Was This Huge River Delta on Mars the Place Where its Oceans Finally Disappeared?

For some time, scientists have known that Mars was once a much warmer and wetter environment than it is today. However, between 4.2 and 3.7 billion years ago, its atmosphere was slowly stripped away, which turned the surface into the cold and desiccated place we know today. Even after multiple missions have confirmed the presence of ancient lake beds and rivers, there are still unanswered questions about how much water Mars once had.

One of the most important unanswered questions is whether or not large seas or an ocean ever existed in the northern lowlands. According to a new study by an international team of scientists, the Hypanis Valles ancient river system is actually the remains of a river delta. The presence of this geological feature is an indication that this river system once emptied into an ancient Martian sea in Mars’ northern hemisphere.

For the sake of their study, which recently appeared in the journal Earth and Planetary Science Letters under the title “The Hypanis Valles delta: The last highstand of a sea on early Mars?” – the international team consulted data from the Mars Reconnaissance Orbiter (MRO)  and the 2001 Mars Odyssey probe to investigate the morphology, sedimentary architecture, and depositional environment of the Hypanis Valles region.

This delta is what separates the southern highlands from the northern lowlands, where an ancient ocean is once believed to have existed – a theory which has remained unproven. Based on data from the MRO’s High Resolution Imaging Science Experiment (HiRISE) instrument and the 2001 Odyssey’s THermal EMission Imaging System (THEMIS), the team found compelling evidence that a large body of water once covered the northern third of Mars.

As Joel Davis – a postdoctoral researcher in the Planetary Surface Group at the Natural History Museum and a co-author of the paper – explained in a recent NHM press release:

“A Martian ocean means that Mars probably had a very Earth-like water cycle, with rivers, lakes, and now oceans, all of which probably interacted as part of a planet-wide system. We think this Earth-like hydrological cycle was active about 3.7 billion years ago, and started to shut down sometime after that. Our study is not definitive proof for an ocean, but these geological features are very hard to explain without one.”

Determining whether or not Mars had standing bodies of water in the past has been no easy challenge, mainly because Mars lacks the kinds of apparent indications of lakes and oceans on its surface (like fine-grained sand deposits or clear shorelines). As a result, scientists have had to look for other means of identifying where water flowed and sand was deposited, which is where sedimentary fans come into play.

In this case, the fan identified was a river delta, which form when a river slows down in the presence of a slower-moving or still body of water. This causes any small sediments that are being carried by the river to settle on the ground and form geological features (e.g. small islands at the mouth of the river) over time. In the past, river deltas have been found on Mars, but only in craters where water flowed into a lake.

Case in point, the Curiosity rover, which has been studying the Gale Crater since it landed there in 2012, has discovered abundant evidence that the crater was once a lake. This evidence included clay minerals at the base of Mount Sharp, as well as sedimentary deposits and channels discovered in the crater wall and Mount Sharp that could only be explained by water flowing into the crater.

Further Reading: Natural History Museum, Earth and Planetary Science Letters