According to a study by scientists, methane in the atmosphere of Mars lasts less than a year. Sergio Fonti from the Universita del Salento in Italy and Giuseppe Marzo from NASA’s Ames Research Center in Mountain View, California, have used observations from NASA’s Mars Global Surveyor spacecraft to track the evolution of the gas over 3 martian years.
“Only small amounts of methane are present in the martian atmosphere, coming from very localized sources,” Fonti said. “We’ve looked at changes in concentrations of the gas and found that there are seasonal and also annual variations. The source of the methane could be geological activity or it could be biological — we can’t tell at this point. However, it appears that the upper limit for methane lifetime is less than a year in the martian atmosphere.”
Levels of methane are highest in autumn in the northern hemisphere, with localized peaks of 70 parts per billion, although methane can be detected across most of the planet at this time of year. There is a sharp decrease in winter, with only a faint band between 40° and 50° north. Concentrations start to build again in spring and rise more rapidly in summer, spreading across the planet.
“One of the interesting things that we’ve found is that in summer, although the general distribution pattern is much the same as in autumn, there are actually higher levels of methane in the southern hemisphere,” said Fonti. “This could be because of the natural circulation occurring in the atmosphere, but has to be confirmed by appropriate computer simulations.”
There are three regions in the northern hemisphere where methane concentrations are systematically higher: Tharsis and Elysium, the two main volcano provinces, and Arabia Terrae, which has high levels of underground water ice. Levels are highest over Tharsis, where geological processes, including magmatism, hydrothermal, and geothermal activity, could be ongoing.
“It’s evident that the highest concentrations are associated with the warmest seasons and locations where there are favorable geological and, hence, biological conditions such as geothermal activity and strong hydration,” Fonti said. “The higher energy available in summer could trigger the release of gases from geological processes or outbreaks of biological activity.”
The mechanisms for removing methane from the atmosphere are also not clear. Photochemical processes would not break down the gas quickly enough to match observations. However, wind-driven processes can add strong oxidizers to the atmosphere, such as the highly reactive salt perchlorate, which could soak up methane more rapidly.
Martian years are nearly twice as long as Earth years. The team used observations from the Thermal Emission Spectrometer (TES) on Mars Global Surveyor between July 1999 and October 2004, which corresponds to 3 martian years. The team studied one of the characteristic spectral features of methane in nearly 3 million TES observations, averaging data together to eliminate noise.
“Our study is the first time that data from an orbiting spectrometer has been used to monitor methane over an extended period,” said Fonti. “The huge TES dataset has allowed us to follow the methane cycle in the martian atmosphere with unprecedented accuracy and completeness. Our observations will be very useful in constraining the origins and significance of martian methane.”
Methane was first detected in the martian atmosphere by ground-based telescopes in 2003 and confirmed a year later by the European Space Agency’s (ESA) Mars Express spacecraft. Observations using ground based telescopes showed the first evidence of a seasonal cycle last year.
The atmosphere on Mars consists of 95 percent carbon dioxide, 3 percent nitrogen, 1.6 percent argon, and contains traces of oxygen and water, as well as methane.
