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Tropics of Saturn’s Moon Titan No Tropical Paradise On Some Days

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(Above) This image of Titan shows data taken with Cassini’s visual and infrared mapping spectrometer during the last three flybys of Titan.

Astronomers have identified a storm cell on Titan the size of the country of India. The storm system appeared in April 2008 in the moon’s tropical region, an area not known for its cloudiness.

Using the Gemini North Telescope and NASA Infrared Telescope Facility on Hawaii’s Mauna Kea volcano, a team of astronomers from the University of Hawaii, the Lowell Observatory, and the California Institute of Technology found a significant mass of methane clouds in a cold desert area where no clouds were expected.

Large cloud outbursts such as these are thought to be associated with significant amounts of precipitation and probably play a major part in shaping the geological features on the surface of Titan..

The paper, “Storms in the tropics of Titan,” appears in the August 13 issue of Nature.


Revelations in Saturn’s Rings Continue as Equinox Approaches

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(Above) The Cassini spacecraft captured this image of a small object in the outer portion of Saturn’s B ring casting a shadow on the rings as Saturn approaches its August 2009 equinox.

Thanks to a special play of sunlight and shadow as Saturn continues its march towards its August 11 equinox, recent images captured by NASA’s Cassini spacecraft are revealing new three-dimensional objects and structures in the planet’s otherwise flat rings. The Cassini spacecraft captured this image of a small object in the outer portion of Saturn’s B ring casting a shadow on the rings as Saturn approaches its August 2009 equinox.

This new moonlet, situated about 300 miles (480 kilometers), inward from the outer edge of the B ring, was found by detection of its shadow which stretches 25 miles, or 41 kilometers, across the rings. The shadow length implies the moonlet is protruding about 660 feet, or 200 meters, above the ring plane. If the moonlet is orbiting in the same plane as the ring material surrounding it, which is likely, it must be about 1,300 feet, or 400 meters, across. This object is not attended by a propeller feature, unlike the band of moonlets discovered in Saturn’s A ring earlier by Cassini. The A ring moonlets, which have not been directly imaged, were found because of the propeller-like narrow gaps on either side of them that they create as they orbit within the rings. The lack of a propeller feature surrounding the new moonlet is likely because the B ring is dense, and the ring material in a dense ring would be expected to fill in any gaps around the moonlet more quickly than in a less dense region like the mid-A ring. Also, it may simply be harder in the first place for a moonlet to create propeller-like gaps in a dense ring.

The search for three-dimensional structures in Saturn’s rings has been a major goal of the imaging team during Cassini’s “Equinox Mission,” the two-year period containing exact equinox — that moment when the sun is seen directly overhead at noon at the planet’s equator. This novel illumination geometry, which occurs every half-Saturn-year, or about 15 Earth years, lowers the sun’s angle to the ring plane and causes out-of-plane structures to cast long shadows across the rings’ broad expanse, making them easy to detect.


Tiny Saturn Moon Could Be Targeted in Search for ET Life

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(Above) Cassini imaging scientists used views like this one to help them identify the source locations for individual jets spurting ice particles, water vapor and trace organic compounds from the surface of Saturn’s moon Enceladus.

Plumes spewing from a tiny moon of Saturn – a moon roughly the width of Arizona – are filled with molecules that suggest that the moon, Enceladus, is likely another place in the solar system to look for life, Cassini scientist Jonathan Lunine of The University of Arizona Lunar and Planetary Laboratory said.

When NASA’s Cassini spacecraft flew through a plume erupting from Enceladus early last October, its Ion and Neutral Mass Spectrometer instrument measured ammonia, argon 40 and an abundance of carbon-bearing molecules, or “organics,” entrained in the water vapor.

Lunine is on the team reporting the results in the July 23 issue of the journal Nature.

Cassini discovered water vapor and particles spewing from Enceladus in a previous, more distant flyby in 2005. Since then, scientists have been trying to determine if the source of the jets is liquid.

“The fact that there’s ammonia on Enceladus is important because it argues the plumes are erupting from a region of liquid water beneath the surface of Enceladus, rather than erupting from what is just warm ice,” Lunine said.

Ammonia acts as antifreeze. Water containing ammonia remains liquid at temperatures as low as minus 143 degrees Fahrenheit.

Cassini has measured temperatures higher than minus 136 degrees Fahrenheit near the fractures where Enceladus shoots out its water vapor plumes, so “We think we have an excellent argument for a liquid water interior,” said Hunter Waite of the Southwest Research Institute in San Antonio, Texas, lead scientist for Cassini’s Ion and Neutral Mass Spectrometer experiment.

Argon 40, an isotope of argon, which is a decay product of potassium, also strengthens the argument for a liquid water source, Lunine said. Rocks on Earth and elsewhere, including Saturn’s giant moon Titan, give off argon 40.

“The fact that we found a lot of argon 40 also argues for liquid water,” Lunine said. Liquid water most likely circulating through Enceladus’ rocky core is the best explanation for all the argon 40 detected, he said.

The Cassini team also discovered such carbon-bearing molecules as methane, formaldehyde, ethanol and hydrocarbons are plentiful in the plumes.

Given other recently reported Cassini evidence for sodium and potassium in Saturn’s E ring – a ring made of material that comes from Enceladus, there must be a salty, liquid layer in Enceladus that “seems like a pretty good environment for life,” Lunine said.

“What I think is really interesting now is that we have four places in the outer solar system with interior oceans,” he said.

Scientists have evidence that Saturn’s Titan and Jupiter’s moons Europa and Ganymede also have oceans.

Mars, Titan, Europa and now Enceladus seem to be good sites to search for extraterrestrial life, Lunine added.


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