Written by Jia-Rui Cook
NASA’s Jet Propulsion Laboratory
Pasadena, CA – From a distance, most of the Saturnian moon Dione resembles a bland cueball.
Thanks to close-up images of a 500-mile-long (800-kilometer-long) mountain on the moon from NASA’s Cassini spacecraft, scientists have found more evidence for the idea that Dione was likely active in the past. It could still be active now.
 The Cassini spacecraft looks down, almost directly at the north pole of Dione. The feature just left of the terminator at bottom is Janiculum Dorsa, a long, roughly north-south trending ridge. (Image credit: NASA/JPL/Space Science Institute)
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NASA’s Cassini Spacecraft data suggests Wild Weather for Saturn’s Moon Titan this Summer
May 23, 2013 |
Written by Jia-Rui C. Cook
NASA’s Jet Propulsion Laboratory
Pasadena, CA – Saturn’s moon Titan might be in for some wild weather as it heads into its spring and summer, if two new models are correct. Scientists think that as the seasons change in Titan’s northern hemisphere, waves could ripple across the moon’s hydrocarbon seas, and hurricanes could begin to swirl over these areas, too.
The model predicting waves tries to explain data from the moon obtained so far by NASA’s Cassini spacecraft. Both models help mission team members plan when and where to look for unusual atmospheric disturbances as Titan summer approaches.
 Ligeia Mare, shown in here in data obtained by NASA’s Cassini spacecraft, is the second largest known body of liquid on Saturn’s moon Titan. It is filled with liquid hydrocarbons, such as ethane and methane, and is one of the many seas and lakes that bejewel Titan’s north polar region. Cassini has yet to observe waves on Ligeia Mare and will look again during its next encounter on May 23rd, 2013. (Image credit: NASA/JPL-Caltech/ASI/Cornell)
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NASA’s Cassini spacecraft spots huge Hurricane at Saturn’s North Pole
April 30, 2013 |
Written by Dr. Tony Phillips
Science at NASA
Washington, D.C. – 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 mph(150 meters per second). The hurricane swirls inside a large, mysterious, six-sided weather pattern known as the hexagon.
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NASA says Saturn to make it’s closest approach to Earth April 28th
April 26, 2013 |
Written by Dr. Tony Phillips
Science at NASA
Washington, D.C. – The Solar System is a beautiful place filled with wonders that NASA space probes are only beginning to discover. There’s a tendency, though, for people to become indifferent; every year Hubble, Cassini, MESSENGER and other spacecraft beam back gigabytes of jaw-dropping images. After a while, you don’t have any more “gasps” left in you.
Well, maybe just one more. Inhale deeply, because at the end of April, Saturn will put on a breathtaking display.
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NASA’s Cassini spacecraft sees Ice Clouds forming in atmosphere of Saturn’s moon Titan
April 12, 2013 |
Written by Jia-Rui C. Cook
NASA’s Jet Propulsion Laboratory
Pasadena, CA – An ice cloud taking shape over Titan’s south pole is the latest sign that the change of seasons is setting off a cascade of radical changes in the atmosphere of Saturn’s largest moon.
Made from an unknown ice, this type of cloud has long hung over Titan’s north pole, where it is now fading, according to observations made by the composite infrared spectrometer (CIRS) on NASA’s Cassini spacecraft.
 The recently formed south polar vortex stands out in the color-swaddled atmosphere of Saturn’s largest moon, Titan, in this natural color view from NASA’s Cassini spacecraft. (Image credit: NASA/JPL-Caltech/Space Science Institute)
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NASA’s Jet Propulsion Laboratory studies atmospheric chemistry of Saturn’s moon Titan
April 4, 2013 |
Written by Jia-Rui C. Cook
NASA’s Jet Propulsion Laboratory
Pasadena, CA – A laboratory experiment at NASA’s Jet Propulsion Laboratory, Pasadena, CA, simulating the atmosphere of Saturn’s moon Titan suggests complex organic chemistry that could eventually lead to the building blocks of life extends lower in the atmosphere than previously thought.
The results now point out another region on the moon that could brew up prebiotic materials. The paper was published in Nature Communications this week.
 The colorful globe of Saturn’s largest moon, Titan, passes in front of the planet and its rings in this true color snapshot from NASA’s Cassini spacecraft. (Image credit: NASA/JPL-Caltech/Space Science Institute)
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NASA’s Cassini spacecraft observations show the craters on Saturn’s Moon Titan disappearing
January 18, 2013 |
Written by Jia-Rui Cook
NASA’s Jet Propulsion Laboratory
Pasadena, CA – Titan’s siblings must be jealous. While most of Saturn’s moons display their ancient faces pockmarked by thousands of craters, Titan – Saturn’s largest moon – may look much younger than it really is because its craters are getting erased.
Dunes of exotic, hydrocarbon sand are slowly but steadily filling in its craters, according to new research using observations from NASA’s Cassini spacecraft.
 This set of images from the radar instrument on NASA’s Cassini spacecraft shows a relatively “fresh” crater called Sinlap (left) and an extremely degraded crater called Soi (right). Sinlap has a depth-to-diameter ratio close to what we see on Jupiter’s moon Ganymede. Soi has a shallow depth compared to similar craters on Ganymede. These craters are both about 50 miles (80 kilometers) in diameter. (Image credit: NASA/JPL-Caltech/ASI/GSFC)
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NASA’s Cassini Spacecraft data suggests there maybe Ice on the Lakes of Saturn’s moon Titan
January 12, 2013 |
Written by Jia-Rui Cook
NASA’s Jet Propulsion Laboratory
Pasadena, CA – It’s not exactly icing on a cake, but it could be icing on a lake. A new paper by scientists on NASA’s Cassini mission finds that blocks of hydrocarbon ice might decorate the surface of existing lakes and seas of liquid hydrocarbon on Saturn’s moon Titan.
The presence of ice floes might explain some of the mixed readings Cassini has seen in the reflectivity of the surfaces of lakes on Titan.
 This artist’s concept envisions what hydrocarbon ice forming on a liquid hydrocarbon sea of Saturn’s moon Titan might look like. (Image credit: NASA/JPL-Caltech/USGS)
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NASA’s Cassini spacecraft to take first images of Saturn’s Transit of Venus from deep space
December 21, 2012 |
Written by Dr. Tony Phillips
Science at NASA
Washington, D.C. – Last June, astronomers urged sky watchers to observe the transit of Venus. It was a once in a lifetime opportunity, they said. The black disk of the second planet wouldn’t crawl across the face of the sun again for more than 100 years.
In fact, it’s happening again this week–not on Earth, but Saturn.
“On Friday, December 21st, there will be a transit of Venus visible from Saturn, and we will be watching it using the Cassini spacecraft,” says Phil Nicholson, a Cassini science team member from Cornell University. “This will be the first time a transit of Venus has been observed from deep space.”
 A transit of Venus seen from Earth on June 6th, 2012. (Photo credit: Bum-Suk Yeom of Daejeon, South Korea)
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NASA’s Cassini spacecraft takes image of River on Saturn’s Moon Titan that looks like Earth’s Nile River
December 16, 2012 |
Written by Jia-Rui Cook
NASA’s Jet Propulsion Laboratory
Pasadena, CA – Scientists with NASA’s Cassini mission have spotted what appears to be a miniature, extraterrestrial likeness of Earth’s Nile River: a river valley on Saturn’s moon Titan that stretches more than 200 miles (400 kilometers) from its “headwaters” to a large sea.
It is the first time images have revealed a river system this vast and in such high resolution anywhere other than Earth.
 This image from NASA’s Cassini spacecraft shows a vast river system on Saturn’s moon Titan. It is the first time images from space have revealed a river system so vast and in such high resolution anywhere other than Earth. (Image Credit: NASA/JPL-Caltech/ASI)
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