The Evolution of Astronomical Observatory Design
Total Page:16
File Type:pdf, Size:1020Kb
Load more
Recommended publications
-
Edwin Powell Hubble Papers: Finding Aid
http://oac.cdlib.org/findaid/ark:/13030/tf7b69n8rd Online items available Edwin Powell Hubble Papers: Finding Aid Processed by Ronald S. Brashear, completed December 12, 1997; machine-readable finding aid created by Xiuzhi Zhou and updated by Diann Benti in June 2017. The Huntington Library, Art Collections, and Botanical Gardens Manuscripts Department 1151 Oxford Road San Marino, California 91108 Phone: (626) 405-2191 Email: [email protected] URL: http://www.huntington.org © 1998 The Huntington Library. All rights reserved. Edwin Powell Hubble Papers: mssHUB 1-1098 1 Finding Aid Overview of the Collection Title: Edwin Powell Hubble Papers Dates (inclusive): 1900-1989 Collection Number: mssHUB 1-1098 Creator: Hubble, Edwin, 1889-1953. Extent: 1300 pieces, plus ephemera in 34 boxes Repository: The Huntington Library, Art Collections, and Botanical Gardens. Manuscripts Department 1151 Oxford Road San Marino, California 91108 Phone: (626) 405-2191 Email: [email protected] URL: http://www.huntington.org Abstract: This collection contains the papers of Edwin P. Hubble (1889-1953), an astronomer at the Mount Wilson Observatory near Pasadena, California. as well as the diaries and biographical memoirs of his wife, Grace Burke Hubble. Language: English. Access Open to qualified researchers by prior application through the Reader Services Department. For more information, contact Reader Services. Publication Rights The Huntington Library does not require that researchers request permission to quote from or publish images of this material, nor does it charge fees for such activities. The responsibility for identifying the copyright holder, if there is one, and obtaining necessary permissions rests with the researcher. Preferred Citation [Identification of item]. -
Telescopes and Binoculars
Continuing Education Course Approved by the American Board of Opticianry Telescopes and Binoculars National Academy of Opticianry 8401 Corporate Drive #605 Landover, MD 20785 800-229-4828 phone 301-577-3880 fax www.nao.org Copyright© 2015 by the National Academy of Opticianry. All rights reserved. No part of this text may be reproduced without permission in writing from the publisher. 2 National Academy of Opticianry PREFACE: This continuing education course was prepared under the auspices of the National Academy of Opticianry and is designed to be convenient, cost effective and practical for the Optician. The skills and knowledge required to practice the profession of Opticianry will continue to change in the future as advances in technology are applied to the eye care specialty. Higher rates of obsolescence will result in an increased tempo of change as well as knowledge to meet these changes. The National Academy of Opticianry recognizes the need to provide a Continuing Education Program for all Opticians. This course has been developed as a part of the overall program to enable Opticians to develop and improve their technical knowledge and skills in their chosen profession. The National Academy of Opticianry INSTRUCTIONS: Read and study the material. After you feel that you understand the material thoroughly take the test following the instructions given at the beginning of the test. Upon completion of the test, mail the answer sheet to the National Academy of Opticianry, 8401 Corporate Drive, Suite 605, Landover, Maryland 20785 or fax it to 301-577-3880. Be sure you complete the evaluation form on the answer sheet. -
Researchers Hunting Exoplanets with Superconducting Arrays
Cryocoolers, a Brief Overview .............................. 8 NASA Preps Four Telescope Missions .............. 37 Lake Shore Celebrates 50 Years ....................... 22 ICCRT Recap ..................................................... 38 Recovering Cold Energy and Waste Heat ............ 32 3-D Printing from Aqueous Materials .................. 40 Exoplanet Hunt with ADR-Cooled Superconducting Detector Arrays | 34 Volume 34 Number 3 Researchers Hunting Exoplanets with Superconducting Arrays The key to revealing the exoplanets tucked away around the universe may just be locked up in the advancement of Microwave Kinetic Inductance Detectors (MKIDs), an array of superconducting de- tectors made from platinum sillicide and housed in a cryostat at 100 mK. An astronomy team led by Dr. Benjamin Mazin at the University of California Santa Barbara is using MKID arrays for research on two telescopes, the Hale telescope at Palomar Observatory near San Diego and the Subaru telescope located at the Maunakea Observatory on Hawaii. Mazin began work on MKIDs nearly two decades ago while working under Dr. Jonas Zmuidzinas at Caltech, who co-pioneered the detectors for cosmic microwave background astronomy with Dr. Henry LeDuc at JPL. A look inside the DARKNESS cryostat. Image: Mazin Mazin has since adapted and ad- vanced the technology for the direct im- aging of exoplanets. With direct imaging, telescopes detect light from the planet itself, recording either the self-luminous thermal infrared light that young—and still hot—planets give off, or reflected light from a star that bounces off a planet and then towards the detector. Researchers have previously relied on indirect methods to search for exo- planets, including the radial velocity technique that looks at the spectrum of a star as it’s pushed and pulled by its planetary companions; and transit pho- tometry, where a dip in the brightness of a star is detected as planets cross in front The astronomy team working with Dr. -
The JWST/Nircam Coronagraph: Mask Design and Fabrication
The JWST/NIRCam coronagraph: mask design and fabrication John E. Krista, Kunjithapatham Balasubramaniana, Charles A. Beichmana, Pierre M. Echternacha, Joseph J. Greena, Kurt M. Liewera, Richard E. Mullera, Eugene Serabyna, Stuart B. Shaklana, John T. Traugera, Daniel W. Wilsona, Scott D. Hornerb, Yalan Maob, Stephen F. Somersteinb, Gopal Vasudevanb, Douglas M. Kellyc, Marcia J. Riekec aJet Propulsion Laboratory/California Institute of Technology, 4800 Oak Grove Drive, Pasasdena, CA, USA 91109; bLockheed Martin Advanced Technology Center, Palo Alto, CA, USA 94303; cUniversity of Arizona, Tucson, AZ, USA 85721 ABSTRACT The NIRCam instrument on the James Webb Space Telescope will provide coronagraphic imaging from λ=1-5 µm of high contrast sources such as extrasolar planets and circumstellar disks. A Lyot coronagraph with a variety of circular and wedge-shaped occulting masks and matching Lyot pupil stops will be implemented. The occulters approximate grayscale transmission profiles using halftone binary patterns comprising wavelength-sized metal dots on anti-reflection coated sapphire substrates. The mask patterns are being created in the Micro Devices Laboratory at the Jet Propulsion Laboratory using electron beam lithography. Samples of these occulters have been successfully evaluated in a coronagraphic testbed. In a separate process, the complex apertures that form the Lyot stops will be deposited onto optical wedges. The NIRCam coronagraph flight components are expected to be completed this year. Keywords: NIRCam, JWST, James Webb Space Telescope, coronagraph 1. INTRODUCTION 1.1 The planet/star contrast problem Observations of extrasolar planet formation (e.g. protoplanetary disks) and planetary systems are hampered by the large contrast differences between these targets and their much brighter stars. -
Sirius - Wikipedia Coordinates: 06 H 4 5 M 08.9 1 7 3 S, −1 6 ° 4 2 ′ 5 8.01 7 ″
12/2/2018 Sirius - Wikipedia Coordinates: 06 h 4 5 m 08.9 1 7 3 s, −1 6 ° 4 2 ′ 5 8.01 7 ″ Sirius Sirius (/ˈsɪriəs/, a romanization of Greek Σείριος, Seirios, lit. "glowing" or "scorching") is a star system Sirius A and B and the brightest star in the Earth's night sky. With a visual apparent magnitude of −1.46, it is almost twice as bright as Canopus, the next brightest star. The system has the Bayer designation Alpha Canis Majoris (α CMa). What the naked eye perceives as a single star is a binary star system, consisting of a white main-sequence star of spectral type A0 or A1, termed Sirius A, and a faint white dwarf companion of spectral type DA2, called Sirius B. The distance separating Sirius A from its companion varies between 8.2 and 31.5 AU.[24] Sirius appears bright because of its intrinsic luminosity and its proximity to Earth. At a distance of 2.6 parsecs (8.6 ly), as determined by the Hipparcos astrometry satellite,[2][25][26] the Sirius system is one of Earth's near neighbours. Sirius is gradually moving closer to the Solar System, so it will slightly increase in brightness over the next 60,000 years. After that time its distance will begin to increase and it will become fainter, but it will continue to be the brightest star in the Earth's night sky for the next 210,000 years.[27] The position of Sirius (circled). Sirius A is about twice as massive as the Sun (M☉) and has an absolute visual magnitude of 1.42. -
Thestargazer
The StarGazer http://www.raclub.org/ Newsletter of the Rappahannock Astronomy Club No. 2 Vol. 7 August 2018–October 2018 Pilgrimage to the Great Refractor By Scott Busby “Time always takes from us those things we hold most dear” The Yerkes Observatory belongs to the Department of Astronomy and Astrophysics of the University of Chicago (UChicago). Established in 1897 on Lake Geneva in Williams Bay, Wisconsin, the observatory, situated on a 78-acre park site, houses all the Department’s activities. Most of the important history of Yerkes Observatory can be found at astro.uchicago.edu. I won’t elaborate too much on its history here; suffice it to say that this great observatory was the result of the hard work and dedication of George Ellery Hale (1868– 1938). Hale had a unique ability to talk wealthy tycoons into funding his astronomical endeavors—pun intended. We can thank him for some of the great telescopes of our time. Some of the more familiar are the 60- and 100-inch Hooker reflecting telescopes on Mount Wilson near Pasadena and his namesake, the Great 200-inch Hale reflecting telescope at Mount Palomar observatory near San Diego. On March 7, 2018, UChicago announced plans to wind down its activities at Yerkes Observatory. As a result, the observatory will close its doors to visitors and researchers on October 1, 2018, with no prospects and no immediate plans to reopen In the last month, my wife Debbie and I decided to take a trip to Williams Bay to visit the Yerkes Observatory and its great 40- The 40-Inch Alvan Clark & Sons Refractor Credit: inch refractor telescope. -
Large Telescopes and Why We Need Them Transcript
Large telescopes and why we need them Transcript Date: Wednesday, 9 May 2012 - 1:00PM Location: Museum of London 9 May 2012 Large Telescopes And Why we Need Them Professor Carolin Crawford Astronomy is a comparatively passive science, in that we can’t engage in laboratory experiments to investigate how the Universe works. To study any cosmic object outside of our Solar System, we can only work with the light it emits that happens to fall on Earth. How much we can interpret and understand about the Universe around us depends on how well we can collect and analyse that light. This talk is about the first part of that problem: how we improve the collection of light. The key problem for astronomers is that all stars, nebulae and galaxies are so very far away that they appear both very small, and very faint - some so much so that they can’t be seen without the help of a telescope. Its role is simply to collect more light than the unaided eye can, making astronomical sources appear both bigger and brighter, or even just to make most of them visible in the first place. A new generation of electronic detectors have made observations with the eye redundant. We now have cameras to record the images directly, or once it has been split into its constituent wavelengths by spectrographs. Even though there are a whole host of ingenious and complex instruments that enable us to record and analyse the light, they are still only able to work with the light they receive in the first place. -
Demonstration of Vortex Coronagraph Concepts for On-Axis Telescopes on the Palomar Stellar Double Coronagraph
Demonstration of vortex coronagraph concepts for on-axis telescopes on the Palomar Stellar Double Coronagraph Dimitri Maweta, Chris Sheltonb, James Wallaceb, Michael Bottomc, Jonas Kuhnb, Bertrand Mennessonb, Rick Burrussb, Randy Bartosb, Laurent Pueyod, Alexis Carlottie, and Eugene Serabynb aEuropean Southern Observatory, Alonso de C´ordova 3107, Vitacura, Casilla 19001, Chile; bJet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91109, USA; cCalifornia Institute of Technology, Pasadena, CA 91106, USA; dSpace Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218, USA; eInstitut de Plan´etologieet d'Astrophysique de Grenoble (IPAG), University Joseph Fourier, CNRS, BP 53, 38041, Grenoble, France; ABSTRACT Here we present preliminary results of the integration of two recently proposed vortex coronagraph (VC) concepts for on-axis telescopes on the Stellar Double Coronagraph (SDC) bench behind PALM-3000, the extreme adaptive optics system of the 200-inch Hale telescope of Palomar observatory. The multi-stage vortex coronagraph (MSVC) uses the ability of the vortex to move light in and out of apertures through multiple VC in series to restore the nominal attenuation capability of the charge 2 vortex regardless of the aperture obscurations. The ring-apodized vortex coronagraph (RAVC) is a one-stage apodizer exploiting the VC Lyot-plane amplitude distribution in order to perfectly null the diffraction from any central obscuration size, and for any vortex topological charge. The RAVC is thus a simple concept that makes the VC immune to diffraction effects of the secondary mirror. It combines a vortex phase mask in the image plane with a single pupil-based amplitude ring apodizer, tailor-made to exploit the unique convolution properties of the VC at the Lyot-stop plane. -
Lick Observatory Records: Photographs UA.036.Ser.07
http://oac.cdlib.org/findaid/ark:/13030/c81z4932 Online items available Lick Observatory Records: Photographs UA.036.Ser.07 Kate Dundon, Alix Norton, Maureen Carey, Christine Turk, Alex Moore University of California, Santa Cruz 2016 1156 High Street Santa Cruz 95064 [email protected] URL: http://guides.library.ucsc.edu/speccoll Lick Observatory Records: UA.036.Ser.07 1 Photographs UA.036.Ser.07 Contributing Institution: University of California, Santa Cruz Title: Lick Observatory Records: Photographs Creator: Lick Observatory Identifier/Call Number: UA.036.Ser.07 Physical Description: 101.62 Linear Feet127 boxes Date (inclusive): circa 1870-2002 Language of Material: English . https://n2t.net/ark:/38305/f19c6wg4 Conditions Governing Access Collection is open for research. Conditions Governing Use Property rights for this collection reside with the University of California. Literary rights, including copyright, are retained by the creators and their heirs. The publication or use of any work protected by copyright beyond that allowed by fair use for research or educational purposes requires written permission from the copyright owner. Responsibility for obtaining permissions, and for any use rests exclusively with the user. Preferred Citation Lick Observatory Records: Photographs. UA36 Ser.7. Special Collections and Archives, University Library, University of California, Santa Cruz. Alternative Format Available Images from this collection are available through UCSC Library Digital Collections. Historical note These photographs were produced or collected by Lick observatory staff and faculty, as well as UCSC Library personnel. Many of the early photographs of the major instruments and Observatory buildings were taken by Henry E. Matthews, who served as secretary to the Lick Trust during the planning and construction of the Observatory. -
Effective Aperture 3.6–4.9 M) 4.7 M 186″ Segmented, MMT (6×1.8 M) F
Effective Effective Mirror type Name Site Built aperture aperture (m) (in) 10.4 m 409″ Segmented, Gran Telescopio Roque de los Muchachos 2006/9 36 Canarias (GTC) Obs., Canary Islands, Spain 10 m 394″ Segmented, Keck 1 Mauna Kea Observatories, 1993 36 Hawaii, USA 10 m 394″ Segmented, Keck 2 Mauna Kea Observatories, 1996 36 Hawaii, USA 9.8 m 386″ Segmented, Southern African South African Astronomical 2005 91 Large Telescope Obs., Northern Cape, South (SALT) Africa 9.2 m 362″ Segmented, Hobby-Eberly McDonald Observatory, 1997 91 Telescope (HET) Texas, USA (11 m × 9.8 m mirror) 8.4 m×2 330″×2 Multiple Large Binocular Mount Graham 2004 (can use mirror, 2 Telescope (LBT) Internationals Obs., Phased- Arizona array optics for combined 11.9 m[2]) 8.2 m 323″ Single Subaru (JNLT) Mauna Kea Observatories, 1999 Hawaii, USA 8.2 m 323″ Single VLT UT1 (Antu) Paranal Observatory, 1998 Antofagasta Region, Chile 8.2 m 323″ Single VLT UT2 (Kueyen) Paranal Observatory, 1999 Antofagasta Region, Chile 8.2 m 323″ Single VLT UT3 (Melipal) Paranal Observatory, 2000 Antofagasta Region, Chile 8.2 m 323″ Single VLT UT4 (Yepun) Paranal Observatory, 2001 Antofagasta Region, Chile 8.1 m 318″ Single Gemini North Mauna Kea Observatories, 1999 (Gillett) Hawaii, USA 8.1 m 318″ Single Gemini South Cerro Pachón (CTIO), 2001 Coquimbo Region, Chile 6.5 m 256″ Honeycomb Magellan 1 Las Campanas Obs., 2000 (Walter Baade) Coquimbo Region, Chile 6.5 m 256″ Honeycomb Magellan 2 Las Campanas Obs., 2002 (Landon Clay) Coquimbo Region, Chile 6.5 m 256″ Single MMT (1 x 6.5 M1) F. -
George Willis Ritchey: Astrophotographer by Robert Anderson
S P R I N G Q U A R T E R / M A R C H 2 0 1 9 George Willis Ritchey: Astrophotographer By Robert Anderson A century ago, Mount Wilson Observatory lost a brilliant astronomer — George Willis Ritchey. When George Ellery Hale left Yerkes Observatory in 1904 to create Mount Wilson, Ritchey was one of four staff members he brought with him. Hale knew he would be indispensable to the new endeavor. And Ritchey was. He designed and built almost every early telescope and optical component on the mountain. Yet for all his contributions, a clash of egos with Hale and charges of disloyalty lead to his dismissal on October 31, 1919. The story of this unpleasant affair is well told by astronomer Donald Osterbrock in his 1993 book, Pauper & Prince: Ritchey, Hale, and Big American Telescopes. It is also the best account of the master optician and his genius (from which much of the information in this article is derived). On the centennial of Ritchey’s On ecember th, , eorge itchey took his rst departure, let’s celebrate his amazing work instead. photograph with the new 60-inch Telescope on Mount Wilson. He chose the Orion Nebula. Perhaps the most Ritchey wore many hats. He was an astronomer, a photographed object in the night sky, recording details of telescope designer, and an expert optician. He took the its glowing gases is a true test of an astrophotographer’s technology of mirror grinding to new levels of perfection equipment and skills. Credit: Carnegie Observatories. —such that his 60-inch mirror grinding machine now rests in the Smithsonian. -
Historyofthetelescope
HISTORY OF THE TELESCOPE Pedro Ré http://pedroreastrophotography.com/ Contents Joseph von Fraunhofer (1787 - 1826) and the Great Dorpat refractor .................................................. 3 Alvan Clark (1804-1887), George Bassett Clark (1827-1891) and Alvan Graham Clark (1832-1897): American makers of telescope optics. .................................................................................................. 13 William Parsons (1800-1867) e o Leviatã de Parsonstown (in Portuguese) ......................................... 21 O Telescópio de Craig (1852) (in Portuguese) ...................................................................................... 29 The 25-inch Newall Refractor ............................................................................................................... 37 The Kew Photoheliograph ..................................................................................................................... 43 O Grande Telescópio de Melbourne (in Portuguese) ........................................................................... 51 O Grande Refractor da Exposição de Paris (1900) (in Portuguese) ...................................................... 61 William Lassell’s (1799-1880) Telescopes and the discovery of Triton ................................................ 71 James Nasmyth’s (1808-1890) telescopes ............................................................................................ 77 The 36-inch Crosley Reflector ..............................................................................................................