Early reports of Red planet irrigation canals might have been greatly overstated, created by optical illusions and an intense desire for neighbors, but we're working with much better equipment and we can now absolutely say that Mars had water. Loads of it. That noise you hear is the "Looking for Martian Life" group having an awesome party.
Early images of "canals" tracing the surface of Mars were artifacts created by imperfections in early telescopes and the human eye, and while we still struggle along with the latter we've upgraded the hell out of the former. Current observations are images images are taken from the HiRISE orbiter, three hundred kilometers above the Martian surface (a tad closer than the original millions of miles). The original observers didn't have the option of just going there and having a look, you see.
The high-resolution images show unmistakable paleoshorelines, series of strandlines defining a four-hundred meter deep lake extending over thirty square kilometers. The shorelines are a particularly exciting place as land-water borders are among the most ecologically active regions on any planet - and the best at recording how that happened. Fossils and chemical evidence of organisms can be buried in the sediments, and now we know where to look on Mars.
The discovery of the ex-lake, which evaporated during one of Mars' massive environmental changes, has massive implications just by existing - but we're more awesome than that. The scanned shoreline is already an excellent contestant for the next "Where do we want to land on Mars?" competition so watch that sedimentary-space to see what happens."Most of the research on Mars has focused 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," said Nicholas Warner, Department of Earth Science and Engineering at Imperial College London who along with colleagues 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 analyzed 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.
The team 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 recent 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 be to survey 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.
Image Credits NASA/JPL: Some scientists believe that on an earlier, wetter Mars some craters may have served as beds for ancient lakes. An extremely interesting feature of the Gusev Crater is the large channel that enters it from the south. This may have been a source of water that produced a large lake within the crater.
Provided by The Daily Galaxy - Casey Kazan / Imperial College London and Eurekalert.org
