Gas giants continue to be great
places to observe at a safe distance.
This is the first time since 1990
that we have had such a huge storm erupting on Saturn and this gives us an
opportunity to collect a lot of new data.
Enjoy the images.
Super Storm on Saturn
May 19, 2011: NASA's Cassini spacecraft and a European Southern
Observatory ground-based telescope are tracking the growth of a giant
early-spring storm in Saturn's northern hemisphere so powerful that it
stretches around the entire planet. The rare storm has been wreaking havoc for
months and shooting plumes of gas high into the planet's atmosphere.
This false-color infrared image shows clouds of large ammonia ice
particles dredged up by the powerful storm. Credit: Cassini.
"Nothing on Earth comes close to this powerful storm," says
Leigh Fletcher, a Cassini team scientist at the University of Oxford in the
United Kingdom, and lead author of a study that appeared in this week's edition
of Science Magazine. "A storm like this is rare. This is only the sixth
one to be recorded since 1876, and the last was way back in 1990."
Cassini's radio and plasma wave science instrument first detected the
large disturbance in December 2010, and amateur astronomers have been watching
it ever since through backyard telescopes. As it rapidly expanded, the
storm's core developed into a giant, powerful thunderstorm, producing a
3,000-mile-wide (5,000-kilometer-wide) dark vortex possibly similar to
Jupiter's Great Red Spot.
This is the first major storm on Saturn observed by an orbiting
spacecraft and studied at thermal infrared wavelengths. Infrared
observations are key because heat tells researchers a great deal about
conditions inside the storm, including temperatures, winds, and atmospheric
composition. Temperature data were provided by the Very Large Telescope (VLT) on
Cerro Paranal in Chile and Cassini's composite infrared spectrometer (CIRS),
operated by NASA's Goddard Space Flight Center in Greenbelt, Md.
"Our new observations show that the storm had a major effect on
the atmosphere, transporting energy and material over great distances --
creating meandering jet streams and forming giant vortices -- and disrupting
Saturn's seasonal [weather patterns]," said Glenn Orton, a paper
co-author, based at NASA's Jet Propulsion Laboratory in Pasadena, Calif.
The violence of the storm -- the strongest disturbances ever detected
in Saturn's stratosphere -- took researchers by surprise. What started as an
ordinary disturbance deep in Saturn's atmosphere punched through the planet's
serene cloud cover to roil the high layer known as the stratosphere.
Thermal infrared images of Saturn from the Very Large Telescope Imager
and Spectrometer for the mid-Infrared (VISIR) instrument on the European
Southern Observatory's Very Large Telescope, on Cerro Paranal , Chile ,
appear at center and on the right. An amateur visible-light image from Trevor
Barry, of Broken Hill , Australia , appears on the left. The
images were obtained on Jan. 19, 2011.
"On Earth, the lower stratosphere is where commercial airplanes
generally fly to avoid storms which can cause turbulence," says Brigette
Hesman, a scientist at the University
of Maryland in College Park who works on the CIRS team at
Goddard and is the second author on the paper. "If you were flying in an
airplane on Saturn, this storm would reach so high up, it would probably be
impossible to avoid it."
A separate analysis using Cassini's visual and infrared mapping
spectrometer, led by Kevin Baines of JPL, confirmed the storm is very violent,
dredging up deep material in volumes several times larger than previous storms.
Other Cassini scientists are studying the evolving storm and, they say, a more
extensive picture will emerge soon.
Stay tuned to Science@NASA for updates.
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