A CaSSIS and HiRISE map of the Clay-bearing Unit at the ExoMars 2022 landing site in Oxia Planum

被引:12
|
作者
Bridges, John [1 ]
Tornabene, Livio [2 ]
Mandon, Lucia [3 ]
Quantin-Nataf, Cathy [4 ]
Patel, Manish R. R. [5 ]
Thomas, Nicolas [6 ]
Cremonese, Gabriele [7 ]
Munaretto, Giovanni [7 ,8 ]
Pommerol, Antoine [6 ]
Pajola, Maurizio [7 ]
Bowen, Adam Parkes [1 ]
机构
[1] Univ Leicester, Sch Phys & Astron, Space Pk Leicester, Leicester LE1 7RH, England
[2] Western Univ, Inst Space & Earth Explorat, Dept Earth Sci, 1151 Richmond St, London, ON N6A 3K7, Canada
[3] Univ Paris, Sorbonne Univ, Univ PSL, LESIA,CNRS,Observ Paris, 5 Pl Janssen, F-92195 Meudon, France
[4] Univ Claude Bernard Lyon 1, 43 Blvd 11 Novembre 1918, F-69100 Villeurbanne, France
[5] Open Univ, Sch Phys Sci, Walton Hall, Milton Keynes MK7 6AA, England
[6] Univ Bern, Phys Inst, Hsch Str 6, 3012 Bern, Switzerland
[7] INAF Astron Observ Padova, Vicolo Osservatorio 4, I-35122 Padua, PD, Italy
[8] Univ Padua, Dept Phys & Astron, Padua, Italy
基金
加拿大自然科学与工程研究理事会;
关键词
ExoMars rover; Oxia Planum; Clay; CaSSIS; HiRISE; OLIVINE DISSOLUTION; GALE CRATER; YELLOWKNIFE BAY; MARS; HABITABILITY; SIZE;
D O I
10.1016/j.pss.2022.105429
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
In preparation for the operations of the ExoMars Rosalind Franklin rover, characterising its landing site in Oxia Planum is essential. Of particular interest is the extensive Clay-bearing Unit present at the site, a key target in the search for biosignatures. In this paper we provide a map based on variations in colour and spectral information within this unit, covering the 1 sigma landing envelope of the rover along with a 1 km buffer to account for minor shifts of the landing envelope ahead of launch (referred to going forward as the 1 sigma+ landing envelope). We used imagery from the Colour and Stereo Surface Imaging System (CaSSIS) and High Resolution Imaging Science Experiment (HiRISE) instruments, along with CaSSIS Band Ratio Composites with enhanced colour sensitivity to the presence of ferric (Fe3+) and ferrous (Fe2+) iron bearing materials. Our map is of a far higher resolution (map scale 1:2000) than those previously available and, in contrast to previously available maps of this unit, differentiates between an Orange Subunit and a Blue Subunit which make up the Clay-bearing Unit. This mapping covered the-91% of the 1 sigma+ landing envelope where there was CaSSIS coverage and split the Clay-bearing Unit into three categories: one for each of the clay subunits, and another for exposures of the Clay-bearing Unit where either both subunits were too intermixed to reliably separate, or where it was difficult to determine which of the two were present. The results from our mapping shows that at least similar to 35% of the 1 sigma+ envelope is covered by exposures of the Clay-bearing Unit: similar to 18% by the Orange Subunit, similar to 9% the Blue Subunit, and similar to 12% were classified as Indeterminate. The spread of these two subunits varied substantially over the 1 sigma+ landing envelope, with the south-east half of the landing envelope dominated by the Orange Subunit (similar to 70% exposures in this area belonging to the Orange Subunit, similar to 10% to the Blue Subunit and similar to 20% to the Indeterminate category), while the north-west has more sporadic exposures of the Clay-bearing Unit (similar to 22% Orange, similar to 37% Blue and similar to 41% Indeterminate). The colour distinction between the two subunits is thought to be due to constituent mineralogical differences rather than differences in dust coverage of the two subunits. The scale of the fracturing present in the two subunits has also been assessed in this study, via qualitative observations of the fracture length and quantitative mapping out of fracture networks. While there were differences in the scale of fracturing between the two subunits, these were not as great as had previously been identified.
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页数:18
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