Methane

Methane is the lightest of the hydrocarbons, consisting of a single carbon atom bonded to four hydrogen atoms in a tetrahedral configuration. It is volatile, and tends to break down quite quickly by being oxidized, so presence of atmospheric methane is often considered to be an indication of the presence of life. However, methane can also be produced be non-biological processes such as volcanic activity. Methane is also an efficient greenhouse gas, contributes to global warming and may be a useful gas for the process of terraforming.

Methane is of particular interest for missions to Mars, as it may be possible to produce it in situ using locally-available raw materials. This would make it an ideal fuel for rovers and rocket engines.

This article discusses organic (?) methane discoveries on Mars.

Discovery in Atmosphere

There have been reports of methane in the Martian atmosphere, but these are at the edge of the instrument's error bars. Curiosity detected sudden spikes in methane which are hard to explain (since methane should be well mixed in the atmosphere) unless the burst of methane appeared very close to the rover.

Further, early reports put methane 10 times higher than later reports. This is hard to explain, since methane should have a half life of ~300 years in Martian conditions. For these reasons, detection of methane should be regarded as preliminary, and we may wish to wait for stronger data.

See Photochemistry for a discussion on how methane breaks down in the Martian Atmosphere.

In 2004, the Mars Express mission detected methane in the Martian atmosphere at a level of approx. 10 parts per billion. This was later confirmed by Earth-based spectroscopy. Methane is quickly decomposed in the martian atmosphere, so some source, either geologic or biological, is replenishing the gas.

Methane plumes have been detected over areas thought to have had water in the past.

Synthesis of methane

Production of methane on the surface of Mars would likely be via the Sabatier reaction:

CO₂ + 4H₂   ↔   CH₄ + 2H₂O

The forward reaction takes place in the presence of high temperatures and pressures, in the presence of a nickel catalyst. All of the raw materials should be available on the surface of Mars:

• The atmosphere contains a high proportion of carbon dioxide.
• Hydrogen could be obtained by electrolysis of indigenous water (although some schemes call for the hydrogen to be imported).

This process could also be used during a trip to or from Mars to scrub CO₂ from a spacecraft atmosphere.

Instead of nickel, a catalyst made out of ruthenium or alumina could be used.

Uses for methane

Methane works well as a rocket fuel, and a number of LOX/methane fueled rockets are under development, including the XCOR XR5M15, Northrop Grumman TR408, the SpaceX Starship and Booster as well as the Blue Origin rockets.

Methane fuel cells have recently been demonstrated, and these would work well for powering rovers, semi-portable equipment or as backup generators. It can play an important part in an energy storage‎ infrastructure.

Carbon in the form of pyrolytic graphite could be recovered from methane by pyrolyzing it:

CH₄ + heat   →   2H₂ + C

The graphite so formed could be used for ablative surfaces, reinforcement of polymer materials, furnace linings or control elements in nuclear reactors.

See also

• The Curious Case for Methane on Mars: Methane and Active Organics Discovered on Mars

External Links

• Wikipedia article on Methane
• Wikipedia article on the Sabatier reaction
• ESA press release on detection of methane by Mars Express