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TOPIC: Titan


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RE: Titan
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This radar image shows the entire scene in which hydrocarbon lakes were first discovered on Titan, near its north pole (see Lakes on Titan). This image was acquired on July 22, 2006, by Cassini's radar instrument in synthetic aperture mode.

TITAN09112
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Credit NASA

The most striking landforms are the lakes: dark patches, some circular, some irregular, many with apparently steep rims, over much of the terrain north of 70 degrees latitude. The most convincing lake forms occur at the narrowest, central part of the scene, which is at the highest latitudes. Here they have short, stubby channels leading into them, and brighter areas within that indicate either dried-up lakes or that we are seeing through a transparent liquid.
The image also shows the considerable variation in the kinds of surface features found at different latitudes. Beginning at the left (20 degrees north by 142 degrees west) and heading north, a circular feature about 75 kilometres in diameter is seen, which could be either an impact crater or a volcanic caldera. Other less distinct circular forms are seen next, possibly including some dried lakes, followed by some ridge-like terrain with dark meandering channels or valleys. The dark lakes begin to appear next (at about 70 degrees north), with more distinct lakes in the middle of the scene, where the swath is closest to the pole and starts to descend to the south. Farther on, apparently dry lakes and canyons begin to dominate, and the region becomes more complex and etched. At the extreme right end, dunes similar to those seen previously mingle with brighter features. The swath ends at 13 degrees north by 347 degrees west.

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This pair of images, taken by the Cassini spacecraft radar mapper on two different Titan passes on Dec. 11, 2006 (T21 left), and Oct. 29, 2005 (T8 right), represent two different views of a field of dunes located near 9.4 degrees south latitude by 290 degrees west longitude.

titan9111
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Credit: NASA/JPL

The images were taken in synthetic aperture mode and have a resolution of approximately 500 metres. North is toward the top of both images, and each image is approximately 400 kilometres long by 275 kilometres wide. The images are different only because the radar instrument illuminated the dunes from different directions. Acting somewhat like a flash camera, the radar sends out microwave pulses and makes an image from the pulses after they are reflected back. Imagine that both the ¿camera¿ and the ¿flash¿ come from the left in the left image and from the top in the right image.
Most obvious differences are seen in the large bright feature at the centre of both images. At left, its left edge is brighter, emphasizing the more steep slopes there. Farther left, the dunes are more clearly defined in the right image as their faces are caught by the illumination. However, since the dunes are visible in both images, it is likely that the materials making up the dark and light stripes are also somehow different. More detailed studies of how materials on Titan reflect and scatter at different angles are giving us clues about what different materials might be present in this cold and distant world.

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T23
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T23, January 13th, Titan flyby details are now available.

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titan09102_lake
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NASA/JPL/Space Science Institute

This radar image was acquired by the Cassini radar instrument in synthetic aperture mode on July 22, 2006. The image is centred near 80 degrees north, 35 degrees west and is about 140 kilometres across. Smallest details in this image are about 500 metres across.

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Scientists report definitive evidence of the presence of lakes filled with liquid methane on Saturn's moon Titan in this week's journal Nature cover story.
Radar imaging data from a July 22, 2006, flyby provide convincing evidence for large bodies of liquid on Titan today. A new false-colour radar view gives a taste of what Cassini saw. Some highlights of the article follow below.

Titan lakes
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Credit: NASA/JPL/USGS

This radar image was acquired by the Cassini radar instrument in synthetic aperture mode on July 22, 2006. The image is centred near 80 degrees north, 35 degrees west and is about 140 kilometres across. Smallest details in this image are about 500 metres across.

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Titan's lakes revealed
The existence of oceans or lakes of liquid methane on Saturn's moon Titan was predicted more than twenty years ago. But with a dense haze preventing a closer look, it has not been possible to confirm their presence. Until the Cassini flyby of 22 July 2006 that is. Radar imaging data from the flyby, published this week, provide convincing evidence for large bodies of liquid. The cover gives a taste of what Cassini saw. Intensity in this image (colourised — though not as a representation of what the human eye would see) is proportional to the logarithm of radar backscatter cross-section. The lakes, darker than the surrounding terrain, are emphasized here by tinting regions of low backscatter blue and radar-brighter regions tan. The strip of radar imagery is about 140 km wide, and is foreshortened to simulate an oblique view of the highest latitude region, seen from a point to its west.

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This image of Titan was taken by the Cassini spaceprobe on December 31, 2006, when it was approximately 1,232,479 kilometres away.

titan74331
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Credit: NASA/JPL/Space Science Institute

The image was taken using the CL1 and CB3 filters.

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This image of Titan was taken by the Cassini spaceprobe on December 28, 2006, when it was approximately 30,108 kilometres away.

Titan21079
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Credit: NASA/JPL/Space Science Institute

The image was taken using the CB3 and CL2 filters.

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As Cassini continues its flybys of Titan, the imaging science team continues to improve its ability to tease out surface details hidden in the unprocessed images. This mosaic provides the best view yet obtained by Cassini's cameras, showing terrain on the moon's sub-Saturn hemisphere -- the side of the moon that always faces toward Saturn.
This mosaic has better resolution, both in pixel scale and from improved signal-to-noise, compared to previous views of the area.

PIA08352b
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Credit: NASA/JPL/Space Science Institute

The view is centred on terrain in the Fensal-Aztlan region on Titan, at 0.03 degrees south latitude, 22.18 degrees west longitude. The mosaic covers an area 3,500 kilometres north to south and 3,600 kilometres west to east. North is up.
The mosaic consists of 17 frames taken using a spectral filter sensitive to wavelengths of infrared light centred at 938 nanometers.
The images in this mosaic were taken using the Cassini spacecraft narrow-angle camera at distances ranging from 81,200 to 119,500 kilometres and at a sun-Titan-spacecraft, or phase, angle of about 25 degrees. The original image scale ranged from 470 to 700 metres per pixel. Because the actual resolution on Titan is a few times the pixel scale, this orthographic projection mosaic was scaled to 1 kilometre per pixel.

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Map of Titan
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This global digital map of Titan was created using data taken by the Cassini spacecraft Imaging Science Subsystem (ISS). The data here consist of images taken using a filter centred at 938 nanometres, allowing researchers to examine albedo (or inherent brightness) variations across the surface of Titan. Due to the scattering of light by Titan's dense atmosphere, no topographic shading is visible in these images.
The map is an equidistant projection and has a scale of 2 kilometres per pixel. Equidistant projections preserve distances on a body, with some distortion of area and direction. Actual resolution varies greatly across the map, with the best coverage near the centre and edges of the map and the worst coverage on the trailing hemisphere (centred around 270 degrees west longitude).

TitanMAP
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Credit: NASA/JPL/Space Science Institute

The mean radius of Titan used for projection of this map is 2,575 kilometres.

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