首页> 外文期刊>Icarus: International Journal of Solar System Studies >Crater-based dating of geological units on Mars: Methods and application for the new global geological map
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Crater-based dating of geological units on Mars: Methods and application for the new global geological map

机译:火星上基于火山口的地质单位测年:新的全球地质地图的方法和应用

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The new, post-Viking generation of Mars orbital imaging and topographical data provide significant higher-resolution details of surface morphologies, which induced a new effort to photo-geologically map the surface of Mars at 1:20,000,000 scale. Although from unit superposition relations a relative stratigraphical framework can be compiled, it was the ambition of this mapping project to provide absolute unit age constraints through crater statistics. In this study, the crater counting method is described in detail, starting with the selection of image data, type locations (both from the mapper's and crater counter's perspectives) and the identification of impact craters. We describe the criteria used to validate and analyse measured crater populations, and to derive and interpret crater model ages. We provide examples of how geological information about the unit's resurfacing history can be retrieved from crater size-frequency distributions. Three cases illustrate short-, intermediate, and long-term resurfacing histories. In addition, we introduce an interpretation-independent visualisation of the crater resurfacing history that uses the reduction of the crater population in a given size range relative to the expected population given the observed crater density at larger sizes. From a set of potential type locations, 48 areas from 22 globally mapped units were deemed suitable for crater counting. Because resurfacing ages were derived from crater statistics, these secondary ages were used to define the unit age rather than the base age. Using the methods described herein, we modelled ages that are consistent with the interpreted stratigraphy. Our derived model ages allow age assignments to be included in unit names. We discuss the limitations of using the crater dating technique for global-scale geological mapping. Finally, we present recommendations for the documentation and presentation of crater statistics in publications.
机译:北欧海盗之后的新一代火星轨道成像和地形数据提供了表面形态的更高分辨率的详细信息,这引发了一项新的工作,即以1:20,000,000的比例对火星表面进行了光学地质成像。尽管可以从单元叠加关系中建立相对的地层框架,但此映射项目的目标是通过火山口统计数据提供绝对的单元年龄约束。在这项研究中,将详细介绍陨石坑计数方法,首先从图像数据的选择,类型位置(从制图仪和陨石坑计数器的角度出发)以及撞击坑的识别开始。我们描述了用于验证和分析测得的陨石坑数量以及推导和解释陨石坑模型年龄的标准。我们提供了一些示例,说明如何从陨石坑的大小-频率分布中检索有关单元重铺历史的地质信息。三个案例说明了短期,中期和长期的重铺历史。此外,我们介绍了火山口重铺历史的独立于解释的可视化方法,该方法使用给定尺寸范围内的火山口数量相对于预期人口的减少(在较大尺寸下观察到的火山口密度)。从一组潜在的类型位置来看,来自22个全局映射单位的48个区域被认为适合于火山口计数。由于表面年龄是从火山口统计数据中得出的,因此这些次生年龄用于定义单位年龄而不是基本年龄。使用本文所述的方法,我们对与解释地层一致的年龄进行了建模。我们导出的模型年龄允许将年龄分配包含在单位名称中。我们讨论了使用火山口测年技术进行全球规模地质测绘的局限性。最后,我们提出有关火山口统计资料的文档编制和介绍的建议。

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