Acidalia Mena, Mars: A key region to test the ocean hypothesis

Acidalia Mena，火星：检验海洋假说的关键区域

• 批准号: 413241974
• 负责人: Professor Dr. Harald Hiesinger
• 金额: --
• 依托单位: Institut für Planetologie
• 依托单位国家: 德国
• 项目类别: Research Grants
• 财政年份: 2018
• 资助国家: 德国
• 起止时间: 2017-12-31 至 2018-12-31
• 项目状态: 已结题
• 来源: https://gepris.dfg.de/gepris/projekt/413241974?language=en
• 关键词: Acidalia; Mena; Mars; key; region

The primary goal of our study is to geologically map the Acidalia Mensa region in the northern hemisphere of Mars at a scale of 1:200,000. The investigation will mostly rely on data of the THermal Emission Imaging Spectrometer (THEMIS) with a pixel scale of 100 m per pixel, augmented by data of the HiRISE, CTX, and HRSC cameras, as well as topography data of the MOLA laser altimeter. Acidalia Mensa is a topographically high-standing terrain north of the proposed shoreline of a putative former ocean on Mars. On the basis of our new geologic map, we propose to vigorously test the ocean hypothesis. The significantly improved quality of available modern imaging and topography data will allow us to geologically map the area in unprecedented detail, which will significantly increase our understanding of the regional geology as well as the existence and evolution of the putative ocean. On the basis of our geologic map we will select key areas for further high-resolution studies. We expect new insights into the geology and structure of the study area, which will allow us to understand its history and evolution. Besides generating a new geologic map, we propose to derive absolute model ages of the map units, decipher the stratigraphy of the area, calculate thermal inertias to estimate grain size distributions, and to perform morphometric measurements of relevant surface features. Results of these investigations, in concert with the geologic map, will be used to test the ocean hypothesis. Some key scientific questions of our study include: 1. What are the building blocks of Acidalia Mensa and what is their relationship to the surrounding Vastitas Borealis Formation? 2. Is there a genetic link between the Acidalia Mensa region and the southern highlands? 3. Is there evidence for a former north-polar ocean? 4. Was Acidalia Mensa surrounded by the putative ocean or did the ocean cover the study region? 5. How old is the Acidalia Mensa plateau and what is its stratigraphic relationship to the surrounding terrain? 6. Given the subdued morphology of impact craters, how much material has been removed from the Acidalia Mensa plateau?

我们研究的主要目标是以1：20万的比例绘制火星北方半球的Acidalia Mensa地区的地质图。调查将主要依靠热发射成像光谱仪（THEMIS）的数据，每像素100米的像素尺度，由HiRISE，CTX和HRSC相机的数据以及MOLA激光高度计的地形数据增强。Acidalia Mensa是一个地势较高的地形，位于火星上一个假定的前海洋的拟议海岸线以北。在我们新的地质图的基础上，我们提议大力检验海洋假说。现有现代成像和地形数据的质量大大提高，将使我们能够以前所未有的详细程度绘制该地区的地质图，这将大大增加我们对区域地质以及假定海洋的存在和演变的了解。根据我们的地质图，我们将选择关键地区进行进一步的高分辨率研究。我们期待对研究区域的地质和结构有新的见解，这将使我们能够了解其历史和演变。除了生成一个新的地质图，我们建议得出的绝对模型年龄的地图单位，破译该地区的地层，计算热惯量估计粒度分布，并进行形态测量的相关表面特征。这些调查的结果，连同地质图，将被用来检验海洋假说。我们研究的一些关键科学问题包括：1。什么是Acidalia Mensa的组成部分，它们与周围的Vastitas Borealis地层有什么关系？2. Acidalia Mensa地区和南部高地之间是否存在遗传联系？3.是否有证据表明曾经有过北极海洋？4. Acidalia Mensa是被假定的海洋包围还是海洋覆盖了研究区域？5.门萨高原的历史有多长？它与周围地形的地层关系如何？6.考虑到撞击坑的柔和形态，有多少物质从门萨高原上被移走了？