 | | |
| | Mars Express reveals wind-blown deposits on Mars
3 February 2012
| Syrtis Major, discovered in 1659 by Christaan Huygens, is a volcanic province on Mars. The image is centred on approximately 16°N/73°E. The High-Resolution Stereo Camera (HRSC) on ESA’s Mars Express collected the data for this image on 8 June 2011 during orbit 9487. The image has a ground resolution of approximately 19 m per pixel. The image size is approximately 90x180 km.
Credits: ESA/DLR/FU Berlin (G. Neukum) | |  |  | |
| |
| | | A wider contextual image of Syrtis Major. The smaller rectangle shows the region covered in this Mars Express HRSC image release.
Credits: NASA MGS MOLA Science Team | | | | |
| |
| | | Syrtis Major is a volcanic province on Mars. This image from the High-Resolution Stereo Camera on ESA’s Mars Express orbiter shows lava flows in box 1. Filled craters and partly filled craters can be seen in box 2. The prevailing wind direction can be judged from the dispersal of the lighter-toned material. The smaller craters illustrate this clearly. The largest crater in the picture, highlighted in box 3, has a small central peak and contains a small dune field of darker-toned dunes. ESA’s Mars Express collected the data for this image on 8 June 2011 during orbit 9487. The image has a ground resolution of approximately 19 m per pixel.
Credits: ESA/DLR/FU Berlin (G. Neukum) | | | | |
| |
| | | Syrtis Major, discovered in 1659 by Christaan Huygens, is a volcanic province on Mars. The image is centred on approximately 16°N/73°E. The image was created using a Digital Terrain Model (DTM) obtained from the High-Resolution Stereo Camera on ESA’s Mars Express spacecraft. Elevation data from the DTM is colour coded: purple indicates the lowest-lying regions and grey the highest. The scale is in metres. The data for these images were collected on 8 June 2011 during orbit 9487. The images have a ground resolution of approximately 19 m per pixel.
Credits: ESA/DLR/FU Berlin (G. Neukum) | | | | |
| |
| | | Syrtis Major, discovered in 1659 by Christaan Huygens, is a volcanic province on Mars. The image is centred on approximately 16°N/73°E. The High-Resolution Stereo Camera on ESA’s Mars Express collected the data for these images on 8 June 2011 during orbit 9487. The images have a ground resolution of approximately 19 m per pixel. It was derived from the nadir channel, which provides the highest detail of all the channels.
Credits: ESA/DLR/FU Berlin (G. Neukum) | | | | |
| |
| | | Syrtis Major, discovered in 1659 by Christaan Huygens, is a volcanic province on Mars. The image is centred on approximately 16°N/73°E. The High-Resolution Stereo Camera on ESA’s Mars Express collected the data for these images on 8 June 2011 during orbit 9487. The images have a ground resolution of approximately 19 m per pixel. This perspective view has been calculated from the Digital Terrain Model derived from the stereo channels. Some ancient lava flow fronts are seen in the foreground and a lighter-toned butte is emerging on the right.
Credits: ESA/DLR/FU Berlin (G. Neukum) | | | | |
| |
| | | Syrtis Major, discovered in 1659 by Christaan Huygens, is a volcanic province on Mars. The image is centred on approximately 16°N/73°E. The High-Resolution Stereo Camera on ESA’s Mars Express collected the data for these images on 8 June 2011 during orbit 9487. The images have a ground resolution of approximately 19 m per pixel. This perspective view has been calculated from the Digital Terrain Model derived from the stereo channels. Some ancient lava flow fronts are seen in the foreground and a lighter-toned butte is emerging on the right.
Credits: ESA/DLR/FU Berlin (G. Neukum) | | | | |
| |
| | | Syrtis Major, discovered in 1659 by Christaan Huygens, is a volcanic province on Mars. The image is centred on approximately 16°N/73°E. The High-Resolution Stereo Camera on ESA’s Mars Express collected the data for these images on 8 June 2011 during orbit 9487. The images have a ground resolution of approximately 19 m per pixel. This perspective view has been calculated from the Digital Terrain Model derived from the stereo channels. Some ancient lava flow fronts are seen in the foreground and a lighter-toned butte is emerging on the right.
Credits: ESA/DLR/FU Berlin (G. Neukum) | | | | |
| |
| | | Syrtis Major, discovered in 1659 by Christaan Huygens, is a volcanic province on Mars. The image is centred on approximately 16°N/73°E. The High-Resolution Stereo Camera on ESA’s Mars Express collected the data for these images on 8 June 2011 during orbit 9487. The images have a ground resolution of approximately 19 m per pixel. This perspective view has been calculated from the Digital Terrain Model derived from the stereo channels. Some ancient lava flow fronts are seen in the foreground and a lighter-toned butte is emerging on the right.
Credits: ESA/DLR/FU Berlin (G. Neukum) | | | | |
| |
| | | Syrtis Major, discovered in 1659 by Christaan Huygens, is a volcanic province on Mars. The image is centred on approximately 16°N/73°E. The High-Resolution Stereo Camera on ESA’s Mars Express collected the data for these images on 8 June 2011 during orbit 9487. The image combines data from the nadir channel and one stereo channel to produce this 3D image. Stereoscopic glasses are required to see the 3D effect.
Credits: ESA/DLR/FU Berlin (G. Neukum) | | | | |
| |
Traces of Martian life
HI-RES JPEG (Size: 
HI-RES TIFF (Size: 
HI-RES JPEG (Size: 
HI-RES JPEG (Size: 
HI-RES JPEG (Size: 
HI-RES JPEG (Size: 
HI-RES JPEG (Size: 
HI-RES JPEG (Size: 
HI-RES JPEG (Size: 
HI-RES JPEG (Size: 
HI-RES JPEG (Size: