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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. -
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. -
Redalyc.Búsqueda General Con La Cámara Mosaico CCD Del
Revista Mexicana de Física ISSN: 0035-001X [email protected] Sociedad Mexicana de Física A.C. México Ferrín, I.; Leal, C.; Hernandez, J. Búsqueda general con la cámara mosaico CCD del telescopio Schmidt de 1m del Observatorio Nacional de Venezuela Revista Mexicana de Física, vol. 52, núm. 3, mayo, 2006, pp. 9-11 Sociedad Mexicana de Física A.C. Distrito Federal, México Disponible en: http://www.redalyc.org/articulo.oa?id=57020393003 Cómo citar el artículo Número completo Sistema de Información Científica Más información del artículo Red de Revistas Científicas de América Latina, el Caribe, España y Portugal Página de la revista en redalyc.org Proyecto académico sin fines de lucro, desarrollado bajo la iniciativa de acceso abierto ASTROFISICA´ REVISTA MEXICANA DE FISICA´ S 52 (3) 9–11 MAYO 2006 Busqueda´ general con la camara´ mosaico CCD del telescopio Schmidt de 1m del Observatorio Nacional de Venezuela I. Ferr´ın y C. Leal Facultad de Ciencias, Departamento de F´ısica, Centro de Astrof´ısica Teorica,´ Universidad de Los Andes Merida,´ Venezuela J. Hernandez Centro de investigaciones de astronom´ıa, CIDA, Merida,´ Venezuela Recibido el 25 de noviembre de 2003; aceptado el 12 de octubre de 2004 En el presente trabajo se muestran los resultados del programa de busqueda´ y seguimiento de diversos objetos astronomicos:´ estrellas variables, supernovas y objetos en movimiento dentro del Sistema Solar. Para ello estamos utilizando el telescopio Schmidt de 1m de diametro´ del Observatorio Nacional de Venezuela, el cual tiene acoplado una camara´ mosaico CCD de 67 Megap´ıxeles, en un arreglo de 4 £ 4 CCDs, cada uno de 2048 £ 2048 p´ıxeles. -
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. -
Artificial Intelligence at the Jet Propulsion Laboratory
AI Magazine Volume 18 Number 1 (1997) (© AAAI) Articles Making an Impact Artificial Intelligence at the Jet Propulsion Laboratory Steve Chien, Dennis DeCoste, Richard Doyle, and Paul Stolorz ■ The National Aeronautics and Space Administra- described here is in the context of the remote- tion (NASA) is being challenged to perform more agent autonomy technology experiment that frequent and intensive space-exploration mis- will fly on the New Millennium Deep Space sions at greatly reduced cost. Nowhere is this One Mission in 1998 (a collaborative effort challenge more acute than among robotic plane- involving JPL and NASA Ames). Many of the tary exploration missions that the Jet Propulsion AI technologists who work at NASA expected Laboratory (JPL) conducts for NASA. This article describes recent and ongoing work on spacecraft to have the opportunity to build an intelli- autonomy and ground systems that builds on a gent spacecraft at some point in their careers; legacy of existing success at JPL applying AI tech- we are surprised and delighted that it has niques to challenging computational problems in come this early. planning and scheduling, real-time monitoring By the year 2000, we expect to demonstrate and control, scientific data analysis, and design NASA spacecraft possessing on-board automat- automation. ed goal-level closed-loop control in the plan- ning and scheduling of activities to achieve mission goals, maneuvering and pointing to execute these activities, and detecting and I research and technology development resolving of faults to continue the mission reached critical mass at the Jet Propul- without requiring ground support. At this Asion Laboratory (JPL) about five years point, mission accomplishment can begin to ago. -
Discovery of Remarkable Opposition Surges on Pluto and Charon
50th Lunar and Planetary Science Conference 2019 (LPI Contrib. No. 2132) 1723.pdf Discovery of Remarkable Opposition Surges on Pluto and Charon. B. J. Buratti1, M. D. Hicks1, E. Kramer1, J. Bauer2. 1Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91109; bon- [email protected]; 2University of Maryland Department of Astronomy, College Park, MD 20742 Introduction: The July 2015 encounter of the New Observations: Our full request of four nights was Horizons spacecraft with Pluto brought a large Kuiper assigned to this project in 2018 and observations in Belt Object into sharp focus for the first time [1]. Pluto JHK wavelengths (1.2, 1.6 and 2.2 µm) were obtained is a dynamic body with the first-ever active glaciers on all nights. One night was slightly cirussy, and fur- observed outside the Earth, possible clouds, snow, sea- ther data analysis beyond the usual pipeline processing sonal volatile transport, and at least two types of the [2] is required to fully reduce this data. Luckily, this dark, elusive material that is ubiquitous in the outer night was the least critical, being slightly smaller in Solar System and that may be tied to the origin of life solar phase angle than our fourth night, which was ob- on Earth. But as spectacular as this flyby was, it repre- tained at our maximum phase angle. sented an instant in time, leaving out the long temporal baseline that is required to capture, understand, and Table 1-2018 JHK data obtained at opposition model the seasonal events and the types of geologic Time (civil) Solar phase angle (°) Longitude (°) processes that were observed on Pluto – and that hap- July 11 0.008 35 pen on 100-year time scales, at least. -
Site Preservation at Palomar Observatory Robert J
SITE PRESERVATION AT PALOMAR OBSERVATORY ROBERT J. BRUCATO Palomar Observatory, California Institute of Technology, Pasadena, CA 91125 ABSTRACT Palomar Mountain was selected as the site of the 200-inch Hale Telescope in 1934. Since then, and especially over the past decade, the population growth of southern California has had a growing adverse impact on the observatory's environment. In 1981, a very active program was initiated to work with the local governmental agencies to prevent further deterioration of the conditions as the area continues to become increasingly urbanized. The character and scope of the program are described in the paper, as well as more general observations relating to the site preservations process. INTRODUCTION The Palomar Observatory, like many of the major optical observatories in the world, is faced with the prospect of increased man-made interference. The most obvious form of this interference is sky glow, or light pollution, from artificial lighting, but the effects of air pollution, aircraft operations and radio frequency interference are also important. To meet these threats, Gerry Neugebauer (the Director of Palomar Observatory) and I have had to expend a greater fraction of our resources to protect our facilities. The aim of this paper is to describe the situation at Palomar and to share our experience. To be sure, the different local conditions make the situation at each observatory a unique case, but there certainly are elements of this issue that are common to all. HISTORICAL BACKGROUND Palomar Mountain is located in the northern part of San Diego County, about 70 km (about 45 miles) from the city of San Diego and about 160 km (about 100 miles) from the Los Angeles basin to the west-northwest. -
The Sitian Project
An Acad Bras Cienc (2021) 93(Suppl. 1): e20200628 DOI 10.1590/0001-3765202120200628 Anais da Academia Brasileira de Ciências | Annals of the Brazilian Academy of Sciences Printed ISSN 0001-3765 I Online ISSN 1678-2690 www.scielo.br/aabc | www.fb.com/aabcjournal PHYSICAL SCIENCES The SiTian Project JIFENG LIU, ROBERTO SORIA, XUE-FENG WU, HONG WU & ZHAOHUI SHANG Abstract: SiTian is an ambitious ground-based all-sky optical monitoring project, developed by the Chinese Academy of Sciences. The concept is an integrated network of dozens of 1-m-class telescopes deployed partly in China and partly at various other sites around the world. The main science goals are the detection, identification and monitoring of optical transients (such as gravitational wave events, fast radio bursts, supernovae) on the largely unknown timescales of less than 1 day; SiTian will also provide a treasure trove of data for studies of AGN, quasars, variable stars, planets, asteroids, and microlensing events. To achieve those goals, SiTian will scan at least 10,000 square deg of sky every 30 min, down to a detection limit of V ≈ 21 mag. The scans will produce simultaneous light-curves in 3 optical bands. In addition, SiTian will include at least three 4-m telescopes specifically allocated for follow-up spectroscopy of the most interesting targets. We plan to complete the installation of 72 telescopes by 2030 and start full scientific operations in 2032. Key words: surveys, telescopes, transients, relativistic processes. INTRODUCTION a 6.7-m filled aperture) with a 9.6 square deg field of view (Ivezić et al.