The size, evolution, and duration of standing bodies of water, such as lakes, on Mars' surface are still a matter of great debate.

MOLA Science Team; image composition: S. Adeli (DLR) There is a wealth of evidence, collected over the past few decades, suggesting liquid water was abundant in the early history of Mars. However, the size, evolution, and duration of standing bodies of water such as lakes on Mars' surface are still a matter of great debate. A recent study paints a detailed picture of the rise and fall of standing bodies of water in a region of Mars that once hosted one of its largest lakes. The study uses data from several spacecraft operating at Mars.



Mars' surface is speckled with basins thought to have once hosted extensive lakes and rivers. The basins left behind by these long since dried-up bodies of water capture an important record of the geological and environmental conditions endured by the regions, making them prime candidates for exploration and study.



A recent paper describes a study of an area of Mars’ surface known as the Terra Sirenum region, carried out by Solmaz Adeli, Ernst Hauber, Laetitia Le Deit, and Ralf Jaumann, which is thought to have played host to one of the largest lakes on Mars. The body of water, known as the Eridania Lake, once covered an area of over a million square kilometers before dividing into smaller isolated lakes and eventually disappearing altogether along with the rest of the water on the planet.



This study focuses on the geological events that occurred before, during, and after the transformation of the gargantuan Eridania Lake into its hypothesized smaller lakes by looking closely at four ancient basins. Each of the four basins — Atlantis Chaos, Simois Colles, Caralis Chaos, and an unnamed basin referred to in the study as the Northern Basin – hosted its own individual lake following the fragmentation of the Eridania Lake.



By combining data from the High Resolution Stereo Camera (HRSC) on ESA's Mars Express with images from both the High Resolution Imaging Science Experiment (HiRISE) and Context Camera (CTX) on NASA's Mars Reconnaissance Orbiter (MRO), the team has built up a detailed geological map for the region and accurately modeled the ages of the mapped units. This, complimented by data from MRO's mineral-finding Compact Reconnaissance Imaging Spectrometer (CRISM), used to characterize the distribution and nature of materials in the area, has enabled the team to interpret the geological history of the region, creating a detailed time frame of its formation and suggesting the most likely mechanisms that led to it.



MOLA Science Team "What we have done here is to combine different methods and vast amounts of data, including the newest available, to give a new perspective on the events that unfolded around one of Mars' most extensive lakes," said lead author of the study Solmaz Adeli, from the Institute of Planetary Research, German Aerospace Center (DLR). "This is not the first time this region has been studied, but by combining pieces of the morphological and mineralogical puzzle we are able to paint a much clearer picture of when material formed, how this important terrain evolved, and how the environment that shaped it changed."



"Very few geological maps have previously been produced for this area," said Ralf Jaumann from the DLR and the Free University of Berlin, Germany. "Now, we have investigated the relationships between key geological features in great detail, allowing us to much better constrain our knowledge of past martian climate, aqueous processes, and morphological evolution."



The oldest geological terrain, dating back to Mars' Noachian period around 4 billion years ago, is on the highlands that surround the basins. On top of this ancient, cratered surface relentlessly dented by a period of extreme asteroid and meteorite impact, can be seen a younger layer of material which was deposited through the air as dust and ash.



"This younger layer of material sits on the uplands atop the older material, moulded into flat-topped and steep-flanked structures known as Mesas," said Ernst Hauber from DLR. In the basins themselves, rather than having been sliced into Mesas by wind and water movement, the team found that this material had cracked and eroded to form dramatic knobs of material that extend up to 2,000 feet (600 meters) from the basin floors.



"What this tells us," continued Hauber, "is that when the material was deposited the Eridania Lake was still very much present, but the water level fell to the point that it was split into a series of smaller lakes early in the Hesperian period, and later in that period the individual basins too began to run dry."

