This is an artist's conception of NASA's Mars Atmosphere and Volatile Evolution MissioN (MAVEN) Mars orbiter. This image shows an artist concept of NASA's Mars Atmosphere and Volatile Evolution (MAVEN) mission.
Learn more about the agency's next Red Planet mission during a live event on June 17.
The Red Planet's surface has been visited by eight NASA spacecraft.
Managed by the Mars Exploration Program and the Jet Propulsion Laboratory for NASA’s Science Mission Directorate NASA’s Jet Propulsion Laboratory, Pasadena, Calif., will provide Program management via the Mars Program Office, as well as navigation support, the Deep Space Network, and the Electra telecommunications relay hardware and operations.
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.The goal of the Mars Atmosphere and Volatile EvolutioN (MAVEN) program is to determine the role that loss of atmospheric gas to space played in changing the Martian climate through time. This animation is a shorter clip from the video "Curiosity and MAVEN Explore Mars." The Remote Sensing package aboard the MAVEN spacecraft, was conceived, designed and built by the University of Colorado’s Laboratory for Atmospheric and Space Physics (CU/LASP) at Boulder. Graphic illustrating the MAVEN spacecraft encountering plasma layers at Mars. Solar Wind Ion Analyzer (SWIA) The SWIA instrument measures the solar wind and ion density and velocity in the magnetosheath of Mars. The MAVEN Solar Wind Ion Analyzer will study ions in the Martian atmosphere, a key component for better understanding the planet's evolution. Technicians and engineers oversee MAVEN after it was attached to a processing stand. These profiles show the brightness of auroras in Mars’ atmosphere at different altitudes. The close encounter between comet Siding Spring and Mars flooded the planet with an invisible tide of charged particles from the comet's coma. NASA Goddard Space Flight Center in Greenbelt, Maryland, will manage the MAVEN mission and provide instruments. A lunar eclipse, a solar eclipse and Mars has a close encounter with a comet. This animation shows a proton aurora at Mars. The ninth will be the first that includes a roundtrip ticket in its flight plan. 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. The Solar Wind Electron Analyzer (SWEA) is a part of the Particles and Fields (P & F) Package and measures the solar wind and ionospheric electrons. The team also fueled the rover's sky crane to get ready for this summer's history-making launch. First, a solar wind proton approaches Mars at high speed and encounters a cloud of hydrogen surrounding the planet. When you navigate with a compass you can orient yourself thanks to Earth's global magnetic field. MAVEN will determine how much of the Martian atmosphere has been lost over time by measuring the current rate of escape to space and gathering enough information about the relevant processes to allow extrapolation backward in time.MAVEN’s principal investigator is based at the University of Colorado at Boulder’s Laboratory for Atmospheric and Space Physics. Download a coloring sheet of NASA MAVEN orbiter and Curiosity rover working together at Mars.
Vaneeza Rupani's essay was chosen as the name for the small spacecraft, which will mark NASA's first attempt at powered flight on another planet. The team also fueled the rover's sky crane to get ready for this summer's history-making launch.
NASA's Mars Atmosphere and Volatile Evolution (MAVEN) spacecraft has obtained its first observations of the extended upper atmosphere surrounding Mars. MAVEN Wind Ion Analyzer – NASA’s Mars Exploration Program. 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. Goals: Deduce magneto-plasma topology in and above the Martian ionosphere based on electron spectra and pitch angle distributions; Measure atmospheric electron impact ionization effects; Observations:
While Curiosity will not be able to see MAVEN as it arrives at Mars, the rover welcomes the orbiter's discoveries...
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