News on Saturn
- The small Saturn-moon Phoebe looks more like a failed planet than a moon
- The origin and age of Titans atmosphere
- Saturns constantly changing F-ring
- Lakes on Titan is like a Namibia mudflat
- Historic clase-encounter with Saturn-moon Tethys
- Measurments of Saturns Aurora and magnetic field
- Saturn streches teh surface on its moon Enceladus
- New amazing images of ice-moon Rhea
- Discovery of thin oxygen atmosphere around Dione
- Titans changing wheather
- Cassini's closest Dione flyby
- The vast sand-dune plains on Titan
- The making of Saturns rings
- The shepparding moons
- Is Titans climate stable?
- Now model explains Titans lakes and storms
- Bad wheather on saturn-moon Titan
- Saturn moon may affect planet's magnetosphere
- Alignment of Saturnian moons
- Cassini only 99km over Saturn-moon Dione
- Cassiini to make 2 close moon-flybys in 1 day
- New higher resolution images of Saturn-moon Enceladus
- Saturns interplanetary dust-storm
- Satirns giant storm has lasted 200 days
- Comets gave Titan atmosphere
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Spring on Titan
Thursday, 23 September 2010 11:52
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| Solar system - Saturn |
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The northern hemisphere of Saturn's moon Titan is set for mainly fine spring weather, with polar skies clearing since the equinox in August last year.
A group led by Sébastien Rodriguez, a Cassini VIMS team collaborator based at Université Paris Diderot, France, has analyzed more than 2,000 VIMS (visual and infrared mapping spectrometer) images to create the first long-term study of Titan's weather using observational data that also includes the equinox. Equinox is when the sun shines directly over the equator, and it occurred in Aug. 2009.
Rodriguez is presenting the results and new images at the European Planetary Science Congress in Rome on Sept. 22. Though Titan's surface is far colder and lacks liquid water, this moon is a kind of "sister world" to Earth because it has a surface covered with organic material and an atmosphere whose chemical composition harkens back to an early Earth. Titan has a hydrological cycle similar to Earth's, though Titan's cycle depends on methane and ethane rather than water. A season on Titan lasts about seven Earth years. Rodriguez and colleagues observed significant atmospheric changes between July 2004 (early summer in Titan's southern hemisphere) and April 2010 (the start of northern spring). The images showed that cloud activity has recently decreased near both of Titan's poles. These regions had been heavily overcast during the late southern summer until 2008, a few months before the equinox. Over the past six years, the scientists found that clouds clustered in three distinct latitude regions of Titan: large clouds at the north pole, patchy clouds at the south pole and a narrow belt around 40 degrees south. "However, we are now seeing evidence of a seasonal circulation turnover on Titan – the clouds at the south pole completely disappeared just before the equinox and the clouds in the north are thinning out," Rodriguez said. "This agrees with predictions from models and we are expecting to see cloud activity reverse from one hemisphere to another in the coming decade as southern winter approaches."
Source: The Cassini homepage |





