Volume: 04, Issue: 21 06/14/2006 
Red spots on Jupiter, photographed by amateur astronomer Christopher Go on May 28, 2006. Image credit: NASA, ESA, A. Simon-Miller, and I. de Pater (University of California Berkeley).
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Red Oval BA photographed by astronomers using the Hubble Space Telescope in April 2006. Image credit: NASA, ESA, A. Simon-Miller, and I. de Pater (University of California Berkeley).
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Hubble snaps baby pictures of Jupiter's "Red Spot Jr." Image credit: NASA, ESA, A. Simon-Miller, and I. de Pater (University of California Berkeley).
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Other Articles in This Issue:
NASA’s FUSE Finds Infant Solar System Awash in Carbon
Spitzer Helps Solve Mystery of Space Dust
First Images from NASA’s CloudSat
Planetary Times Summer Hiatus
 

Huge Storms Converge

The two biggest storms in the solar system are about to bump into each other in plain view of backyard telescopes.

Storm number one is the Great Red Spot, twice as wide as Earth, with winds blowing 350 mph. The behemoth has been spinning around Jupiter for hundreds of years.

Storm number two is Oval BA, also known as “Red Jr.,” a youngster of a storm only six years old. Compared to the Great Red Spot, Red Jr. is half its size, able to swallow Earth merely once, but it blows just as hard as its older cousin.

The two are converging. The closest approach will be the 4th of July, according to Amy Simon-Miller of the Goddard Space Flight Center who has been monitoring the storms using the Hubble Space Telescope.

“There won’t be a head-on collision,” she says. “The Great Red Spot is not going to ‘eat’ Oval BA or anything like that.” But the storms’ outer bands will pass quite close to one another – and no one knows exactly what will happen.

Similar encounters have happened before, notes JPL’s Glenn Orton, a colleague of Simon-Miller. “Oval BA and the Great Red Spot pass each other approximately every two years.” Previous encounters in 2002 and 2004 were anticlimactic. Aside from some “roughing” around the edges, both storms survived apparently unaltered.

This time might be different. Simon-Miller and Orton think Red Jr. could lose its red color, ironically, by passing too close to the Great Red Spot.

Red Jr./Oval BA was not always red. For five years, 2000 to 2005, the storm was pure white like many other small “white ovals” circling the planet. In 2006 astronomers noticed a change: a red vortex formed inside the storm, the same color as the powerful Great Red Spot. This was a sign, researchers believed, that Oval BA was intensifying.

The color of the Great Red Spot itself is a mystery. A popular theory holds that the storm dredges up material from deep inside Jupiter’s atmosphere, lifting it above the highest clouds where solar ultraviolet rays turn “chromophores” (color-changing compounds) red. Oval BA turned red when it became strong enough to perform the same trick.

Bumping up against the Great Red Spot, however, could weaken Oval BA, turning it white again. Simon-Miller explains: “We believe the Great Red Spot will push Oval BA toward a southern jet stream, which is blowing against the oval’s counterclockwise rotation.” This would slow Oval BA’s spin, possibly reversing the process that reddened it in the first place.

What will actually happen? “We’ll see,” she said, "That’s what telescopes are for."

Note to sky watchers: Jupiter is easy to find. It pops up out of the evening twilight before any other star, surprisingly bright. Look for it halfway up the southeastern sky at sunset.

For more information, please visit the following websites:
http://www.nasa.gov/vision/universe/solarsystem/05jun_redperil.html
http://science.nasa.gov/headlines/y2006/02mar_redjr.htm.

    
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