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1
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- Ganesh Sankaranarayanan
- Graduate Student
- Electrical Engineering
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2
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- 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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3
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- 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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4
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5
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- Electromagnetic radiation
- The visible world (We see very little!)
- Radio spectrum
- X-ray, UV,IR spectrum
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6
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7
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8
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9
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- 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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10
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11
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12
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13
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- 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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14
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15
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16
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17
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- 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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18
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19
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- 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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20
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21
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22
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23
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24
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25
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- 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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26
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- 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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27
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- Located in Socorro, NM
- 27 antennas interferometer
- Each antenna 25 meters( 82 feet) in diameter
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28
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29
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- Atacama desert, Chile
- 64 radio telescopes
- 12 meter (39 feet) wide dish antenna
- Expected to operate in 2011
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30
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- Europe
- Westerbork Synthesis Radio Telescope (WSRT) , Netherlands
- The Ryle Telescope, United Kingdom
- Australia
- Asia
- Giant Meterwave Radio Telescope(GMRT) , India
- Nobeyama millimeter array ,Japan
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31
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- UAI established in 1999
- 7ft dish
- Currently building motion control and receivers for 21cm hydrogen lines
(1420 MHz)
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32
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- 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
- 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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33
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