NASA Probe Gets Close-Up Views of Large Hurricane on Saturn

[Date Prev] [Date Next] [Thread Prev] [Thread Next] [Date Index] [Thread Index]

 



April 29, 2013

Dwayne Brown 
Headquarters, Washington 
202-358-1726 
dwayne.c.brown@xxxxxxxx 

Jia-Rui C. Cook 
Jet Propulsion Laboratory, Pasadena, Calif. 
818-354-0850 
jccook@xxxxxxxxxxxx 

RELEASE: 13-121

NASA PROBE GETS CLOSE-UP VIEWS OF LARGE HURRICANE ON SATURN

WASHINGTON -- NASA's Cassini spacecraft has provided scientists the 
first close-up, visible-light views of a behemoth hurricane swirling 
around Saturn's north pole. 

In high-resolution pictures and video, scientists see the hurricane's 
eye is about 1,250 miles (2,000 kilometers) wide, 20 times larger 
than the average hurricane eye on Earth. Thin, bright clouds at the 
outer edge of the hurricane are traveling 330 miles per hour (150 
meters per second). The hurricane swirls inside a large, mysterious, 
six-sided weather pattern known as the hexagon. 

"We did a double take when we saw this vortex because it looks so much 
like a hurricane on Earth," said Andrew Ingersoll, a Cassini imaging 
team member at the California Institute of Technology in Pasadena. 
"But there it is at Saturn, on a much larger scale, and it is somehow 
getting by on the small amounts of water vapor in Saturn's hydrogen 
atmosphere." 

Scientists will be studying the hurricane to gain insight into 
hurricanes on Earth, which feed off warm ocean water. Although there 
is no body of water close to these clouds high in Saturn's 
atmosphere, learning how these Saturnian storms use water vapor could 
tell scientists more about how terrestrial hurricanes are generated 
and sustained. 

Both a terrestrial hurricane and Saturn's north polar vortex have a 
central eye with no clouds or very low clouds. Other similar features 
include high clouds forming an eye wall, other high clouds spiraling 
around the eye, and a counter-clockwise spin in the northern 
hemisphere. 

A major difference between the hurricanes is that the one on Saturn is 
much bigger than its counterparts on Earth and spins surprisingly 
fast. At Saturn, the wind in the eye wall blows more than four times 
faster than hurricane force winds on Earth. Unlike terrestrial 
hurricanes, which tend to move, the Saturnian hurricane is locked 
onto the planet's north pole. On Earth, hurricanes tend to drift 
northward because of the forces acting on the fast swirls of wind as 
the planet rotates. The one on Saturn does not drift and is already 
as far north as it can be. 

"The polar hurricane has nowhere else to go, and that's likely why 
it's stuck at the pole," said Kunio Sayanagi, a Cassini imaging team 
associate at Hampton University in Hampton, Va. 

Scientists believe the massive storm has been churning for years. When 
Cassini arrived in the Saturn system in 2004, Saturn's north pole was 
dark because the planet was in the middle of its north polar winter. 
During that time, Cassini's composite infrared spectrometer and 
visual and infrared mapping spectrometer detected a great vortex, but 
a visible-light view had to wait for the passing of the equinox in 
August 2009. Only then did sunlight begin flooding Saturn's northern 
hemisphere. The view required a change in the angle of Cassini's 
orbits around Saturn so the spacecraft could see the poles. 

"Such a stunning and mesmerizing view of the hurricane-like storm at 
the north pole is only possible because Cassini is on a sportier 
course, with orbits tilted to loop the spacecraft above and below 
Saturn's equatorial plane," said Scott Edgington, Cassini deputy 
project scientist at NASA's Jet Propulsion Laboratory (JPL) in 
Pasadena, Calif. "You cannot see the polar regions very well from an 
equatorial orbit. Observing the planet from different vantage points 
reveals more about the cloud layers that cover the entirety of the 
planet." 

Cassini changes its orbital inclination for such an observing campaign 
only once every few years. Because the spacecraft uses flybys of 
Saturn's moon Titan to change the angle of its orbit, the inclined 
trajectories require attentive oversight from navigators. The path 
requires careful planning years in advance and sticking very 
precisely to the planned itinerary to ensure enough propellant is 
available for the spacecraft to reach future planned orbits and 
encounters. 

The Cassini-Huygens mission is a cooperative project of NASA, the 
European Space Agency and the Italian Space Agency. JPL manages the 
Cassini-Huygens mission for NASA's Science Mission Directorate in 
Washington. The Cassini orbiter and its two onboard cameras were 
designed, developed and assembled at JPL. The imaging team consists 
of scientists from the United States, the United Kingdom, France and 
Germany. The imaging operations center is based at the Space Science 
Institute in Boulder, Colo. 

Images and two versions of a movie of the hurricane can be viewed 
online at: 

http://go.nasa.gov/17tmHzo 

For more information about Cassini and its mission, visit: 

http://www.nasa.gov/cassini 

	
-end-



To subscribe to the list, send a message to: 
hqnews-subscribe@xxxxxxxxxxxxxxxxxxxxxx
To remove your address from the list, send a message to:
hqnews-unsubscribe@xxxxxxxxxxxxxxxxxxxxxx



[Index of Archives]     [JPL News]     [Cassini News From Saturn]     [NASA Marshall Space Flight Center News]     [NASA Science News]     [James Web Space Telescope News]     [JPL Home]     [NASA KSC]     [NTSB]     [Deep Creek Hot Springs]     [Yosemite Discussion]     [NSF]     [Telescopes]

  Powered by Linux