Anaglyph image of Hebes Chasma
Anaglyph image of Hebes Chasma
Anaglyph images of the surface of Mars are produced using the nadir channel in the HRSC camera system, which is directed vertically down towards the planet surface, and one of the stereo channels aligned at an oblique angle. Red-blue (cyan) or red-green-blue spectacles create a three-dimensional impression of the landscape. The Hebes Chasma basin, almost eight kilometres deep, stretches 315 kilometres along a west-east direction and 125 kilometres from north to south. At its centre, the flat-topped mountain is around 100 kilometres long, some 8000 metres high, and varies in width between 10 and 20 kilometres.
Copyright note:
As a joint undertaking by DLR, ESA and FU Berlin, the Mars Express HRSC images are published under a Creative Commons licence since December 2014: ESA/DLR/FU Berlin, CC BY-SA 3.0 IGO. This licence will also apply to all HRSC images released to date.