DOCSLIB.ORG

Sky in Google Earth

Total Page：16

File Type：pdf, Size：1020Kb

Download full-text PDF Read full-text
Sky in Google Earth VOL 24 ISSUE 03 Space Telescope Science Institute Interacting Galaxy Pair Image Credit: NASA, ESA, and the Hubble Heritage Team (STScI/AURA) http://Hubblesite.org/newscenter/archive/releases/2007/36/ SKY IN GOO G LE EARTH C. Christian, [email protected], and A. Conti, [email protected] fter spending hours roaming our home planet via GOO G LE EARTH , it a “basemap.” SKY also contains stick figures of constellations, labeling just seemed natural to wonder if we might ramble through the SKY of selected objects from astronomical catalogues, Hubble press-release in the same manner. Although we arrived by different paths, we images with explanations, and other features, such as tours. A found we shared that same vision. By late 2005, we were collaborating in Each tour is a sequence of locations linked by some theme that you have an experiment to use the technology of GOO G LE EARTH as an interface to the downloaded into your Places in GOO G LE EARTH /SKY. For example, a tour of universe of astronomical data and information. some interesting Hubble images can be downloaded from the gSKY website. We had an opportunity to give a “Tech Talk” at the Googleplex in Mountain Detailed instructions about all aspects of using GOO G LE EARTH and SKY are View, California, where we introduced googlers to the treasure trove of found at the GOO G LE EARTH website: http://earth.google.com/userguide/. 2007 Hubble data and the standards and protocols of astronomical archives. The Hubble press-release images were embedded in SKY only after going Members of the GOO G LE EARTH team were intrigued by the possibilities and through a painstaking process of checking and adjusting their alignments enthusiastic about our modest experimentation with their technology. on the basemap. To make this process even more complicated, the In August 2007, our dream became a reality with the release of SKY IN basemap is constructed from a projection involving the Earth’s geometry GOO G LE EARTH , a feature incorporated in GOO G LE EARTH version 4.2, which and coordinate system. The explanations are from the original press allows the user to begin roaming the sky with a click of a button (http:// releases by the Office of Public Outreach; each is linked to the object’s earth.google.com). pages at the Astronomical Data System, SIMBAD , and The data in the Digitized Sky Survey and the Sloan Digital Sky Survey the NASA/IPAC EXTRA G ALACTIC ATABA S E D . All the press- Continued FALL forms the foundation of SKY. Colleagues at the University of Pittsburgh release images are tagged to conform to the Virtual page 3 and the Google Pittsburgh facility processed and merged this data into Astronomy Multimedia Project recommendations DIRECTOR’S PERSPECTIVE Possible Multi-Cycle Treasury Program M. Mountain, [email protected] f everything goes according to plan, next August the Kennedy Space Center will host a spectacular sight: two space shuttles, poised on adjacent launch pads, ready to go into space. Atlantis will be heading to the Hubble Space Telescope for the last servicing mission; Endeavor will be prepared, if necessary, to rescue the crew of the Atlantis. This dramatic display of strategic assets Iwill testify to NASA’s commitment to space science. The primary goal of Servicing Mission 4 (SM4) is to maximize the Great Observatory Origins Deep Survey and the Cosmic Evolution Survey. scientific return from Hubble over the following five years. There is little question that complementary and supplementary programs Here at the Space Telescope Science Institute, we have the responsibility using WFC3 will be proposed in Cycle 17. to ensure that the science flowing from the newly refurbished Hubble fully In another example, the panchromatic capabilities of WFC3 and ACS justifies the incredible investment the nation, NASA, and the astronaut offer the potential of mapping the star-formation properties in nearby corps are making in this last servicing mission. Thus, we are inviting input galaxies (such as M33), perhaps coupled with metallicity and kinematic from the community about a possible new class of very large observing analyses using observations by COS and STIS. programs following SM4. As yet another—STIS, COS, and perhaps even the FGS might feature After SM4, Hubble will have new gyros, batteries, and more powerful strongly in concerted investigations of the characteristics of transiting instrumentation than ever before in its history. The Wide Field Camera 3 (and non-transiting) extrasolar planets. (WFC3) and Cosmic Origins Spectrograph (COS) will be installed. If all These are just some areas that might profit from very large allocations goes well, we will also have a new Fine Guidance Sensor (FGS) and a of Hubble time. In order to assess the appetite of the community for such repaired Space Telescope Imaging Spectrograph (STIS). NASA is even programs, we are soliciting white papers that describe projects in this exploring how to repair the Advanced Camera for Surveys (ACS), which category. This solicitation in no way pre-selects or restricts the science topics. was Hubble’s imaging workhorse until it died in late January 2007. Not You may submit ideas for any combination of imaging and spectroscopy. until Webb flies in 2013 will the community have access to so powerful a If you are opposed to the establishment of this type of program, you space observatory as the refurbished Hubble will be after SM4. may also submit a white paper outlining your concerns. For example, you So how should we allocate time after this last visit to Hubble? What could describe the science that you envision being adversely impacted, or programs should we contemplate? Are our current modes of operation advocate a greater overall allocation to small and medium programs. sufficient, or are there science questions that demand greater resources? If, and only if, we find really compelling ideas for a new Multi-Cycle As one example, Hubble has devoted extensive resources to probing Treasury (MCT) program, we anticipate allocating 2,000 orbits— the high-redshift universe through deep-imaging surveys on a variety of distributed over the last few months of Cycle 17 (150 to 200 orbits) and scales, from the Hubble Deep Field and the Ultra Deep Field through the through Cycles 18 and 19—to this category. Up to 600 orbits would be 2 DIRECTOR’S PERSPECTIVE subsidized from director’s discretionary time. The remaining orbits (up to 1200) would be taken from the General Observer allocations in Cycles 18 and 19, drawn predominantly from the time currently set aside for large and Treasury programs. MCT programs should, therefore, have relatively little impact on the number of small and medium programs allocated in those cycles, and there will still be an opportunity to apply for standard large and Treasury programs. By this time next year, if all goes well, we will be entering a new era of space science capabilities with the post-SM4 Hubble. We are looking to the science community to make this a new era of discovery. W Figure 1: Astronauts training to fix The Space Telescope Imaging Spectrograph (STIS) in the Neutral Buoyancy Laboratory (NBL). SKY IN GOO G LE EARTH from page 1 and vetted by the International Virtual Observatory Alliance (http://www.communicatingastronomy. org/repository). Within minutes of the SKY release, a new community blossomed with comments, speculations, and additions. This delighted us, because SKY is intended to be an organic, growing technology for professionals, amateurs, and novices to use—where they all can contribute and collaborate. Many professional astronomers have jumped at the opportunity to share data, including stars with exoplanets from Geoff Marcy, overlays of the constellations from the Naval Observatory and the Institute, and the sky as seen by the Infrared Astronomical Satellite contributed by the University of Washington. We are continuing to work on new features for SKY Figure 1: SKY IN GOO G LE EARTH showing constellation stick figures, locations related to Hubble data, such as catalogs, links to the of Hubble images (the blue symbols) and the main features of the viewport, Hubble Legacy Archive, the Multimission Archive at including the navigation control in the upper right. The left menus are the search Space Telescope, and the National Virtual Observatory. feature, the folders of resources the user has downloaded (middle section) and We have already released a layer of Galaxy Evolution the resources that are downloaded automatically with SKY (lower left section). Explorer images, a tour of the most popular Hubble images as described above, and a file that shows the location of Hubble and its orbit that can be downloaded from the gSky webpage http://Hubblesite. org/explore_astronomy/gSKY/. Orbits and positions for other satellites will be available on that site and viewable in both GOO G LE EARTH and SKY. Continued The purpose of the gSky page is to make it easier for anyone—public page 4 users, educators, students, amateurs, and professional astronomers—to 3 Figure 3: The tour of great HST images. Figure 2: A portion of SKY showing part of the constellation Orion, including Download from the gSKY website: http:// the constellation stick figure, the classic constellation drawing contributed Hubblesite.org/explore_astronomy/gSKY /, by a SKY user, and the location of the Hubble mosiac entitled “Fire and Fury open in the SKY mode of GOO G LE EARTH . Click on of Stellar Birth.” Clicking on the blue HubbleSite symbol allows the user “STScI’s Best of Hubble” under Places, and then hit to zoom in to see the high-resolution Hubble Orion image. the play button. Figure 5: Hubble Space Telescope position, its orbit and an information “balloon” regarding the satellite.
Load more

Recommended publications
  • 7 Planetary Rings Matthew S
    7 Planetary Rings Matthew S. Tiscareno Center for Radiophysics and Space Research, Cornell University, Ithaca, NY, USA 1Introduction..................................................... 311 1.1 Orbital Elements ..................................................... 312 1.2 Roche Limits, Roche Lobes, and Roche Critical Densities .................... 313 1.3 Optical Depth ....................................................... 316 2 Rings by Planetary System .......................................... 317 2.1 The Rings of Jupiter ................................................... 317 2.2 The Rings of Saturn ................................................... 319 2.3 The Rings of Uranus .................................................. 320 2.4 The Rings of Neptune ................................................. 323 2.5 Unconfirmed Ring Systems ............................................. 324 2.5.1 Mars ............................................................... 324 2.5.2 Pluto ............................................................... 325 2.5.3 Rhea and Other Moons ................................................ 325 2.5.4 Exoplanets ........................................................... 327 3RingsbyType.................................................... 328 3.1 Dense Broad Disks ................................................... 328 3.1.1 Spiral Waves ......................................................... 329 3.1.2 Gap Edges and Moonlet Wakes .......................................... 333 3.1.3 Radial Structure .....................................................
    [Show full text]
  • Planetary Ring Systems Edited by Matthew S
    Cambridge University Press 978-1-107-11382-4 — Planetary Ring Systems Edited by Matthew S. Tiscareno , Carl D. Murray Frontmatter More Information Planetary Ring Systems Properties, Structure, and Evolution Planetary rings are among the most intriguing structures of our solar system and have fas- cinated generations of astronomers. Collating emerging knowledge in the field, this volume reviews our current understanding of ring systems with reference to the rings of Saturn, Uranus, Neptune, and more. Written by leading experts, the history of ring research and the basics of ring-particle orbits is followed by a review of the known planetary ring sys- tems. All aspects of ring system science are described in detail, including specific dynamical processes, types of structures, thermal properties, their origins, and investigations using com- puter simulations and laboratory experiments. The concluding chapters discuss the prospects of future missions to planetary rings, the ways in which ring science informs and is informed by the study of other astrophysical disks, and a perspective on the field’s future. Researchers of all levels benefit from this thorough and engaging presentation. MATTHEW S. TISCARENO is a Senior Research Scientist at the SETI Institute, California. He is a Participating Scientist and an Imaging Team Associate with the Cassini- Huygens mission. His research output includes solar system dynamics and space-based observations of the outer solar system. CARL D. MURRAYis Professor of Mathematics and Astronomy at Queen Mary Univer- sity of London. He has contributed to numerous ring and moon discoveries as an original member of the Imaging Team with the Cassini-Huygens mission and he is co-author of the textbook Solar System Dynamics (1999).
    [Show full text]
  • The Sky Tonight
    MARCH POUTŪ-TE-RANGI HIGHLIGHTS Conjunction of Saturn and the Moon A conjunction is when two astronomical objects appear close in the sky as seen THE- SKY TONIGHT- - from Earth. The planets, along with the TE AHUA O TE RAKI I TENEI PO Sun and the Moon, appear to travel across Brightest Stars our sky roughly following a path called the At this time of the year, we can see the ecliptic. Each body travels at its own speed, three brightest stars in the night sky. sometimes entering ‘retrograde’ where they The brightness of a star, as seen from seem to move backwards for a period of time Earth, is measured as its apparent (though the backwards motion is only from magnitude. Pictured on the cover is our vantage point, and in fact the planets Sirius, the brightest star in our night sky, are still orbiting the Sun normally). which is 8.6 light-years away. Sometimes these celestial bodies will cross With an apparent magnitude of −1.46, paths along the ecliptic line and occupy the this star can be found in the constellation same space in our sky, though they are still Canis Major, high in the northern sky. millions of kilometres away from each other. Sirius is actually a binary star system, consisting of Sirius A which is twice the On March 19, the Moon and Saturn will be size of the Sun, and a faint white dwarf in conjunction. While the unaided eye will companion named Sirius B. only see Saturn as a bright star-like object (Saturn is the eighth brightest object in our Sirius is almost twice as bright as the night sky), a telescope can offer a spectacular second brightest star in the night sky, view of the ringed planet close to our Moon.
    [Show full text]
  • Educator's Guide: Orion
    Legends of the Night Sky Orion Educator’s Guide Grades K - 8 Written By: Dr. Phil Wymer, Ph.D. & Art Klinger Legends of the Night Sky: Orion Educator’s Guide Table of Contents Introduction………………………………………………………………....3 Constellations; General Overview……………………………………..4 Orion…………………………………………………………………………..22 Scorpius……………………………………………………………………….36 Canis Major…………………………………………………………………..45 Canis Minor…………………………………………………………………..52 Lesson Plans………………………………………………………………….56 Coloring Book…………………………………………………………………….….57 Hand Angles……………………………………………………………………….…64 Constellation Research..…………………………………………………….……71 When and Where to View Orion…………………………………….……..…77 Angles For Locating Orion..…………………………………………...……….78 Overhead Projector Punch Out of Orion……………………………………82 Where on Earth is: Thrace, Lemnos, and Crete?.............................83 Appendix………………………………………………………………………86 Copyright©2003, Audio Visual Imagineering, Inc. 2 Legends of the Night Sky: Orion Educator’s Guide Introduction It is our belief that “Legends of the Night sky: Orion” is the best multi-grade (K – 8), multi-disciplinary education package on the market today. It consists of a humorous 24-minute show and educator’s package. The Orion Educator’s Guide is designed for Planetarians, Teachers, and parents. The information is researched, organized, and laid out so that the educator need not spend hours coming up with lesson plans or labs. This has already been accomplished by certified educators. The guide is written to alleviate the fear of space and the night sky (that many elementary and middle school teachers have) when it comes to that section of the science lesson plan. It is an excellent tool that allows the parents to be a part of the learning experience. The guide is devised in such a way that there are plenty of visuals to assist the educator and student in finding the Winter constellations.
    [Show full text]
  • Stories in the Sky
    8 Stories in the Sky In modern times, astronomers count 88 constellations, but many of these constellations go back to ancient times. ere were many groups of people from long ago who told mythological stories about these shapes in the sky. Recommended Reading Once Upon a Starry Night, by Jacqueline Mitton and Christina Balit A Walk rough the Heavens: A Guide to Stars and Constellations and their Legends (4th edition), by Milton D. Heifetz and Will Tirion, p.57- 58, stories of Bootes and Canis Major (not for students in the southern hemisphere) A Walk rough the Southern Sky: A Guide to Stars and Constellations and their Legends (2nd edition), by Milton D. Heifetz and Will Tirion, p.79- 82, stories of Carina and Centarus (not for students in the northern hemisphere) ACTIVITY Build a Planisphere Follow the instructions on the following page to learn to make and use a planisphere: experienceastronomy.com/planisphere LESSON 8 Lesson 8: Job 38:31-32 Can |you |bind |the |chains |of |the P|leiades |or |loose |the |cords |of O|rion? Can |you |lead |forth |the Mazzaroth |in |their |season, |or |can |you |guide |the B|ear |with |its |children? Lesson 8: Job 38:31-32 Can you bind the chains of the Pleiades or loose the cords of Orion? Can you lead forth the Mazzaroth in their season, or can you guide the Bear with its children? Lesson 8: Job 38:31-32 Question: How many constellations are there in the whole sky? Answer: 88 LESSON 8 Stories in the Sky Lesson 8 Quiz 1.
    [Show full text]
  • Giant Planets in the OGLE Fields Francois Fressin, Tristan Guillot, Vincent Morello, Frédéric Pont
    Interpreting and predicting the yield of transit surveys: Giant planets in the OGLE fields Francois Fressin, Tristan Guillot, Vincent Morello, Frédéric Pont To cite this version: Francois Fressin, Tristan Guillot, Vincent Morello, Frédéric Pont. Interpreting and predicting the yield of transit surveys: Giant planets in the OGLE fields. Astronomy and Astrophysics - A&A, EDP Sciences, 2007, pp.A&A. hal-00140833v2 HAL Id: hal-00140833 https://hal.archives-ouvertes.fr/hal-00140833v2 Submitted on 13 Apr 2007 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. Astronomy & Astrophysics manuscript no. corotlux˙v3.08.hyper16679 April 15, 2007 (DOI: will be inserted by hand later) Interpreting and predicting the yield of transit surveys: Giant planets in the OGLE fields F. Fressin1, T. Guillot2, V.Morello2 and F. Pont3 1 Observatoire de la Cˆote d’Azur, Laboratoire Gemini, CNRS UMR 6203, B.P. 4229, 06304 Nice Cedex 4, France e-mail: [email protected] 2 Observatoire de la Cˆote d’Azur, Laboratoire Cassiop´ee, CNRS UMR 6202, B.P. 4229, 06304 Nice Cedex 4, France 3 Geneva University Observatory, Switzerland A&A, in press. Received: January 18, 2007, Accepted: April 8, 2007.
    [Show full text]
  • A Basic Requirement for Studying the Heavens Is Determining Where In
    Abasic requirement for studying the heavens is determining where in the sky things are. To specify sky positions, astronomers have developed several coordinate systems. Each uses a coordinate grid projected on to the celestial sphere, in analogy to the geographic coordinate system used on the surface of the Earth. The coordinate systems differ only in their choice of the fundamental plane, which divides the sky into two equal hemispheres along a great circle (the fundamental plane of the geographic system is the Earth's equator) . Each coordinate system is named for its choice of fundamental plane. The equatorial coordinate system is probably the most widely used celestial coordinate system. It is also the one most closely related to the geographic coordinate system, because they use the same fun­ damental plane and the same poles. The projection of the Earth's equator onto the celestial sphere is called the celestial equator. Similarly, projecting the geographic poles on to the celest ial sphere defines the north and south celestial poles. However, there is an important difference between the equatorial and geographic coordinate systems: the geographic system is fixed to the Earth; it rotates as the Earth does . The equatorial system is fixed to the stars, so it appears to rotate across the sky with the stars, but of course it's really the Earth rotating under the fixed sky. The latitudinal (latitude-like) angle of the equatorial system is called declination (Dec for short) . It measures the angle of an object above or below the celestial equator. The longitud inal angle is called the right ascension (RA for short).
    [Show full text]
  • Astronomy 2008 Index
    Astronomy Magazine Article Title Index 10 rising stars of astronomy, 8:60–8:63 1.5 million galaxies revealed, 3:41–3:43 185 million years before the dinosaurs’ demise, did an asteroid nearly end life on Earth?, 4:34–4:39 A Aligned aurorae, 8:27 All about the Veil Nebula, 6:56–6:61 Amateur astronomy’s greatest generation, 8:68–8:71 Amateurs see fireballs from U.S. satellite kill, 7:24 Another Earth, 6:13 Another super-Earth discovered, 9:21 Antares gang, The, 7:18 Antimatter traced, 5:23 Are big-planet systems uncommon?, 10:23 Are super-sized Earths the new frontier?, 11:26–11:31 Are these space rocks from Mercury?, 11:32–11:37 Are we done yet?, 4:14 Are we looking for life in the right places?, 7:28–7:33 Ask the aliens, 3:12 Asteroid sleuths find the dino killer, 1:20 Astro-humiliation, 10:14 Astroimaging over ancient Greece, 12:64–12:69 Astronaut rescue rocket revs up, 11:22 Astronomers spy a giant particle accelerator in the sky, 5:21 Astronomers unearth a star’s death secrets, 10:18 Astronomers witness alien star flip-out, 6:27 Astronomy magazine’s first 35 years, 8:supplement Astronomy’s guide to Go-to telescopes, 10:supplement Auroral storm trigger confirmed, 11:18 B Backstage at Astronomy, 8:76–8:82 Basking in the Sun, 5:16 Biggest planet’s 5 deepest mysteries, The, 1:38–1:43 Binary pulsar test affirms relativity, 10:21 Binocular Telescope snaps first image, 6:21 Black hole sets a record, 2:20 Black holes wind up galaxy arms, 9:19 Brightest starburst galaxy discovered, 12:23 C Calling all space probes, 10:64–10:65 Calling on Cassiopeia, 11:76 Canada to launch new asteroid hunter, 11:19 Canada’s handy robot, 1:24 Cannibal next door, The, 3:38 Capture images of our local star, 4:66–4:67 Cassini confirms Titan lakes, 12:27 Cassini scopes Saturn’s two-toned moon, 1:25 Cassini “tastes” Enceladus’ plumes, 7:26 Cepheus’ fall delights, 10:85 Choose the dome that’s right for you, 5:70–5:71 Clearing the air about seeing vs.
    [Show full text]
  • Publications of the Astronomical Society of the Pacific 108: 8-34, 1996 January
    Publications of the Astronomical Society of the Pacific 108: 8-34, 1996 January Invited Review Paper Astrophysics in 1995 Virginia Trimble Department of Astronomy, University of Maryland, College Park, Maryland 20742-2421 and Department of Physics, University of California, Irvine, California 92717-4575 Peter J. T. Leonard Department of Astronomy, University of Maryland, College Park, Maryland 20742-2421 Received 1995 October 26; accepted 1995 October 27 ABSTRACT. Ap95 differs from Ap91 to Ap94 primarily in Ap number. That is, it once again attempts to highlight some areas of our mutual science where a major event has occurred during the year (a possible solution of the Type II supernova problem, the faintness of quasar host galaxies, the collision of Shoemaker-Levy 9 with Jupiter), but also to focus on some topics where dogged determination is producing more gradual advances (dense star clusters, the second-parameter problem, inventories of nearby objects, and dark-matter candidates). In moderate departure from the rules of Ap92-94, there has been some deliberate up-dating of topics discussed previously. The topics are only partly ordered from nearby to far away. 1. INTRODUCTION Journal. Another, less publicized, change of editors has "For crying out loud," we can hear you saying, "is it modified the journal so much that Vinod Krishan's Bulletin them again!" Well, yes. This is the fifth annual mustering of of the Astronomical Society of India (BASI in the references) the sheep and goats of astronomical/astrophysical research, has been added to the list of journals to be scanned regularly. based on journals that reached library shelves between 1 Oc- Last year, we worried a bit about paying too much atten- tober 1994 and 30 September 1995.
    [Show full text]
  • Calibrating Star Formation Rates on the Galactic Mesoscale
    Calibrating Star Formation Rates on the Galactic Mesoscale Matthew S. Povich Assistant Professor, Department of Physics & Astronomy California State Polytechnic University, Pomona, CA USA Key Collaborators Penn State University of University of Leisa Townsley Wisconsin Arizona Patrick Broos Edward Churchwell John Bieging Konstantin Getman Barbara Whitney Nathan Smith Eric Feigelson Marilyn Meade University of Brian Babler Mike Kuhn Exeter Michigan State Cal Poly Pomona Tim Naylor Laura Chomiuk Alex Rudolph * PhD student Remington Sexton*1 1 Now at UCR Max Planck Institute Nicole Sanchez*2 for Astronomy 2 Now at Fisk U. Alec Vinson*3 Thomas Robitaille 3 Now at UCLA Anoush Kazarians** ** Undergrad Some Definitions • Microscale Star Formation - Local 500 pc volume, ~10 pc scale clouds, (e.g. Heiderman et al. 2010, Lada et al. 2010, 2012, 2013, Gutermuth et al. 2011, Evans et al. 2014). - Few O stars, ONC is most massive cluster. • Macroscale Star Formation — Extragalactic studies, including starbursts (e.g. Kennicutt 1998, Gao & Solomon 2004, Kennicutt et al. 2009) or parts of galaxies at 0.1-1 kpc scales (e.g. Calzetti et al. 2007, Faesi et al. 2014) • Mesoscale Star Formation - Case Study: The Carina Nebula Complex (Povich et al. 2011a,b) - Comparative Studies: Chomiuk & Povich (2011), MYStIX (+ MAGIX?) The Schmidt-Kennicutt “Law” Schmidt (1959): N ∑SFR = A∑gas based on observations of stars and gas in the Solar neighborhood. Kennicutt (1998): N = 1.4±0.15 (slope of line fit to data in plot) for a sample of normal, disk galaxies (filled circles, open circles for galaxy centers) and starburst galaxies (squares). Star formation rate (SFR) surface density Star formation Gas surface density Mesoscale Case Study: The Chandra Carina Complex Project (CCCP) • Use wide-field, high-resolution, multiwavelength datasets to directly observe the young stellar population of the Great Nebula in Carina and measure its star formation rate (SFR).
    [Show full text]
  • Property Map
    PROPERTY MAP [email protected] THELINEHOTEL.COM/DC Housed in a neoclassical church that has been thoughtfully renovated to preserve the building’s architectural features — including 60-foot vaulted ceilings, millwork and brass detailing, and large copper entry doors —the 20th century structure sits alongside a contextual addition connected through the lobby. The LINE DC includes 220 guest rooms, a number of dining and drinking options, a live broadcast radio station and a rooftop with sweeping views encompassing the Washington Monument and the Washington National Cathedral. G F E D C B A A SPA LEVEL D LOBBY LEVEL F MONUMENT VIEW FITNESS CENTER • BROTHERS & SISTERS MASTER SUITE • THE CUP WE ALL RACE 4 B CARINA FULL SERVICE RADIO G ROOFTOP CARINA & CARINA EAST ARGO & PAVO VELA ROOFTOP LYRA & LYNX C STREET LEVEL GUEST ROOMS LOCATED • RESTAURANTS BANNEKER EAST, WEST E MEZZANINE ON FLOORS 1–7 • COFFEE SHOP CENTER, & FOYER • A RAKE’S PROGRESS [email protected] STREET LEVEL O LOAIN EIT WEST W.C. STAIRS ARINA W.C. W.C. ELEVATORS BANNEER FOYER ENTER EIT STAIRS STAIRS EIT TO ARINA ELEVATORS ARAE EAST EAST W.C. STAIRS EIT EIT PORTEORE [email protected] LOBBY LEVEL SPOEN ENLIS EIT STAIRS W.C. BROS STAIRS ARO PAVO SIS P D.R. TE UP ELEVATORS WE ALL RAE UEST ROOMS BROTERS SISTERS EIN FULL SERVIE RAIO STAIRS STAIRS LYRA LYN ELEVATORS W.C. STAIRS [email protected] MEZZANINE A RAES EIT PRORESS STAIRS W.C. ELEVATORS EIT UEST ROOMS A RAE PRORESS PR EIT W.C. EIT STAIRS A RAES EIT PRORESS STAIRS [email protected] MONUMENT VIEW MASTER SUITE BEROOM WC OUTOOR LIVIN TERRAE AREA [email protected] ROOFTOP EIT W.C.
    [Show full text]
  • ESO Annual Report 2004 ESO Annual Report 2004 Presented to the Council by the Director General Dr
    ESO Annual Report 2004 ESO Annual Report 2004 presented to the Council by the Director General Dr. Catherine Cesarsky View of La Silla from the 3.6-m telescope. ESO is the foremost intergovernmental European Science and Technology organi- sation in the field of ground-based as- trophysics. It is supported by eleven coun- tries: Belgium, Denmark, France, Finland, Germany, Italy, the Netherlands, Portugal, Sweden, Switzerland and the United Kingdom. Created in 1962, ESO provides state-of- the-art research facilities to European astronomers and astrophysicists. In pur- suit of this task, ESO’s activities cover a wide spectrum including the design and construction of world-class ground-based observational facilities for the member- state scientists, large telescope projects, design of innovative scientific instruments, developing new and advanced techno- logies, furthering European co-operation and carrying out European educational programmes. ESO operates at three sites in the Ataca- ma desert region of Chile. The first site The VLT is a most unusual telescope, is at La Silla, a mountain 600 km north of based on the latest technology. It is not Santiago de Chile, at 2 400 m altitude. just one, but an array of 4 telescopes, It is equipped with several optical tele- each with a main mirror of 8.2-m diame- scopes with mirror diameters of up to ter. With one such telescope, images 3.6-metres. The 3.5-m New Technology of celestial objects as faint as magnitude Telescope (NTT) was the first in the 30 have been obtained in a one-hour ex- world to have a computer-controlled main posure.
    [Show full text]