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Salt flat indicates some of the last vestiges of Martian surface water

Date:
August 7, 2015
Source:
University of Colorado at Boulder
Summary:
Mars turned cold and dry long ago, but researchers have discovered evidence of an ancient lake that likely represents some of the last potentially habitable surface water ever to exist on the Red Planet.
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This is a perspective rendering of the Martian chloride deposit.
Credit: LASP / Brian Hynek

Mars turned cold and dry long ago, but researchers at the University of Colorado Boulder have discovered evidence of an ancient lake that likely represents some of the last potentially habitable surface water ever to exist on the Red Planet.

The study, published in the journal Geology, examined an 18-square-mile chloride salt deposit (roughly the size of the city of Boulder) in the planet's Meridiani region near the Mars Opportunity rover's landing site. As seen on Earth in locations such as Utah's Bonneville Salt Flats, large-scale salt deposits are considered to be evidence of evaporated bodies of water.

Digital terrain mapping and mineralogical analysis of the features surrounding the deposit indicate that this one-time lakebed is no older than 3.6 billion years old, well after the time period when Mars is thought to have been warm enough to sustain large amounts of surface water planet-wide. Planetary scientists believe that the solar system formed approximately 4.6 billion years ago.

"This was a long-lived lake, and we were able to put a very good time boundary on its maximum age," said Brian Hynek, a research associate at the Laboratory for Atmospheric and Space Physics (LASP) at CU-Boulder and lead author of the study. "We can be pretty certain that this is one of the last instances of a sizeable lake on Mars."

Based on the extent and thickness of the salt, the researchers estimate that the lake was only about 8 percent as salty as Earth's oceans and therefore may have been hospitable to microbial life.

"By salinity alone, it certainly seems as though this lake would have been habitable throughout much of its existence," said Hynek, who is also an associate professor in the Department of Geological Sciences at CU-Boulder and director of the CU Center for Astrobiology. He noted, however, that other factors such as acidity levels were not included in the scope of the study.


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Materials provided by University of Colorado at Boulder. Note: Content may be edited for style and length.


Journal Reference:

  1. Brian M. Hynek, Mikki K. Osterloo, Kathryn S. Kierein-Young. Late-stage formation of Martian chloride salts through ponding and evaporation. Geology, 2015; G36895.1 DOI: 10.1130/G36895.1

Cite This Page:

University of Colorado at Boulder. "Salt flat indicates some of the last vestiges of Martian surface water." ScienceDaily. ScienceDaily, 7 August 2015. <www.sciencedaily.com/releases/2015/08/150807110738.htm>.
University of Colorado at Boulder. (2015, August 7). Salt flat indicates some of the last vestiges of Martian surface water. ScienceDaily. Retrieved May 23, 2017 from www.sciencedaily.com/releases/2015/08/150807110738.htm
University of Colorado at Boulder. "Salt flat indicates some of the last vestiges of Martian surface water." ScienceDaily. www.sciencedaily.com/releases/2015/08/150807110738.htm (accessed May 23, 2017).

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