Goodwin Arthur, Garwood Russell J, Tartèse Romain
Department of Earth and Environmental Sciences, The University of Manchester, Manchester, United Kingdom.
Earth Sciences Department, Natural History Museum, London, United Kingdom.
Astrobiology. 2022 Jun;22(6):755-767. doi: 10.1089/ast.2021.0069. Epub 2022 Feb 25.
The regolith breccia Northwest Africa (NWA) 7034 and paired samples are unique meteorite representatives of the martian crust. They are water rich, lithologically varied, and preserve the oldest martian zircon grains yet discovered that formed 4500-4300 Ma. The meteorite thus provides us with an invaluable record of the crustal and environmental conditions on early Mars. Resetting of some radioisotopic chronometers occurred in response to a major thermal disturbance event 1500-1400 Ma, likely caused by an impactor that brecciated and redeposited NWA 7034 near the surface in an ejecta blanket. Lithologies comprising NWA 7034 were then aqueously altered by a long-lasting impact-induced hydrothermal system, before being excavated and ejected by a subsequent impact at 5-15 Ma. This review compiles chronological and petrological information into an overarching geochronological summary for NWA 7034 and paired samples. We then provide a synopsis for the volatile (HO, C) inventory and hydrothermal alteration history of NWA 7034. From this geochronological history and volatile inventory, we interpret and assess two potential periods of martian habitability: (1) an early window of pre-Noachian planetary habitability, and (2) impact-derived hydrothermal systems that allowed intermittent habitable crater environments well into the Amazonian.
西北非洲(NWA)7034号陨石角砾岩及其配对样本是火星地壳独特的陨石代表。它们富含水,岩性多样,并保存了迄今发现的最古老的火星锆石颗粒,这些锆石形成于45亿至43亿年前。因此,这块陨石为我们提供了早期火星地壳和环境状况的宝贵记录。一些放射性同位素计时仪在15亿至14亿年前的一次重大热扰动事件中被重置,这可能是由一个撞击体造成的,该撞击体将NWA 7034号陨石角砾化并重新沉积在地表附近的喷射毯中。构成NWA 7034号陨石的岩性随后被一个长期的撞击诱导热液系统水合改变,之后在500万至1500万年前被随后的一次撞击挖掘并喷射出来。本综述将年代学和岩石学信息汇编成一个关于NWA 7034号陨石及其配对样本的总体地质年代学总结。然后,我们提供了NWA 7034号陨石挥发性物质(氢、碳)含量和热液蚀变历史的概要。根据这一地质年代学历史和挥发性物质含量,我们解释并评估了火星宜居性的两个潜在时期:(1)诺亚纪前行星宜居性的早期窗口,以及(2)撞击衍生的热液系统,这些系统使得在亚马逊纪时期间歇性的宜居陨石坑环境得以存在。