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TOPIC: Titan


L

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This image of Titan was taken by the Cassini space probe was taken on July 03, 2006 when it was approximately 159,843 kilometres away.

N00063422

The image was taken using the CL1 and CB3 filters.

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L

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This image of Titan was taken by the Cassini space probe was taken on July 03, 2006 when it was approximately 164,203 kilometres away.

N00063416

The image was taken using the CL1 and CB3 filters.

-- Edited by Blobrana at 13:45, 2006-07-04

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L

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This image of Titan was taken by the Cassini space probe was taken on July 02, 2006 when it was approximately 160,785 kilometres away.

W00015736

The image was taken using the CL3 and CL2 filters.


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L

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This image of Titan was taken by the Cassini space probe was taken on July 02, 2006 when it was approximately 183,007 kilometres away.

N00063394

The image was taken using the CL1 and CB3 filters.

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Two years after reaching Saturn, the Cassini spacecraft is halfway to completing its orbital mission.
On July 2, Cassini will perform its 16th flyby of Saturn's largest moon, Titan, at an altitude of 1,906 kms.
Cassini will focus on the interactions between Titan's atmosphere and the magnetosphere that surrounds Saturn. Cassini will also study Titan's surface to enable a better understanding of its properties and composition.

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L

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What happened to Titan's craters? NASA's Cassini mission should have seen hundreds of impact craters on Saturn's giant moon, but so far it has only spotted a handful.
The latest clues in the mystery of the missing craters suggest a conspiracy between volcanoes, rain and settling soot - perhaps aided by an eggshell-thin crust.

Recent radar views of Saturn's moon Titan from the close flyby of the Cassini probe shows a striking variety of surface structures, including a first glimpse of craters formed by meteors.
A team led by Steve Wall of NASA's Jet Propulsion Laboratory in Pasadena, California, says it is surprising there are so few craters, compared with the pock-marked face of the bare, icy Saturnian moon Rhea.
Wall and colleagues conclude Titan's surface is either geologically active -- so outflows of material from 'cold volcanoes' have covered traces of old craters -- or it has such a thin icy crust over softer material that the craters flatten like dents in soft sand and then become covered by dust.
As well as two craters of 280 and 50 miles across, the new images of Titan show a range of other features.
The Cassini spacecraft's imaged a long strip of Titan's surface, reaching from high in the southern hemisphere to high in the northern during its third close fly-by of Titan. Cassini passed only about 1,000 miles above the surface, showing features as small as a few hundred feet across.
The study appears in this week's issue of the journal Nature.

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L

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This image of Titan was taken by the Cassini space probe on June 02, 2006, when it was approximately 2,342,944 kilometres away.

N00062243
Credit NASA

The image was taken using the CL1 and CL2 filters.

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L

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This image of Titan was taken by the Cassini spaceprobe on May 20, 2006 when it was approximately 55,989 kilometres away.

W00015211

The image was taken using the CB3 and CL2 filters.

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L

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This image of Titan was taken by the Cassini spaceprobe on May 18, 2006 when it was approximately 1,177,940 kilometres away.

N00061620

The image was taken using the IRP0 and CB3 filters.

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L

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This image was taken with the Cassini Synthetic Aperture Radar instrument on Oct. 28, 2005.

This was the fourth flyby of Titan during which radar images were obtained, and this pass considerably expanded the coverage of Titan's surface.
The swath is about 6,150 kilometres long, extending from 7 degrees north to 18 degrees south latitude and 179 west to 320 west longitude.


Expand (1.68mb, 7218 x 766)
Credit NASA/JPL

The spatial resolution of the radar images ranges from about 300 meters per pixel to about 1.5 kilometres per pixel. It covers the area where the Huygens probe landed (eastern end of the swath), giving geologic context for the landing site.
The most ubiquitous features in this swath are "cat scratches," which are interpreted as longitudinal dunes and were first seen in the February 2005 flyby.

Also prominent are long, bright ridges, concentrated near the eastern end of the swath. These may be tectonic in origin, and are seen for the first time here. No impact craters are seen, indicating a young surface.

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