Mount Sharp, officially known as Aeolis Mons, forms the central peak within a very large crater named Gale that is 155 km in diameter.
The mountain stands about 5 km tall, its lower flanks exposing hundreds of rock layers. The rock layers – alternating between lake, river and wind deposits – bear witness to the repeated filling and evaporation of a lake much larger and longer-lasting than any previously examined close-up.
“If our hypothesis for Mount Sharp holds up, it challenges the notion that warm and wet conditions were transient, local, or only underground on Mars. A more radical explanation is that Mars’ ancient, thicker atmosphere raised temperatures above freezing globally, but so far we don’t know how the atmosphere did that,” said team member Dr Ashwin Vasavada of NASA’s Jet Propulsion Laboratory in Pasadena, California.
“We are making headway in solving the mystery of Mount Sharp. Where there’s now a mountain, there may have once been a series of lakes,” added team member Dr John Grotzinger of the California Institute of Technology in Pasadena.
Curiosity currently is investigating the lowest sedimentary layers of Mount Sharp, a section of rock 150 m high, dubbed the Murray formation. Rivers carried sand and silt to the lake, depositing the sediments at the mouth of the river to form deltas similar to those found at river mouths on Earth. This cycle occurred over and over again.
“The great thing about a lake that occurs repeatedly, over and over, is that each time it comes back it is another experiment to tell you how the environment works,” Dr Grotzinger said.
“As Curiosity climbs higher on Mount Sharp, we will have a series of experiments to show patterns in how the atmosphere and the water and the sediments interact. We may see how the chemistry changed in the lakes over time.”
“This is a hypothesis supported by what we have observed so far, providing a framework for testing in the coming year.”
After the Gale crater filled to a height of at least a few hundred meters and the sediments hardened into rock, the accumulated layers of sediment were sculpted over time into a mountainous shape by wind erosion that carved away the material between the crater perimeter and what is now the edge of the mountain.
On the 8-km journey from the rover’s landing site to its current work site at the base of Mount Sharp, Curiosity uncovered clues about the changing shape of the crater floor during the era of lakes.
“We found sedimentary rocks suggestive of small, ancient deltas stacked on top of one another. Curiosity crossed a boundary from an environment dominated by rivers to an environment dominated by lakes,” said team member Dr Sanjeev Gupta of Imperial College in London.
“Knowledge we’re gaining about Mars’ environmental evolution by deciphering how Mount Sharp formed will help guide plans for future missions to seek signs of Martian life,” said Dr Michael Meyer, lead scientist for the Mars Exploration Program at NASA headquarters in Washington, DC.