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27 August 2004

Radio astronomy

Part 2. Spinoffs, discoveries and resources

Jeffrey M. Lichtman
Radio Astronomy Contributing Editor

Australian Hans Michlamyr and his 3.7-meter (12-feet) diameter stretched parabola antenna. Click image to enlarge.

In Part 1, I covered the basics of radio astronomy. Here we will look at some radio spinoffs and discoveries. I will also cover some resources for amateur radio observers.

Spinoffs of radio astronomy

Technological advances in radio astronomy have enhanced existing technology and ushered in new ideas and technology in other fields, all while contributing to what we know about the universe. Here are some examples of technologies that have been influenced in some way by radio astronomy:

  • Sensitive microwave receiving systems
  • High gain antennas
  • Low noise receiver technology
  • Cryogenics
  • Data correlation and signal processing
  • Image restoration
  • Advanced time and frequency standards
  • Remote sensing, navigation and geodesy

Notable radio astronomy discoveries

Signals from the first pulsar.

While contributing to technology, radio astronomy has made some remarkable discoveries. One such discovery is the pulsar.

In 1967, Jocelyn Bell, a doctoral student at Cambridge University detected some sporadic pulses while doing some observations. She at first suspected terrestrial interference. But after recalibrating the receiver, the
pulses still appeared.

This signals reappeared on observing records for quite some time. They were even given the name LGM (Little Green Men). Further investigation showed a movement of one degree each day, which suggested a source in outer space. This radio source became CP1919 in the Cambridge catalog.

Anthony Hewish and Martin Ryle shared the Nobel Prize for the discovery of the pulsar. Jocelyn Bell never received special recognition for her discovery.

Simplified radio sky noise diagram adapted from John Kraus. Click image to enlarge.

Another major radio astronomy discovery was the 3 K (7 cm) microwave background radiation from the expansion of the universe. This was discovered by Arno Penzias and Robert Wilson of Bell Labs.

Other radio astronomy discoveries include many radio galaxies, 21-cm hydrogen emission, hydrocarbon molecules in protostellar clouds and SETI research.

More information about radio astronomy discoveries can be found at the web site of the National Radio Astronomy Observatory (NRAO). For example, here is a recent NRAO news release:

Radio Astronomers lift "fog" on Milky Way's dark heart

Dave Finley, National Radio Astronomy Observatory, 01 April 2004.

BERKELEY – Thirty years after astronomers discovered the mysterious object at the exact center of our Milky Way Galaxy, an international team of scientists has finally succeeded in directly measuring the size of that object, which surrounds a black hole nearly four million times more massive than the Sun. This is the closest telescopic approach to a black hole so far and puts a major frontier of astrophysics within reach of future observations. The scientists used the National Science Foundation's Very Long Baseline Array (VLBA) radio telescope to make the breakthrough.

The Very Long Baseline Array, part of the National Radio Astronomy Observatory, is a continent-wide radio-telescope system, with 10, 240-ton dish antennas ranging from Hawaii to the Caribbean. It provides the greatest resolving power, or ability to see fine detail, of any telescope in astronomy, on Earth or in space. The National Radio Astronomy Observatory is a facility of the National Science Foundation, operated under cooperative agreement by Associated Universities, Inc.
www.berkeley.edu/news/media/releases/2004/04/01_01_srgA.shtml)

The amateur effort: Society of Amateur Radio Astronomers

The Society of Amateur Radio Astronomers (SARA) is an international society of dedicated enthusiasts who mentor, trade technical information, and do their own observations of the radio sky. SARA is a scientific, non-profit organization founded for the sole purpose of supporting amateur radio astronomy. SARA was founded in 1981 by Jeffrey M. Lichtman. It's co-founder was Lt. Col. R. W. P. Patterson (U.S. Army, Ret). Today SARA has hundreds of members worldwide. The group consists of optical astronomers, ham radio operators, engineers, teachers and non-technical persons. Many of our members are new to the field, and membership is extended to all who have an interest in radio astronomy.

SARA 2004 group photo at the National Radio Astronomy Observatory (NRAO). Photograph by Dr. Paul Shuch. Click image to enlarge.


The SARA Mentor Program

SARA is very involved in the education and mentoring of those interested in radio astronomy. Over the years, many enthusiasts have received guidance and training in this discipline. If you would like to learn more and need a mentor, click here.

SARA has active mentors in many parts of the United States and also some foreign countries. For special requests about SARA, please contact me at jmlras@mindspring.com. I will be happy to entertain your requests.

Radio astronomy information sources

Photo Gallery (NASA)
http://nssdc.gsfc.nasa.gov/photo_gallery/photogallery-jupiter.html

Basics of Radio Astronomy (Free Workbook)
http://www2.jpl.nasa.gov/radioastronomy/

Society of Amateur Radio Astronomers
http://www.qsl.net/SARA/

SETI League
http://www.setileague.org

National Radio Astronomy Observatory
http://www.nrao.edu/

Arecibo Radio Observatory
http://www.naic.edu/

Jodrell Bank Radio Observatory
http://www.jb.man.ac.uk/

Acknowledgments

Dr. Edwin V. Bell, II, NASA
Cindy Brooman, Jerry Ehman, Ohio State University
Gary Bloom, Society of Amateur Radio Astronomers
Dave Finley, National Radio Astronomy Observatory
Geoffrey Bower, University of California-Berkeley

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