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University of Sulaimani
College of Education
Physics Department
Karbin kamaran
Karbin.ph@gmail.com
Rawezh Othman
rawezhothman1@gmail.com
2016-2017
Radio Telescope
Types of Telescopes
Millimeter Telescopes
Sub-Millimeter Telescopes
Infrared Telescope
Optical Telescopes
Ultraviolet Telescopes
X-ray Telescopes
Gamma-ray Telescopes
Radio Telescopes







Outline
History
Some picture radio telescope
Why we use Radio Telescope
Types of Radio Telescope
Basic and Diagram Radio Telescope
Advantages and Disadvantages Radio Telescope
The sky seen at the radio telescope
Information about china Radio Telescope
History
 The early history of radio astronomy begins
in 1894 with sir Olivier Lodge.
 like much in science it was discovered
accidentally by Karl Jansky
 first radio telescope built by Karl Jansky .in
1931.
History
Some picture radio telescope
Why we use Radio Telescope
 Planet observation…
 Stars observation…
 Seeing between stars…
 Observing energetic objects…
 Seen stars not light…
Types of Radio Telescope
 Ther are many difernt size and desing of
radio telescope.
 There are three main sort
• Haystack radio telescope
• Westford radio telescope
• Arecibo and China radio telescope
Types of Radio Telescope
• Haystack radio telescope
- Controlled by remote
- We can Used for education
- Usually smaler tlescopes
Haystack radio telescope
Types of Radio Telescope
• Westford radio telescope
- Dome shaped tlescope
- Discovered in 1961
- Used in communications technilogy
Westford radio telescope
Types of Radio Telescope
• Arecibo radio telescope
• China radio telescope
We have only two version from these types
Arecibo and China radio telescope
Basic Radio Telescope
 Basic componet of a radio Telescope
• Dish
• Receiver
• Amplifier
• Computer and Recorder devices
Diagram Radio Telescope
Diagram Radio Telescope
Dish
Amplifier
Computer
and
Recorder devices
Receiver
Advantages Radio Telescope
And
Disadvantages RadioTelescope
Advantages Radio Telescope
They work day and night
They can see much further distance objects
They are simple technology
They are Cheap to build
Can be operate in bad weather
Radio Telescope are much larger due to
Wavelength Size
Disadvantages RadioTelescope
 They have to be very very big
 They are too heavy to lift into space
 Affected by other radio waves
The sky seen
at the Radio Telescope
For Understand
A Flattened Earth
The sky seen at the Radio Telescope
The sky seen at optical wavelengths The sky seen at the radio telescopeVS
Information about china Radio Telescope
 Location: PINGTANG county
GUIZHOU province
 Built: 2011-2016
 Dimeter: 500m
 Deep:138m
Thank you for every one
Discussion Time

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Radio telescope

Editor's Notes

  1. Shar7e history kae The early history of radio astronomy begins in 1894, with Sir Oliver Lodge. Lodge attempted detection of radiation from the sun at centimeter wavelengths. Unfortunately over the next forty years, further attempts also failed due to inadequate detection techniques. The more recent history of radio astronomy begins in 1931 when an American engineer named Karl Jansky, while working for Bell Telephone Laboratories, conducted experiments on radio wavelength interference. Jansky detected three separate groups of static; local thunderstorms, distant thunderstorms and a steady hisstype static of unknown origin. The unknown source that Jansky found is the center of the Milky Way as he was able to show by determining its position on the sky. Jansky was the first to detect radio emission from the Galaxy. The image above shows Jansky standing with his antenna (Photo courtesy of Bell Laboratories). This rotatable antenna looks similar to a merry-go-round; the rotation allowed it to move along with the static. The work done by Jansky included receiving frequencies in the range of 15 to 30 MHz (approximately 15-m wavelengths). Jansky published three reports on his findings, which were largely ignored for many years to come. The field of radio astronomy would eventually recognize him with a unit named for him; the Jansky is equivalent to 10^(-26) watts per m^2 per Hz.