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Mars' valleys and volcanoes

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This image, taken by the High Resolution Stereo Camera (HRSC) on board ESA’s Mars Express spacecraft, shows Crater Hale in the Argyre basin of the southern hemisphere of Mars.

The image is centred at latitude 36° South and longitude 324° East. The image was taken with a ground resolution of about 40 metres per pixel during Mars Express orbit 533 in June 2004.

Crater Hale, with its terraced walls, central peak and a part of the inner ring is visible in the upper (eastern) part of the image.

Credits: ESA/DLR/FU Berlin (G. Neukum)
On 2 May 2004, the High-Resolution Stereo Camera (HRSC) on board the ESA Mars Express spacecraft obtained this image from the central area of the Valles Marineris canyon, called Melas Chasma.

This image was taken at a resolution of approximately 30 metres per pixel. The displayed region is located at the southern rim of the Melas Chasma, centred at Mars latitude 11° S and Mars longitude 286° E. The images were taken on orbit 360 of Mars Express.

This perspective view was created by using the nadir (vertical view) channel and one stereo channel of the HRSC to produce a digital model of the terrain. Please note that image resolution has been reduced for use on the internet.

Credits: ESA/DLR/FU Berlin (G. Neukum)
 
Credits: ESA/DLR/FU Berlin (G. Neukum)
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