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Jarosite in the Noctis Labyrinthus Region of Mars | NASA MRO Light toned layered pit depression on surface of Mars This image, acquired on Nov. 24, 2015 by the High Resolution Imaging Science Experiment (HiRISE) camera aboard NASA's Mars Reconnaissance Orbiter, shows the western side of an elongated pit depression in the eastern Noctis Labyrinthus region of Mars. Along the pit's upper wall is a light-toned layered deposit. Noctis Labyrinthus is a huge region of tectonically controlled…

Jarosite in the Noctis Labyrinthus Region of Mars

Toro Crater, Mars - The different colors reflect different mineral composition on the Martian surface. (Taken 12/1/11 by the High Resolution Imaging Science Experiment on NASA's Mars Reconnaissance Orbiter).

Toro Crater, Mars - The different colors reflect different mineral composition on the Martian surface. (Taken by the High Resolution Imaging Science Experiment on NASA's Mars Reconnaissance Orbiter).

A piece of Mars: Wind ha blown the dark, rippled sand between jagged hills, from top to bottom in this frame (663 m or 2175 ft across). Regardless of the terrain, sand finds a way to get through -- just like at the beach, it manages to get everywhere. (HiRISE ESP_037494_1685, NASA/JPL/Univ. of Arizona)

In this image, SETI Institute’s Lori Fenton explains that wind has blown the dark, rippled sand between jagged Martian hills, from top to bottom in this frame

Hebes Chasma : Este abismo marciano, mais de 4 vezes mais largas e profundas como o Grand Canyon , é um fechado , quase 8 km ( 4,97 milhas ) cocho -Deep alongamento 315 km ( 195,73 milhas ) em uma direção leste-oeste e 125 km ( 77,67 milhas ) de norte a sul em seu ponto mais largo. Ele fica a cerca de 300 km ( 186,41 milhas ) ao norte da grande canyon Valles Marineris .

Hebes Chasm on Mars. It forms a giant trough nearly miles km) deep, of Valles Marineris, the largest canyon system in the solar system. Taken with the High Resolution Stereo Camera on Mars Express.

The Syrtis Major Volcanic Province. Acquired by the High Resolution Stereo Camera on ESA’s Mars Express Satellite, this image depicts a detailed region of the Martian Nili Fossae Graben system. This system is an area of great interest to geologists due to the variety of its landscape. The graben system contains numerous troughs, plateaus, impact craters and depressions.

The Syrtis Major Volcanic Province - The Martian Surface Acquired by the High Resolution Stereo Camera on ESA’s Mars Express Satellite, this image depicts a detailed region of the Martian Nili Fossae Graben system. This system is an area of great.

The north polar cap of Mars, with water ice clouds sweeping over the plains of Vastitas Borealis. The ice cap spans roughly 1000 kilometers. Observed by the Mars Express orbiter in May 2014.

ESA / DLR / FU Berlin / Bill Dunford Clouds Over the North The north polar cap of Mars, with water ice clouds sweeping over the plains of Vastitas Borealis. The ice cap spans roughly 1000 kilometers. Observed by the Mars Express orbiter in May

Enhanced color image of a hill in the Candor Colles region of #CandorChasma, #Mars.

Long ago, in the largest canyon system in our solar system, vibrations from "marsquakes" shook soft sediments that had accumulated in Martian lakes.