Contours seen on Mars may have been created by run-off rainwater, say scientists who found that branching angles of the valleys on the red planet were very similar to those found in arid landscapes on Earth. The surface of Mars bears imprints of structures that resemble fluvial steam networks on Earth. Scientists therefore assume that there must have been once enough water on the red planet to feed water streams that incised their path into the soil.
For years, however, scientists have been debating the source from which this water must have originated. A study, published in Science Advances, suggests that the branching structure of the former river networks on Mars has striking similarities with terrestrial arid landscapes. Using statistics from all mapped river valleys on Mars, researchers conclude that the contours still visible today must have been created by superficial run-off of rainwater.
Consequently, the influence of groundwater seepage from the soil can be excluded as a dominant process for shaping these features. The distribution of the branching angles of the valleys on Mars is very similar to those found in arid landscapes on Earth. This implies that there must have been a similar hydrological environment with sporadic heavy rainfall events on Mars over a prolonged period of time and that this rainwater may have run off quickly over the surface shaping the valley networks.
This is how river valleys develop in arid regions on Earth. For example, in Arizona, researchers observed the same valley network patterns in a landscape where astronauts are training for future Mars missions. Valleys in arid regions fork at a narrow angle.
The branching angles on Mars are comparatively low. Seybold therefore rules out the influence of groundwater sapping as the major channel forming process on Mars. River networks that are formed by re-emerging groundwater, as found, for example, in Florida, tend to have much wider branching angles between the two tributaries and do not match the narrow angles of streams in arid areas. Conditions such as those found in terrestrial arid landscapes today probably prevailed on Mars for only a relatively short period about 3.6 to 3.8 billion years ago.
In that period, the atmosphere on Mars may have been much denser than it is today. "Recent research shows that there must have been much more water on Mars than previously assumed," said Hansjorg Seybold, a professor at ETH Zurich.
One hypothesis suggests that the northern third of Mars was covered by an ocean at that time. Water evaporated, condensed around the high volcanoes of the highlands to the south of the ocean and led to heavy precipitation. As a result, rivers formed, which left traces that can still be observed on Mars today. The big question is where the water has disappeared to over time. "It's likely that most of it evaporated into space. But it could still be found in the vicinity of Mars. This is a question for a future space mission," said Seybold.
