
If all goes according to plan, at 09:31 GMT on Monday March 14th, a Russian Proton launcher is scheduled to lift-off from the Baikonaur Cosmodrome Kazakhstan, sending the first part of the European ExoMars mission on its way to Mars.
With its suite of high-tech instruments, the Trace Gas Orbiter (TGO) should arrive at the Red Planet on October 19th, 2016, after a journey of 496 million kilometres (308 million miles). While Its main mission is to photograph the Red Planet and analyse its air, the TGO is also carrying a small Mars lander, dubbed Schiaparelli, after the man who first thought he saw canali (as in “groves” or “channels”) on Mars in the 1870s, and thus inadvertently sparked the entire “canals on Mars mythos.

A key goal for the TGO mission is to analyse the methane gas which has frequently been detected on Mars by various missions. Methane can either be generated in a biological process, such as microbes decomposing organic matter, or geological ones involving chemical processes in hot liquid water under the surface. However, it also tends to be broken down by ultraviolet radiation within a few hundred years, so for it to be detected at all on Mars means whatever is producing it is liable to be an active process, and identifying what that process actually is – organic or inorganic – is a crucial part of furthering our understanding of Mars, and could have major ramifications for future missions.
“TGO will be like a big nose in space,” according to Jorge Vago, an ExoMars project scientist. “It will analyse Mars’ methane in more detail than any previous mission and try to determine its origins.”
In addition, TGO will monitor seasonal changes in Mars’ atmospheric composition and temperature in order to create and refine detailed models of the Martian atmosphere. Its instruments will also map the subsurface hydrogen to a depth of a metre, with improved spatial resolution compared with previous measurements. This could reveal deposits of water-ice hidden just below the surface, which, along with locations identified as sources of the trace gases, could influence the choice of landing sites of future missions.
TGO’s findings will also be used to help plan the second phase of the ExoMars mission, due to fly in 2018 (or possibly 2020 due to budget concerns). This will be a solar-powered rover unit, slightly larger than NASA’s MER rovers, Spirit and Opportunity. It’s also a rover with a long gestation period, having been under development for almost 20 years.
Originally designed to be a much bigger vehicle, ExoMars was going to be a joint ESA / NASA undertaking, with ESA supplying the rover and NASA some of the science instruments and the launch vehicle. However, in 2012, NASA arbitrarily withdrew from the project, forcing Europe to go back to the drawing board and seek Russian support for the mission (Russia is supplying the launch vehicle and the landing platform for the rover, as well as some of the science instruments carried aboard both the rover and TGO).

Unlike NASA’s Curiosity mission (but like NASA’s upcoming Mars 2020 mission), ExoMars is intended to directly seek out evidence of current or past microbial life on Mars. As such, the findings from TGO could be key in the selection of the final landing site for the rover. In addition, TGO will also act as the primary communications relay between the rover and Earth.
It is also as a communications relay that TGO will support the Schiaparelli lander. Officially named the Entry, Descent and Landing Demonstrator Module (EDM), Schiaparelli is intended to help ESA in developing the technology for landing on the surface of Mars with a controlled landing orientation and touchdown velocity. Obviously, a safe entry, descent and controlled landing capability is crucial to the success of the ExoMars rover mission, and Schiaparelli will help in determining the final design and development requirements for the rover’s landing systems.



















