After-effects of Saturn's super storm shine on (w/ Video)

(Phys.org)—The heat-seeking capabilities of the international Cassini spacecraft and two ground-based telescopes have provided the first look at the aftermath of Saturn's 'Great Springtime Storm'. Concealed from the naked eye, a giant oval vortex is persisting long after the visible effects of the storm subsided.

The ground-based observations were made by the Very Large Telescope of the in Chile, and NASA's Infrared Telescope Facility at the summit of Mauna Kea in Hawaii.

The vivid cloud structures that wreaked havoc across wide swathes of the mid-northern latitudes of Saturn's atmosphere captured the imaginations of amateur and professional astronomers alike, from its first appearance in December 2010 through much of 2011.

But in new reports that focus on the temperatures, winds and composition of Saturn's atmosphere, scientists find that the spectacular cloud displays were only part of the story.

Much of the associated activity took place beyond the reach of visible-light cameras, and the after-effects are still continuing today.

"It's the first time we've seen anything like it on any planet in the Solar System," says Leigh Fletcher from the University of Oxford, UK, lead author of the Icarus paper.

This animation shows the evolution of Saturn's 'Great Springtime Storm' in the planet's stratosphere. It is based on observations performed at mid-infrared wavelengths. As clouds broke out in Saturn's stormy troposphere, waves of heat traveled hundreds of kilometers upwards, depositing their energy as two vast 'beacons' of hot air in the stratosphere in January 2011. Both hotspots traveled in a westerly direction around the planet, but the larger of the two traveled much faster, lapping the smaller one before they merged to create an enormous vortex that for a brief period, in late June 2011, covered about 62 000 km - almost one quarter of the planet's circumference at the mid-northern latitudes affected by the storm. The giant vortex was visible only to infrared cameras, and persisted long after the clouds from the storm had faded away in the troposphere. Since July 2011, the giant hot vortex has been shrinking and cooling at a very slow pace. It is still present in Saturn's stratosphere, where it has shrunk to less than half of its greatest extent, and is expected to disappear completely by the end of 2013. The animation is based on mid-infrared data collected by NASA/ESA/ASI's Cassini spacecraft, ESO's Very Large Telescope and NASA's Infrared Telescope Facility. Credit: ESA/C. Carreau

"It's extremely unusual, as we can only see the vortex at – we can't tell that it is there simply by looking at the ."

As the visible storm erupted in the roiling cloud deck of Saturn's , waves of energy rippled hundreds of kilometres upwards, depositing their energy as two vast 'beacons' of hot air in the stratosphere.

The were expected to cool down and dissipate, but by late April 2011 – by which time bright cloud material had encircled the entire planet – the hot spots had merged to create an enormous vortex that for a brief period exceeded even the size of Jupiter's famous Great Red Spot.

Furthermore, the temperature of the vortex was far higher than expected, some 80ºC warmer than the surrounding atmosphere. At the same time, huge spikes in the amount of gases like ethylene and acetylene were detected.

Much like the Great Red Spot, Saturn's vortex also cuts off the atmosphere in its core from the surrounding environment, constraining its unique chemistry and high temperatures within the walls of the powerful winds whipping around the edge.

"But Jupiter's vortex is embedded deep down in the turbulent 'weather zone', whereas the vast vortex on Saturn is higher up in the atmosphere where, normally, you wouldn't expect anything like it to have formed," says Dr Fletcher.

"Although there are parallels to be drawn between the two, the mechanisms by which they were formed and the length of time they are going to exist seem to be very different."

Jupiter's famous has raged for at least 300 years, but after traversing the planet once every 120 days since May 2011, Saturn's large beacon is cooling and shrinking. Scientists expect it to fade away completely by the end of 2013.

The question now remains as to whether Saturn's storm-generating energy has been sapped or if there will be a repeat performance.

The outburst already caught observers by surprise by arriving during the planet's northern hemisphere spring, years ahead of the predictably stormy summer season.

"The beauty is that Cassini will be operating until the Saturn system reaches its summer solstice in 2017, so if there is another global event like this, we'll be there to see it," says ESA's Cassini project scientist Nicolas Altobelli.


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Journal information: Icarus

Citation: After-effects of Saturn's super storm shine on (w/ Video) (2012, October 25) retrieved 20 September 2020 from https://phys.org/news/2012-10-after-effects-saturn-super-storm-video.html
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