Traces of recent water found on Mars
The southern hemisphere of Mars is home to a crater that contains very well-preserved gullies and debris flow deposits.
Washington: The southern hemisphere of Mars is home to a crater that contains very well-preserved gullies and debris flow deposits.
The geomorphological attributes of these landforms provide evidence that they were formed by the action of liquid water in geologically recent time.
When sediment on a slope becomes saturated with water, the mixture may become too heavy to remain in place, leading to a flow of debris and water as a single-phase unit. This is called a debris flow. Debris flows on Earth often cause significant material destruction and even human casualties, when they occur in built-up areas. During a debris flow, a mixture of stones, gravel, clay and water moves rapidly down a slope. When the sediment subsequently stops, it displays characteristic surface features such as lobate deposits and paired levees along flow channels.
It is these landforms that Andreas Johnsson has identified on Mars. The research group has been able to compare the landforms on Mars with known debris flows on Svalbard with the aid of aerial photography and field studies. The debris flows on Mars provide evidence that liquid water has been present in the region.
Johnsson of the Department of Earth Sciences, University of Gothenburg, said their fieldwork on Svalbard confirmed our interpretation of the Martian deposits. What surprised them was that the crater in which these debris flows have formed is so young.
Crater statistics allowed Johnsson and his co-authors to determine that the age of the crater to be approximately 200,000 years. This means that the crater was formed long after the most recent proposed ice age on Mars, which ended around 400,000 years ago.
Johnsson said gullies are common on Mars, but the ones which have been studied previously are older, and the sediments where they have formed are associated with the most recent ice age.
He said that their study crater on Mars is far too young to have been influenced by theconditions that were prevalent then. This suggests that the meltwater-related processes that formed these deposits have been exceptionally effective also in more recent times.