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KSC-MRO-wet-rehersal.jpg
Practice, Practice, Practice: 'Wet Dress Rehearsal'
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KSC-MRO_Encapsulation.jpg
Spacecraft Shrouded: Encapsulation
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MRO_data.jpg
34 Terabits of Data
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mars_orbiters.jpg
Spacecraft Comparison
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The Art of Exploration
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MRO_thumbs_up.jpg
Last Stop: Launch Pad
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This panoramic image, dubbed "Rub al Khali," was taken by Opportunity on the plains of Meridiani during the rover's 456th to 464th sols on Mars.
Opportunity's 'Rub al Khali' Panorama
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This Mars Global Surveyor (MGS) Mars Orbiter Camera (MOC) image shows a 1.5 meters per pixel (~5 ft/pixel) view of three aligned meteor impact craters on the floor of a much larger crater in the Noachis Terra region. The craters may have formed together from a single event in which the impactor (the meteor) was broken into three pieces.
Triple Impact
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MRO_Orb_Up_7_19.jpg
Fueled for Flight
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This Mars Global Surveyor (MGS) Mars Orbiter Camera (MOC) image shows a curved, pitted ridge in Isidis Planitia. This feature may be a remnant of a once more-extensive layer of material that covered the present, cratered surface.
Curved and Pitted Ridge
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If a human with perfect vision donned a spacesuit and stepped onto the martian surface, the view would be as clear as this sweeping panorama taken by Spirit.
'Everest' Panorama; 20-20 Vision
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MRO_Fairing.jpg
Fairing Preparing for Farewell
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Opportunity's wheels dug more than 10 centimeters (4 inches) deep into the soft, sandy material of a wind-shaped ripple in Mars' Meridiani Planum region during the rover's 446th martian day, or sol (April 26, 2005).
Looking Back at 'Purgatory Dune'
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20050615-01.jpg
Bringing the Blast: Upper Stage Rocket Arrives at Kennedy Space Center
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This image is an artist's concept of a view looking down on NASA's Mars Reconnaissance Orbiter. The spacecraft is pictured using its Shallow Subsurface Radar instrument (SHARAD) to "look" under the surface of Mars.
Mars Reconnaissance Orbiter's Radar, Top View (Artist's Concept)
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MRO-SHARAD-top-view.jpg
The Mars Reconnaissance Orbiter using its SHARAD radar (top view)
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MRO-SHARAD-side-view.jpg
The Mars Reconnaissance Orbiter using the SHARAD radar (side view)
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MRO-MOI.jpg
The Mars Reconnaissance Orbiter during its Mars Orbit Insertion
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MRO-Mars-Climate-Sounder.jpg
The Mars Reconnaissance Orbiter using its Mars Climate Sounder instrument
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Hamilton_G21258_cover.jpg
Olivine-Rich Bedrock Around Nili Fossae
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This Mars Global Surveyor (MGS) Mars Orbiter Camera (MOC) image shows dark slope streaks coming down the slopes of a knob in western Amazonis Planitia. All of the surfaces in this image are mantled by dust. On the slopes, mass movement of dry dust has created the streaks.
Slope-Streaked Knob
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This false color image shows a region with craters of different ages located at the margin of Acidalia Planitia. This image was collected during the Northern Spring season. The THEMIS VIS camera is capable of capturing color images of the Martian surface using five different color filters. In this mode of operation, the spatial resolution and coverage of the image must be reduced to accommodate the additional data volume produced from using multiple filters. To make a color image, three of the five filter images (each in grayscale) are selected. Each is contrast enhanced and then converted to a red, green, or blue intensity image. These three images are then combined to produce a full color, single image. Because the THEMIS color filters don't span the full range of colors seen by the human eye, a color THEMIS image does not represent true color. Also, because each single-filter image is contrast enhanced before inclusion in the three-color image, the apparent color variation of the scene is exaggerated. Nevertheless, the color variation that does appear is representative of some change in color, however subtle, in the actual scene. Note that the long edges of THEMIS color images typically contain color artifacts that do not represent surface variation.
Cratered Acidalia Planitia
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A portion of an exposure of bedrock dubbed "Larry's Outcrop" shows little layering in this view, in contrast to nearby outcrops called "Methuselah" and "Jibsheet."
Larry's Outcrop' in False Color
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20050518-01.jpg
Getting Closer to Countdown: Spacecraft Undergoes Readiness Tests
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This Mars Global Surveyor (MGS) Mars Orbiter Camera (MOC) image shows cross-cutting fault scarps among graben features in northern Tempe Terra. Graben form in regions where the crust of the planet has been extended; such features are common in the regions surrounding the vast "Tharsis Bulge" on Mars.
Cross-Cutting Faults
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