Rounded Stones on Mars are Evidence of Flowing Water
NASA’s Curiosity rover has returned images of what may have been a riverbed on Mars. The observations were made with Curiosity’s stereo camera and reveal areas with densly packed gravel and pebbles. The pebbles are cemented together like concrete. After studying the size and shape of the pebbles, a team of scientists has reported that the features are clear evidence of flowing water on ancient Mars. According to the study, the depth of the liquid ranged between 0.03 meters to 0.9 meters.
“In order to have moved and formed these rounded pebbles, there must have been flowing water with a… flow rate of about 1 meter per second – or 3.6 km/h – slightly faster than a typical natural Danish stream.”
- Morten Bo Madsen, head of the Mars research group at the Niels Bohr Institute
Why is this research important to Astrobiology?
The potential for life on Mars (and other celestial bodies beyond Earth) is on of the major areas of study for astrobiologists. NASA’s Astrobiology Program lists the search for life in our solar system as one of the program’s major goals in the NASA Astrobiology Roadmap.
Because life as we know it requires liquid water to survive, the questions about life’s potential on Mars currently center around whether or not environments with liquid water once existed on the surface of the planet. This new research supports the idea that liquid was indeed present, indicating that habitats where life could have gained a foothold may have once been present on ancient Mars.
Where can you read more about this research?
The scientific paper, "Martian Fluvial Conglomerates at Gale Crater" was published in the journal Science under lead author R.M.E. Williams. The abstract is available at: http://www.sciencemag.org/content/340/6136/1068
Astrobiology Magazine contacted Dr. Rebecca Williams, lead author of the study, with some additional questions about his research:
Astrobiology Magazine: Is there any other process that could have created these formations? Why is flowing water the most likely explanation?
Williams: The rounded shape of the pebbles is a testament to a transport process, either wind or water. Rocks that exceed a few mm in size are too large to move by wind. The typical pebble size is around 1 cm, and the largest rocks are 4 cm across. Thus, at this size, fluvial transport is the most likely process.
AM: How widespread are these features in the Curiosity landing site? Are they commonly seen in the area that the rover has explored so far?
Williams: We’ve encountered a half-dozen outcrops of these water-transported conglomerated during our journey across Bradbury Rise. These are patchy occurrences and we are hoping to find more exposures as we travel back across this terrain en route to Mount Sharp. The MSL science team has a number of hypotheses for how these conglomerates relate to other rocks in this area, including the ones we have drilled near Glenelg, and seeing additional conglomerates will help refine our understanding of the overall ancient environment.
AM: Why is the study area named ‘Hottah’?
Williams: The MSL science team names rocks and other science targets for ease of reference. Generally the names are for noteworthy geological sites on Earth. At noteworthy sites, we also pay tribute to the memory of individuals who have contributed significantly to the mission.
AM: How can you tell the depth and flow rate of the water that created these features?
Williams: Using what we know about the physics of water flow and the motion of rocks in rivers, we can estimate the minimum water flow conditions required to move rocks of this size on Mars.
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