Univ Lyon, Univ Lyon 1, ENS Lyon, CNRS, LGL-TPE, 2 Rue Raphael Dubois, F-69622 Villeurbanne, France, France.
Institut d'Astrophysique Spatiale, Univ Paris Sud, CNRS, UMR 8617, Univ Paris-Saclay, Bat 120-121, F-91405 Orsay, France.
Astrobiology. 2021 Mar;21(3):345-366. doi: 10.1089/ast.2019.2191. Epub 2021 Jan 5.
The European Space Agency (ESA) and Roscosmos ExoMars mission will launch the "Rosalind Franklin" rover in 2022 for a landing on Mars in 2023.The goals of the mission are to search for signs of past and present life on Mars, investigate the water/geochemical environment as a function of depth in the shallow subsurface, and characterize the surface environment. To meet these scientific objectives while minimizing the risk for landing, a 5-year-long landing site selection process was conducted by ESA, during which eight candidate sites were down selected to one: Oxia Planum. Oxia Planum is a 200 km-wide low-relief terrain characterized by hydrous clay-bearing bedrock units located at the southwest margin of Arabia Terra. This region exhibits Noachian-aged terrains. We show in this study that the selected landing site has recorded at least two distinct aqueous environments, both of which occurred during the Noachian: (1) a first phase that led to the deposition and alteration of ∼100 m of layered clay-rich deposits and (2) a second phase of a fluviodeltaic system that postdates the widespread clay-rich layered unit. Rounded isolated buttes that overlie the clay-bearing unit may also be related to aqueous processes. Our study also details the formation of an unaltered mafic-rich dark resistant unit likely of Amazonian age that caps the other units and possibly originated from volcanism. Oxia Planum shows evidence for intense erosion from morphology (inverted features) and crater statistics. Due to these erosional processes, two types of Noachian sedimentary rocks are currently exposed. We also expect rocks at the surface to have been exposed to cosmic bombardment only recently, minimizing organic matter damage.
欧洲航天局(ESA)和俄罗斯 Roscosmos ExoMars 任务将于 2022 年发射“罗莎琳德·富兰克林”漫游者,于 2023 年在火星着陆。该任务的目标是在火星上寻找过去和现在生命的迹象,研究水/地球化学环境作为浅层地下深处的函数,并对表面环境进行特征描述。为了满足这些科学目标,同时将着陆风险降到最低,ESA 进行了长达 5 年的着陆点选择过程,在此过程中,8 个候选着陆点被缩减到 1 个:Oxia Planum。Oxia Planum 是一个 200 公里宽的低地势地形,其特征是在阿拉伯 Terra 的西南边缘存在含有水合粘土的基岩单元。这一区域显示出了诺亚纪地貌。我们在这项研究中表明,所选着陆点至少记录了两个不同的水相环境,这两个环境都发生在诺亚纪:(1)导致沉积和改造约 100m 的层状粘土丰富的沉积物的第一阶段;(2)在广泛的富含粘土的层状单元之后发生的河流三角洲系统的第二阶段。覆盖含粘土单元的孤立但独立的圆形孤丘也可能与水相过程有关。我们的研究还详细描述了形成一个未改变的富含镁铁质的深黑色抵抗单元的过程,其可能具有亚马逊纪年龄,覆盖了其他单元,并且可能源自火山作用。Oxia Planum 显示出强烈侵蚀的证据,包括地貌(倒置特征)和陨石坑统计数据。由于这些侵蚀过程,目前有两种诺亚纪沉积岩暴露出来。我们还预计,表面的岩石最近才暴露在宇宙撞击之下,最大限度地减少了有机物的破坏。