首页> 外文期刊>Journal of geophysical research. Planets >A synthesis of Martian aqueous mineralogy after 1 Mars yearof observations from the Mars Reconnaissance Orbiter
【24h】

A synthesis of Martian aqueous mineralogy after 1 Mars yearof observations from the Mars Reconnaissance Orbiter

机译:在火星侦察轨道飞行器观测到火星1年后合成的火星含水矿物学

获取原文
获取原文并翻译 | 示例
       

摘要

Martian aqueous mineral deposits have been examined and characterized using dataacquired during Mars Reconnaissance Orbiter's (MRO) primary science phase, includingCompact Reconnaissance Imaging Spectrometer for Mars hyperspectral imagescovering the 0.4-3.9 pm wavelength range, coordinated with higher—spatial resolutionHiRISE and Context Imager images. MRO's new high-resolution measurements,combined with earlier data from Thermal Emission Spectrometer; Thermal EmissionImaging System; and Observatoire pour la Mineralogie, L'Eau, les Glaces et l'Activitiê onMars Express, indicate that aqueous minerals are both diverse and widespread on theMartian surface. The aqueous minerals occur in 9-10 classes of deposits characterized bydistinct mineral assemblages, morphologies, and geologic settings. Phyllosilicates occurin several settings: in compositionally layered blankets hundreds of meters thick,superposed on eroded Noachian terrains; in lower layers of intracrater depositional fans;in layers with potential chlorides in sediments on intercrater plains; and as thousands ofdeep exposures in craters and escarpments. Carbonate-bearing rocks form a thin unitsurrounding the Isidis basin. Hydrated silica occurs with hydrated sulfates in thinstratified deposits surrounding Valles Marineris. Hydrated sulfates also occur togetherwith crystalline ferric minerals in thick, layered deposits in Terra Meridiani and in VallesMarineris and together with kaolinite in deposits that partially infill some highlandcraters. In this paper we describe each of the classes of deposits, review hypotheses fortheir origins, identify new questions posed by existing measurements, and consider theirimplications for ancient habitable environments. On the basis of current data, two to fiveclasses of Noachian-aged deposits containing phyllosilicates and carbonates may haveformed in aqueous environments with pH and water activities suitable for life.
机译:火星含水矿物沉积物已在火星侦察轨道器(MRO)的主要科学阶段得到了检查和表征,包括用于0.4-3.9 pm波长范围的火星高光谱图像的紧凑侦察成像光谱仪,并与更高的空间分辨率HiRISE和Context Imager图像相协调。 MRO的新高分辨率测量结果与热发射光谱仪的早期数据相结合;热发射成像系统; Mars Express上的L'Eau,les Glaces等人的《矿物观察站》和《火星快报》指出,火成岩上的含水矿物质既多样又广泛。含水矿物存在于9-10类沉积物中,其特征是矿物组合,形态和地质环境不同。层状硅酸盐存在于多种环境中:在数百米厚的组成分层的毛毯中,叠加在受侵蚀的Noachian地形上;在火山口内沉积扇的下层;在火山口平原沉积物中含潜在氯化物的层;以及成千上万的火山口和悬崖陡壁暴雨。含碳酸盐的岩石在伊迪斯盆地周围形成一个薄的单元。水合二氧化硅与水合硫酸盐一起发生在Valles Marineris周围的薄层沉积物中。水合硫酸盐也与结晶铁矿一起出现在Terra Meridiani和VallesMarineris的厚而分层的矿床中,以及高岭石的矿床中,这些矿床部分填充了一些高地陨石。在本文中,我们描述了每一类矿床,审查了其成因的假说,确定了现有测量提出的新问题,并考虑了它们对古代可居住环境的影响。根据目前的数据,在pH和水活度适合生活的水环境中,可能形成了两到五类的含有页硅酸盐和碳酸盐的诺亚纪年龄沉积物。

著录项

相似文献

  • 外文文献
  • 中文文献
  • 专利
获取原文

客服邮箱:kefu@zhangqiaokeyan.com

京公网安备:11010802029741号 ICP备案号:京ICP备15016152号-6 六维联合信息科技 (北京) 有限公司©版权所有
  • 客服微信

  • 服务号