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EXOMARS ROVER: EXPOSING THE REALITY OF LIFE ON THE RED PLANET

Article originally written for AKKA UK: Original post on my LinkedIn Account

Dedicated AKKA employees are helping to conduct the research and development of the ExoMars 2020 mission by developing and building the ExoMars Rover, a mission which sets out to uncover the history of the Red Planet.

 

The complete mission will see European and Russian Space agencies, ESA and Rocosmos, join forces to look for signs of life on Mars, and the ExoMars Rover itself will play an integral role in providing key insights into future manned missions.


The UK’s €205million contribution is the second largest, and Airbus D&S is the prime contractor of the ExoMars Rover. Working at Airbus D&S, some of our own engineers are providing the knowledge and expertise crucial to the success of this visionary frontier.

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ESA has stated that the Rover will land on a site with a ‘high potential of having well-preserved organic material’, and will search for signs of past or present life by drilling a hole (2m maximum) into the planet’s surface to investigate the mineralogy. In 2017, ESA decided they would study both Oxia Planum and Mawrth Vallis as possible touchdown sites for the ExoMars Rover. Located in Mars’ northern hemisphere, studies have shown both these sites are likely to harbour evidence of previous water activity.
The Rover’s cleverly designed drill includes an infrared spectrometer which will characterise the mineralogy exposed by the borehole. Then, in the heart of the vehicle, there will be a laboratory which will perform a detailed chemical, physical and spectral analysis on the crushed sample. The MOMA (Mars Organic Molecule Analyser) and mass spectrometer have been provided by NASA.

However, it has taken a feat of complex and rigorous testing to get the team to where they are now. Since the project’s origin, many prototypes of the ExoMars Rover have been produced, each with a name as exotic as the next: Bridget, Bruno, and Bryan- the latter being the latest. Having now finalised the design of the Rover, the Stevenage team is focusing on testing the Rover, including vibration and structure testing.

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Once the final tests have been carried out, the team will then need to complete the final version of the Rover later this year. Although this comes two years before the launch date, it is critical to the success of the mission: the Rover will need to be integrated into the spacecraft which comprises the Russian launch vehicle, ESA carrier module and Russian lander. This all requires final assembly before being launched in Summer 2020.

The ExoMars Rover will be held in a descent module which will disconnect from the rest of the ExoMars craft upon entering Mars’ atmosphere. This descent module will see the Rover safely to the surface of Mars, where it can begin its mission. The ExoMars Trace Gas Orbiter which was launched in 2016, will continue to orbit Mars, studying the atmosphere and supporting communications between the Rover and the ESOC (European Space Operations Centre). We can expect the Rover to land 9 months after the launch, which is expected to be January 2021.

 

The Rover boasts many intelligent features, one of which is its ability for autonomous navigation. During its expedition, the Rover will travel several kilometres; as the ExoMars Trace Gas Orbiter only passes over the Rover approximately twice per sol, and as it can also take up to 24 minutes for signals from Mars to reach Earth, it is essential that the ExoMars Rover is able to assess its surroundings, selecting the safest path of travel for itself.
Using the topmost cameras, the Rover will process a 3D image of the Martian terrain, classifying each of the obstacles into different risk categories and using this information to plan a safe path across the planet. The only navigational input which Earth needs to determine is the final destination of the Rover. 

NASA IMG - Vera Rubin Ridge.jpg

The Curiosity Mars Rover takes a photo of the Gale Crater from the 'Vera Rubin Ridge' - October 2017

Still, the Airbus D&S team has had much to consider in their extensive designing of the Rover vehicle. There will be many external challenges facing the Rover upon its Mars touchdown, one of which is the extreme shifts in the planet’s surface temperature. At night, Mars’ temperature can drop to -130°C and even in the Summer the temperature won’t rise above 5°C.


Working to accommodate such a cold environment has proven to be a challenging venture. Materials which constitute the ExoMars Rover can become very brittle when they are exposed to these cool climates; as such, any abrasions or impacts to the vehicle will be far more damaging.
Furthermore, as the shift in temperature between night and day is so drastic (upwards of a 90°C shift), the rates of expansion and contraction across the materials which make up the Rover will vary considerably, acting to tear the components of the vehicle apart.

Indeed, knowing that the Martian landscape is covered in abrasive sand is integral to the design of the vehicle; not only will the vehicle’s tread pull up sand as it moves across the surface, but also Mars is prone to huge dust storms, one of which is predicted to set in around the same time the ExoMars mission is due to take place. Though the rover is due to land outside of the main dust storm season, it is bound to encounter these routine storms during its 7-12-month operational period.
Taking into consideration Mars’ atmospheric pressure, which is about 1% the density of Earth’s, it is unlikely that these winds will cause serious damage upon impact. However, on rare occasion, these storms can be planet-wide and can produce a haze of dust which enshrouds the entire surface of Mars; not ideal for the solar-powered ExoMars Rover, as the dust storms can block the light to its solar arrays.
Furthermore, the dust particles on Mars are small and slightly electrostatic, meaning that when they inevitably do stick to the surface of the Rover, any incidents of them getting into the machinery and gears can have hazardous consequences.

NASA IMG - Mars dust storm.jpg

2001 images taken from the Mars Orbiter Camera on NASA's Mars Global Surveyor Orbiter shows Mars as a global dust-storm consumes the planet. The two images were taken roughly a month apart.

In addition to these debilitating storms, Mars is highly irradiated. Software and electronics that have not been sufficiently protected will not stand a chance when journeying across the surface.

As a result, the team has worked hard to address the challenges facing the ExoMars Rover, and is well on its way to meeting the 2018 project deadline.
ExoMars is a groundbreaking mission which will be the first mission to combine the capability to move across the surface and study Mars at depth. Operations will be monitored and controlled via the ROCC (Rover Operations Control Centre) in Turin, Italy.

We’re wishing our engineers favourable Martian weather for the upcoming mission.

SOURCES:

 

[1] http://abyss.uoregon.edu/~js/ast121/lectures/lec02.html

 

[2] http://www.math.nus.edu.sg/aslaksen/gem-projects/hm/0102-1-stonehenge/sun.htm

 

[3] Clark, Stuart. ‘The Unknown Universe in 10 Chapters’, Chapter 1, p. 20.

 

[4] http://abyss.uoregon.edu/~js/ast121/lectures/lec02.html

 

[5] Clark, Stuart. P. 25

 

[6] Clark, Stuart, p. 22

 

[7] https://www.space.com/15787-johannes-kepler.html

 

[8] Clark, Stuart, p. 23

 

[9] https://www.space.com/15787-johannes-kepler.html

 

[10] 1-3 of Kepler’s laws: http://hyperphysics.phy-astr.gsu.edu/hbase/kepler.html

 

[11] Clark, Stuart, p.28

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