Categories: ObservingSaturn

Violent Polar Cyclones on Saturn Imaged in Unprecedented Detail by Cassini

[/caption]

The Cassini mission has released some of the most detailed images of Saturn’s poles yet, revealing vast cyclones churning up the gas giant’s atmosphere in the north and south. These observations show very similar storms to the south pole observations imaged by the NASA spacecraft in 2006, only in far better detail. It is believed the north and south cyclones are generated by violent thunderstorms deep inside Saturn’s atmosphere; water condensing inside these storms output heat, fuelling the vortex extending 2,500 miles (4,000 kilometres) in diameter. The smallest features resolved are 120 kilometre (75 mile)-wide cumulus clouds rotating at velocities in excess of 325 mph (530 kph), more than twice the wind speed possible on Earth…

and the mystery north pole hexagon is still there.

Images of the large cyclones at the north (left) and south (right) poles of Saturn taken in June 2008 by the visual and infrared mapping spectrometer onboard the Cassini spacecraft (NASA/JPL/University of Arizona)
Cassini has wowed scientists with these brand new views of Saturn’s north pole. With detail at 10-times higher resolution than previously attained, Cassini has shown that both poles have vast swirling cyclones that highlight regions of planet-wide storm activity.

These are truly massive cyclones, hundreds of times stronger than the most giant hurricanes on Earth,” said Kevin Baines, Cassini scientist on the visual and infrared mapping spectrometer at NASA’s Jet Propulsion Laboratory. “Dozens of puffy, convectively formed cumulus clouds swirl around both poles, betraying the presence of giant thunderstorms lurking beneath. Thunderstorms are the likely engine for these giant weather systems.”

The Saturn hexagon as seen by Voyager 1 in 1980 (NASA)
Interestingly, the northern storm observation still shows the mysterious hexagonal shape (as originally verified in 2006, after a sighting by Voyager 1 in 1980), only in far greater detail. Scientists are still uncertain why the northern cyclone should take such a stable form; the clouds within the hexagonal shape spin at high speeds without interfering with its six-sided shape.

Previous observations appeared to show an outer ring of high clouds surrounding a region thought to be clear air with a few puffy clouds circulating around the pole. These brand new images reveal a far more complex picture. The circulating clouds are actually smaller convective storms forming other, more distinct rings.

Oblique view of Saturns south polar vortex (NASA)

Tony DelGenio of NASA’s Goddard Institute for Space Studies in New York and Cassini imaging team member explains the scene: “What looked like puffy clouds in lower resolution images [from 2006] are turning out to be deep convective structures seen through the atmospheric haze. One of them has punched through to a higher altitude and created its own little vortex.”

These clouds push high above the main weather system, casting long shadows, indicating they are 25-45 miles (40-70 km) above the vortex rings (pictured above). These also appears to be an inner ring of clear air (the “eye” of the storm) over the poles, that appeared bigger in previous observations.

For me, the most perplexing feature to come out of these new Cassini observations is the enduring hexagonal shape in the circulating clouds. In 2006 when the lower-resolution north pole observations were released, many made the assumption that it was an unstable transient feature, appearing for a short period, only to disappear soon afterwards. But over a year later, the hexagon remains, as six-sided as ever. I’d guess this shape could be some atmospheric standing wave, what do you think?

See the Cassini video of the north pole hexagon being buffetted by the high-speed winds surrounding it »

Source: Space.com

Ian O'Neill

[Follow me on Twitter (@astroengine)] [Check out my space blog: Astroengine.com] [Check out my radio show: Astroengine Live!] Hello! My name is Ian O'Neill and I've been writing for the Universe Today since December 2007. I am a solar physics doctor, but my space interests are wide-ranging. Since becoming a science writer I have been drawn to the more extreme astrophysics concepts (like black hole dynamics), high energy physics (getting excited about the LHC!) and general space colonization efforts. I am also heavily involved with the Mars Homestead project (run by the Mars Foundation), an international organization to advance our settlement concepts on Mars. I also run my own space physics blog: Astroengine.com, be sure to check it out!

Recent Posts

How Could Astronauts Call for Help from the Moon?

Exploring the Moon poses significant risks, with its extreme environment and hazardous terrain presenting numerous…

9 hours ago

There Was a 15 Minute Warning Before Tonga Volcano Exploded

Volcanoes are not restricted to the land, there are many undersea versions. One such undersea…

10 hours ago

Main Sequence and White Dwarf Binaries are Hiding in Plain Sight

Some binary stars are unusual. They contain a main sequence star like our Sun, while…

11 hours ago

What a Misplaced Meteorite Told Us About Mars

11 million years ago, Mars was a frigid, dry, dead world, just like it is…

13 hours ago

Uranus is Getting Colder and Now We Know Why

Uranus is an oddball among the Solar System's planets. While most planets' axis of rotation…

16 hours ago

How Scientists Repurposed a Camera on ESA’s Mars Express Mission

A camera aboard the Mars Express orbiter finds a new lease on life. Sometimes, limitations…

19 hours ago