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Layers within a Crater in Lucus Planum via HiRISE Mars No

Layers within a Crater in Lucus Planum via HiRISE Mars No

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Layers within a Crater in Lucus Planum, via HiRISE No Time For Me, Mars

tumblr_oe6a2q4mks1rlz4gso1_1280 Layers within a crater in Lucus Planum. Beautiful Mars series.

Yardangs showing a suite of textures. (a) MFF etched material within Nicholson Crater

Planet Four: Probing Springtime Winds on Mars by Mapping the Southern Polar CO2 Jet Deposits

This 3D, or stereo anaglyph, view shows the upcoming science destination for NASA's Mars rover Curiosity, a region dubbed "Glenelg," where three different ...

Craters within craters in Cimmeria (THEMIS_IOTD_20160928)

Sand motion in Pasteur crater. (Top) HiRISE image PSP_001756_1995, December 11,

A Fading Impact Crater in Lucus Planum

Images of layers in Juventae Chasma showing changes in orbiter camera resolution from the Viking orbiters

Persistent Aeolian Activity at Endeavour Crater, Meridiani Planum, Mars

Nicholson Crater Central Mound, as seen by HiRISE. Click on image to see dark slope streak being diverted by an obstacle.

Evidence for two fundamental types of layered ejecta craters on Mars and proposed nomenclature system

Map of sample craters

Morphology and mineralogy of Libya Montes layered delta deposits, Mars: Implications for long-term aqueous alteration

Windy Mars: A dynamic planet as seen by the HiRISE camera

The delicate rays extending beyond the halo are also significantly faded. Only the individual craters remain distinctly dark in the new ...

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The HiRISE camera on NASA's Mars Reconnaissance Orbiter captured this unusual crater or pit on the

Formation[edit]

Composite demonstrating relative resolution of 7 different cameras that imaged Mars:HiRISE (Mars Reconnaissance Orbiter), THEMIS VIS (Mars Odyssey), ...

Windy Mars: A dynamic planet as seen by the HiRISE camera

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Gullies on Mars

Dunes and Ripples in Valles Marineris

Bedding orientation measurements from six locations around margin of Gale Crater mound (Mars).

Euphrates crater, a possible source of the Pasteur crater sands. Downslope motion is apparent

Another Well-Preserved Impact Crater

Persistent Aeolian Activity at Endeavour Crater, Meridiani Planum, Mars

Upper limits on the atmospheric pressure of early Mars. Comparison of model crater size–

Crater displaying layers, as seen by HiRISE under HiWish program

Lava flow and crater ejecta, as seen by HiRISE. Impact penetrated into light-toned material then spread it on darker surface. Scale bar is 500 meters long.

Dejnev Crater Floor, as seen by HiRISE. Scale bar is 500 meters long. Click on image to see large pits.

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A Meteoroid Smashed Into the Side of a Crater on Mars and Then Started a Landslide

Close up of the crater captured by the MRO's HiRISE instrument. Credit: NASA/JPL/University of Arizona

Columbus Crater Layers, as seen by HiRISE. This false-color image is about

The planet Mars: a global view (Viking 1 Orbiter mosaic [NASA])

Aeolian Dune Sediment Flux Heterogeneity in Meridiani Planum, Mars

3-D images reveal features of Martian polar ice caps. This cut-away

Places on Mars to Look for Microbes, Lichens, .

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Aeolis quadrangle

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Coarse-grained ripples I. Sol 072-074, the wheel scuff into ''Serpent'' ripple at the rim of Bonneville crater (see Figure 51a for location in HiRISE image) ...

Sunlight was just starting to reach the high Northern latitudes in late winter when HiRISE captured

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Typical crater floor polygons. (left) CTX image of a 14 km-sized

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Candidate-landing sites at Eberswalde and Holden craters. (a) Regional context showing

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Artist's impression of a global view of Mars, centered on the Meridiani Planum region. Credit: Air and Space Museum/Smithsonian Institution

Elysium quadrangle

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(Top) Locations outlined on Mars Global Surveyor (

This Oct. 25, 2016, image shows the area where the European Space Agency's

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FRB_528262238EDR_F0580774FHAZ00302M_

Foros (crater)

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Close-up of layers in a pit on crater floor, as seen by HiRISE

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Strata in Becquerel Crater. (A) MOLA topography reveals that deposits infill a significant

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Dark layer exposed in the wall of a possible collapse formation in Ophir Planum (3

Model for the mineralogic evolution of Mars surface environments through time (after Bibring et al

All content in this area was uploaded by Oded Aharonson …

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Close view of layers in crater, as seen by HiRISE under HiWish program

Curiosity update: Change of plans

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Deep impact craters in the Isidis and southwestern Utopia Planitia regions of Mars: High target material strength as a possible cause

Boulder abundances and size-frequency distributions on Oxia Planum-Mars: Scientific implications for the 2020 ESA ExoMars rover

Curiosity's view of Mount Sharp (September 9, 2015).

This inner slope of a Martian crater has several of the seasonal dark streaks called “recurrent slope lineae,” or RSL, which were caputred by the HiRISE ...

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Mean sand flux over Nili Patera as a function of solar longitude. The sand

Localization of the studied dune fields between 65 1 N and 65 1 S from Hayward

Dilly Crater, as seen by HiRISE.

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A global view on the mineralogical composition of dark dunes on Mars

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( A ) Three-dimensional view of the stratified deposit within Becquerel crater. This

Athabasca Valles Streamlined Form, as seen by HiRISE. Click on image to see layers.

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The sand flux is derived from measuring ripples migration from the correlation of HiRISE images in MY30 (2010–2011) using COSI-Corr (see Methods).

Beagle (crater)

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