ESAESA ScienceCassini-Huygens
   
Unique insights into a ringed world
About Cassini-Huygens
About Saturn
About Titan
Meet the team
Multimedia
VideoTalkCassini-Huygens imagesCassini-Huygens videosTitan virtual tourHygens probe descent - multilingual CD-romDownload wallpapersDownload screensavers3D Flash 'model'SOI animationWaiting for Titan - the human side of Huygens
Watch the event
Services
Comments
 
 
 
 
Article Images
New images from Titan
 
15 January 2005

Download:
 HI-RES PNG (Size: 213 kb)  HI-RES TIFF (Size: 1117 kb)
This image was returned on 14 January 2005, by ESA's Huygens probe during its successful descent to land on Titan. This is the colour view, following processing to add reflection spectra data, gives a better indication of the actual colour of the surface. Initially thought to be rocks or ice blocks, they are more pebble-sized. The two rock-like objects just below the middle of the image are about 15 centimetres (left) and 4 centimetres (centre) across respectively, at a distance of about 85 centimetres from Huygens. The surface is darker than originally expected, consisting of a mixture of water and hydrocarbon ice. There is also evidence of erosion at the base of these objects, indicating possible fluvial activity.

Credits: ESA/NASA/JPL/University of Arizona
 
 
Download:
 HI-RES PNG (Size: 386 kb)  HI-RES TIFF (Size: 807 kb)
This raw image was returned yesterday, 14 January 2005, by ESA's Huygens probe during its successful descent to land on Titan. Sizes have been added to indicate scale of these features. Initially thought to be rocks or ice blocks, they are more pebble-sized. The two rock-like objects just below the middle of the image are about 15 centimetres (left) and 4 centimetres (centre) across respectively, at a distance of about 85 centimetres from Huygens. The surface is darker than originally expected, consisting of a mixture of water and hydrocarbon ice. There is also evidence of erosion at the base of these objects, indicating possible fluvial activity.

Credits: ESA/NASA/JPL/University of Arizona

Credits: ESA/NASA/JPL/University of Arizona

 
 
Huygens' view of Titan
Download:
 HI-RES JPEG (Size: 10 kb)  HI-RES TIFF (Size: 88 kb)
This composite was produced from images returned on 14 January 2005, by ESA's Huygens probe during its successful descent to land on Titan. It shows the boundary between the lighter-coloured uplifted terrain, marked with what appear to be drainage channels, and darker lower areas. These images were taken from an altitude of about 8 kilometres with a resolution of about 20 metres per pixel.

Credits: ESA/NASA/JPL/University of Arizona
 
 
Download:
 HI-RES JPEG (Size: 167 kb)  HI-RES TIFF (Size: 377 kb)
This composite was produced from images returned yesterday, 14 January 2005, by ESA's Huygens probe during its successful descent to land on Titan. It shows a full 360-degree view around Huygens. The left-hand side, behind Huygens, shows a boundary between light and dark areas. The white streaks seen near this boundary could be ground 'fog' of methane or ethane vapour, as they were not immediately visible from higher altitudes. As the probe descended, it drifted over a plateau (centre of image) and was heading towards its landing site in a dark area (right). This dark area is possibly a drainage channel which might still contain liquid material. From the drift of the probe, the wind speed has been estimated at around 6-7 metres per second. These images were taken from an altitude of about 8 kilometres with a resolution of about 20 metres per pixel.

Credits: ESA/NASA/JPL/University of Arizona
 


At Saturn and Titan
At Saturn and TitanViews on approach to Saturn
Huygens raw images
First image of Titan
Sounds of Titan
Related articles
Huygens lands in Titanian mudView from ten kilometres highFirst images from TitanEurope reaches new frontier – Huygens lands on TitanRadio astronomers confirm Huygens entry in the atmosphere of Titan
Related links
NASA JPL Cassini-Huygens siteItalian Space Agency (ASI)
 
 
 
   Copyright 2000 - 2010 © European Space Agency. All rights reserved.