Methane 'belches' detected on Mars

© NASA/JPL/CALTECH/MSSS

The US space agency's (Nasa) Curiosity rover has detected the intermittent "belching" of methane gas on Mars.

The robot sees very low-level amounts constantly in the background, but it also has monitored a number of short-lived spikes that are 10 times higher.

Methane on the Red Planet is intriguing because here on Earth, 95% of the gas comes from microbial organisms.

Researchers have hung on to the hope that the molecule's signature at Mars might also indicate a life presence.

The Curiosity team cannot identify the source of its methane, but the leading candidate is underground stores that are periodically disturbed.

Curiosity scientist Sushil Atreya said it was possible that so-called clathrates were involved.

"These are molecular cages of water-ice in which methane gas is trapped. From time to time, these could be destabilised, perhaps by some mechanical or thermal stress, and the methane gas would be released to find its way up through cracks or fissures in the rock to enter the atmosphere," the University of Michigan professor told BBC News.

This, of course, still leaves open the question of how the methane (CH4) got into the clathrate stores in the first place.

It could have come from Martian bugs; it could also have come from a natural process, such as serpentinisation, which sees methane produced when water interacts with certain rock types.

At the moment, it is all speculation. But at least Curiosity has now made the detection.

Enriched samples

It was concerning that for many months the robot could not see a gas that was being observed by orbiting spacecraft at Mars and by telescopes at Earth.

People were beginning to wonder if the other sightings were reliable.

Curiosity is located in a deep bowl on Mars' equator known as Gale Crater.

It has been sucking in Martian air and scanning its components since shortly after landing in August 2012.

For gases that have very low concentrations in the atmosphere, the robot can employ a special technique in which it expels the most abundant molecule - carbon dioxide - before analysing the sample.

This has the effect of enriching and amplifying any residual chemistry.

And in doing this for methane, Curiosity finds that there is a persistent signature of about 0.7 parts per billion by volume.

To put that in context, in Earth's atmosphere, you would expect to see around 1,750 parts per billion by volume of air. It is the difference between a few tens of thousands of tonnes in Mars' air, and the many billions of tonnes that exist in Earth's atmosphere.

The background detection is a bit lower than theoretical models had anticipated. It was thought that just the action of sunlight on the carbon compounds in cosmic dust falling to Mars would release a certain level of CH4.

"I don't think there is a big disagreement there; our result is to within an order of magnitude. That's quite satisfying," said Dr Paul Mahaffy, the lead investigator on Curiosity's Surface Analysis at Mars instrument.

Life's preference

The spikes in methane that Curiosity saw occurred on four occasions during the course of a two-month period.

They varied between about 7 and 9 parts per billion by volume.

It is likely, the team says, that the gas is being released relatively nearby, either within the crater or just outside.

Curiosity's weather station suggests it is blowing in from the north, from the direction of the crater rim.

One way to investigate whether the methane on Mars has a biological or a geological origin would be to study the types, or isotopes, of carbon atom in the gas.

On Earth, life favours a lighter version of the element (carbon-12), over a heavier one (carbon-13).

A high C-12 to C-13 ratio in ancient Earth rocks has been interpreted as evidence that biological activity existed on our world as much as four billion years ago.

If scientists could find similar evidence on Mars, it would be startling. But, sadly, the volumes of methane detected by Curiosity are simply too small to run this kind of experiment.

"If we had enriched our sample during one of the peaks, we might have had a shot at looking at these isotopes," explained Dr Mahaffy.

"I think there is still some hope. If the methane comes back, and we can enrich it, we'll certainly be trying."

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