Small radio telescope for hydrogen 21cm emission line

In summary, a small radio telescope for hydrogen 21cm emission line is a specialized telescope that detects the emission of the hydrogen atom at a wavelength of 21 centimeters. It works by using a dedicated receiver connected to a computer, and can provide insights into the distribution and movement of hydrogen gas in the universe. This type of telescope is different from others because of its specific purpose and can be used by anyone with the necessary knowledge and equipment, but is primarily utilized by professional astronomers and researchers for studying the universe.
  • #1
Kimmo
1
0
Hi

I am trying to figure out if there is call for a small, commercial, educational radio telescope to measure the 21cm emission line of hydrogen.

We have been developing an instrument with the following characteristics:

- The antenna would have a size of about 1m x 1m.
Because the beamwidth of such an antenna is relatively large, about 14 degrees, it is enough to have a 'manual stand' for the antenna.
Furthermore, it is not necessary to track the motion of the sky during observations; a typical integration of the HI line would take a couple of
minutes.
The stand would have simple digital setting circles, similar to those used with Dobsonian telescopes. A simple computer program transforms the desired galactic coordinates to altitude and azimuth, and the user then manually points the antenna.

- A low-noise amplifier is attached to the antenna.

- The receiver itself transforms the original signal at around 1420 MHz to a lower frequency, say, between 0-3 MHz, which is then read by an analog-to-digital converter. The receiver is kept as simple as possible so that it can be used to demonstrate the basic components of a radio receiver (local oscillator, mixer, amplifier stages etc.)

- Analog-to-digital converter is used to digitize the signal. An ordinary computer is used to calculate the spectrum of the digitized signal
by using fast Fourier transform. The width of the spectrum could be about 3 MHz, so that it includes the hydrogen line plus some background
emission around the line. Software on a computer is used to integrate (sum up) the spectra so that good enough signal-to-noise ratio
is achieved.

- The spectra can be saved so that external programs can be used to analyze the spectra.

- The most interesting project that can be made with this telescope is probably the measurement of galactic rotation curve.
As an example of this project see
www.haystack.mit.edu/edu/undergrad/srt/SRT Projects/rotation.html

- In addition, one can use this instrument to measure radio emission from the Sun. With some luck, one can detect radio bursts from the Sun. Other sources than the Sun are difficult to observe with this small telescope.

- This instrument is intended to measure hydrogen emission mainly along the galactic plane where the emission is at strongest.

- This instrument could be used at schools, colleges and universities.

So, in principle the telescope would be similar to the SRT (Small Radio Telescope) that was developed at Haystack observatory
(see www.haystack.mit.edu/edu/undergrad/srt/oldsrt.html ), although smaller, lighter and without motorized tracking.
Consequently, the price would be much less than the price of about $6000 for the SRT (SRT is not produced anymore).

What is your opinion, do you think that teachers and students would find this instrument useful and interesting ?


Kimmo Lehtinen
University of Helsinki, Finland
 
Astronomy news on Phys.org
  • #2



Dear Kimmo Lehtinen,

Thank you for sharing your idea for a small, commercial, educational radio telescope. As a scientist in the field of radio astronomy, I believe there is definitely a call for such an instrument. Here are some of my thoughts on your proposed design and its potential uses:

- The antenna size of 1m x 1m is suitable for detecting the 21cm emission line of hydrogen, which is a widely studied and important feature in radio astronomy. The manual stand with digital setting circles makes it easy to point the antenna in the desired direction, and the non-requirement for tracking the motion of the sky during observations is a great advantage for educational purposes.

- The inclusion of a low-noise amplifier and a simple receiver with basic components is a good approach for demonstrating the fundamentals of radio receivers. This could be a valuable learning tool for students interested in radio astronomy or engineering.

- The use of an analog-to-digital converter and a computer for data analysis is a cost-effective and efficient method for obtaining spectra. This would allow students to conduct their own observations and analyze the data, which is a great way to engage them in hands-on learning.

- The potential projects that can be carried out with this telescope, such as measuring galactic rotation curves and detecting radio bursts from the Sun, are interesting and relevant to current research in radio astronomy. This would provide students with a real-world application of their learning and may spark their interest in pursuing further studies in the field.

- The price point of this telescope is significantly lower than that of the SRT, making it more accessible for educational institutions. I believe that teachers and students would find this instrument both useful and interesting, as it provides a practical and affordable way to study radio astronomy.

In summary, I believe that your proposed design for a small, commercial, educational radio telescope has great potential for use in schools, colleges, and universities. It combines simplicity, affordability, and practicality, making it a valuable tool for teaching and learning about radio astronomy. Thank you for sharing your idea and I wish you the best in its development.

 

FAQ: Small radio telescope for hydrogen 21cm emission line

What is a small radio telescope for hydrogen 21cm emission line?

A small radio telescope for hydrogen 21cm emission line is a type of telescope that is specifically designed to detect the emission of the hydrogen atom at a wavelength of 21 centimeters. This emission line is used to study the distribution and movement of hydrogen gas in the universe.

How does a small radio telescope for hydrogen 21cm emission line work?

A small radio telescope for hydrogen 21cm emission line works by using a specially designed receiver that can detect the emission of the hydrogen atom at a wavelength of 21 centimeters. This receiver is connected to a computer which processes the data and creates an image of the detected hydrogen gas in the universe.

What can we learn from using a small radio telescope for hydrogen 21cm emission line?

Using a small radio telescope for hydrogen 21cm emission line, we can learn about the distribution and movement of hydrogen gas in the universe. This can provide insights into the formation and evolution of galaxies, as well as the structure of the universe itself.

How is a small radio telescope for hydrogen 21cm emission line different from other types of telescopes?

A small radio telescope for hydrogen 21cm emission line is different from other types of telescopes because it is specifically designed to detect the hydrogen emission line at a wavelength of 21 centimeters. Other telescopes may use different wavelengths or may be designed for different purposes, such as detecting visible light or infrared radiation.

Can anyone use a small radio telescope for hydrogen 21cm emission line?

Yes, anyone can use a small radio telescope for hydrogen 21cm emission line as long as they have the necessary knowledge and equipment. However, these telescopes are often used by professional astronomers and researchers for studying the universe and are not typically available for personal use.

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