“MAVEN has been a tremendous success,” said Bruce Jakosky, MAVEN principal investigator and LASP associate director for science. “The spacecraft and instruments continue to operate as planned, and we’re looking forward to further exploration of the Martian upper atmosphere and its influence on climate.”
MAVEN’s selfie was made by looking at ultraviolet wavelengths of sunlight reflected off of components of the spacecraft. The image was obtained with the Imaging Ultraviolet Spectrograph (IUVS) instrument, built at LASP, that normally looks at ultraviolet emissions from the Martian upper atmosphere. The IUVS instrument is mounted on a platform at the end of a 1.2-m boom (its own “selfie stick”), and by rotating around the boom can look back at the spacecraft. The selfie was made from 21 different images, obtained with the IUVS in different orientations, that have been stitched together.
“We never expected MAVEN to be able to take its own picture this way, but MAVEN has already surprised us many times with its outstanding performance at Mars,” said Nick Schneider, lead scientist for the IUVS instrument and a CU Boulder professor of astrophysical and planetary sciences. “We think this is the first ultraviolet selfie taken by a spacecraft.”
The MAVEN team in LASP includes researchers and students at both the graduate and undergraduate level. MAVEN has been streaming back to Earth since the spacecraft went into orbit around Mars on Sept. 14, 2014. LASP provided two instruments for MAVEN and leads science operations and education and outreach for the mission.
During its time at Mars, MAVEN has made the following discoveries and science results, among others:
- Acquired compelling evidence that the loss of atmosphere to space has been a major driver of climate change on Mars.
- Determined that the stripping of ions from the upper atmosphere to space during a solar storm can be enhanced by a factor of 10 or more, possibly making these storms a major driver of loss of the atmosphere through time.
- Discovered two new types of Martian aurorae – diffuse aurora and proton aurora. Neither type has a direct connection to the local or global magnetic field or to magnetic cusps, as aurorae do on Earth.
- MAVEN has made direct observations of a metal-ion layer in the Martian ionosphere, the first direct detection on any planet other than the Earth. The ions are produced by a steady influx of incoming interplanetary dust.
- Demonstrated that the majority of the CO2 on the planet has been lost to space and that there isn’t enough left to terraform the planet by warming it, even if the CO2 could be released and put back into the atmosphere.
Next year, engineers will initiate an aerobraking maneuver by skimming the spacecraft through Mars’ upper atmosphere to slow it down. This will reduce the highest altitude in MAVEN’s orbit to enhance its ability to serve as a communications relay for data from rovers on the surface. Currently, MAVEN carries out about one relay pass per week with one of the rovers. This number will increase after NASA’s InSight mission lands on Mars in November.
MAVEN completed its primary mission in November 2015 and has been operating in an extended mission since that time, continuing its productive investigation of Mars’ upper atmosphere and exploring additional opportunities for science that the new relay orbit will bring.
NASA’s Goddard Space Flight Center in Greenbelt, Maryland, manages the MAVEN project and provided two science instruments for the mission. Lockheed Martin built the spacecraft and is responsible for mission operations. The University of California at Berkeley’s Space Sciences Laboratory also provided four science instruments for the mission. NASA’s Jet Propulsion Laboratory in Pasadena, California, provides navigation and Deep Space Network support, as well as the Electra telecommunications relay hardware and operations.