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Three Radio Astronomy Futures:

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Title: Three Radio Astronomy Futures:


1
  • Three Radio Astronomy Futures
  • ALMA, EVLA, SKA

Mark T. Adams Assistant Director, EPO National
Radio Astronomy Observatory http//www.nrao.edu
Osher Lifelong Learning Institute University of
Virginia 18 September 2008
2
Electromagnetic Spectrum
The Domain of Radio Astronomy Wavelength 15
meters to 0.3 millimeter Frequency 20 MHz
to 1.0 THz 1 THz 1,000 GHz 1,000,000 MHz
3
Green Bank Telescope
  • Dedicated in 2000 in Green Bank, WV
  • Located in National Radio Quiet Zone
  • 100 x 110m dish 2 acres of collecting area
  • Weighs 17M lbs largest moving structure on land
  • Studies pulsars, complex molecules, neutral
    hydrogen

4
Very Large Array
  • Built in 197s, Dedicated in1980
  • 27 antennas in a reconfigurable array

Studies Black holes, proto-planetary disks around
young stars, Galactic Center, cosmology
5
Very Long Baseline Array
  • Operated from Socorro, NM
  • Ten antennas
  • Hawaii to the Caribbean
  • Highest resolution astronomical telescope
  • Dedicated 1993

6
NRAO Technology Center
  • Radio Astronomy technology signal processing
    push state-of-the-art
  • NTC scientists, engineers, Technicians perform
    the required Research Development

7
The Invisible UniverseWhy Do Radio Astronomy?
  • Radio complements other wavelengths

H o r s e h e a d N e b u l a
Optical Infrared Radio
8
The Invisible UniverseHydrogen
Optical image of M81 Group (DSS)
9
The Invisible UniverseCenter of our Galaxy
10
Expanded Very Large Array
http//www.aoc.nrao.edu/evla
11
Expanded Very Large Array
  • Leverages the VLA to Enable the Next-Generation
    cm-wavelength Telescope
  • builds on existing infrastructure 27 antennas,
    Track, facilities, people
  • An International Collaboration United States,
    Canada, and Mexico
  • Implements state-of-the-art technology
  • Correlator
  • wideband receivers 1 - 50 GHz
  • fiber-optic data transmission system
  • digital electronics
  • Software

12
EVLA Science Themes
Magnetic Universe
Measure the strength and structure of the cosmic
magnetic field
Obscured Universe
Sgr A
Image young stars massive black holes in dust
enshrouded environments
13
EVLA Correlator
  • WIDAR Wideband Interferometric Digital
    Architecture
  • WIDAR is an Innovative method for digital
    correlation of very wideband signals from a radio
    interferometer
  • 40 x 1015 Ops / sec

invented by Brent Carlson Peter Dewdney at
Dominion Radio Astrophysical Observatory
14
Atacama Large Millimeter/submillimeter Array
http//www.alma.nrao.edu http//www.alma.cl
15
ALMA Science Schedule
  • Key Science
  • Cosmic Origins Planets, Stars, Galaxies
  • The Cold Universe
  • Timeline
  • 1995 site testing in Chile Begins
  • 1998 Design Development Start
  • 2007 First ALMA Antennas Arrive in Chile
  • 2010 First Science
  • 2013 ALMA Fully Operational

16
ALMA Location
  • mm / sub-mm radiation is blocked by water in the
    atmosphere
  • MM / sub-mm telescopes must be located at very
    dry, high altitude sites
  • Chajnantor plain in northern chile (Atacama
    Desert ) is the best

17
Altiplano de ChajnantorRegion II, Chile
18
ALMA Antennas in Chile
3 Melco Antennas
VertexRSI
19
ALMA Transporter
Concept
Reality Sep 07
20
Square Kilometre Array
  • 1994 Community begins to Consider A Next-Gen
    Radio Telescope With A Square Kilometre (250
    Acres) of Collecting Area
  • Scientific Objectives
  • Technology
  • Cost

21
Square Kilometre Array
  • Key Science Projects
  • Cradle of Life
  • Gravity Tests Using Pulsars Black Holes
  • Origin Evolution of Cosmic Magnetism
  • Galaxy Evolution Cosmology
  • Probing the Dark Ages

22
Square Kilometre Arraynew technology
23
Square Kilometre Array
  • Pathfinder Technology development projects
    underway in United States, Europe, South Africa,
    Australia
  • Likely To Be 3 Separate SKA Telescope Systems
  • SKA-Hi, SKA-Mid, SKA-Low
  • Construction Cost 1- 2B USD for Each
  • EVLA COMPLETE in 2012 SKA PATHFINDER
  • SKA Fully Realized Operational 2025
  • http//www.skatelescope.org

24
Radio Astronomy discoveries Cosmic Microwave
Background Quasars Pulsars Gravitational
Lenses Dark Matter Masers Gravitational
Waves First Extra-solar PlanetsStay Tuned for
the EVLA, ALMA, SKA the Scientific frontiers
they will open
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