Saturn’s wind mystery is starting to unravel

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  Last updated August 28, 2019 at 11:35 am


Saturn’s interior might flow like honey, and it might solve the mystery of why winds stop at a certain depth inside the giant gas planet.

Cassini’s view of Saturn and its main rings. Credit: NASA/JPL – Caltech/Space Science Institute

A new study argues that Saturn’s interior flows like honey due to its magnetic field, which may help solve the mystery of why the planet’s powerful winds stop 8,500km inside the giant gas planet.

Unlike Earth, Saturn has no solid surface; it is a gaseous planet, consisting mostly of hydrogen and helium that move around fluidly.

Strong winds, known as jet streams, form the appearance of stripes on Saturn’s exterior – similar but less stark than those on Jupiter.

Cassini offered a glimpse below Saturn’s clouds

Study co-author, Navid Constantinou from The Australian National University (ANU), says the recent space mission Cassini offered a glimpse of what goes on below Saturn’s cloud tops.

“At the end of its mission, Cassini dived into Saturn and made detailed measurements of Saturn’s gravitational field.”

“The measurements revealed that these jet streams continue about 8,500 km inside Saturn, which is roughly 15 per cent of the distance towards the planet’s centre,” he says.

Constantinou says the study may help solve the mystery of why Saturn’s jet streams stop at a certain depth.

“Deep into Saturn, where the pressure is high, the gas becomes a liquid that conducts electricity and is more strongly influenced by the planet’s magnetic field.”

“An electrically conducting, flowing liquid will bend or distort a magnetic field. We showed that the distortion of the magnetic field makes the fluid more viscous, like honey.”

The mystery of what goes on inside Saturn is starting to be unveiled

The team’s theoretical model indicates this viscous effect from the magnetic field could be the reason why the jet streams terminate at depths beyond 8,500 km.

“The mysteries of what goes on inside Saturn and the other gas giants in our Solar System are now slowly starting to be unveiled,” Constantinou says.

“Our findings provide a promising way for interpreting the data from planetary missions and offer a better understanding of the planets in our Solar System and beyond.”

The results are published in the Physical Review Fluids journal.


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