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Quantum fluctuations in space, science, exploration and other cosmic fields... served up regularly by MSNBC.com science editor Alan Boyle since 2002.

Alan Boyle covers the physical sciences, anthropology, technological innovation and space science and exploration for MSNBC.com. He is a winner of the AAAS Science Journalism Award, the NASW Science-in-Society Award and other honors; a contributor to "A Field Guide for Science Writers"; and a member of the board of the Council for the Advancement of Science Writing.

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Springtime stunners from Saturn

Posted: Monday, September 21, 2009 7:42 PM by Alan Boyle


NASA / JPL / SSI
Click for slideshow: Saturn's rings have darkened almost to invisibility in this
portrait captured by the Cassini orbiter on Aug. 12, just after equinox. This view
highlights the start of spring for Saturn's northern hemisphere. Click on the image
to see a slideshow featuring pictures from the ringed planet and its moons.

The Cassini orbiter has sent back a spectacular set of pictures taken during Saturn’s equinox, including a moody portrait of the giant planet's rings at their darkest. Taken together, the pictures reveal that Saturn’s rings are bumpier, more active and more complex than previously thought.

An equinox simply marks the precise time in a planet's orbital cycle when day and night are of equal lengths. It's one of the traditional markers of seasonal change. Thus, the photos herald the return of spring to Saturn’s northern hemisphere after almost 30 earthly years (which means fall has begun in the south).

On Earth, this week's equinox puts people in a mind to think of fall leaves (in, say, New England) or spring flowers (in Australia). On Saturn, however, the main significance of the Aug. 11 equinox is that it provided scientists with an unprecedented opportunity to see how the giant planet's rings are structured.

Because Saturn's orbital cycle is nearly 30 Earth years long, Cassini's equinox encounter marked the first time scientists could take a close-up look at the rings under conditions that were ideal for fine-resolution observations.

"It's like putting on 3-D glasses and seeing the third dimension for the first time, " Bob Pappalardo, Cassini project scientist at NASA's Jet Propulsion Laboratory, explained today in a news release. "This is among the most important events Cassini has shown us."

Because Saturn's rings are edge-on with respect to the sun during the equinox, the shadows cast by small features within the rings are grossly exaggerated, like the shadows of trick-or-treaters at sunset. Those bumps, ruffles and peaks go unnoticed when sunlight falls upon the rings on an angle. The peculiar circumstances of the equinox revealed, however, that such features are actually not small at all. Some of them rise as high above the main plane of the rings as the Rocky Mountains on Earth, NASA said.

Ripples and ridges in the rings
That plane is nowhere near as flat as a plain. In the old days, scientists thought the rings were only 30 feet (10 meters) thick in the main rings (designated by the letters A through D). Cassini's observations confirm that the rings actually ripple up and down in vertical formations spanning as much as 500 miles (800 kilometers). Scientists don't yet know what caused those ripples.

"It looks like something happened in the early 1980s to get this pattern going, but we are still trying to figure out what could have disturbed such a large part of the rings," said Cornell University's Matthew Hedman, a Cassini imaging team associate.

There's a lot going on within those rippling rings: Cassini's shadow pictures helped astronomers spot a wall of ring particles that rose as high as 2.5 miles (4 kilometers), whipped up by the gravitational influence of the Saturnian moon Daphnis.

"We thought the plane of the rings was no taller than two stories of a modern-day building, and instead we've come across walls more than two miles high," said Carolyn Porco, a planetary scientist at the Colorado-based Space Science Institute who leads the Cassini imaging team. "Isn't that the most outrageous thing you could imagine? It truly is like something out of science fiction."

Cassini also spotted streaky clouds of tiny particles floating above the ring plane. That phenomenon suggests that yard-wide bits of interplanetary debris are continuing to rain down upon the rings, throwing up those clouds and contributing to the evolution of the rings. There are also larger-sized "moonlets" that apparently stir up the ring material, creating clumps that whirl like propellers.

Cassini's previous observations confirmed that the rings are made up of chunks of ice and gunk, in varying sizes. During the equinox, those chunks and bits cooled down to new lows, as recorded by the orbiter's Composite Infrared Spectrometer. Temperatures in the A ring, for example, dipped to 382 degrees below zero Fahrenheit (43 Kelvin). That's not quite as chilly as the permanently shadowed craters at our moon's south pole, which last week was dubbed the coldest spot in the solar system. But it's pretty darn close.

See the full show
Our latest Saturn slideshow presents a selection of the equinox pictures, and for more, you can click on over to the Web sites for the Cassini-Huygens mission and the Cassini imaging team. Here's a NASA slideshow complete with spacey audio track, and a video explaining the geometry behind the equinox mission.

I don't think there's any doubt that the highlight of today's selection is the full frontal image of Saturn, its rings and its moons, captured on the day after equinox. In a large-format version of the image, you can spot the moon Janus in the lower left, Epimetheus near the middle bottom, Pandora outside the rings on the right, and Atlas inside Saturn's thin F ring on the right.

Did you spot them all? If so, that's because the picture has been enhanced to make the rings and moons more visible. The bright side of the rings was made 20 times brighter relative to the planet itself, and the dark side's brightness has been bumped up 60 times. The moons have also been brightened by a factor of 30 to 60. Without the brightening, the rings would essentially fade to black, according to the imaging team.

In an e-mail exchange, Porco told me that more equinox pictures will be coming from the Cassini team. "But they will be like the ones we captured as the sun was setting, probably more moon shadows, and images taken here and there," she said.

Porco said she was deeply satisfied with Cassini's coverage of Saturn's equinox, and noted that "it will be a very long time before any of us sees anything like this again." Almost 15 years, to be precise.

"This has been a moving spectacle to behold, and one that has left us with far greater insight into the workings of Saturn's rings than any of us could have imagined," she said in a news release summarizing the latest findings. "We always knew it would be good. Instead, it's been extraordinary."

Update for 7:25 p.m. ET Sept. 22: Check out Brian Williams' take on the new pictures from Saturn, which aired on "NBC Nightly News." 

More about Saturn:


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Comments

Although not an exquisite discovery in the grand scheme of the Cosmos...too bad Carl Sagan isn't around to witness things like this.  R.I.P.
Beautiful picture and great writeup Alan!  The rings of Saturn have intrigued people for many centuries, thanks to Galileo and his funny little viewing tube.  The Cassini orbiter has done great work for many years and hopefully it will last much longer.
It seems like the coolest way to study the rings would be to orbit Cassini just "above" them. Couldn't you get close enough then to actually *see* "ring stuff" moving and colliding.  Or is everything moving so ridiculously fast it would just be a blur anyway(like looking at the shoulder of a freeway whizzing past next to your car) at least until you were obliterated by some inbound "ring rock".   It seems like maybe you could get into a syncronous orbit with the rings and then just "inch closer and closer" to see what happens.  

Is that a stupid question? I'm a reasonably bright person; though, admittedly, not a rocket scientist by trade.
Kyle, what you suggest could yield some magnificent images and possible insight as to the details of the orbital mechanics of the rings. Here's what makes that difficult and expensive:

The center of the orbit of Saturn's rings must coincide with the center of mass of Saturn. The center of the orbit (or focus, if a non-circular elliptical orbit) of a satellite orbiting Saturn must also coincide with Saturn's center of mass.

This means you couldn't be in a stable orbit "above," or parallel to, Saturn's rings. The satellite's orbit would have to cross the rings in two places, and a destructive collision would be all but inevitable.

It might be possible, with enough fuel (requiring a more fuel-hungry launch vehicle to lift the extra fuel), to be in an UNstable orbit "above" the rings and use fuel for "station-keeping." It also might be possible to very gradually merge the orbit of a satellite with the rings by "inching closer and closer" if the satellite were covered with tough air-bags like the Mars lander. This would require some great software with inputs from multi-directional radar, maneuvering thrusters that would be somehow protected by the air bags and still not burn them up when fired, and, again, a lot of fuel.
Thanks Bruce, the center of mass problem occurred to me after I wrote that.  So... plan B.  If we don't mind destroying a probe, we might be able to throw something into such an orbit that for a short time before being obliterated crossing the ring plane, it were psuedo-syncronous, and get some of those ring shots that way. Effectively inching closer and closer, but with no intention of surviving the trip.  Maybe...  
omg...
saturn so0 efFen pretTy...
i think i want to0 live there...
Wow! Space is beautiful, like art!

http://www.viewposters.com/posters/subjects/astronomy



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