compare it to images previously obtained at Palomar. More computers using a type of artificial intelligence software sift through the results to identify the most An innovative sky survey has begun returning interesting "transient" sources-those that vary in images that will be used to detect unprecedented brightness or position. numbers of powerful cosmic explosions-called supernovae-in distant galaxies, and variable Within minutes of a candidate transient's discovery, brightness stars in our own Milky Way. -
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Printer Friendly - - science news articles online technology magazine articles Printer Friendly Beyond Pluto We are only beginning to discover how vast and strange our solar system truly is By Kathy A. Svitil Illustrations by Don Foley DISCOVER Vol. 25 No. 11 | November 2004 | Astronomy & Physics As a child, Mike Brown had all the trappings of an astronomer-in-the-making, with space books, rocket drawings, and a poster of the planets on his bedroom wall. On it, Pluto was depicted as “this crazy and very eccentric planet,” he says. “It was everyone’s favorite crazy planet.” Brown still recalls the mnemonic he learned for the names of the planets: Martha visits every Monday and—a for asteroids—just stays until noon, period. “The ‘period,’ for Pluto, was always suspicious,” Brown says with a laugh. “It didn’t seem to fit. So maybe that was when I first got the idea that Pluto didn’t belong.” Nowadays Brown, a planetary astronomer at Caltech, has no doubt about Pluto’s place in the solar system: “Pluto is not a planet. There is no logical reason to call Pluto a planet.” Like a growing number of his colleagues, Brown believes Pluto is best understood as the largest known member of the Kuiper belt, a band of rocky, icy miniplanets that orbit the sun in a swath stretching from beyond Neptune to a distance of nearly 5 billion miles. “I don’t think it denigrates Pluto at all to say that it is not a planet. I think Pluto is a fascinating and interesting world, and being the largest Kuiper belt object is an honorable thing to be.” No longer is Pluto a lonely outpost in an otherwise empty frontier. -
Spitzer Pipeline Commissioning Observations of DR 6
Spitzer Pipeline Commissioning Observations of DR 6 Sean J. Carey, Jeonghee Rho, William T. Reach, William J. Glaccum, Bidushi Bhattacharya, Mark Lacy, Seppo Laine, Patrick J. Lowrance, Brant O. Nelson, Daniel Stern, Jason A. Surace, Gillian Wilson (Spitzer Science Center) and the IRAC Instrument Team (SAO) Introduction: As part of the Science Verification phase of the In-Orbit Checkout of Spitzer, IRAC observed the HII region DR 6 and the associated infrared cluster DB7 An 8 mm image of a 1.5 by 1.5 degree region centered on (Dutra & Bica 2001). DR 6 is at a distance of 1.0 kpc (Comerón & Torra 2001) . The DR6 from MSX. The HII region is part of the much larger intent of the experiment was to make a representative observation of a region of high structures of the Cygnus X region. Near the HII region are source density and structure similar to observations that will be conducted by general several infrared-dark filaments which are dense molecular observers of Galactic star formation. In addition, these observations provide a stress cores (Carey et al. 1998). test of the IRAC data pipeline and the SSC post-BCD software, including the mosaicer, point source extraction and bandmerging software. Observations: DR 6 was imaged by IRAC using 12s high dynamic range mode on 27 November 2003. High dynamic range observations consist of set of a 0.6s frame and a 12s frame at each pointing. The map is 20 by 10 arcminutes in size with four dithers at each map position. The total integration time per pixel is 43.2 seconds and the map took 20 minutes to complete. -
The X-Ray Universe 2017
The X-ray Universe 2017 6−9 June 2017 Centro Congressi Frentani Rome, Italy A conference organised by the European Space Agency XMM-Newton Science Operations Centre National Institute for Astrophysics, Italian Space Agency University Roma Tre, La Sapienza University ABSTRACT BOOK Oral Communications and Posters Edited by Simone Migliari, Jan-Uwe Ness Organising Committees Scientific Organising Committee M. Arnaud Commissariat ´al’´energie atomique Saclay, Gif sur Yvette, France D. Barret (chair) Institut de Recherche en Astrophysique et Plan´etologie, France G. Branduardi-Raymont Mullard Space Science Laboratory, Dorking, Surrey, United Kingdom L. Brenneman Smithsonian Astrophysical Observatory, Cambridge, USA M. Brusa Universit`adi Bologna, Italy M. Cappi Istituto Nazionale di Astrofisica, Bologna, Italy E. Churazov Max-Planck-Institut f¨urAstrophysik, Garching, Germany A. Decourchelle Commissariat ´al’´energie atomique Saclay, Gif sur Yvette, France N. Degenaar University of Amsterdam, the Netherlands A. Fabian University of Cambridge, United Kingdom F. Fiore Osservatorio Astronomico di Roma, Monteporzio Catone, Italy F. Harrison California Institute of Technology, Pasadena, USA M. Hernanz Institute of Space Sciences (CSIC-IEEC), Barcelona, Spain A. Hornschemeier Goddard Space Flight Center, Greenbelt, USA V. Karas Academy of Sciences, Prague, Czech Republic C. Kouveliotou George Washington University, Washington DC, USA G. Matt Universit`adegli Studi Roma Tre, Roma, Italy Y. Naz´e Universit´ede Li`ege, Belgium T. Ohashi Tokyo Metropolitan University, Japan I. Papadakis University of Crete, Heraklion, Greece J. Hjorth University of Copenhagen, Denmark K. Poppenhaeger Queen’s University Belfast, United Kingdom N. Rea Instituto de Ciencias del Espacio (CSIC-IEEC), Spain T. Reiprich Bonn University, Germany M. Salvato Max-Planck-Institut f¨urextraterrestrische Physik, Garching, Germany N. -
As the Dome of Twilight Sinks Below The
As the dome of twilight sinks below the horizon, a mechanical corps de ballet starts a slow-motion pirouette with each dancer keeping the unblinking eye of a telescope locked on a single spot in the heavens. Shutters open and ancient photons, ending a journey that may have started before the earth was born, collide with sensors that store an electron to mark that photon's arrival. With the dance in motion the directors sit back to watch the show; another imaging session has begun... Image by Marcus Stevens A Full and Proper Kit An introduction to the gear of astro-photography The young recruit is silly – 'e thinks o' suicide; 'E's lost his gutter-devil; 'e 'asn't got 'is pride; But day by day they kicks him, which 'elps 'im on a bit, Till 'e finds 'isself one mornin' with a full an' proper kit. Rudyard Kipling Like the young recruit in Kipling's poem 'The 'Eathen', a deep-sky imaging beginner starts with little in the way of equipment or skill. With 'older' imagers urging him onward, providing him with the benefit of the mistakes that they had made during their journey and allowing him access to the equipment they've built or collected, the newcomer gains the 'equipment' he needs, be it gear or skills, to excel at the art. At that time he has acquired a 'full and proper kit' and ceases to be a recruit. This paper is a discussion of hardware, software, methods and actions that a newcomer might find useful. It is not meant to be an in-depth discussion of all forms of astro-photography; that would take many books and more knowledge than I have available. -
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. -
Comparative Kbology: Using Surface Spectra of Triton
COMPARATIVE KBOLOGY: USING SURFACE SPECTRA OF TRITON, PLUTO, AND CHARON TO INVESTIGATE ATMOSPHERIC, SURFACE, AND INTERIOR PROCESSES ON KUIPER BELT OBJECTS by BRYAN JASON HOLLER B.S., Astronomy (High Honors), University of Maryland, College Park, 2012 B.S., Physics, University of Maryland, College Park, 2012 M.S., Astronomy, University of Colorado, 2015 A thesis submitted to the Faculty of the Graduate School of the University of Colorado in partial fulfillment of the requirement for the degree of Doctor of Philosophy Department of Astrophysical and Planetary Sciences 2016 This thesis entitled: Comparative KBOlogy: Using spectra of Triton, Pluto, and Charon to investigate atmospheric, surface, and interior processes on KBOs written by Bryan Jason Holler has been approved for the Department of Astrophysical and Planetary Sciences Dr. Leslie Young Dr. Fran Bagenal Date The final copy of this thesis has been examined by the signatories, and we find that both the content and the form meet acceptable presentation standards of scholarly work in the above mentioned discipline. ii ABSTRACT Holler, Bryan Jason (Ph.D., Astrophysical and Planetary Sciences) Comparative KBOlogy: Using spectra of Triton, Pluto, and Charon to investigate atmospheric, surface, and interior processes on KBOs Thesis directed by Dr. Leslie Young This thesis presents analyses of the surface compositions of the icy outer Solar System objects Triton, Pluto, and Charon. Pluto and its satellite Charon are Kuiper Belt Objects (KBOs) while Triton, the largest of Neptune’s satellites, is a former member of the KBO population. Near-infrared spectra of Triton and Pluto were obtained over the previous 10+ years with the SpeX instrument at the IRTF and of Charon in Summer 2015 with the OSIRIS instrument at Keck. -
The Big Eye Vol 2 No 1
Friends of Palomar Observatory P.O. Box 200 Palomar Mountain, CA 92060-0200 The Big Eye The Newsletter of the Friends of Palomar Observatory Vol. 2, No. 1 Solar System Now Palomar’s Astronomical Has Eight Planets Bandwidth The International Astronomical Union (IAU) recently downgraded the status of Pluto to that of a “dwarf plan- For the past three years, astronomers at the et,” a designation that will also be applied to the spheri- California Institute of Technology’s Palomar Obser- cal body discovered last year by California Institute of vatory in Southern California have been using the Technology planetary scientist Mike Brown and his col- High Performance Wireless Research and Education leagues. The decision means that only the rocky worlds Network (HPWREN) as the data transfer cyberin- of the inner solar system and the gas giants of the outer frastructure to further our understanding of the uni- system will hereafter be designated as planets. verse. Recent applications include the study of some The ruling effectively settles a year-long controversy of the most cataclysmic explosions in the universe, about whether the spherical body announced last year and the hunt for extrasolar planets, and the discovery informally named “Xena” would rise to planetary status. of our solar system’s tenth planet. The data for all Somewhat larger than Pluto, the body has been informally this research is transferred via HPWREN from the known as Xena since the formal announcement of its remote mountain observatory to college campuses discovery on July 29, 2005, by Brown and his co-discov- hundreds of miles away. -
The Outskirts of Cygnus OB2 ⋆
Astronomy & Astrophysics manuscript no. 9917 c ESO 2008 May 27, 2008 The outskirts of Cygnus OB2 ? F. Comeron´ 1??, A. Pasquali2, F. Figueras3, and J. Torra3 1 European Southern Observatory, Karl-Schwarzschild-Strasse 2, D-85748 Garching, Germany e-mail: [email protected] 2 Max-Planck-Institut fur¨ Astronomie, Konigstuhl¨ 17, D-69117 Heidelberg, Germany e-mail: [email protected] 3 Departament d'Astronomia i Meteorologia, Universitat de Barcelona, E-08028 Barcelona, Spain e-mail: [email protected], [email protected] Received; accepted ABSTRACT Context. Cygnus OB2 is one of the richest OB associations in the local Galaxy, and is located in a vast complex containing several other associations, clusters, molecular clouds, and HII regions. However, the stellar content of Cygnus OB2 and its surroundings remains rather poorly known largely due to the considerable reddening in its direction at visible wavelength. Aims. We investigate the possible existence of an extended halo of early-type stars around Cygnus OB2, which is hinted at by near- infrared color-color diagrams, and its relationship to Cygnus OB2 itself, as well as to the nearby association Cygnus OB9 and to the star forming regions in the Cygnus X North complex. Methods. Candidate selection is made with photometry in the 2MASS all-sky point source catalog. The early-type nature of the selected candidates is conrmed or discarded through our infrared spectroscopy at low resolution. In addition, spectral classications in the visible are presented for many lightly-reddened stars. Results. A total of 96 early-type stars are identied in the targeted region, which amounts to nearly half of the observed sample. -
Asteroids Near and Far
Asteroids Near and Far David J. Tholen Institute for Astronomy University of Hawaii Subaru 20th Anniversary 2019 November 22 Subaru and Near-Earth Asteroids ● Wide, deep imaging one of Subaru's strengths ● One of my earliest uses of Subaru was to look for asteroids interior to the Earth's orbit ● Introduced the term “apohele” to refer to this type of object (to distinguish from Amor, Apollo, Aten near-Earth objects) ● The motivation... Asteroid aphelia circa 2000 The Search for Apohele ● UHAS81 discovered 2004 Dec 13 with Subaru ● Later designated 2004 XZ130 ● At the time of discovery, had the smallest semimajor axis of any known asteroid Orbit of 2004 XZ130 Asteroid aphelia circa 2019 List of Known Apohele Object Aphelion Distance (AU) 2019 AQ3 0.77 2019 LF6 0.79 (418265) 2008 EA32 0.80 2018 JB3 0.88 2013 TQ5 0.89 (164294) 2004 XZ130 0.90 2006 WE4 0.93 2017 YH 0.94 2013 JX28 0.94 (413563) 2005 TG45 0.94 2006 KZ39 0.94 2015 ME131 0.95 2010 XB11 0.95 2014 FO47 0.96 (481817) 2008 UL90 0.96 2017 XA1 0.97 2012 VE46 0.97 (434326) 2004 JG6 0.97 (163693) Atira 0.98 Discovery of Apophis ● Most famous of the objects discovered during the search for Apohele ● Discovered 2004 June 19 UT ● Not a Subaru discovery, yet Subaru played a role that few people know about ● A stack of the three discovery images... Apophis on 2004 June 19 UT Subaru and Apophis ● UHAS55 identified as object of interest in Subaru images taken 2004 June 17 UT ● Motion faster than 90 arcsec/hr at solar elongation of 56 deg ● Attempted to recover on 2004 June 19 UT with Bok 2.29-m