Signs of ancient flowing water on Mars



by Staff Writers



Paris (ESA) Feb 22, 2019



This image from ESA's Mars Express shows a network of dried-up valleys on Mars, and comprises data gathered on 19 November 2018 during Mars Express orbit 18831. The ground resolution is approximately 14 m/pixel and the images are centered at 66 E/17 S. This image was created using data from the nadir and colour channels of the High Resolution Stereo Camera (HRSC). The nadir channel is aligned perpendicular to the surface of Mars, as if looking straight down at the surface. North is to the right. See detailed related images and captions here

These images from ESA's Mars Express satellite show a branching, desiccated system of trenches and valleys, signs of ancient water flow that hint at a warmer, wetter past for the Red Planet.

We see Mars as a cold, dry world, but plenty of evidence suggests that this was not always the case. Research in past years instead increasingly indicates that the planet once had a thicker, denser atmosphere that was able to lock in far greater amounts of warmth, and therefore facilitate and support the flow of liquid water on the surface below.

While this is no longer the case, we see clear signs of past water activity tracing across the martian surface. This image shows one such region: a system of valleys in the southern highlands of Mars, located east of a large, well-known impact crater called Huygens and north of Hellas, the largest impact basin on the planet.

At 3.5 to four billion years old, the southern highlands are some of the oldest and most heavily cratered parts of Mars, with many signs of ancient water flow observed here.

The topography of this region suggests that water flowed downhill from the north (right in the main colour, topography and 3D images) to the south (left), carving out valleys up to two kilometres across and 200 metres deep as it did so.

We see these valleys as they stand today, having undergone significant and heavy erosion since they were formed. This erosion is visible in the form of broken down, smoothed, fragmented and dissected valley rims, especially in the valleys cutting from east to west.

Overall, the valley system appears to branch out significantly, forming a pattern a little like tree branches stemming from a central trunk. This kind of morphology is known as 'dendritic' - the term is derived from the Greek word for tree (dendron), and it is easy to see why. Various channels split off from the central valley, forming little tributaries that often split again on their journey outwards.

This kind of dendritic structure is also seen in drainage systems on Earth. A particularly good example is that of the Yarlung Tsangpo river, which snakes its way from its source in western Tibet down through China, India, and Bangladesh.

In the case of this image of Mars, these branching channels were likely formed by surface water runoff from a once-strong river flow, combined with extensive rainfall. This flow is thought to have cut through existing terrain on Mars, forging new paths and carving a new landscape.

While it is unclear where all of this water came from originally - precipitation, groundwater, melting glaciers? - all of this required a far warmer and more watery past for Mars than the planet we see today.

A tantalising question raised by this warmer and wetter climate is whether conditions would have been suitable for life - a topic at the heart of Mars exploration. Next year, ESA and Roscosmos will launch the ExoMars mission comprising a rover - recently named Rosalind Franklin - and a surface science platform.

The rover will drive to interesting locations to drill below the surface in search for signs of life - the first mission of its kind. Meanwhile, the ExoMars Trace Gas Orbiter continues to analyse the atmosphere in greater detail than ever, with a particular interest for gases potentially related to biological or geological activity, and to identify subsurface locations where water-ice or hydrated minerals are present.

This succession of spacecraft at Mars - both in orbit and on the surface - ensures ESA's long-term presence in Mars science and exploration. The next step that ESA together with international partners are considering is returning a sample of Mars to Earth - an ambitious task that will provide scientific treasures for generations to come.



Related Links

Mars Express at ESA

Mars News and Information at MarsDaily.com

Lunar Dreams and more





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Paris (ESA) Nov 26, 2018

