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Mystery of Jupiter's colourful bands 'solved'

Mystery of Jupiter's colourful bands 'solved'
By: Sky News Posted On: August 10, 2018 View: 11

Mystery of Jupiter's colourful bands 'solved'

Scientists may have solved the mystery of Jupiter's colourful bands.

The gas giant Jupiter's famous bands of cloud have been observed by astronomers for more than 100 years, but until now scientists have not been sure how accurately they reflect what was happening deep inside the planet.

Now, a number-crunching study into how magnetic fields affect atmospheric flows has revealed that at their possible deepest, they never dive more than 3% into the planet itself.

Powerful jet streams flow east through the Jupiter's atmosphere - jet streams which last year NASA established move similar to Earth's.

Spectral analysis of the light reflecting from Jupiter has shown the bands are made of clouds of ammonia in the outer atmosphere, giving the planet its striking stripes of white, red, orange, brown and yellow.

Observations by researchers in Australia and the United States have now helped develop a picture of what's happening beneath these clouds.

This image captures a high-altitude cloud formation surrounded by swirling patterns in the atmosphere of Jupiter's North North Temperate Belt region. The North North Temperate Belt is one of Jupiter's many colorful, swirling cloud bands. Scientists have wondered for decades how deep these bands extend. Gravity measurements collected by Juno during its close flybys discovered that these bands of flowing atmosphere actually penetrate deep into the planet, to a depth of about 1,900 miles (3,000 kil
Image: Cloud formation in Jupiter's upper atmosphere. Pic: NASA

Dr Navid Constantinou, from Australia's ANU research school of earth sciences, said: "We know a lot about the jet streams in Earth's atmosphere and the key role they play in the weather and climate, but we still have a lot to learn about Jupiter's atmosphere.

"Scientists have long debated how deep the jet streams reach beneath the surfaces of Jupiter and other gas giants, and why they do not appear in the sun's interior."

Evidence recently produced by NASA's spacecraft Juno, which conducted multiple fly-bys of the gas giant, suggested the jet streams reached up to 1,860 miles (3,000km) below Jupiter's clouds.

Another member of the research team, Dr Jeffrey Parker from Livermore National Laboratory in the US, said their theory showed how the jet streams were suppressed by the planet's magnetic field.

"The gas in the interior of Jupiter is magnetised, so we think our new theory explains why the jet streams go as deep as they do under the gas giant's surface but don't go any deeper," said Dr Parker.

Juno entered Jupiter's orbit on 4 July 2016. Pic: NASA
Image: Juno entered Jupiter's orbit on 4 July 2016. Pic: NASA

The team compared their observations of Jupiter's bands with the ways that our own planet's atmosphere works.

"Earth's jet streams have a huge impact on the weather and climate by acting as a barrier and making it harder for air on either side of them to exchange properties such as heat, moisture and carbon," said Dr Constantinou.

Unlike the jet streams on Earth, which are wavy and irregular, those on Jupiter are relatively straight compared to its axis.

"There are no continents and mountains below Jupiter's atmosphere to obstruct the path of the jet streams," Dr Parker said.

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"This makes the jet streams on Jupiter simpler. By studying Jupiter, not only do we unravel the mysteries in the interior of the gas giant, but we can also use Jupiter as a laboratory for studying how atmospheric flows work in general."

The study, titled Magnetic Suppression of Zonal Flows on a Beta Plane, has been published in The Astrophysical Journal.

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