Spectacular satellite images suggest that Mars was warm enough to sustain lakes three billion years ago, a period that was previously thought to be too cold and arid to sustain water on the surface, according to research published today in the journal Geology.
The research, by a team from Imperial College London and University College London (UCL), suggests that during the Hesperian Epoch, approximately 3 billion years ago, Mars had lakes made of melted ice, each around 20km wide, along parts of the equator.
Earlier research had suggested that Mars had a warm and wet early history but that between 4 billion and 3.8 billion years ago, before the Hesperian Epoch, the planet lost most of its atmosphere and became cold and dry. In the new study, the researchers analysed detailed images from NASA's Mars Reconnaissance Orbiter, which is currently circling the red planet, and concluded that there were later episodes where Mars experienced warm and wet periods.
The researchers say that there may have been increased volcanic activity, meteorite impacts or shifts in Mars' orbit during this period to warm Mars' atmosphere enough to melt the ice. This would have created gases that thickened the atmosphere for a temporary period, trapping more sunlight and making it warm enough for liquid water to be sustained.
Lead author of the study, Dr Nicholas Warner, from the Department of Earth Science and Engineering at Imperial College London, says:
"Most of the research on Mars has focussed on its early history and the recent past. Scientists had largely overlooked the Hesperian Epoch as it was thought that Mars was then a frozen wasteland. Excitingly, our study now shows that this middle period in Mars' history was much more dynamic than we previously thought."
The researchers used the images from the Mars Reconnaissance Orbiter to analyse several flat-floored depressions located above Ares Vallis, which is a giant gorge that runs 2,000 km across the equator of Mars. Scientists have previously been unable to explain how these depressions formed, but believed that the depressions may have been created by a process known as sublimation, where ice changes directly from its solid state into a gas without becoming liquid water. The loss of ice would have created cavities between the soil particles, which would have caused the ground to collapse into a depression.
In the new study, the researchers analysed the depressions and discovered a series of small sinuous channels that connected them together. The researchers say these channels could only be formed by running water, and not by ice turning directly into gas.
The scientists were able to lend further weight to their conclusions by comparing the Mars images to images of thermokarst landscapes that are found on Earth today, in places such as Siberia and Alaska. Thermokarst landscapes are areas where permafrost is melting, creating lakes that are interconnected by the same type of drainage channels found on Mars.
The team believe the melting ice would have created lakes and that a rise in water levels may have caused some of the lakes to burst their banks, which enabled water to carve a pathway through the frozen ground from the higher lakes and drain into the lower lying lakes, creating permanent channels between them.
Professor Jan-Peter Muller, Mullard Space Science Laboratory, Department of Space Climate Physics at University College London, was responsible for mapping the 3D shape of the surface of Mars. He adds:
"We can now model the 3D shape of Mars' surface down to sub-metre resolution, at least as good as any commercial satellite orbiting the Earth. This allows us to test our hypotheses in a much more rigorous manner than ever before."
The researchers determined the age of the lakes by counting crater impacts, a method originally developed by NASA scientists to determine the age of geological features on the moon. More craters around a geological feature indicate that an area is older than a region with fewer meteorite impacts. In the study, the scientists counted more than 35,000 crater impacts in the region around the lakes, and determined that the lakes formed approximately three billion years ago. The scientists are unsure how long the warm and wet periods lasted during the Hesperian epoch or how long the lakes sustained liquid water in them.
The researchers say their study may have implications for astrobiologists who are looking for evidence of life on Mars. The team say these lake beds indicate regions on the planet where it could have been warm and wet, potentially creating habitats that may have once been suitable for microbial life. The team say these areas may be good targets for future robotic missions.
The next step will see the team extend their survey to other areas along the equator of Mars so that they can ascertain how widespread these lakes were during the Hesperian Epoch. The team will focus their surveys on a region at the mouth of Ares Vallis called Chryse Planitia, where preliminary surveys of satellite images have suggested that this area may have also supported lakes.
The study was a collaboration between the Department of Earth Science and Engineering at Imperial College London and Space Physics at UCL. The project was funded by the Science and Technology Facilities Council, the Royal Society and the Leverhulme Trust.
Notes to editors:
1. *** Images and 3 D virtual reality video ***
Images are from the Context Camera (CTX) onboard NASA's Mars Reconnaissance Orbiter (MRO).
NASA Context Camera image of crater near Ares Vallis. The floor of the crater shows several irregular, flat-floored depressions that are interpreted as ancient lake basins. Scale bar is 10 km.
Download image: https://fileexchange.imperial.ac.uk/files/6e8a67a9d25/Fig.1_Lakes.jpg
NASA Context Camera image of depressions interpreted as ancient lake basins. Note channel connecting depressions in bottom right providing clear evidence of liquid exchange between depressions. Depression in centre is ~4 km wide.
Download image: https://fileexchange.imperial.ac.uk/files/4af0a2d480/Fig.2_Lakes.jpg
NASA Context Camera image of depressions interpreted as ancient lake basins. Note channel connecting depressions in bottom right providing clear evidence of liquid exchange between depressions. Depression in centre is ~3 km wide.
Download image: https://fileexchange.imperial.ac.uk/files/fa19869025d/Fig.3_Lakes.jpg
Close-up image from Fig.2_Lakes.jpg of channel connecting depressions. Fig.5 shows scale and arrows indicating channel.
Download image: https://fileexchange.imperial.ac.uk/files/9e1cfab32ff/Fig.5_Channel.jpg
Download image: https://fileexchange.imperial.ac.uk/files/9267947b628/Fig.5_Channel.jpg
PLEASE NOTE THAT COLOURS REPRESENT ELEVATION.
These images show topographic data for depressions interpreted as ancient lakes. Topography data illustrate that channels connect depressions of different depths suggesting lakes drained from shallower to deeper depressions.
Main depression in right hand image is ~40 metres deep.
Main depression at top left in left image is ~100 metres deep.
Download image: https://fileexchange.imperial.ac.uk/files/b64830dde6d/Fig.6_Topographic_image.jpg
3D virtual reality video of Ares Vallis
3D virtual reality video of Ares Vallis, which is a giant gorge that runs 2000 km across the equator of Mars. The lakes and their interconnecting channels can be seen a third of the way through the video. Dr Sanjeev Gupta, Imperial College London, is on hand to offer journalists a commentary about what they are seeing in the video. Please contact Colin Smith, +44 (0)207 594 6712, to arrange a telephone interview.
Topographic image is a 3D map constructed from a CTX stereo image pair by Prof. Jan-Peter Muller's team at Mullard Space Science Laboratory, Department of Space Climate Physics at University College London.
Ares Vallis 3D Movie © 2006 Planetary Visions. Stereoscopic animation by Andrew Wayne. Based on input image and topographic data from the High-resolution Stereo Camera (HRSC) onboard ESA's Mars Express spacecraft © UCL/ESA/DLR/FU Berlin.
2. "Hesperian equatorial thermokarst lakes in Ares Vallis as evidence for transient warm conditions on Mars", Geology, JANUARY 2010, vol. 38, p. 71-74.
Dr Sanjeev Gupta (1),Nicholas Warner (1), Jung-Rack Kim (2), Shih-Yuan Lin (2), and Jan Peter Muller (2)
(1) Department of Earth Science and Engineering, Imperial College London
(2) Mullard Space Science Laboratory, Department of Space Climate Physics, University College London, Holmbury St Mary Surrey RH5 6NT, UK
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