About the ExoMars Mission
Innovative technologies... enabling new science
ExoMars is the first mission in ESA's Aurora Exploration Programme. ExoMars will pursue important science and technology objectives aimed at extending Europe's capabilities in planetary exploration.
It will demonstrate the descent and landing of a large payload on Mars; the navigation and operation of a mobile scientific platform; a novel drill to obtain subsurface samples; a sample processing and distribution system; and meet challenging planetary protection and cleanliness levels necessary to achieve the mission’s ambitious scientific goals.
Establishing whether life ever existed, or is still active on Mars today, is one of the outstanding questions of our time. It is also a prerequisite to prepare for the future human exploration of the Red Planet.
Exobiology and geology research
ExoMars will deploy a Rover carrying a comprehensive suite of analytical instruments dedicated to exobiology and geology research: the Pasteur payload. The Rover will travel several kilometres searching for traces of past and present signs of life, collecting and analysing samples from within surface rocks and from the subsurface, down to a depth of 2 metres.
The ExoMars Rover mission will be complemented by the Humboldt payload, to be accommodated on the Lander. Following the Rover's egress, the Humboldt station will be activated to study the environment and measure planetary geophysics parameters important for understanding Mars’s evolution and habitability.
Additionally, data from engineering sensors necessary for Entry, Descent, and Landing (EDL) will provide an opportunity to perform vital descent science measurements.
Planetary protection
Based on the Outer Space Treaty, the Committee On Space Research (COSPAR) has established a planetary protection policy that ExoMars adheres to.
The implementation of planetary protection requirements for ExoMars comprise restrictions on impact probabilities for flight hardware not intended to directly contact Mars, and biological and organic contamination control for all spacecraft elements. Specifically parts of the spacecraft that come into contact with the samples from Mars have to be sterile and clean to avoid compromising the life-detection experiments.
Mobility and drilling capabilities
Recent discoveries from ESA's Mars Express have revealed multiple deposits containing salt and clay minerals that can only form in the presence of liquid water. This reinforces the hypothesis that ancient Mars may have been wetter, and possibly warmer, than it is today.
NASA's Mars Exploration Rovers (Spirit and Opportunity) were conceived as robotic geologists and they have demonstrated the past existence of wet environments on Mars. Their results have persuaded the scientific community that mobility is a must-have requirement for future missions.
ExoMars will have instruments to investigate whether life ever arose on the Red Planet. It will also be the first mission combining mobility and access to subsurface locations where organic molecules may be well-preserved; thus allowing, for the first time, to investigate Mars's third dimension: depth. This alone assures that ExoMars will break new scientific ground.
Finally, the many technologies developed for this project, will allow ESA to prepare for international collaboration on future missions, such as Mars Sample Return.
Last update: 5 March 2008
Rate this
Views
Share
- Currently 0 out of 5 Stars.
- 1
- 2
- 3
- 4
- 5
Rating: 0/5 (0 votes cast)Thank you for rating!
You have already rated this page, you can only rate it once!
Your rating has been changed, thanks for rating!