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Animation of MAVEN orbiting Mars
September 22, 2014
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NASA
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NASA's Mars Atmosphere and Volatile EvolutioN, or MAVEN, spacecraft, mounted atop a United Launch Alliance Atlas V rocket, rolls out from Cape Canaveral Air Force Station's Vertical Integration Fac...
MAVEN Rolls to the Launch Pad
Artist’s conception of MAVEN’s Imaging UltraViolet Spectrograph (IUVS) observing the “Christmas Lights Aurora" on Mars. MAVEN observations show that aurora on Mars is similar to Earth’s "Northern L...
Artist's Concept of MAVEN Observing Aurora on Mars
Conceptual image of wind (blue arrows) flowing over rugged Martian terrain and generating disturbances that propagate upward as atmospheric gravity waves (grey lines).
Artist's Concept of Wind Flowing over Martian Terrain
MAVEN selfie with Mars in the background.
MAVEN Selfie with Mars in the Background
The payload fairing for the Mars Atmosphere and Volatile Evolution, or MAVEN, spacecraft arrives at the Payload Hazardous Servicing Facility at NASA's Kennedy Space Center in Florida.
MAVEN's Payload Fairing Arrives
This image shows an artist concept of NASA's Mars Atmosphere and Volatile Evolution (MAVEN) mission.
Artist Concept of NASA's Mars Atmosphere and Volatile Evolution (MAVEN)
Two days before the scheduled launch to Mars, the United Launch Alliance Atlas V rocket and NASA's Mars Atmosphere and Volatile Evolution (MAVEN) spacecraft rolled out of the Cape Canaveral Air For...
Mars-Bound MAVEN at the Launch Pad
The Martian surface bears ample evidence of flowing water in its youth, from crater lakes and riverbeds to minerals that only form in water. But today Mars is cold and dry, and scientists think tha...
Investigating the Martian Atmosphere
The Imaging Ultraviolet Spectrograph (IUVS) is a part of the Remote Sensing (RS) Package and measures global characteristics of the upper atmosphere and ionosphere via remote sensing.
Imaging Ultraviolet Spectrograph
Phobos as observed by MAVEN's Imaging Ultraviolet Spectrograph.
Phobos Observed by MAVEN
Artist’s rendering of a solar storm hitting Mars and stripping ions from the planet's upper atmosphere.
Visualizing a Solar Storm's Effect on Mars Atmosphere
Mars's thick early atmosphere was likely lost to space, and the Sun is a potential culprit. When high-energy solar photons strike the upper Martian atmosphere they can ionize gas molecules, causing...
MAVEN: Mars Atmospheric Loss: Plasma Processes
This artist's concept shows the MAVEN spacecraft in orbit around the Red Planet, with a fanciful image of her home planet in the background.
MAVEN to Mars
The first demonstration of NASA's MAVEN Mars orbiter's capability to relay data from a Mars surface mission, on Nov. 6, 2014, included this and other images from NASA's Curiosity Mars rover. The im...
Image Relayed by MAVEN from Curiosity Mars Rover
The Neutral Gas and Ion Mass Spectrometer (NGIMS) measures the composition and isotopes of thermal neutrals and ions.
Neutral Gas and Ion Mass Spectrometer for MAVEN Spacecraft
This graphic depicts paths by which carbon has been exchanged among Martian interior, surface rocks, polar caps, waters and atmosphere, and also depicts a mechanism by which it is lost from the atm...
Carbon Exchange and Loss Processes on Mars
Inside Kennedy’s Payload Hazardous Servicing Facility technicians clean the electricity-producing solar arrays for the Mars Atmosphere and Volatile Evolution (MAVEN) spacecraft Aug. 28.
Technicians at KSC Prep Solar Panels
This image of the Mars night side shows ultraviolet emission from nitric oxide (abbreviated NO)
Mars' Nightside Atmosphere
Energetic particles from a large solar storm in September 2017 were seen both in Mars orbit by NASA's MAVEN orbiter, and on the surface of Mars by NASA's Curiosity Mars rover.
Solar Storm's Radiation at Martian Orbit and Surface
This illustration shows the MAVEN spacecraft and the limb of Mars.
MAVEN Artist's Concept Orbiting Mars
This artist's concept depicts the early Martian environment (left) - believed to contain liquid water and a thicker atmosphere - versus the cold, dry environment seen at Mars today (right).
The Look of a Young Mars
This image is a stereo, panoramic view of various trenches dug by NASA's Phoenix Mars Lander. The images that make up this panorama were taken by Phoenix's Surface Stereo Imager at about 4 p.m., lo...
Phoenix Trenches (3-D)
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
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
This ultraviolet image near Mars’ South Pole was taken by MAVEN on July 10 2016 and shows the atmosphere and surface during southern spring.
Ultraviolet Image Near Mars' South Pole
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