Skip to main content

What’s up with the methane on Mars? Curiosity is finding out

A selfie of NASA's Curiosity Mars rover taken at a location nicknamed "Mary Anning" after a 19th century English paleontologist.
NASA’s Curiosity Mars rover took this selfie at a location nicknamed “Mary Anning” after a 19th century English paleontologist. NASA/JPL-Caltech/MSSS

Something complicated is going on with the presence of methane on Mars. Methane is an important chemical for astrobiologists because it can be created by living animals and microbes, although it can also be created by non-organic processes as well. Previous studies have found indications of methane on Mars — but not consistently. Some instruments have found methane there, others have not. Now, a new study hopes to unravel this mystery by examining the differences in methane levels between Martian day and night.

Methane on Mars was detected above the surface of the Gale Crater by the Curiosity rover, but not in the high atmosphere by the Trace Gas Orbiter (TGO), a European Space Agency spacecraft in orbit around the planet which takes highly accurate readings. This came as a surprise to scientists.

Recommended Videos

“When the Trace Gas Orbiter came on board in 2016, I was fully expecting the orbiter team to report that there’s a small amount of methane everywhere on Mars,” said Chris Webster, lead of the Tunable Laser Spectrometer (TLS) instrument in the Sample Analysis at Mars (SAM) chemistry lab aboard the Curiosity rover. “But when the European team announced that it saw no methane, I was definitely shocked.”

Please enable Javascript to view this content

To try to understand what was happening, Webster’s team considered the possibility that the methane was coming from the rover itself. “So we looked at correlations with the pointing of the rover, the ground, the crushing of rocks, the wheel degradation — you name it,” Webster said. “I cannot overstate the effort the team has put into looking at every little detail to make sure those measurements are correct, and they are.”

So the next possibility was that somehow both Curiosity and the TGO readings were correct, and that differences were due to Mars’s day-night cycle. The TLS instrument on Curiosity operates mostly at night, as it requires a lot of power, while the TGO operates during the day as it needs sunlight. Co-author John E. Moores explained that the methane could build up at night when the atmosphere is calm, and be dissipated during the day by the warmth of the sun affecting the atmosphere.

“Any atmosphere near a planet’s surface goes through a cycle during the day,” Moores said. “So I realized no instrument, especially an orbiting one, would see anything.”

Further experiments using Curiosity support this theory, showing that methane levels were effectively zero during the day in the Gale Crater.

So that may answer what is happening in this particular region, although there remains a larger question about the global methane levels on Mars. Unless Gale Crater is the only place where methane is leaking out of the rocks, which seems unlikely, some methane should still be visible to the orbiter.

The researchers are now undertaking more experiments to find out what is happening to the methane between the surface level and the atmosphere.

Georgina Torbet
Georgina has been the space writer at Digital Trends space writer for six years, covering human space exploration, planetary…
Check out this incredible cloud atlas of Mars
Arsia Mons Elongated Cloud (AMEC): This elongated cloud has formed as a result of wind encountering the Arsia Mons mountains. It forms almost every day during a specific season, from early morning until noon.

Photographing a beautiful sky is a great passion for many here on Earth, but it can be just as striking on another planet too. Researchers recently presented a stunning new "cloud atlas" of Mars: a database containing 20 years' worth of images of clouds and storms observed on the red planet.

The cloud atlas is available online, inviting you to browse the many images of martian weather captured by the Mars Express spacecraft. This European Space Agency mission has been in orbit around Mars since 2005, and has taken hundreds of images of the planet using its High Resolution Stereo Camera (HRSC) instrument.

Read more
Perseverance rover gears up for a big climb to the rim of the Jezero Crater
One of the navigation cameras aboard NASA’s Perseverance Mars rover captured this view looking back at the “Bright Angel” area on July 30, the 1,224th Martian day, or sol, of the mission.

The Perseverance rover on Mars is set to begin its newest challenge: a slog up the rim of the Jezero Crater that will take months to complete. The rover will face steep slopes and difficult terrain, testing its wheels and suspension system, but its efforts should help to uncover rocks from the most ancient part of the Mars crust.

Since the rover landed in the Jezero Crater in 2021, it has been exploring the floor of the crater and the site of an ancient river delta. This area was chosen because it was once home to an ancient lake, so the rock cores that the rover has collected will help to uncover information about the history of water on Mars -- which is vital to determine if the planet could ever have been habitable.

Read more
Mars has ‘oceans’ worth’ of water – but it’s deep underground
More than 3 billion years ago, Mars was warm, wet, and had an atmosphere that could have supported life. This artist's rendering shows what the planet may have looked like with global oceans based on today's topography.

One of the key issues for getting humans to Mars is finding a way to get them water. Scientists know that millions of years ago, Mars was covered in oceans, but the planet lost its water over time and now has virtually no liquid water on its surface. Now, though, researchers have identified what they believe could be oceans' worth of water on Mars. There's just one snag: it's deep underground.

The research used data from NASA's now-retired InSight lander, which used a seismometer and other instruments to investigate the planet's interior. They found evidence of what appears to be a large underground reservoir of water, enough to cover the entire planet in about a mile of ocean. But it's inaccessible, being located between 7 to 13 miles beneath the planet's surface. The water is located in between cracks in a portion of the interior called the mid-crust, which sits beneath the dry upper crust that is drillable from the surface.

Read more