“We don’t yet know where methane on Mars comes from,” tweeted Thomas Zurbuchen, NASA’s Associate Administrator for the Science Mission Directorate. “A leading idea is that methane on Mars is being released from underground reservoirs created by past biology. But sometimes, methane is a sign of geology rather than biology.”
Hundreds of millions of miles from Earth, NASA’s Curiosity rover has caught a whiff of methane on the Red Planet. On four occasions in late 2013 and 2014, the rover sniffed the air and found relatively intense concentrations of methane—a ten-fold increase compared to earlier measurements. This confirmed earlier detections of methane on Mars from ground-based observatories on Earth.
“Given this surprising result, we’ve reorganized the weekend to run a follow-up experiment,” Ashwin R. Vasavada, the project scientist for the mission, wrote to the science team in an email that was obtained by The Times. The mission’s controllers on Earth sent new instructions to the rover on Friday to follow up on the readings, bumping previously planned science work. The results of these observations are expected back on the ground on Monday.
NASA acknowledged the methane detection in a statement Saturday afternoon, but called it an “early science result.” The agency’s spokesperson added, “To maintain scientific integrity, the project science team will continue to analyze the data before confirming results.”
While methane is actually odorless and colorless, to many researchers, methane is sweet. To exobiologists, writes NASA, it is the aroma of life. To planetary scientists, it is a greenhouse gas and a key ingredient of atmospheres on a variety of worlds. On Mars, it is a scientific bonanza.
Here on Earth, most methane comes from life—mainly from anaerobic microbes called methanogens, such as in the guts of cows but also from the decay of plant matter and other biological processes in places like wetlands. Does methane on Mars suggest life there, too?
Mike Mumma of the Goddard Space Flight Center in Greenbelt, MD says, “A leading idea is that methane on Mars is being released from underground reservoirs created by past biology.”
Sometimes methane is a sign of geology rather than biology. On Earth, for instance, volcanoes produce methane. There are no currently active volcanoes on Mars, but scientists are studying the possibilities of methane being released through other geological processes as well. These processes involve reactions of carbon from carbonate rocks or CO2 gas, with hydrogen from liquid water. At the right temperatures these reactions produce methane. The methane Curiosity has been sniffing could be evidence of these reactions.
On our planet, methane can come from many sources including oil and gas systems, coal mining, landfills and wastewater, and microbial metabolism in wetland ecosystems. Charles Miller of NASA’s Jet Propulsion Laboratory and his team are using data from NASA’s airborne CARVE mission to investigate methane emissions from thawing permafrost and tundra, and what these emissions mean for the sensitivity of Arctic ecosystems to warming. Data from CARVE shows increasing methane emissions persisting deeper into the cold season, as climate change keeps sub-surface soil temperatures above freezing later into the autumn as far north as the North Slope of Alaska. This knowledge should help improve the accuracy of global carbon cycle models.
At the other end of the solar system, NASA’s New Horizons spacecraft has found methane on Pluto. Some mountains on the dwarf planet are dusted with methane “snow.” Pluto’s atmosphere is, essentially, a 1000 mile-high bubble of nitrogen spiced with methane and other less abundant gases. On Pluto, methane reacts with UV sunlight to produce a type of extraterrestrial smog. On Saturn’s giant moon Titan, methane appears in liquid form, filling lakes and seas. It is also present in Titan’s atmosphere, being broken apart by UV rays to create some of the same smog-like particles found on Pluto.
Wherever it comes from, methane is an important greenhouse gas, approximately 25 times more potent per molecule than carbon dioxide over a 100-year period. One reason scientists track methane is to quantify methane’s contribution to greenhouse warming. Additionally, the breakup of methane can lead to the destruction of ozone. Earth’s ozone layer is crucial to protecting life on our planet from harsh solar ultraviolet rays. Mars has an ozone layer, too, (several of them, in fact) even more fragile than Earth’s. Methane could pose a threat to ozone on the red planet.
“Since the big methane spikes of 2013 and 2014, the gas has subsided but not vanished. Curiosity is currently sensing methane at very low, yet still variable, levels,” says Mumma.
Mumma is looking forward to measurements from a new spacecraft that could clarify what’s going on. Europe’s Trace Gas Orbiter was launched in March and will orbit Mars in October of 2016. This spacecraft will be able to monitor methane as well as other trace gases Curiosity is detecting. Within a year of its arrival, the Trace Gas Orbiter will attempt to map the entire planet and identify areas of methane release.
“Once we know where the gas is coming from, we could target future missions to investigate the methane at its source,” said Mumma.
Image credit: JPL/Caltech