Radio Wave Technique Could Detect Alien Planets

**American Patriot** · April 19th, 2011, 15:21

New Radio Wave Technique Could Detect Alien Planets

SPACE.com Staff
Date: 18 April 2011 Time: 03:38 PM ET

Images of Jupiter’s northern UV auroras were obtained using the Advanced Camera for Surveys onboard the Hubble Space Telescope in February 2007.
CREDIT: Boston University/NASA.

Radio waves from the auroras of planets like Jupiter could be used to detect exoplanets that orbit at large distances from their parent star, according to a new study.

Auroras are flares of ultraviolet light in the upper atmosphere of planets.

Scientists at the University of Leicester in England have shown that emissions from the radio aurora of planets such as Jupiter and Saturn could be detectable by radio telescopes such as the European Low Frequency Array, or LOFAR. Construction of the LOFAR radio telescope, with stations primarily located in the Netherlands, will be completed later this year.

"This is the first study to predict the radio emissions by exoplanetary systems similar to those we find at Jupiter or Saturn," said Jonathan Nichols, who is presenting the study's results today (April 18) at the Royal Astronomical Society's National Astronomy Meeting in Wales.

"At both planets, we see radio waves associated with auroras generated by interactions with ionized gas escaping from the volcanic moons, Io and Enceladus," Nichols said. "Our study shows that we could detect emissions from radio auroras from Jupiter-like systems orbiting at distances as far out as Pluto." [The Strangest Alien Planets]

Nichols examined how the radio emissions of Jupiter-like exoplanets would be affected by the rotation rate of the planet, the rate of plasma outflow from a moon, the orbital distance of the planet and the ultraviolet brightness of the parent star.

In his study, Nichols found that in many scenarios, exoplanets orbiting stars that emit bright ultraviolet light would generate enough radio power to be detectable from Earth. In fact, for the brightest stars and fastest moving planets, the radio emissions would be detectable from systems up to 150 light-years away from Earth. [Video: Mapping Alien Worlds: A How-To Guide]
"In our solar system, we have a stable system with outer gas giants and inner terrestrial planets, like Earth, where life has been able to evolve," Nichols said. "Being able to detect Jupiter-like planets may help us find planetary systems like our own, with other planets that are capable of supporting life."

Finding alien planets that orbit at large distances from their star remains a challenge, and of the hundreds of exoplanets that have been detected to date, less than 10 percent orbit at distances equivalent to the outer planets in our own solar system.

Most exoplanets have been found using the so-called transit method, which detects the dimming of light as a planet moves — or transits — in front of a star. Another technique looks for a wobble effect as a star is tugged by the gravity of an orbiting planet. With both of these methods, it is easiest to detect planets that closely orbit the star and move very quickly.

"Jupiter and Saturn take 12 and 30 years respectively to orbit the sun, so you would have to be incredibly lucky or look for a very long time to spot them by a transit or a wobble," Nichols said.

The results have been accepted for publication in an upcoming issue of the Monthly Notices of the Royal Astronomical Society.

**American Patriot** · April 19th, 2011, 15:23

Technically this isn't a "new idea"... but because we can indeed pick up signals from Jupiter and Saturn generated in the atmosphere, this means that we can use those same antennas to pick up and perhaps pinpoint the location in the sky where other planets might generate similar signals.

Using shortwave radios for instance.

**American Patriot** · April 19th, 2011, 15:25

http://www.spacetoday.org/SolSys/Jup...iterRadio.html

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The Planet Jupiter:

How To Hear Radio Signals From Jupiter

RADIO IMAGE OF JUPITER

Jupiter is a source of powerful bursts of natural radio waves that can produce exotic sounds when picked up on Earth using simple antennas and shortwave receivers.

Even though human ears can't hear the radio waves directly, they make an exciting listening experience when converted to audio signals by a receiver.

It's not E.T. phoning home. The shortwave radio signals from Jupiter aren't a sign of extraterrestrial intelligence. The emissions are generated naturally by plasma instabilities in Jupiter's magnetosphere.

Pulsing power beam. Most space physicists say that ionized gas in the upper atmosphere above Jupiter's magnetic poles sometimes behaves like a powerful radio laser or maser. The radiation can be so intense that Jupiter frequently outshines the Sun as a source of radio energy at ham radio wavelengths.

Where does the radio laser get so much power? It starts on Jupiter's volcanic moon Io.

Tidal forces from Jupiter and its other large satellites superheat the interior of the moon Io and make it the most volcanic body in the Solar System.

Volcanic materials are thrown far above Io's surface. Much of that enters orbit around Jupiter, forming a huge gaseous donut around the giant planet.

With a diameter the size of Io's orbit, the electrically conducting "Io torus," as it's known, spans 525,000 miles and has an important impact on Jupiter's magnetic environment.

Two trillion watts. As Io's orbital motion carries it through this magnetized ring of ionized gas, a huge electrical current flows between Io and Jupiter. Carrying about two trillion watts of power, it's the biggest DC electrical circuit in the Solar System.

Unlike the ordinary kind of DC circuit we know using batteries and wires, plasma physicists believe that current in the Io-Jupiter system is carried by a type of magnetic plasma wave called Alfven waves.

However it works, this awesome current is the power source for plasma waves that give rise to the laser radio signals that travel away from Jupiter's magnetic poles in cone-shaped beams.

The beams rotate with the giant planet every 9 hours and 55 minutes making Jupiter something like a slow-turning pulsar. When the beams sweep past our planet Earth, listeners here can pick up the Jovian radio bursts in the shortwave bands between 15 and 40 MHz.

RADIO IMAGE OF JUPITER

The radio images of Jupiter on this page were recorded by the Australia Telescope National Facility (ATNF) of the Commonwealth Scientific and Industrial Research Organisation (CISRO). The Australia Telescope is a set of eight radio-receiving dish antennas at three sites in New South Wales. It is the largest single astronomical institution in Australia. The image at the top of this page was received by ATNF at a wavelength of 22cm. The image immediately above was received by ATNF at a wavelength of 13cm. By comparison, the amateur Radio JOVE telescopes observe Jupiter at wavelengths near 1500 cm.

Radio JOVE. Thanks to a NASA project known as Radio JOVE, the pleasure of listening to Jupiter's broadcast of exotic sounds is no longer reserved for professional astronomers.

Amateur astronomers, ham radio enthusiasts, shortwave listeners and students in middle schools, high schools and colleges can tune in, too.

NASA scientists at the Goddard Space Flight Center in Maryland, along with others at the University of Florida, are helping the public tune in and inspiring thousands to look up and listen to the biggest planet in the Solar System.

NASA has come up with a $115 radiotelescope kit that a school science class or other interested observers can put together. The kit includes all of the parts required to construct a 20 MHz radio receiver.

It comes with the necessary transmission cables and wire for the dual antennas, which are of a common type that ham radio operators call half-wave dipoles. Each antenna is about 20 feet long. They should be mounted 20 feet apart.

The kit doesn't include the PVC pipe recommended for mounting the wires. However, PVC is inexpensive at local hardware stores. Alternatively, wood could be used for mounting the antennas.

How sensitive is it? The kit makes a radiotelescope capable of detecting the giant planet hundreds of millions of miles away from Earth.

Bill Pine is a California high school teacher who is distributing the NASA Radio JOVE kits through The INSPIRE Project, Inc., a non-profit educational corporation, to schools, amateur radio operators and other interested individuals.

Once they build their own radiotelescopes, the new amateur astronomers make observations, which help scientists monitor activity in Jupiter's enormous magnetosphere.

What does it sound like? When it comes to sound effects, NASA says woodpeckers and ocean waves can't hold a candle to Jupiter.

There are two varieties of Jovian radio bursts:

Through the loudspeaker of a shortwave receiver, the so-called "L-burst" sounds like ocean waves crashing on a distant beach. The "L" stands for long. If a recording is slowed down dramatically, the S-burst sound like eerie drifting whistlers.
Through the loudspeaker of a shortwave receiver, the so-called "S-burst" produces a staccato of rapid popping sound with a beat that reminds some of woodpeckers. The "S" stands for short.

Sample Sounds. To listen to the sounds of Jupiter, click these spectrum images of 25 MHz radio bursts from Jupiter captured on tape at the University of Florida Radio Observatory.

S-BURSTS
L-BURSTS

Student Observing Party. One of the first Radio JOVE student teams was at the Lexington Traditional Magnet School in Lexington, Kentucky. Students, teachers and parents set up an observing station on a teacher's farm at Mt. Sterling, Kentucky, on Oct. 22, 1999. Signals from Jupiter came through loud and clear.

What if you can't build one? For those who can't build their own radiotelescope, there is an online observatory where anyone can monitor Jupiter and receive live data on the World Wide Web.

The University of Florida Radio Observatory (UFRO), in a central Florida pine forest near the mouth of the Suwannee River, has an array antennas capturing shortwave radio signals from Jupiter and the Sun.

UFRO has been collecting Jupiter radio data there since the mid-1950's. Today, it is known as North America's best facility for low-frequency planetary radio astronomy.

The Sun also shines. Like Jupiter, the Sun is a powerful source of shortwave radio bursts. Solar radio activity is especially high around the so-called solar maximum, which began in the year 2000.

Recording solar bursts is another way to test the completed Radio JOVE Project radiotelescope kits and learn about the powerful processes that produce solar storms and flares.

Bonus Audio. In addition to receiving natural radio signals from Jupiter, you now can listen to ten seconds of very low frequency audio sounds of Jupiter captured by the Cassini spacecraft as it passed by in 2000 on its way to Saturn. The low radio frequencies received by Cassini were converted by NASA to sound wave frequencies for this RealAudio file.

Learn more about Jupiter and radioastronomy

Exploring Jupiter main page
Planet Jupiter NASA JPL Galileo

Moons and Rings

Radio JOVE Project NASA Goddard Space Flight Center

brochure
visitor center
How to join
equipment photos
recommended readings

The Sounds of Jupiter NASA
University of Florida Radio Astronomy Observatory online

equipment
live data

Jupiter Radio Japan
The Discovery of Jupiter's Radio Emissions

Jovian Decametric Radio Emission

Exploring Jupiter's Magnetosphere American Geophysical Union

Read more about the Solar System . . .
Star:	The Sun
Inner Planets:	Mercury	Venus	Earth	Mars
Outer Planets:	Jupiter	Saturn	Uranus	Neptune	Pluto
Other Bodies:	Moons	Asteroids	Comets
Beyond:	Pioneers	Voyagers