MARSIS set to reveal more from Mars

Image: Mars Express in orbit around Mars with the MARSIS antenna unfurled.

The deployment will begin on 2nd May and continue until 12th May by which time the booms will be outstretched to their final position. Each of the two main radar booms, are folded into a box like an accordion. On release the box opens and the elastic energy of the compressed glass fibre booms (40 metres long) allows them to gently unfold - hence the time period over which the deployment happens.

Confirmation of the overall success of the operation will require several days of analysis. Once the deployment is complete, the MARSIS instrument will undergo three weeks of testing before commissioning and start of actual science investigations, just as one of the prime regions of interest for radar observations will come in the right position through the natural evolution of the spacecraft's orbit.

Professor Iwan Williams from Queen Mary University of London, a co-investigator on MARSIS, eagerly awaits data from the instrument, "It will be good to see the booms of MARSIS deployed - better late than never! The deployment is taking place at a time when the conditions are optimised - as the search for sub-surface water can only take place when the pericentre of the orbit is in the dark (or at night). MARSIS will also act as an atmospheric probe and may even be able to detect meteors in the Martian atmosphere."

The deployment of the three MARSIS radar booms is an operation which will take place in three phases, in a window spanning from 2 to 12 May 2005. These operations will be initiated and monitored from ESA's European Space Operations Centre (ESOC) in Darmstadt, Germany. Each boom will be deployed separately, with the two 20-metre 'dipole' booms to be unfurled first and the 7-metre 'monopole' boom to follow a few days later.

The prime objective of MARSIS is to map the distribution of water and ice in the upper portions of the Martian crust. Using techniques similar to oil prospecting on Earth, the instrument will analyse reflections of radio waves in the upper 2-3 km of the Martian crust to reveal the subsurface structure. It will be able to distinguish between dry, frozen and wet soil.

The deployment of MARSIS was originally scheduled to take place in April 2004. However, final computer simulations prior to deployment revealed the possibility of a whiplash effect before they extended to their resting position - with the potential for the booms to hit the spacecraft. This has now been resolved.

The three booms of MARSIS consist of a pair of 20-metre hollow cylinders, each 2.5 centimetres and a 7-metre boom.

Once deployed it is anticipated that MARSIS will continue to probe the subsurface of Mars until at least until the end of November 2005 - and beyond if the mission is further extended.

The principal investigator for MARSIS is Professor Giovanni Picardi from Universita di Roma La Sapienza, Rome, Italy. UK scientists from Imperial College, Queen Mary University of London and Bristol University are involved in investigating the significance of ground water/ice on the Martian surface, data analysis and the detection of sub glacial lakes.

Source: PPARC