Jansky’s Experiment
المؤلف:
Diane Fisher Miller
المصدر:
Basics of Radio Astronomy
الجزء والصفحة:
p 3
24-2-2016
1883
Jansky’s Experiment
As often happens in science, RF radiation from outer space was first discovered while someone was looking for something else. Karl G. Jansky (1905-1950) worked as a radio engineer at the Bell Telephone Laboratories in Holmdel, New Jersey. In 1931, he was assigned to study radio frequency interference from thunderstorms in order to help Bell design an antenna that would minimize static when beaming radio-telephone signals across the ocean. He built an awkward looking contraption that looked more like a wooden merry-go-round than like any modern-day antenna, much less a radio telescope. It was tuned to respond to radiation at a wavelength of 14.6 meters and rotated in a complete circle on old Ford tires every 20 minutes. The antenna was connected to a receiver and the antenna’s output was recorded on a strip-chart recorder.
Jansky’s Antenna that First Detected Extraterrestrial RF Radiation
He was able to attribute some of the static (a term used by radio engineers for noise produced by unmodulated RF radiation) to thunderstorms nearby and some of it to thunderstorms farther away, but some of it he couldn’t place. He called it “ . . . a steady hiss type static of unknown origin.”
As his antenna rotated, he found that the direction from which this unknown static originated changed gradually, going through almost a complete circle in 24 hours. No astronomer himself, it took him a while to surmise that the static must be of extraterrestrial origin, since it seemed to be correlated with the rotation of Earth.
He at first thought the source was the sun. However, he observed that the radiation peaked about 4 minutes earlier each day. He knew that Earth, in one complete orbit around the sun, necessarily makes one more revolution on its axis with respect to the sun than the approximately 365 revolutions Earth has made about its own axis. Thus, with respect to the stars, a year is actually one day longer than the number of sunrises or sunsets observed on Earth. So, the rotation period of Earth with respect to the stars (known to astronomers as a sidereal day) is about 4 minutes shorter than a solar day (the rotation period of Earth with respect to the sun). Jansky therefore concluded that the source of this radiation must be much farther away than the sun. With further investigation, he identified the source as the Milky Way and, in 1933, published his findings.
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