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This picture was taken during the Martian summer with only small patches of ice remaining at the surface; they show up as bright, somewhat blue, spots on slopes that provide some shading from the Sun.
Sand Dunes Near the North Pole
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This crater, formed in 2008, exposes shallow, clean ice that is not uncommon in the middle-to-high latitudes on Mars.
Icy New Impact
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This unnamed impact crater is about 8 kilometers in diameter and contains numerous gullies.
Bright Gully Deposits on Mars
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An image showing a rocket firing. The rocket is on a train track to replicate the forces a supersonic spacecraft would experience prior to landing.
NASA Fires Up Rocket Sled Hardware at China Lake
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Science team leaders for NASA's Mars Science Laboratory mission have chosen "Mount Sharp" as an informal name for the mountain beside the chosen landing site for the mission's rover, Curiosity.
Robert Sharp
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The landing site for NASA's Mars rover Curiosity was chosen for giving the mission access to examine the lower layers of a mountain inside Gale Crater.
'Mount Sharp' on Mars Compared to Three Big Mountains on Earth
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Curiosity, the big rover of NASA's Mars Science Laboratory mission, will land in August 2012 near the foot of a mountain inside Gale Crater.
'Mount Sharp' Inside Gale Crater, Mars
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This image shows the target landing area for Curiosity, the rover of NASA's Mars Science Laboratory mission.
Destination for Mars Rover Curiosity
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The Magnetometer (MAG) is a part of the Particles and Fields (P & F) Package and measures interplanetary solar wind and ionospheric magnetic fields.
MAVEN Magnetometer
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The Solar Wind Electron Analyzer (SWEA) is a part of the Particles and Fields (P & F) Package and will measure the solar wind and ionospheric electrons.
Solar Wind Electron Analyzer for MAVEN Spacecraft
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The Solar Wind Ion Analyzer (SWIA) is a part of the Particles and Fields (P & F) Package and measures the solar wind and magnetosheath ion density and velocity.
Solar Wind Ion Analyzer for MAVEN Spacecraft
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The Solar Energetic Particle (SEP) instrument is part of the Particles and Fields (P & F) Package and determines the impact of SEPs on the upper atmosphere.
Solar Energetic Particle Instrument for MAVEN Spacecraft
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The Suprathermal and Thermal Ion Composition (STATIC) instrument is part of the Particles and Fields (P & F) Package and measures thermal ions to moderate energy escaping ions.
Suprathermal And Thermal Ion Composition Instrument for MAVEN Spacecraft
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The Langmuir Probe and Waves (LPW) instrument is part of the Particles and Fields (P & F) Package and determines ionospheric properties and wave heating of escaping ions and solar EUV input to the atmosphere.
Langmuir Probe And Waves Instrument for MAVEN Spacecraft
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A towering dust devil, casts a serpentine shadow over the Martian surface in this image acquired by the High Resolution Imaging Science Experiment (HiRISE) camera on NASA's Mars Reconnaissance Orbiter.
The Serpent Dust Devil of Mars
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The MAVEN spacecraft core structure is successfully lowered and mated to the hydrazine propulsion tank and boat tail assembly at Lockheed Martin, Denver.
MAVEN Stucture Tank Integration
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The Thermal Emission Imaging System (THEMIS) camera on NASA's Mars Odyssey spacecraft has completed an unprecedented full decade of observing Mars from orbit.
Tenth Anniversary Image from Camera on NASA Mars Orbiter
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The MAVEN spacecraft structure is placed into a reaction chamber, where it completed a static loads test to ensure that it will withstand the extreme forces of launch.
MAVEN Spacecraft in Reaction Structure
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A NASA Mars Science Laboratory test rover called the Vehicle System Test Bed, or VSTB, serves as the closest double for Curiosity in evaluations of the mission's hardware and software.
Testing Precision of Movement of Curiosity's Robotic Arm
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This self-portrait from Opportunity shows dust accumulation on the rover's solar panels as the mission approached its fifth Martian winter.
Dusty Mars Rover Selfie
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This image, taken Jan. 26, 2012, shows NASA's no-longer-active Phoenix Mars Lander spacecraft after its second Martian arctic winter.
Phoenix Lander After Second Martian Winter
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The Mars Hand Lens Imager (MAHLI) camera at the end of the robotic arm of NASA's Curiosity rover will use a calibration target attached to a shoulder joint of the arm.
Calibration Target on Curiosity for Camera on Rover's Arm
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This image, taken Jan. 26, 2012, shows the back shell of NASA's Phoenix Mars Lander spacecraft after its second Martian arctic winter.
Phoenix Back Shell After Second Martian Winter
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Near the lower left corner of this view is the three-petal lander platform that NASA's Mars Exploration Rover Spirit drove off in January 2004.
Spirit Lander and Bonneville Crater in Color
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During pre-flight testing in March 2011, the Mars Hand Lens Imager (MAHLI) camera on NASA's Mars rover Curiosity took this image of the MAHLI calibration target under illumination from MAHLI's two ultraviolet LEDs (light emitting diodes).
MAHLI Calibration Target in Ultraviolet Light
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