Scientists have discovered a new type of water cycle on Mars, which is a bit surprising given the generally severe lack of water on the planet. According to a new study, water vapor rises from the lower atmosphere to Mars’ upper atmosphere, and some of it even escapes into space, but this can only happen under very limited conditions. This finding may also help explain how Mars lost most of its water billions of years ago.
The intriguing new results were published in the current issue of the peer-reviewed journal Geophysical Research Letters on April 16, 2019, by researchers from the Moscow Institute of Physics and Technology (MIPT) and the Max Planck Institute for Solar System Research (MPS) in Germany.
Computer simulations showed that, surprisingly, water vapor can rise from the lower atmosphere and pass through the colder middle atmosphere into the upper atmosphere, but only under certain circumstances. This unique movement of water vapor occurs about every two years, during summer in the southern hemisphere. Some of the water vapor is carried by winds to the north pole, while the rest of it decays and escapes into space. This could be how Mars lost most of its water vapor in the distant past, as well.
So how is the water vapor able to pass through the cold barrier in the middle atmosphere? The researchers think there is a previously unknown mechanism at work, which acts sort of like a pump. The middle atmosphere is normally very cold, making it difficult for water vapor to go through it. But twice a day – and only at a certain location and at a certain time of year – that barrier becomes more permeable. At those times, the water vapor can sneak through the middle atmosphere and enter the upper atmosphere.
The water vapor cools in the upper atmosphere, where some of it finds its way to the north pole and sinks downward again. But some of the water molecules are disintegrated by solar radiation at those extreme heights, and escape into space.
The orbit of Mars is a key factor in how this process works. Its orbit is about twice as long as Earth’s, two years, and much more elliptical. It is summer in Mars’ southern hemisphere when the planet is closest to the sun, about 26 million miles (42 million km) closer than at its farthest point, and the summer temperatures in Mars’ southern hemisphere are therefore significantly warmer than summer temperatures in its northern hemisphere. This makes it easier for water vapor to rise through the atmosphere at that time. According to Paul Hartogh from MPS:
When it is summer in the southern hemisphere, at certain times of day water vapor can rise locally with warmer air masses and reach the upper atmosphere.
This, combined with the pump mechanism, means that doing those relatively brief moments, water vapor can actually ascend all the way through the atmosphere, even into space. But there is also another process that can help with this: dust storms. Dust storms on Mars can be monsters, even encircling the entire planet sometimes. The dust particles heat up and can increase the atmospheric temperature by as much as 30 degrees. The dust can also lift water vapor high up into the atmosphere, as noted by Alexander Medvedev from MPS:
The amounts of dust swirling through the atmosphere during such a storm facilitate the transport of water vapor into high air layers.
One huge dust storm was in 2007, and the researchers calculated that it lofted approximately twice as much much vapor in to the upper atmosphere than would normal occur. As explained by Dmitry Shaposhnikov of MIPT, first author of the new study:
Our model shows with unprecedented accuracy how dust in the atmosphere affects the microphysical processes involved in the transformation of ice into water vapor.
As Hartogh also commented:
Apparently, the Martian atmosphere is more permeable to water vapor than that of the Earth. The new seasonal water cycle that has been found contributes massively to Mars’ continuing loss of water.
The Martian atmosphere is also now so thin, it can’t hold onto nearly as much water vapor as it used to a few billion years ago. And even today, it seems that whatever vapor there is can, at times, easily escape out into space. Scientists also think that Mars’ atmosphere overall was once much thicker than it is now, which could have held much more water vapor, like Earth does today. Rain, rivers and lakes were all possible at this time, and perhaps even an ocean in the northern hemisphere, as some scientists now think. Now it is mostly ice on and below the surface, with some evidence for liquid water lakes deeper down, and much less water vapor. How Mars changed so much has long been a mystery to scientists, but now thanks to studies like this one, researchers are finally learning how the planet changed from a more Earth-like world to the cold, dry desert we see today.
Bottom line: Mars doesn’t have a lot of water left, other than ice and some liquid water deeper down, but it does still have an active water cycle in the atmosphere. This new study not only shows how the cycle works, but might also help explain why Mars lost most of its water vapor – and atmosphere overall – in the first place.
Paul Scott Anderson has had a passion for space exploration that began when he was a child when he watched Carl Sagan’s Cosmos. While in school he was known for his passion for space exploration and astronomy. He started his blog The Meridiani Journal in 2005, which was a chronicle of planetary exploration. In 2015, the blog was renamed as Planetaria. While interested in all aspects of space exploration, his primary passion is planetary science. In 2011, he started writing about space on a freelance basis, and now currently writes for AmericaSpace and Futurism (part of Vocal). He has also written for Universe Today and SpaceFlight Insider, and has also been published in The Mars Quarterly and has done supplementary writing for the well-known iOS app Exoplanet for iPhone and iPad.