A Tour of the Largest Ground-Based Telescopes Being Developed

Slides:



Advertisements
Similar presentations
Chapter 6: Telescopes – Portals of Discovery. Visible light is only one type of electromagnetic radiation emitted by stars Each type of EM radiation travels.
Advertisements

Telescope Projects at Steward Observatory Work in Progress Astronomical Society of New York Union College Saturday, 24 October 2009 Peter Wehinger Steward.
Optics and Telescopes Chapter Six. Telescopes The fundamental purpose of any telescope is to gather more light than the naked eye can In many cases telescopes.
Chapter 4 – Stars, Galaxies, and the Universe.  The electromagnetic spectrum includes the entire range of radio waves, infrared radiation, visible light,
1 Astronomical Observational Techniques and Instrumentation RIT Course Number Professor Don Figer Telescopes.
Chapter 6 Telescopes: Portals of Discovery. 6.1 Eyes and Cameras: Everyday Light Sensors Our goals for learning How does your eye form an image? How do.
Observational techniques meeting #3. Mirrors Classical mirrors: polished glass Monolithic block of glass, polished to spec. Largest good one is the 200”
Light and Telescopes Chapter 5. Traditional Telescopes The 4-m Mayall Telescope at Kitt Peak National Observatory (Arizona)
Imaging Science Fundamentals Chester F. Carlson Center for Imaging Science Astronomical Imaging Telescopes and Detectors.
Astronomical Research at TAMU Faculty Future facilities and projects.
The SOAR Telescope MSU’s Laboratory for Astronomical Discovery.
A Few Ways of Acquiring Telescope Time Telescope Committee Astronomical Society of New York October 23, 2009 Peter Wehinger Steward Observatory University.
January 24, 2006Astronomy Chapter 5 Astronomical Instruments How do we learn about objects too far away for spacecraft? How do telescopes work? Do.
Future of Astronomy Astronomy 315 Professor Lee Carkner Lecture 25.
Modern Telescopes and Ancient Skies New Views of the Universe An IU Lifelong Learning Class Tuesdays, May 10, 17, 24 III. 30-meters and beyond.
Optics and Telescopes Chapter Six.
Telescopes. Magnification (make things look bigger) easy to make a telescope with good magnification Collection of large amounts of light (see fainter.
Figuring large off-axis segments to the diffraction limit Hubert Martin Steward Observatory University of Arizona.
Top 5 Optical Telescopes By: Kiana Gathers and Mary Beth Garrett.
Infrared Telescopes 1.
Radiation & Telescopes ____________ radiation: Transmission of energy through space without physical connection through varying electric and magnetic fields.
Observatories and Telescopes Mauna Kea, Hawaii (14,000 ft) Why do telescopes need to be located at high altitude and dry climate ?
Future of Astronomy Astronomy 315 Professor Lee Carkner Lecture 23.
1 New Frontiers with LSST: leveraging world facilities Tony Tyson Director, LSST Project University of California, Davis Science with the 8-10 m telescopes.
25.4 Galaxies and the Universe  Objectives:  Describe the different types of galaxy  Describe the solar system’s position in our galaxy  Describe the.
© 2010 Pearson Education, Inc. Chapter 6 Telescopes: Portals of Discovery.
{ Telescopes Jon Holtzman NMSU Astronomy.  Telescopes are light buckets: bigger buckets collect more light, and faint (far away) objects don’t produce.
Telescope Technologies
Optics and Telescopes. Optics and Telescopes: Guiding Questions 1.How do reflecting and refracting telescopes work? 2.Why is it important that professional.
© 2004 Pearson Education Inc., publishing as Addison-Wesley Telescopes.
1 The LOFT group Who we are Where we came from Where we are going Large Optics Fabrication and Testing ?
Telescopes Notes.
Chapter 6 Telescopes: Portals of Discovery. 6.1 Eyes and Cameras: Everyday Light Sensors Our goals for learning How does your eye form an image? How do.
Telescopes continued… Why is bigger better? Two reasons…
A105 Stars and Galaxies  News Quiz Today  1 st NovaSearch homework due Thursday  First Exam on Thursday, Sept. 28 Today’s APODAPOD.
Light, Optics and Telescopes The Electromagnetic Spectrum.
Copyright © The McGraw-Hill Companies, Inc. Permission required for reproduction or display. Chapter 6 Light and Optics.
Mega Telescopes of the 21 st Century Evolution in the Ground-Space Synergy Dr. Marc Postman (STScI) & Richard Ellis (Caltech) James Webb Space Telescope.
Telescopes Lecture. Standards Understand how knowledge about the universe comes from evidence collected from advanced technology (e.g., telescopes, satellites,
Stars, Galaxies, and the Universe
Future of Astronomy Astronomy 315 Professor Lee Carkner Lecture 25.
Telescopes Telescopes only have a few jobs: 1)Point to a particular point on the sky 2)Collect lots of light and focus it onto a detector 3)Follow the.
1 Astronomical Observational Techniques and Instrumentation Professor Don Figer Telescopes.
Refracting Telescopes 24.2 Tools for Studying Space  A refracting telescope is a telescope that uses a lens to bend or refract light.  Focus The most.
다양한 창문을 통한 우주 내용 왜 다양한 창문 ? 왜 다양한 창문 ? 대기의 영향 대기의 영향 망원경의 성능 망원경의 성능 관측에서 얻는 정보 관측에서 얻는 정보 중요 망원경들 중요 망원경들 차세대 망원경들 차세대 망원경들.
Gina Moraila University of Arizona April 21, 2012.
Optics and Telescopes Chapter Six. Some Guiding Questions 1.Why is it important that telescopes be large? 2.Why do most modern telescopes use a large.
Youth AstroNet Program Introduction This presentation based on information and materials from The Harvard-Smithsonian Center for Astrophysics Science Education.
The GMT Project The Giant Magellan Telescope (GMT)
Youth AstroNet Program Introduction
Chapter 6 Telescopes: Portals of Discovery
Telescopes.
Chapter 6 Telescopes: Portals of Discovery
Observing and exploring space
Facility Concept Design and Study
Planetary Discovery in the era of Spacecraft Exploration Xi Zhang
Telescopes & Detectors
6.3 Telescopes and the Atmosphere
Uber media Process billions of social, demographic, and location signals daily for Fortune 500 companies across retail, automotive, and entertainment .
Telescopes.
4. Telescopes Light gathering power and resolution
Telescopes & Detectors
Seeing into Space!.
Optical Telescopes, Radio Telescopes and Other Technologies Advance Our Understanding of Space Unit E: Topic Three.
Astronomical Observational Techniques and Instrumentation
Telescopes Lecture.
Review When is Orion visible in Arizona?
The Richard F. Caris Mirror Lab
The Largest Telescopes
Telescopes & Detectors
Presentation transcript:

A Tour of the Largest Ground-Based Telescopes Being Developed Big Glass A Tour of the Largest Ground-Based Telescopes Being Developed

Giant Magellan Telescope (GMT) Las Campanas, Chile First Light 2024

Large Binocular Telescope (LBTO) Mt Graham, AZ, 2007

Large Synoptic Survey Telescope (LSST), Cerro Pachon Ridge, Chile First Light 2022

What do All These New Observatories have in Common? They’re built with BIG GLASS: 8.4 meter primary mirrors

Caris Mirror Lab at U of Arizona Steward Observatory

Building the Giant Mirrors Used in these Telescopes

The Honeycomb structure controls weight and adaptation to temperatures Small-scale casting showing honeycomb structure in relation to thickness of mirrored surface One of 1750 alumina-silica cores used in casting an 8.4 meter mirror The Honeycomb structure controls weight and adaptation to temperatures

Special borosilicate glass is melted in the spin-casting operation

Spin-casting the fourth of seven 8 Spin-casting the fourth of seven 8.4-meter mirrors destined for the Giant Magellan Telescope (GMT). The mold cools slowly for three months after casting to prevent introduction of impurities and imperfections Casting the Mirror

Moving the cast blank in preparation for grinding & polishing

Grinding and Polishing Grinding pedestal is visible in the background; back of mirror is ground flat at this station; front is ground to prepare for polishing. Long bar hanging across the left-center is a laser-measuring device to ensure mirror surface is ground to exacting specifications Grinding and Polishing

Polishing the Aspherical (parabolic) surface The final polishing stage deploys a “stressed-lap” polishing tool that consists of a polishing disk which bends actively to match the varying curvature of the surface The entire mirror surface is polished in stages; here a cleaning assembly is lowered onto the surface Polishing the Aspherical (parabolic) surface

When Complete the Seven Segments will comprise the primary mirror for the GMT, totaling 84.5 ft across

GMT’s Mission and Stats Location: Las Campanas Peak, Chile Elevation 8,500 ft 300 nights / year viewing (minimal rainfall) Purposes: search for exoplanets; study dark matter & dark energy; study formation and fate of galaxies Scheduled first light: 2024

LSST Goals will image the entire visible sky every few nights (thus capturing changes and opening up the time-domain window to the observable universe) Map the interior of the Milky Way—our galactic home in 10 years of observing, the goal is to record the greatest movie ever made billions of objects will be imaged in six colors in an unprecedentedly large volume of our universe

LSST Technical Innovations camera (3200 megapixels, the world’s largest digital camera) each image the equivalent of 40 full moons telescope (simultaneous casting of the primary and tertiary mirrors; two aspherical optical surfaces on one substrate) data management (20-30 terabytes of data nightly, nearly instant alerts issued for objects that change in position or brightness) Public facility—access to images and database for amateur astronomers

What other ELTs are in the works (Extremely Large Telescopes) and how do they differ from these? Thirty Meter Telescope (TMT), Mauna Kea, Hawaii European Extremely Large Telescope (E-ELT), Cerro Amazones, Chile Hint: Like the James Webb Space Telescope, these two telescopes will use large numbers of 1.44 meter hexagonal mirrors in coordinated arrays

Thirty Meter Telescope (TMT) Mauna Kea, HI 2022 (date delayed)

TMT Stats 30-meter diameter 492 optical segments (individual mirrors) Mauna Kea Observatory, Hawaii, 13,290 ft Scheduled First Light 2022 Status: delayed by court order driven by Hawaiian protests

European Extremely Large Telescope (E-ELT) Cerro Amazones, Chile, 2024

E-ELT Stats Overall diameter of primary = 39.3 meters 798 individual hexagonal mirror segments Each segment 1.45 meters across, 50 mm thick Located on Cerro Amazones, Chile, at 10,040 ft. Status: budget approved by European First light scheduled for 2024

Relevant Websites Large Synoptic Survey Telescope Giant Magellan Telescope Observatory (this site has many good links, including more detail about Univ. of Az’s manufacture of 8.4 meter mirrors) Thirty Meter Telescope (site may be down) Large Binocular Telescope Observatory Caris Mirror Lab