Santa Fe, New Mexico, USA May 31 – June 5, 2009
Total Page:16
File Type:pdf, Size:1020Kb
Load more
Recommended publications
-
Messier Objects
Messier Objects From the Stocker Astroscience Center at Florida International University Miami Florida The Messier Project Main contributors: • Daniel Puentes • Steven Revesz • Bobby Martinez Charles Messier • Gabriel Salazar • Riya Gandhi • Dr. James Webb – Director, Stocker Astroscience center • All images reduced and combined using MIRA image processing software. (Mirametrics) What are Messier Objects? • Messier objects are a list of astronomical sources compiled by Charles Messier, an 18th and early 19th century astronomer. He created a list of distracting objects to avoid while comet hunting. This list now contains over 110 objects, many of which are the most famous astronomical bodies known. The list contains planetary nebula, star clusters, and other galaxies. - Bobby Martinez The Telescope The telescope used to take these images is an Astronomical Consultants and Equipment (ACE) 24- inch (0.61-meter) Ritchey-Chretien reflecting telescope. It has a focal ratio of F6.2 and is supported on a structure independent of the building that houses it. It is equipped with a Finger Lakes 1kx1k CCD camera cooled to -30o C at the Cassegrain focus. It is equipped with dual filter wheels, the first containing UBVRI scientific filters and the second RGBL color filters. Messier 1 Found 6,500 light years away in the constellation of Taurus, the Crab Nebula (known as M1) is a supernova remnant. The original supernova that formed the crab nebula was observed by Chinese, Japanese and Arab astronomers in 1054 AD as an incredibly bright “Guest star” which was visible for over twenty-two months. The supernova that produced the Crab Nebula is thought to have been an evolved star roughly ten times more massive than the Sun. -
Spatial Distribution of Galactic Globular Clusters: Distance Uncertainties and Dynamical Effects
Juliana Crestani Ribeiro de Souza Spatial Distribution of Galactic Globular Clusters: Distance Uncertainties and Dynamical Effects Porto Alegre 2017 Juliana Crestani Ribeiro de Souza Spatial Distribution of Galactic Globular Clusters: Distance Uncertainties and Dynamical Effects Dissertação elaborada sob orientação do Prof. Dr. Eduardo Luis Damiani Bica, co- orientação do Prof. Dr. Charles José Bon- ato e apresentada ao Instituto de Física da Universidade Federal do Rio Grande do Sul em preenchimento do requisito par- cial para obtenção do título de Mestre em Física. Porto Alegre 2017 Acknowledgements To my parents, who supported me and made this possible, in a time and place where being in a university was just a distant dream. To my dearest friends Elisabeth, Robert, Augusto, and Natália - who so many times helped me go from "I give up" to "I’ll try once more". To my cats Kira, Fen, and Demi - who lazily join me in bed at the end of the day, and make everything worthwhile. "But, first of all, it will be necessary to explain what is our idea of a cluster of stars, and by what means we have obtained it. For an instance, I shall take the phenomenon which presents itself in many clusters: It is that of a number of lucid spots, of equal lustre, scattered over a circular space, in such a manner as to appear gradually more compressed towards the middle; and which compression, in the clusters to which I allude, is generally carried so far, as, by imperceptible degrees, to end in a luminous center, of a resolvable blaze of light." William Herschel, 1789 Abstract We provide a sample of 170 Galactic Globular Clusters (GCs) and analyse its spatial distribution properties. -
Space in Central and Eastern Europe
EU 4+ SPACE IN CENTRAL AND EASTERN EUROPE OPPORTUNITIES AND CHALLENGES FOR THE EUROPEAN SPACE ENDEAVOUR Report 5, September 2007 Charlotte Mathieu, ESPI European Space Policy Institute Report 5, September 2007 1 Short Title: ESPI Report 5, September 2007 Editor, Publisher: ESPI European Space Policy Institute A-1030 Vienna, Schwarzenbergplatz 6 Austria http://www.espi.or.at Tel.: +43 1 718 11 18 - 0 Fax - 99 Copyright: ESPI, September 2007 This report was funded, in part, through a contract with the EUROPEAN SPACE AGENCY (ESA). Rights reserved - No part of this report may be reproduced or transmitted in any form or for any purpose without permission from ESPI. Citations and extracts to be published by other means are subject to mentioning “source: ESPI Report 5, September 2007. All rights reserved” and sample transmission to ESPI before publishing. Price: 11,00 EUR Printed by ESA/ESTEC Compilation, Layout and Design: M. A. Jakob/ESPI and Panthera.cc Report 5, September 2007 2 EU 4+ Executive Summary ....................................................................................... 5 Introduction…………………………………………………………………………………………7 Part I - The New EU Member States Introduction................................................................................................... 9 1. What is really at stake for Europe? ....................................................... 10 1.1. The European space community could benefit from a further cooperation with the ECS ................................................................. 10 1.2. However, their economic weight remains small in the European landscape and they still suffer from organisatorial and funding issues .... 11 1.2.1. Economic weight of the ECS in Europe ........................................... 11 1.2.2. Reality of their impact on competition ............................................ 11 1.2.3. Foreign policy issues ................................................................... 12 1.2.4. Internal challenges ..................................................................... 12 1.3. -
And Ecclesiastical Cosmology
GSJ: VOLUME 6, ISSUE 3, MARCH 2018 101 GSJ: Volume 6, Issue 3, March 2018, Online: ISSN 2320-9186 www.globalscientificjournal.com DEMOLITION HUBBLE'S LAW, BIG BANG THE BASIS OF "MODERN" AND ECCLESIASTICAL COSMOLOGY Author: Weitter Duckss (Slavko Sedic) Zadar Croatia Pусскй Croatian „If two objects are represented by ball bearings and space-time by the stretching of a rubber sheet, the Doppler effect is caused by the rolling of ball bearings over the rubber sheet in order to achieve a particular motion. A cosmological red shift occurs when ball bearings get stuck on the sheet, which is stretched.“ Wikipedia OK, let's check that on our local group of galaxies (the table from my article „Where did the blue spectral shift inside the universe come from?“) galaxies, local groups Redshift km/s Blueshift km/s Sextans B (4.44 ± 0.23 Mly) 300 ± 0 Sextans A 324 ± 2 NGC 3109 403 ± 1 Tucana Dwarf 130 ± ? Leo I 285 ± 2 NGC 6822 -57 ± 2 Andromeda Galaxy -301 ± 1 Leo II (about 690,000 ly) 79 ± 1 Phoenix Dwarf 60 ± 30 SagDIG -79 ± 1 Aquarius Dwarf -141 ± 2 Wolf–Lundmark–Melotte -122 ± 2 Pisces Dwarf -287 ± 0 Antlia Dwarf 362 ± 0 Leo A 0.000067 (z) Pegasus Dwarf Spheroidal -354 ± 3 IC 10 -348 ± 1 NGC 185 -202 ± 3 Canes Venatici I ~ 31 GSJ© 2018 www.globalscientificjournal.com GSJ: VOLUME 6, ISSUE 3, MARCH 2018 102 Andromeda III -351 ± 9 Andromeda II -188 ± 3 Triangulum Galaxy -179 ± 3 Messier 110 -241 ± 3 NGC 147 (2.53 ± 0.11 Mly) -193 ± 3 Small Magellanic Cloud 0.000527 Large Magellanic Cloud - - M32 -200 ± 6 NGC 205 -241 ± 3 IC 1613 -234 ± 1 Carina Dwarf 230 ± 60 Sextans Dwarf 224 ± 2 Ursa Minor Dwarf (200 ± 30 kly) -247 ± 1 Draco Dwarf -292 ± 21 Cassiopeia Dwarf -307 ± 2 Ursa Major II Dwarf - 116 Leo IV 130 Leo V ( 585 kly) 173 Leo T -60 Bootes II -120 Pegasus Dwarf -183 ± 0 Sculptor Dwarf 110 ± 1 Etc. -
The Messier Catalog
The Messier Catalog Messier 1 Messier 2 Messier 3 Messier 4 Messier 5 Crab Nebula globular cluster globular cluster globular cluster globular cluster Messier 6 Messier 7 Messier 8 Messier 9 Messier 10 open cluster open cluster Lagoon Nebula globular cluster globular cluster Butterfly Cluster Ptolemy's Cluster Messier 11 Messier 12 Messier 13 Messier 14 Messier 15 Wild Duck Cluster globular cluster Hercules glob luster globular cluster globular cluster Messier 16 Messier 17 Messier 18 Messier 19 Messier 20 Eagle Nebula The Omega, Swan, open cluster globular cluster Trifid Nebula or Horseshoe Nebula Messier 21 Messier 22 Messier 23 Messier 24 Messier 25 open cluster globular cluster open cluster Milky Way Patch open cluster Messier 26 Messier 27 Messier 28 Messier 29 Messier 30 open cluster Dumbbell Nebula globular cluster open cluster globular cluster Messier 31 Messier 32 Messier 33 Messier 34 Messier 35 Andromeda dwarf Andromeda Galaxy Triangulum Galaxy open cluster open cluster elliptical galaxy Messier 36 Messier 37 Messier 38 Messier 39 Messier 40 open cluster open cluster open cluster open cluster double star Winecke 4 Messier 41 Messier 42/43 Messier 44 Messier 45 Messier 46 open cluster Orion Nebula Praesepe Pleiades open cluster Beehive Cluster Suburu Messier 47 Messier 48 Messier 49 Messier 50 Messier 51 open cluster open cluster elliptical galaxy open cluster Whirlpool Galaxy Messier 52 Messier 53 Messier 54 Messier 55 Messier 56 open cluster globular cluster globular cluster globular cluster globular cluster Messier 57 Messier -
Iván Almár Is Professor of Astronomy at the Konkoly Observatory of the Hungarian Academy of Sciences
Iván Almár is professor of astronomy at the Konkoly Observatory of the Hungarian Academy of Sciences. He has worked in space research (specifically, upper-atmospheric research and satellite geodesy) for more than 50 years. Prof. Almár has been a Member of the IAA since 1984, and was chairman of its Space and Society Commission from 2003 to 2005. He began presenting and publishing papers on planetary protection in 1989. Charles Cockell is professor of geomicrobiology at the Open University, UK. He obtained his PhD from the University of Oxford and held an NRC Associateship at the NASA Ames Research Centre. His interests are in microbe-mineral interactions and life in extreme environments. He is author of several books, including 'Space on Earth' (Macmillan), which explores the links between environmentalism and space exploration. His publications on ethics have focused on the place of microorganisms in environmental ethics and the protection of the space environment. He is Chair of the Earth and Space Foundation. Catharine A. Conley has served as the NASA Planetary Protection Officer since 2006. Prior to this, Conley's research at NASA Ames Research Center focused on the biochemistry and evolution of muscle tissue. Conley has been involved in several spaceflight experiments using the nematode worm, Caenorhabditis elegans, the first of which was flown on the last mission of the Space Shuttle Columbia. Flight hardware was recovered after the tragic accident, and when opened it was found that some spaceflown experimental animals were still alive, a finding of considerable relevance to Planetary Protection. Gernot Groemer has a background in astronomy and astrobiology. -
Stellar Flares with ARIEL
Stellar flares with ARIEL Krisztián Vida & Bálint Seli Konkoly Observatory, Budapest, Hungary Stellar activity as noise ● Photospheric starspots have small contribution to light variations in the IR regime ● Flares are also more prominent at shorter wavelengths Flare of an M-dwarf in multiple passbands ● A possible problem: with transit spectroscopy the removed spectral source is the whole stellar disk, but different activity contribution can cause contamination even in IR regime Rackham, Apai, Giampapa 2018 ● A possible problem: with transit spectroscopy the removed spectral source is the whole stellar disk, but different activity contribution can cause contamination even in IR regime ● This can reach a level of 10+% depending on wavelength and spot confguration Rackham, Apai, Giampapa 2018 ARIEL & stellar activity ● Magnetic activity is an important property of young, fast-rotating stars ● This can have serious consequences on their exoplanets What remains to study for later stages of star/planetary system evolution? Rotation (age) vs. X-ray luminosity ARIEL & stellar activity ● Magnetic activity is an important property of young, fast-rotating stars ● This can have serious consequences on their exoplanets ● Some models already exist discussing the effects of activity on planets, but not much is known on the additive effects and observational confrmation is also missing Model of the atmospheric changes of an Earth-like planet due to a large fare event (Segura et al. 2010) ARIEL & stellar activity ● The interaction of exoplanets and stellar magnetism is crucial for planetary evolution and for the search for life ● Can the system harbor life on long term? (frst signs of life on Eearth dates back to 4Gyr, although complex life based on eukaryotic cells took much longer time to form) ARIEL & stellar activity High resolution photometry can be crucial for fast transients – e.g. -
Astronomy Astrophysics
A&A 641, A76 (2020) https://doi.org/10.1051/0004-6361/202037625 Astronomy & © Ö. H. Detre et al. 2020 Astrophysics Herschel-PACS photometry of the five major moons of Uranus? Ö. H. Detre1, T. G. Müller2, U. Klaas1, G. Marton3,4, H. Linz1, and Z. Balog1,5 1 Max-Planck-Institut für Astronomie (MPIA), Königstuhl 17, 69117 Heidelberg, Germany e-mail: [email protected] 2 Max-Planck-Institut für extraterrestrische Physik (MPE), PO Box 1312, Giessenbachstraße, 85741 Garching, Germany 3 Konkoly Observatory, Research Centre for Astronomy and Earth Sciences, Konkoly Thege-Miklós 15-17, 1121 Budapest, Hungary 4 ELTE Eötvös Loránd University, Institute of Physics, Pázmány Péter 1/A, 1171 Budapest, Hungary 5 Astronomisches Recheninstitut des Zentrums für Astronomie, Mönchhofstrasse 12–14, 69120 Heidelberg, Germany Received 30 January 2020 / Accepted 9 June 2020 ABSTRACT Aims. We aim to determine far-infrared fluxes at 70, 100, and 160 µm for the five major Uranus satellites, Titania, Oberon, Umbriel, Ariel, and Miranda. Our study is based on the available calibration observations at wavelengths taken with the PACS photometer aboard the Herschel Space Observatory. Methods. The bright image of Uranus was subtracted using a scaled Uranus point spread function (PSF) reference established from all maps of each wavelength in an iterative process removing the superimposed moons. The photometry of the satellites was performed using PSF photometry. Thermophysical models of the icy moons were fitted to the photometry of each measurement epoch and auxiliary data at shorter wavelengths. Results. The best-fit thermophysical models provide constraints for important properties of the moons, such as surface roughness and thermal inertia. -
Contributed Paper KONKOLY WIDE-FIELD PLATE ARCHIVE 1
CORE Metadata, citation and similar papers at core.ac.uk Provided by Repository of the Academy's Library Proc. IV Serbian-Bulgarian Astronomical Conference, Belgrade 21{24 April 2004, eds. M. S. Dimitrijevi´c, V. Golev, L. C.ˇ Popovi´c, M. Tsvetkov, Publ. Astron. Soc. "Rudjer Boˇskovi´c" No 5, 2005, 295 - 301 Contributed paper KONKOLY WIDE-FIELD PLATE ARCHIVE 1 2 2 2 2 M. TSVETKOV , L. G. BALAZS´ , A. FRONTO´ , J. KELEMEN , A. HOLL , 1 1 1 3 K. Y. STAVREV , K. TSVETKOVA , A. BORISOVA , D. KALAGLARSKY and 3 R. BOGDANOVSKI 1Institute of Astronomy, Bulgarian Academy of Sciences, 72 Tsarigradsko Shosse blvd., 1784 Sofia, Bulgaria E{mail [email protected] 2Konkoly Observatory, Hungarian Academy of Sciences, Konkoly Thege M. ut 15-17, 1121 Budapest, Hungary E{mail [email protected] 3Space Research Institute, Bulgarian Academy of Sciences, 6 Moskovska str., 1000 Sofia, Bulgaria E{mail [email protected] Abstract. The wide-field photographic observations in Konkoly Observatory were per- formed in the period 1962 { 1997 with the 60/90/180 cm Schmidt telescope in Piszk´estet}o Mountain Station. The archive of the telescope contains more than 13 000 observations de- scribed in the Konkoly plate catalogue. After the preparation of an enlarged version of the catalogue it has been incorporated in the Wide-Field Plate Database installed in the Sofia Sky Archive Data Center with a possible on-line search at http://www.skyarchive.org/search/. Results from the analysis of the catalogue data characterizing the observational activity at Konkoly in the period 1962 { 1997 are presented. -
THE CARE of OBSOLETE INSTRUMENTS Magda Vargha
161 THE CARE OF OBSOLETE INSTRUMENTS Magda Vargha Konkoly Observatory Budapest Hungary is a little country with old traditions. Hungarian celebrate the 950th anniversary of the death of the first king Stephan I this year. As regards astronomy, during the Renaissance in the court of the Hungarian king Matthias I there was a modest flowering in astronomy and this continued until 1526, when because of the Turkish occupation, the region was cut off and remained so for centuries. I do not want to list all the tragic historical events. Rather I would like to emphasize what we know by own experiences: what it means to reconstruct destroyed buildings and to try to collect valuable old items that are thrown away by guilty negligence. Returning to the recent time, according to my experiences that also in peaceful circumstances valuable old things such as books and scientific instruments are in permanent danger. This is true especially when they are not "up to date"but not old enough for antiquarians. Furthermore, the obsolete instruments meet a worse fate. During my working period in the Konkoly Observatory many instruments considered obsolete have been eliminated while the old books have quiet places on our shelves in the library. With respect to survival, there are many differences between instru ments and books. This is the most important difference among them: while an instrument is made in one or in very few copies, the books are printed in hundreds. One source of trouble is that it is very easy for someone to modify or disassemble an instrument to the point where it is unrecognizable. -
EPSC2014-584, 2014 European Planetary Science Congress 2014 Eeuropeapn Planetarsy Science Ccongress C Author(S) 2014
EPSC Abstracts Vol. 9, EPSC2014-584, 2014 European Planetary Science Congress 2014 EEuropeaPn PlanetarSy Science CCongress c Author(s) 2014 Detection limit for the size of exomoons around Kepler planetary candidates and in simulated CHEOPS data A. E. Simon (1,2), Gy. M. Szabó (2,3) and L. L. Kiss (2) (1) Center for Space and Habitability, University of Berne, CH-3012 Bern, Switzerland (2) Konkoly Observatory, Research Centre for Astronomy and Earth Sciences, Hungarian Academy of Sciences, H-1121 Budapest, Hungary (3) Gothard Astrophysical Observatory and Multidisciplinary Research Center of Loránd Eötvös University, H-9700 Szombathely, Hungary Abstract 2. (Un)detectable moon around Ke- The increasing number of detected exoplanets has in- pler candidates? spired a significant interest in the community as to We calculated photometric transit timing variations whether these planets can host a detectable and hab- (PTV : see TTVp in [5]) from simulated observations itable moon [4]. Here we show which are the most with increasing moon size for all Kepler candidates2 to promising Kepler planetary candidates that are capa- determine the minimum radius of a theoretical moon ble to host a detectable moon and what is the best way that can be detected in the Kepler data. to increase our chance of discovering exomoons via the forthcoming CHEOP S space telescope. 1. Introduction Despite the efforts during the past 8 years that aimed on a discovery of an exomoon in the Kepler data [9, 5, 6, 7, 2], there has no firm evidence for an exomoon found as of today [8, 3]. From the analysis of the data provided by the Kepler spacecraft shows an apparent contradiction between the number of examined KOI systems by date and the lack of any firm detection. -
3D Shape of Asteroid (6) Hebe from VLT/SPHERE Imaging: Implications for the Origin of Ordinary H Chondrites M
3D shape of asteroid (6) Hebe from VLT/SPHERE imaging: Implications for the origin of ordinary H chondrites M. Marsset, B. Carry, C. Dumas, J. Hanus, M. Viikinkoski, P. Vernazza, Müller T.G., M. Delbo, E. Jehin, M. Gillon, et al. To cite this version: M. Marsset, B. Carry, C. Dumas, J. Hanus, M. Viikinkoski, et al.. 3D shape of asteroid (6) Hebe from VLT/SPHERE imaging: Implications for the origin of ordinary H chondrites. Astronomy and Astrophysics - A&A, EDP Sciences, 2017, 604, page 1-12. 10.1051/0004-6361/201731021. hal- 01707187 HAL Id: hal-01707187 https://hal.archives-ouvertes.fr/hal-01707187 Submitted on 12 Feb 2018 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. A&A 604, A64 (2017) Astronomy DOI: 10.1051/0004-6361/201731021 & c ESO 2017 Astrophysics 3D shape of asteroid (6) Hebe from VLT/SPHERE imaging: Implications for the origin of ordinary H chondrites? M. Marsset1, B. Carry2; 3, C. Dumas4, J. Hanuš5, M. Viikinkoski6, P. Vernazza7, T. G. Müller8, M. Delbo2, E. Jehin9, M. Gillon9, J. Grice2; 10, B. Yang11, T. Fusco7; 12, J. Berthier3, S.