Potential ExoMars Rover Landing Sites: Aram Dorsam (previously known as Oxia Palus) and Hypanis Delta

Matthew R Balme, The Open University, School of Physical Sciences, Milton Keynes, United Kingdom, Peter M Grindrod, University College London, London, United Kingdom, Sanjeev Gupta, Imperial College London, Department of Earth Science and Engineering, London, United Kingdom, Peter Fawdon, Open University, Milton Keynes, United Kingdom, Jan-Peter Muller, University College London, Mullard Space Science Laboratory, London, United Kingdom, Joseph R Michalski, Planetary Science Institute Tucson, Tucson, AZ, United States and Elliot Sefton-Nash, University of California Los Angeles, Los Angeles, CA, United States
Abstract:
The search for life on Mars is a cornerstone of international solar system exploration. In 2018, the European Space agency will launch the ExoMars Rover to further this. The key science objectives of the ExoMars Rover are to: 1) search for signs of past and present life on Mars; 2) investigate the water/geochemical environment as a function of depth in the shallow subsurface; and 3) to characterise the surface environment. ExoMars will drill into the sub-surface to look for indicators of past life using a variety of complementary techniques, including assessment of morphology (potential fossil organisms), mineralogy (past environments) and a search for organic molecules and their chirality (biomarkers).

The choice of landing site is vital if the objectives are to be met. The landing site must: (i) be ancient (≥3.6 Ga); (ii) show abundant morphological and mineral evidence for long-term, or frequently reoccurring, aqueous activity; (iii) include numerous sedimentary outcrops that (iv) are distributed over the landing region (the typical Rover traverse range is a few km, but ellipse size is ~ 100 by 15 km). Various ‘engineering constraints’ also apply, including: (i) latitude limited to 5º S to 25º N; (ii) maximum altitude of the landing site 2 km below Mars’s datum; and (iii) few steep slopes within the ellipse.

In March 2014, the first ExoMars Landing Site Selection Workshop was held, during which about ten different landing sites were presented and discussed. At the end of the workshop a poll of the workshop participants highlighted four sites as highest priority: Mawrth Vallis, Oxia Planum, Oxia Palus and Hypanis Delta. Of these, our team led proposals for the Oxia Palus and Hypanis Delta sites. The Oxia Palus site has since been renamed “Aram Dorsum” – the name the IAU designated to the inverted channel system that is the most prominent feature of the site. This is inferred to be the remnants of a long-lived, widespread alluvial system that was buried and then recently exhumed. The Hypanis site contains layered terminal deposits from the Hypanis and Sabrina Valles and is inferred to be an ancient environment.

Since the workshop, further mapping and geological studies of these sites have been performed. Here we describe the latest results for these two sites, and why they are appropriate for meeting ExoMars’ goals.

Back to: Reconstructing Habitable Environments on Ancient Mars II Posters