Titan | Universe Today

New images of Titan's surface from the Cassini spacecraft show changes which are evidence of seasonal change. Objects identified earlier as liquid hydrocarbon lakes are shrinking and disappearing over the course of one to several Earth years. Scientists say seasonal temperature variations causing evaporation is the most likely cause for the changes observed. Cassini's Synthetic Aperture Radar (SAR) repeatedly peered through Titan's thick atmosphere, and data show that the lakes exhibit more than an order of magnitude increase in radar return and have disappearing borders between observations, suggesting surface change. These changes cannot be explained without invoking temporal variability, scientists reported at the American Astronomical Society's Division for Planetary Sciences meeting now under way in Fajardo, Puerto Rico.
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Titan appears to be more like Earth all the time, and a new understanding of Titan's hazy atmosphere could provide clues to the evolution of Earth's early atmospheric environment and the development of life on our home planet. Researchers have discovered a series of chemical reactions on Saturn’s largest moon that may shield the moon’s surface from ultraviolet radiation, similar to how Earth’s ozone layer works. The reactions may also be responsible for forming the large organic molecules that compose the moon’s thick and hazy orange atmosphere.
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Titan is the only place in the solar system other than the earth that appears to have large quantities of liquid sitting on the surface. Granted, conditions on Titan are quite different than on Earth. For one thing, it's a lot colder on Titan and the liquids there are various types of hydrocarbons. "Methane is to Titan what water is to the earth," says astronomer Mike Brown (yes, that guy, of Pluto, Eris and Makemake fame.) But now Brown and his colleagues have discovered another similarity. Titan has fog. "All of those bright sparkly reddish white patches (shown in the image here) are fog banks hanging out at the surface in Titan's late southern summer," Brown wrote in his blog.

Wow.
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Titan is just fun. Seems like every other week, another fascinating tidbit emerges about how interesting Saturn's famous moon really is — and how compellingly similar to Earth.

A United States team of astronomers is releasing this image today in Nature. It's an adaptive optics peek at a storm over the wild object's parched, dry desert.

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It's more than a billion kilometers (759 million miles) away, but the more astronomers learn about Titan, the more it looks like Earth.

That's the theme of two talks happening this week at the International Astronomical Union meeting in Rio de Janeiro, Brazil. Two NASA researchers, Rosaly Lopes and Robert M. Nelson of the Jet Propulsion Laboratory in Pasadena, California, are reporting that weather and geology have very similar actions on Earth and Titan — even though Saturn's moon is, on average, 100 degrees C (212 degrees F) colder than Antarctica (and certainly much more frigid than either California or Brazil; lucky astronomers).

The researchers are also reporting a tantalizing clue in the search for life: Titan hosts chemistry much like pre-biotic conditions on Earth.

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Titan's mysterious dark plains will be named after planets in the series of "Dune" science fiction novels by author Frank Herbert. The US Geological Survey Astrogeology Science Center announced the first plain or "planitia" given a name will be designated as Chusuk Planitia. Chusuk was a planet from the Dune series, known for its musical instruments. Chusuk Planitia on Titan is located at 5.0S, 23.5W, and in the picture here is the small, dark area next to the "C" of Chusuk.
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Looking to go somewhere far-flung and exotic? Now is the time to book your excursion, and the Cassini spacecraft has several flyby tours of the moons Titan and Enceladus scheduled for the next few months. Major tour operators say the cost of long-haul flights and summer holidays prices are at an all time low. But with Cassini, you can travel for FREE! just by following the along with Universe Today and the Cassini website. Thrill with some of the closest flybys ever of the mystery moon Titan, and delight in explorations of the geyser plumes of Enceladus. As a special bonus, if you book today, you can experience Saturn's solar equinox, as in August the sun crosses from the southern hemisphere to the north. Wonderful worlds are beckoning – come away starting June 6 with Cassini! It's a worry free vacation. See below for available tour dates! Destination fees do not apply.
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Think Titan looks pretty round?

Not quite, according to new data released today by the Cassini radar team — and slight irregularities in the shape of the bizarre moon may account for the concentration of lakes at the highest latitudes, among other perplexing features. 

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Hang on, and enjoy a virtual flyover of Saturn's moon Titan! Data from Cassini's radar instrument have been used to create new flyover maps of Saturn's largest moon. The maps show the topography of Titan in 3-D, and illustrating the height of the 1,200-meter (4,000-foot) mountain tops, the north polar lake country, the vast dunes more than 100 meters (300 feet) high that crisscross the moon, and the thick flows that may have oozed from possible ice volcanoes. "These flyovers let you take in the bird's-eye sweeping views of Titan, the next best thing to being there," said Randy Kirk, from the Science Center at the U.S. Geological Survey, who created the maps.. "We've mapped many kinds of features, and some of them remind me of Earth. Big seas, small lakes, rivers, dry river channels, mountains and sand dunes with hills poking out of them, lava flows." Click the image above to see one of the movies.
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Once every 15 years, Saturn flashes its paper-thin rings in edge-on formation relative to Earth. 

Because the orbits of Saturn's major satellites are in the ring plane, too, this alignment gives astronomers a rare opportunity to capture a spectacular parade of celestial bodies crossing Saturn's surface.

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Scientists have mapped vast dune fields on Titan that may align with the wind on Saturn’s biggest moon — flowing opposite the way climate models had predicted.

The maps, as above, represent four years of radar data collected by the Cassini spacecraft. They reveal rippled dunes that are generally oriented east-west, which means Titan’s winds probably blow toward the east instead of the west. If so, Titan’s surface winds blow opposite the direction suggested by previous global circulation models. On the example above, the arrows indicate the general wind direction. The dark areas without arrows might have dunes but have not yet been imaged. 

“At Titan there are very few clouds, so determining which way the wind blows is not an easy thing, but by tracking the direction in which Titan’s sand dunes form, we get some insight into the global wind pattern,” says Ralph Lorenz, Cassini radar scientist at Johns Hopkins University in Maryland. “Think of the dunes sort of like a weather vane, pointing us to the direction the winds are blowing.”

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At a meeting last week between NASA and ESA, the two space agencies narrowed down the choices for the next big flagship planetary missons, which will be joint efforts between the US and Europe. A mission to Jupiter and its four largest moons will be the primary mission the two space agencies will focus on, while they continue to plan for another potential mission to visit Saturn's largest moon Titan and Enceladus. The two missions, the Jupiter System Mission and the Titan Saturn System Mission, are the result of NASA and ESA merging their separate mission concepts.
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Recent pictures from the Cassini spacecraft of Titan's south polar region reveal new lake features not seen in images of the same region taken a year earlier. Extensive cloud systems seen in images covering the area during past year suggest that the new lakes could be the result of a large rainstorm and that lakes on Titan owe their presence, size and distribution to the moon’s weather and changing seasons. But there must also be large underground reservoirs as well of the liquids on Titan. Those liquids aren't water, of course, but super-cold hydrocarbons like methane.
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This is perhaps the coolest thing I've ever seen. Ray Villard, the news director for the Hubble Space Telescope, also writes a blog for Discovery called Cosmic Ray (love that name!) He recently wrote about a dragonfly-like robotic device being developed by the Technical University Delft, Wageningen University in the Netherlands. It's call the ExoFly, and Ray described it as a "dragonfly-on-steroids … a nimble flapping aerobot." It could be the next generation of robotic planetary explorers. It's a small, lightweight autonomous machine capable of flying, hovering, landing and taking off like an insect. Ray says this type of vehicle would "open up a new exploration niches that it not easily reachable by rovers or airborne vehicles on far flung worlds." Actually, it might work best in conjunction with a future big rover, flying ahead to search for interesting or dangerous terrain, and the rover would provide a "landing pad" for the ExoFly's home base. While the ExoFly may be small, its name sounds like a potential super hero, and its capabilities could be in the exploration super hero category, as well.

Take a look at the incredible video of the ExoFly below:
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While browsing through Cassini images of Saturn's moon Titan, astronomer Mike Brown and some colleagues noticed a recurring pattern of clouds appearing over the frigid moon's north pole. While a large, stable cloud has been visible in every image of Titan's north pole obtained since its discovery, Brown noticed bright "knots or streaks" in the cloud that appeared on some images but not others, or changed in images taken hours apart. Brown thought these bright features looked similar to cumulus clouds – or even like thunderheads. But how could tropical-like thunderheads be present on a moon where surface temperatures hover around -178°C (-289°F)? Brown believes these clouds are similar to winter-time lake-effect clouds found on Earth, and are due to convection and condensation occurring in the methane and ethane lakes on Titan.
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