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Kasei Valles

Kasei Valles is one of the largest outflow channel systems on Mars that was created by several gigantic flood events over 3 billion years ago.

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Asteroid Vesta

The asteroid Vesta is the third largest body in the asteroid belt (with dimensions of 280 x 270 x 230 kilometer) and one of a few relicts from early times of the solar system.

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Dao and Niger Valles

This complex outflow-channel system on Mars is up to 40 km wide in places. The northern Dao Vallis is about 2400 m deep, the southern Niger Vallis about 1400 m.

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Ulyxis Rupes

Ulyxis Rupes is located in the southern highlands of our neighbour planet Mars. There are many ice deposits and dune formations in this area.

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Valles Marineris

This animation shows a fly-over of the central region of the vast canyon system Valles Marineris, a significant geological structure on Mars.

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Saturnian moon Iapetus

This animation shows a small part of the massive equatorial ridge on Iapetus. The ridge encircles the Saturnian moon along the equator.

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Mawrth Vallis

This large outflow channel is situated north of the Martian dichotomy boundary between the southern highland and the northern lowland.

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Impact crater Nicholson

Nicholson Crater is located northwest of a region called Medusae Fossae on Mars. In the centre of this crater an oblong massif rises around 3.5 km above the floor.