Fotografías || Isla de Gran Canaria

The Phlegra Dorsa region consists of ancient hills that have been surrounded and partially buried by flows from the Cerberus Fossae to the south.

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Central peaks on Mars have some of the most diverse and distinctive rock types.

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This image is of a region slightly to the southwest of where the MSL rover, called Curiosity, will land in August 2012.

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How did this folding occur? On Earth, rocks are commonly folded when deeply buried and subject to high heat and pressure, which can make any rock flow.

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The many large landslides inside Valles Marineris are well known, but there are also landslides elsewhere on Mars.

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This follow-up image to an earlier observation shows that the smaller dark tracks are gone, and the larger ones have faded considerably.

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These layered sediments are of great interest because they are very regular in thicknesses.

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The upper wall of the pit shows at least four distinct layers, each representing a sequence of one or more lava flows.

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This image covers the margin of a lava flow in Elysium Planitia, the youngest flood-lava province on Mars, and highlights terrain that resembles an elephant.

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The differing colors indicate different rock types of alteration. The darkest patches of ground probably consist of volcanic sand that is trapped in relative low areas.

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There are also bright lines present, representing the tracks of dust devils that have already passed through this region.

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West Candor Chasma in central Valles Marineris contains some of the thickest of the fine-grained layered deposits on Mars.

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The opening of Valles Marineris did involve crustal spreading and faulting, but may have had a more complex history.

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Every winter, dunes and other surfaces at these northern latitudes are coated with several tens of centimeters of carbon dioxide frost and ice, plus a minor amount of water frost.

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Gullies remain an interesting feature to study on Mars, especially because we are still learning about their formation and what processes still act on them.

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This observation was taken to investigate the topography near the source of fluids from the Cerberus Fossae fractures in the Elysium Planitia region of Mars.

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Structural features cut through the layered material and strata at this location. Could these features be faults or dikes?

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A dust devil the size of a terrestrial tornado towers above the Martian surface in this late springtime afternoon image of Amazonis Planitia.

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