
SOUTHERN STORMNewly released images of Saturn’s south pole, taken by the Cassini spacecraft in May 2007, show the entire polar region, including a hurricane-like vortex at the core. The bottom image is in infrared, showing dark areas where clouds absorb the planet’s internal heat. The upper, false-color image combines views from many wavelengths. Aqua areas are clouds and haze, not seen over the pole itself.
Hurricanes Ike and Katrina can’t hold a candle to the giant
storm centers on Saturn. Planetary scientists have gotten their closest look yet
at polar hurricanes on the ringed planet, and find that the storms are big
enough to engulf Earth.
Researchers unveiled the images on October 13 in Ithaca, N.Y.,
at the annual meeting of the American Astronomical Society’s Division for
Planetary Sciences.
The Cassini spacecraft, which has been touring Saturn and
its moons since 2004, took the images in July.
Unlike Earth’s hurricanes, which drift across oceans, these
storms are locked to Saturn’s poles. They may be driven by Saturn’s internal
heat, which can create giant weather patterns by causing massive parcels of
atmospheric gases, most likely ammonium hydrosulfide, to rise and fall.
It’s also possible that sunlight trapped in the planet’s
atmosphere could drive the motions, says Andy Ingersoll of the California
Institute of Technology in Pasadena.
“It’s going to be a delicate balance between the internal
heat and the external sunlight,” that creates these features, comments Heidi
Hammel of the Space Science Institute in Boulder, Colo.
Saturn’s storm activity could churn at the boundary where the planet’s internal
atmospheric heat couples with the upper atmosphere, where sunlight is the main
driver, she suggests.

NORTH AND SOUTHThese infrared images show the cyclone at the north pole (left) and at the south pole (right).NASA, JPL, University of Arizona
“We are still in the phase of butterfly collecting, trying
to classify what we see,” Ingersoll says. “The vortices in the solar system
come in all shapes and sizes.”
Other planets, such as Uranus, and especially Neptune, show
signs of possible storm activity at the poles, but observations from Earth of
these planets are too poor to discern detailed structures, notes Hammel. “It’s
possible that we’d have equally fascinating images for Neptune,
should we ever get there.”
At Saturn’s north pole, the new Cassini portraits reveal a
previously unknown cyclone. Because this pole is now in winter and receives no
sunlight, the northern cyclone can only be seen at infrared wavelengths, where
the glow from Saturn’s own internal heat silhouettes thick, swirling clouds. Some
clouds aren’t thick enough or deep enough to block Saturn’s internal glow,
which emerges unobscured at infrared wavelengths.
In this way, the infrared observations not only allow a peek
at the nightside of the planet, “but allow us to see depth, an extra
dimension,” says Kevin Baines of NASA’s Jet Propulsion Laboratory in Pasadena.
Clouds in the cyclone churn at 530 kilometers per hour,
more than twice as fast as the highest wind speeds of hurricanes on Earth.
Surrounding this cyclone is a puzzling hexagon-shaped
structure, first seen by the Voyager 1 and Voyager 2 spacecraft more than 20
years ago, and imaged by Cassini last year. Although the hexagon itself is stationary, small white
clouds inside the structure move at speeds exceeding 500 km/second, whipping
around the hexagon like cars on a racetrack, says Ingersoll.
Intriguingly, the central eye of the northern storm isn’t
clear but is covered by a dark cloud 600 km wide, which Cassini scientists have
dubbed the bellybutton.
At the south pole, where it’s summer, Cassini took images in
visible light and in infrared. The new images show features one-tenth as small
as those seen before. Previous visible-light images showed an outer ring of
high clouds surrounding what appeared to be a relatively cloud-free region, but
the new close-ups reveal a second, inner ring of strong storms.
The outer ring has a diameter of 4,000 km with a wall
of towering clouds 40 to 70 km high. The inner ring has about half the diameter
of the outer one.
Infrared images of the south show that the entire region is
marked by dark cloud spots, an indication of underlying thunderstorm activity
similar to that in the north, notes Baines.
In the south, the central eye is clear. “Darned if I know”
why a hexagon pattern appears only in the north and not in the south, says
Ingersoll.
Cassini scientists plan to take additional images of both
hemispheres in August 2009, when the seasons change and spring comes to the
northern hemisphere.
Found in: Atom & Cosmos and Planetary Science
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