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MAVEN Launching
November 18, 2013
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This is an artist's conception of NASA's Mars Atmosphere and Volatile Evolution MissioN (MAVEN) Mars orbiter.
Artist's Concept of MAVEN
At Cape Canaveral Air Force Station's Space Launch Complex-41 liquid oxygen began flowing into the Atlas first stage booster for the Mars Atmosphere and Volatile Evolution, or MAVEN, mission.
Fueling of MAVEN's Atlas V Rocket Underway
This artist concept depicts NASA’s Space Launch System, which will be the most powerful rocket ever built. It is designed to boost the agency’s Orion spacecraft on deep space missions, including to...
Space Launch System Rocket Clearing the Clouds
At Cape Canaveral Air Force Station in Florida, the United Launch Alliance Atlas V first stage is lifted for stacking at Launch Pad 41 in preparation for the Mars Atmosphere and Volatile Evolution,...
MAVEN's Atlas V Lifted to Launch Pad
These profiles show the brightness of auroras in Mars’ atmosphere at different altitudes. The solid black profile on the right is from a September 2017 solar storm. Barely visible along the vertica...
Martian Aurora 25 Times Brighter Than Prior Brightest
Robert Lin, the late director of the Space Sciences Laboratory, discusses how NASA's MAVEN spacecraft will study the interaction of the Martian atmosphere with the solar wind. MAVEN's findings will...
Studying the Solar Wind on Mars
MAVEN will use its Neutral Gas and Ion Mass Spectrometer to study the interaction of neutral gases and ions in the Martian atmosphere with the solar wind, helping scientists to understand how Mars ...
Searching for Mars' Missing Atmosphere
How did Mars, a once wet planet, lose its early atmosphere? One possibility is through a process called "sputtering," in which atoms are knocked away from the atmosphere due to impacts with energet...
MAVEN: Mars Atmospheric Loss
The MAVEN Electra UHF Transceiver Flight Model is shown here.
MAVEN Electra UHF
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)
Download a PDF of the MAVEN Fact Sheet.
MAVEN Fact Sheet
This visualization shows MAVEN and Comet Siding Spring making their way through the solar system to a close encounter near Mars. This animation maintains a fixed camera above the ecliptic plane of ...
Comet Siding Spring Wide Shots (Fixed)
NASA's Mars Atmosphere and Volatile Evolution, or MAVEN, spacecraft went through weeks of processing to ensure it was ready for a 10-month trip to the Red Planet. Watch as time-lapse video condense...
MAVEN Processing in Minutes
MAVEN selfie composite, annotated
MAVEN Selfie Composite, Annotated
MAVEN positioned atop Atlas V rocket.
MAVEN Positioned Atop Atlas V Rocket
The engineering model of the Extreme Ultraviolet (EUV) sensor that is part of the Langmuir Probe and Waves (LPW)/EUV experiment on MAVEN and will measure the solar EUV input to the atmosphere.
MAVEN Extreme Ultraviolet Sensor
At Cape Canaveral Air Force Station's Space Launch Complex 41 a United Launch Alliance Atlas V rocket stands ready to boost the Mars Atmosphere and Volatile Evolution, or MAVEN, spacecraft on a 10-...
MAVEN Ready for Launch
A map of MAVEN's IUVS’s auroral detections in December 2014 overlaid on Mars’ surface.
Map of Auroral Detections on Mars
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
NASA’s MAVEN (Mars Atmosphere and Volatile EvolutioN) mission acquired stunning views of Mars in two ultraviolet images taken at different points along our neighboring planet’s orbit around the Sun.
MAVEN Spacecraft Stuns with Ultraviolet Views of Red Planet
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
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
The close encounter between comet Siding Spring and Mars flooded the planet with an invisible tide of charged particles from the comet's coma. The dense inner coma reached the surface of the planet...
Close Siding Spring Encounter
This animation shows a proton aurora at Mars. First, a solar wind proton approaches Mars at high speed and encounters a cloud of hydrogen surrounding the planet.
Animation of Proton Aurora at Mars
Aerobraking plan for MAVEN
MAVEN Aerobraking to Achieve Science and Relay Orbit
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