Notes
Slide Show
Outline
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Radio Astronomy
  • Ganesh Sankaranarayanan
  • Graduate Student
  • Electrical Engineering


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UW Campus Observatory
  • Built in 1892
  • Located on 4th and   University St
  • Moved in 1895 to the current location
  • Second Building on campus next to denny hall
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Telescope
  • 6-inch Brashear objective lens
  • Warner & Swasey equatorial mount
  •  90-inch focal length
  • Warner & Swasey  wooden , rests on 3 civil war era cannon balls!
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Visible World
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Electromagnetic spectrum
  • Electromagnetic radiation
  • The visible world (We see very little!)
  • Radio spectrum
  • X-ray, UV,IR spectrum





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History of Radio Astronomy
Serendipity?
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History of Radio Astronomy
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Radio Sources
21-cm Neutral Hydrogen Lines
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Radio Sources
21-cm Neutral Hydrogen lines
Discovery
  • Emission once in few million years
  • 80% Hydrogen in Universe
  • 21-cm emission not obstructed by dust
  • Used to map galaxies and ISM


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Milky Way in 21cm
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M33 Radio and Optical Composite
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Orion Nebula M42
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Radio Sources
Pulsars
  • Discovered in 1967
  • Rapidly rotating neutron star
  • 10-15 km radius
  • Cosmic clocks in the sky
  • First thought to be a signal from aliens (“little green men”)
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Sounds of Pulsars
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Pulsar and Supernova Remnant
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Crab Nebula Pulsar
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Radio Sources
Quasars
  • Quasar : Quasi- stellar radio source
  • Most distant object to emit radio waves
  • Contain super massive black holes in the center
  • Radio emission produced by synchrotron radiation
  • Reflect the stage of universe billions of years ago
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Quasar
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Radio Sources
  MASERS
  • Dense molecular clouds with strong emission
  •     (T > 106 K)
  • MASER action
  • Microwave Amplification by Stimulated Emission of Radiation
  • OH,H2O,SiO, CH3CH2OH and more…


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Water
MASER
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Radio Sources
Cosmic Microwave  Background Radiation
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Cosmic Microwave  Background Radiation
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Radio
Sources
Sun
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Radio Sources Planets
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Radio Telescopes Arecibo
  • Located in Puerto Rico
  • Operated by Cornell and NSF
  • 1000 ft (304.8 m)
  • Used for Astronomy,  atmospheric and planetary studies


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Radio Telescopes
Green Bank Telescope
  • Located in Green bank, West Virginia
  • 485 feet tall -- taller than the Statue of Liberty!
  • 100 by 110 m width
  • World’s Largest steerable radio telescope


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Radio Telescopes
VLI (Very Large Array)
  • Located in Socorro, NM
  • 27 antennas interferometer
  • Each antenna 25 meters( 82 feet) in diameter
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VLBI (Very Large Baseline Array)
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ALMA The Atacama Large Millimeter Array
  • Atacama desert,     Chile
  • 64 radio telescopes
  • 12 meter (39 feet) wide dish antenna
  • Expected to operate in 2011


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Radio Telescopes
around the world
  • Europe
    • Westerbork Synthesis Radio Telescope (WSRT) , Netherlands
    • The Ryle Telescope, United Kingdom
  • Australia
    • Mopra Observatory
  • Asia
    • Giant Meterwave Radio Telescope(GMRT) , India
    • Nobeyama millimeter array ,Japan
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Radio Astronomy at UW
  • UAI established in 1999
  • 7ft dish
  • Currently building motion control and receivers for 21cm hydrogen lines (1420 MHz)


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Future of Radio Astronomy
  • More cost to build radio telescopes
    • Consortium among countries to build future telescopes


  • Major advancements in telescope technologies
    • Better design to control noise over effective area
      • GMRT,ALMA
    • Better angular resolution
  • Encroachment of radio frequencies by ground and satellite communications
    • More power in deciding frequency allocations
    • Better modulation techniques to prevent spill over


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The End