4.5 Article

Occurrence of secondary minerals at Tharsis Montes of Mars: A critical assessment

期刊

ICARUS
卷 378, 期 -, 页码 -

出版社

ACADEMIC PRESS INC ELSEVIER SCIENCE
DOI: 10.1016/j.icarus.2022.114953

关键词

Mars surface; Image processing; Spectroscopy; Geological processes; Mineralogy

资金

  1. SSPO, ISRO Bangalore
  2. SAC, ISRO Ahmedabad
  3. IIT Guwahati
  4. Indian Space Research Organisation, Department of Space through the scheme MOM-AO project
  5. SERB, DST, India

向作者/读者索取更多资源

This study utilized remote spectral analysis to investigate the surface mineralogy of Tharsis Montes on Mars, revealing the distribution of minerals such as olivine, pyroxene, and plagioclase. The presence of dust obscured certain areas but provided unique research opportunities in less dusty regions. The occurrence of secondary mafic mineral phyllosilicates suggests active weathering or hydrothermal alteration in the region.
Identification of phyllosilicates on Mars suggests the existence of an aqueous environment, indicating an active period in its evolutionary history. This study analysed the surface mineralogy of caldera and flank regions of Tharsis Montes using remote spectral analysis. Though a thick layer of dust obscures the surface of Tharsis volcanic province, relatively lesser dust regions provide a unique window for exploration. The reflectance data obtained from CRISM onboard Mars Reconnaissance Orbiter in the visible-infrared region is used for the mineralogical study. Spectral parameter indices were used to identify the distribution of minerals over the caldera and flank regions of Tharsis Montes. The spectral characterisation indicates the well-distributed presence of mafic minerals such as olivine with low-calcium pyroxene and plagioclase with the sparse presence of high calcium pyroxene in the region. The dusty region, typically with a high TES DCI index and low thermal inertia values in the Tharsis Montes, shows a high concentration of olivine. Few regions identified as comparatively dust-free at the caldera and flank show the presence of secondary mafic minerals like Fe-Mg bearing phyllosilicates. Our spectral analysis using nonlinear mixing models with the MICA spectral library indicates the occurrence of absorption features characteristic of hydrated minerals. The occurrence of the secondary mafic minerals, especially the phyllosilicates on Tharsis Montes suggest active weathering or hydrothermal alteration from episodic volcanic activity over time.

作者

我是这篇论文的作者
点击您的名字以认领此论文并将其添加到您的个人资料中。

评论

主要评分

4.5
评分不足

次要评分

新颖性
-
重要性
-
科学严谨性
-
评价这篇论文

推荐

暂无数据
暂无数据