Why Europe’s New Mission To Mars Is Such A Big Deal

Why Europe’s New Mission To Mars Is Such A Big Deal

NASA gets all the glory when it comes to Martian exploration, but two other space agencies are now hoping to change that. Early next week, the European Space Agency and Roscosmos are launching the first phase of their joint ExoMars mission, a major new scientific effort with an badarse goal: discovering signs of life on the Red Planet.

At 10:30am Central European Time (8:30pm AEDT) on March 14, two robotic probes — a Trace Gas Orbiter (TGO) and the Schiaparelli entry, descent and landing demonstrator — will blast off together aboard a Russian Proton rocket from the Baikonur Cosmodrome in Kazakhstan. Thanks to the close proximity of Earth and Mars at the time of launch, it should only take the ExoMars vehicles seven months to reach the Red Planet, on October 19.

The mission: to search for evidence of biologic and geologic activity on Mars and to test technologies for the second phase of ExoMars. Exploration will involve an autonomous rover that will trundle about the surface drilling holes, collecting samples and searching for Martian life forms.

“This is really quite a significant mission for us,” Hakan Svedhem, the ESA’s mission scientist for the TGO, told Gizmodo. “It is certainly a possibility that life exists on Mars today, and we are going there to find out.”

Neither Europe nor Russia has a great track record when it comes to Mars. The ESA has made it to orbit only once with the Mars Express mission in 2003. But while the mission’s orbiter continues to capture stunning images of the Red Planet from above, a companion lander never phoned home after reaching the surface.

Why Europe’s New Mission To Mars Is Such A Big Deal
The ExoMars Trace Gas Orbiter undergoing some final tests before launch on March 14th. Image Credit: ESA

The ExoMars Trace Gas Orbiter undergoing some final tests before launch on March 14. Image Credit: ESA

Russia hasn’t even gotten that far. Following more than a dozen failed attempts to reach Mars by the USSR — along with a few partial successes — in 2011 the Russian space agency launched the Phobos-Grunt probe. The probe’s goal was to collect samples from Mars’ weird little egg-shaped moon, with the intention of returning to Earth in 2014.

In fact, Phobos-Grunt returned quite a bit sooner, after a catastrophic launch malfunction sent the space probe plummeting back into Earth’s atmosphere shortly after reaching orbit. It burned up over the Pacific, inciting a wave of delightfully paranoid alien warfare conspiracy theories.

So as you might imagine, there’s quite a bit of national pride staked on the success of ExoMars. But more exciting still are this mission’s science goals. The TGO is equipped with a suite of instruments that will allow scientists to sniff the Red Planet’s lower atmosphere at parts-per-trillion sensitivity. It will be looking for chemicals that could signal activity on the surface.

Chief among those chemical clues is methane, which remote surveys and NASA’s Curiosity rover have found sporadic evidence for over the past few years.

“Methane is particularly interesting because it can be broken apart by sunlight very quickly,” said Bruce Jakosky of the University of Colorado Boulder, who heads NASA’s Mars Atmosphere and Volatile Evolution, or MAVEN, mission. “If methane is present in the atmosphere at all means it must be resupplied to the atmosphere. That can come about from geologic and biological processes.”

How would we know where the methane is coming from? For starters, we’d have to see what other trace gases are present. Methane in conjunction with sulphur dioxide, for instance, is often taken as a sign of volcanic activity. If methane on Mars is found alongside other hydrocarbons, that could point to a biological source. The TGO is also capable of looking at the ratio of different carbon isotopes present in methane which can help elucidate its origin.

But none of these indicators is a silver bullet for alien life.

“Even if methane is from life, it doesn’t mean life is there today,” Svedhem notes. “It could have been stored underground by various processes and is only being released now.”

We’ll need a suite of follow-up analyses to learn the truth. If the TGO sniffs anything interesting, it will be able to document the area using a high res camera and probe the ground for water ice with its on-board neutron detector. If it finds something really interesting, ESA might eventually follow up with a lander.

Why Europe’s New Mission To Mars Is Such A Big Deal
Artist’s concept of NASA’s MAVEN orbiter, which is studying the Red Planet’s upper atmosphere. Image Credit: NASA

Artist’s concept of NASA’s MAVEN orbiter, which is studying the Red Planet’s upper atmosphere. Image Credit: NASA

Jakosky, for one, is excited to see another spacecraft joining MAVEN in the effort to study Mars’ atmosphere. “One of the things we’ve found over the last several decades of exploring Mars is that it’s a very complex system,” he said. “MAVEN is studying the upper atmosphere and TGO will study the lower. If we’re trying to understand the environment as a whole we need measurements from both.”

We’ll also need to continue doing ground-based exploration which is why the ExoMars 2016 payload includes a small robotic lander. Sciaparelli will touch down on Martian soil on October 19th, after which the ESA reckons it will have two to eight days of battery life to collect some basic meteorological data. But mostly, this lander is a proof of concept. The ESA wants to make sure the lander’s heat shield, parachute and thrusters deliver Sciaparelli gently to the surface — because it’s counting on that same technology to bring a large rover to Mars in 2018.

“We’ve never done this full landing concept in the past,” Svedhem said. “There’s a whole sequence of things we need to demonstrate.”

But first things first, these intrepid space probes need to get off the ground. The ExoMars launch will be taking place on March 14.

The Proton Rocket that will carry ExoMars space probes to orbit. Image Credit: KhSC / ESA


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