中文核心期刊

中国科技核心期刊

中国科学引文数据库（CSCD）来源期刊

中国高校百佳科技期刊

中国宇航学会深空探测技术专业委员会会刊

高级检索

留言板

尊敬的读者、作者、审稿人, 关于本刊的投稿、审稿、编辑和出版的任何问题, 您可以本页添加留言。我们将尽快给您答复。谢谢您的支持!

姓名
邮箱
手机号码
标题
留言内容
验证码
x 关闭 永久关闭

利用CRISM数据探测火星表面含水矿物及其演化

杨懿,金双根,薛岩松

downloadPDF
文章导航> 深空探测学报(中英文）> 2016> 3(2): 187-194
杨懿, 金双根, 薛岩松. 利用CRISM数据探测火星表面含水矿物及其演化[J]. 深空探测学报(中英文）, 2016, 3(2): 187-194. doi: 10.15982/j.issn.2095-7777.2016.02.015
引用本文: 杨懿, 金双根, 薛岩松. 利用CRISM数据探测火星表面含水矿物及其演化[J]. 深空探测学报(中英文）, 2016, 3(2): 187-194.doi:10.15982/j.issn.2095-7777.2016.02.015
shu
YANG Yi, JIN Shuanggen, XUE Yansong. Identification and Geological Evolution of Hydrated Minerals at Holden and Jezero Impact Craters Mars Using MRO CRISM Hyperspectral Data[J]. Journal of Deep Space Exploration, 2016, 3(2): 187-194. doi: 10.15982/j.issn.2095-7777.2016.02.015
Citation: YANG Yi, JIN Shuanggen, XUE Yansong. Identification and Geological Evolution of Hydrated Minerals at Holden and Jezero Impact Craters Mars Using MRO CRISM Hyperspectral Data[J].Journal of Deep Space Exploration, 2016, 3(2): 187-194.doi:10.15982/j.issn.2095-7777.2016.02.015
shu

利用CRISM数据探测火星表面含水矿物及其演化

doi:10.15982/j.issn.2095-7777.2016.02.015
  • 1.

    中国科学院 上海天文台, 上海 200030;中国科学院大学, 北京 100049

  • 2.

    中国科学院 上海天文台, 上海 200030

Identification and Geological Evolution of Hydrated Minerals at Holden and Jezero Impact Craters Mars Using MRO CRISM Hyperspectral Data

  • 1.

    Shanghai Astronomical Observatory, Chinese Academy of Science, Shanghai 200030, China;University of Chinese Academy of Sciences, Beijing 100049, China

  • 2.

    Shanghai Astronomical Observatory, Chinese Academy of Science, Shanghai 200030, China

  • 摘要:火星表层矿物识别是了解火星大气环境变化、表层地质环境的关键因素。通过确定火星表层矿物,分析矿物特性,了解火星的环境状态、地质演化以及火星的未来适居性。火星勘测轨道器(Mars reconnaissance orbiter,MRO)上搭载的紧凑型侦察成像仪(compact reconnaissance imaging spectrometer for Mars,CRISM)是针对火星矿物探测的最新的高光谱成像仪,以很高的光谱分辨率覆盖可见光至近红外波段,为火星表面的矿物分布及区域填图提供了可能。通过光谱匹配及计算CRISM光谱参数综合产品,分析了火星Jezero以及Holden撞击坑内的矿物成分及其演化。Jezero与Holden因其复杂而关键的地质特征,被列为火星2020登陆任务的备选登陆点。对这两个地点的矿物探测与填图分析不仅可进一步分析火星典型地质特征以及演化,而且还可以为未来的火星登陆点分析提供现实意义。在研究区域已检测到与水成蚀变相关的含水硅酸盐类以及碳酸盐类与含水硫酸盐类。水合矿物增加了这些区域曾经含水的可能性,且矿物的多样性表明研究区地质环境经历了不同的变化,其中Jezero地区不同于火星的绝大多数地区从中性环境到酸性环境的演化,有可能经历了从中性环境到碱性环境的演化。
    Abstract:Identification of mineral components in different regions on the Mars is crucial to understand the Martian geology and environmental changes. By recognizing the Martian surface mineral, the Martian's environment condition and geological evolution can be understood. Meanwhile, it can be used for further exploration of the habitability of the Mars. The compact reconnaissance imaging spectrometer for Mars (CRISM) on the Mars reconnaissance orbiter (MRO) is the most recent hyperspectral imager that has reached the Mars in order to detecting the minerals. The spectrometer covers the wavelength from visible to near infrared along with enhanced spectral resolution, which provides the ability to map the mineralogy on Mars. In this paper, based on the spectrum matching and calculating CRISM summary product, mineral composition and geological evolution of the Jezero and Holden craters on the Mars are analyzed. These two craters were proposed as the candidates of the landing sites for the Mars 2020 mission due to their complex geological characteristics. Therefore, identification of mineral components of these two sites can not only further analyze the typical geological characteristics and evolutions of the climate of Mars, but also provide practical significance for the analysis of future landing sites on the Mars. We have detected several kinds of hydrated minerals including carbonate, hydrated silicate and hydrated sulfate in the study areas. These minerals suggested the possibility that the Holden and Jezero craters have experienced long time water-rock interactions. Also, the diversity of the minerals found in these regions indicates the aqueous activities in multiple distinct environments and the different environment changes in the study areas. For example unlike the dominating environment evolution from neutral to acidic on the Mars, the evolution around the Jezero may be from neutral to alkaline.
  • [1] Barlow N G. Mars:an introduction to its interior,surface and atmosphere[M]. Cambridge:Cambridge University Press,2008,303.
    [2] 韩同林. 火星地貌与地质[M]. 北京:地质出版社,2007.Han T L. Martian landforms and geology[M]. Beijing:Geological Publishing House,2007.
    [3] Bibring J P,Soufflot A,Berthé M,et al. OMEGA:Observatoire pour la Minéralogie,l'Eau,les Glaces et l'Activité[J]. Mars Express the Scientific Payload,2004(1240):37-49.
    [4] Bibring J P,Langevin Y,Gendrin A,et al. Mars surface diversity as revealed by the OMEGA/Mars Express observations[J]. Science,2005,307(5715):1576-1581.
    [5] Bibring J P,Langevin Y,Mustard J F,et al. Global mineralogical and aqueous mars history derived from OMEGA/Mars Express data[J]. Science,2006,312(5772):400-404.
    [6] Gendrin A,Mangold N,Bibring J P,et al. Sulfates in martian layered terrains:the OMEGA/Mars Express view[J]. Science,2005,307(5715):1587-1591.
    [7] Yves L,FranOis P,Bibring J P,et al. Sulfates in the north polar region of Mars detected by OMEGA/Mars express[J]. Science,2005,307(5715):1584-1589.
    [8] Murchie S,Arvidson R,Bedini P,et al. Compact reconnaissance imaging spectrometer for Mars (CRISM) on Mars reconnaissance orbiter (MRO)[J]. Journal of Geophysical Research,2007,112(E5):431-433.
    [9] Mustard J F,Murchie S L,Pelkey S M,et al. Hydrated silicate minerals on Mars observed by the Mars reconnaissance orbiter CRISM instrument[J]. Nature,2008,454(7202):305-309.
    [10] Mcguire P C,Bishop J L,Brown A J,et al. An improvement to the volcano-scan algorithm for atmospheric correction of CRISM and OMEGA spectral data[J]. Planetary & Space Science,2009,57(7):809-815.
    [11] Murchie S L,Mustard J F,Ehlmann B L,et al. A synthesis of Martian aqueous mineralogy after 1 Mars year of observations from the Mars reconnaissance orbiter[J]. Journal of Geophysical Research Planets,2009,114(E2):396-412.
    [12] Murchie S L,Seelos F P,Hash C D,et al. Compact reconnaissance imaging spectrometer for Mars investigation and data set from the Mars reconnaissance orbiter's primary science phase[J]. Journal of Geophysical Research,2009(114):1-15.
    [13] 陈述彭. 遥感地学分析[M]. 北京:测绘出版社,1990.Chen S P. Geography analysis for remote sensing[M]. Beijing:Surveying and Mapping Press,1990.
    [14] 浦瑞良,宮鹏. 高光谱遥感及其应用[M]. 北京:高等敎育出版社,2000.Pu R L,Gong P. Hyperspectral remote sensing and its applications[M]. Beijing:Higher Education Press,2000.
    [15] 张良培,张立福. 高光谱遥感[M]. 北京:测绘出版社,2011.Zhang L P,Zhang L F. Hyperspectral remote sensing[M]. Beijing:Surveying and Mapping Press,1990
    [16] Pelkey S M,Mustard J F,Murchie S,et al. CRISM multispectral summary products:parameterizing mineral diversity on Mars from reflectance[J]. Journal of Geophysical Research:Planets,2007,112(E8):1-18.
    [17] Cabrol N A,Grin E A,Newsom H E,et al. Hydrogeologic evolution of Gale crater and its relevance to the exobiological exploration of Mars[J]. Icarus,1999,139(2):235-245.
    [18] Clark R N,King T V V,Klejwa M,et al. High spectral resolution reflectance spectroscopy of minerals[J]. Journal of Geophysical Research:Solid Earth,1990,95(B8):12653-12680.
    [19] Arvidson R E,Poulet F,Bibring J P,et al. Spectral reflectance and morphologic correlations in eastern Terra Meridiani,Mars[J]. Science,2005,307(5715):1591-1594.
    [20] Giese R F. Kaolin minerals; structures and stabilities[J]. Reviews in Mineralogy and Geochemistry,1988,19(1):29-66.
    [21] 张渊智,安璐,黄朝君. 基于天空风化的尖晶石二向性反射特性研究[J]. 深空探测学报,2014,1(3):210-213.Zhang Y Z,An L,Huang Z J. The study of bidirectional reflectance feature of the spinel based on the space weathering[J]. The Journal of Deep Space Exploration,2014,1(3):210-213.
    [22] Gaffey S J. Spectral reflectance of carbonate minerals in the visible and near infrared (O. 35-2.55 microns);calcite,aragonite,and dolomite[J]. American Mineralogist,1986,71(1-2):151-162.
    [23] Hunt G R,Salisbury J W. Visible and near infrared spectra of minerals and rocks:Ⅱ. carbonates[J]. Modern Geology,1971(2):23-30.
    [24] Ehlmann B L,Mustard J F,Murchie S L,et al. Orbital identification of carbonate-bearing rocks on Mars[J]. Science,2008,322(5909):1828-1832.
    [25] Ehlmann B L,Mustard J F,Fassett C I,et al. Clay minerals in delta deposits and organic preservation potential on Mars[J]. Nature Geoscience,2008,1(6):355-358.
    [26] Ehlmann B L,Mustard J F,Swayze G A,et al. Identification of hydrated silicate minerals on Mars using MRO-CRISM:geologic context near Nili Fossae and implications for aqueous alteration[J]. Journal of Geophysical Research:Planets,2009,114(10):1-33.
  • [1] 张玉花, 杨金, 盛松, 印兴峰, 徐亮.“天问一号”火星环绕器推进管路热控设计与分析. 深空探测学报(中英文）, 2023, 10(1): 1-7.doi:10.15982/j.issn.2096-9287.2023.20210086
    [2] 王森, 朱新波, 汪栋硕, 张旭光.火星环绕器全链路时间标定及发射日授时方法. 深空探测学报(中英文）, 2023, 10(2): 1-6.doi:10.15982/j.issn.2096-9287.2023.20210091
    [3] 张玉花, 朱新波, 谢攀, 徐亮.火星环绕探测发展现状与趋势. 深空探测学报(中英文）, 2023, 10(1): 1-8.doi:10.15982/j.issn.2096-9287.2023.20220008
    [4] 柳思聪, 童小华, 刘世杰, 谢欢, 赵慧, 刘大永, 许雄, 叶真, 王超, 刘祥磊.“天问一号”着陆区遥感形貌建模与制图分析. 深空探测学报(中英文）, 2022, 9(3): 338-347.doi:10.15982/j.issn.2096-9287.2022.20220005
    [5] 耿迅, 徐青.一种线阵推扫式行星遥感影像摄影测量快速处理方法. 深空探测学报(中英文）, 2022, 9(3): 348-356.doi:10.15982/j.issn.2096-9287.2022.20210002
    [6] 卢皓, 张辉, 张朕, 于天一, 崔晓峰, 胡晓东, 费立刚.火星车多光谱相机桅杆精确指向控制方法. 深空探测学报(中英文）, 2022, 9(5): 1-6.doi:10.15982/j.issn.2096-9287.2022.20220007
    [7] 尹力, 叶乐佳, 邸凯昌, 刘斌, 孙小珠, 王长焕, 薄正.坡度变化率建模的低分辨率坡度补偿方法. 深空探测学报(中英文）, 2022, 9(3): 311-320.doi:10.15982/j.issn.2096-9287.2022.20210161
    [8] 艾素芬, 向艳超, 雷尧飞, 薛淑艳, 沈宇新, 殷雷, 刘佳, 陈维强.火星车低密度纳米气凝胶隔热材料制备及性能研究. 深空探测学报(中英文）, 2020, 7(5): 466-473.doi:10.15982/j.issn.2096-9287.2020.20200036
    [9] 石海平, 陈燕, 贾阳, 屈严, 刘治钢, 王文强, 彭松.太阳电池阵火星环境发电建模仿真. 深空探测学报(中英文）, 2020, 7(5): 474-480.doi:10.15982/j.issn.2096-9287.2020.20200042
    [10] 孙博文, 何章鸣, 王炯琦.基于神经网络的卫星控制系统故障识别方法. 深空探测学报(中英文）, 2019, 6(4): 369-375.doi:10.15982/j.issn.2095-7777.2019.04.009
    [11] 傅惠民, 杨海峰, 文歆磊.自识别自校准Kalman滤波方法. 深空探测学报(中英文）, 2019, 6(4): 398-402.doi:10.15982/j.issn.2095-7777.2019.04.013
    [12] 孔令高, 张爱兵, 田峥, 郑香脂, 王文静, 刘勇, 丁建京.自主火星探测高集成离子与中性粒子分析仪. 深空探测学报(中英文）, 2019, 6(2): 142-149.doi:10.15982/j.issn.2095-7777.2019.02.005
    [13] 关昭, 乔卫东, 杨建峰, 薛彬, 陶金有.火星多光谱相机的地面几何标定研究. 深空探测学报(中英文）, 2018, 5(5): 465-471.doi:10.15982/j.issn.2095-7777.2018.05.009
    [14] 舒嵘, 徐卫明, 付中梁, 万雄, 袁汝俊.深空探测中的激光诱导击穿光谱探测仪. 深空探测学报(中英文）, 2018, 5(5): 450-457.doi:10.15982/j.issn.2095-7777.2018.05.007
    [15] 李建军, 王大轶.摄动因素对火星环绕段轨道长期影响研究. 深空探测学报(中英文）, 2017, 4(1): 77-81.doi:10.15982/j.issn.2095-7777.2017.01.012
    [16] 于正湜, 崔平远.行星着陆自主导航与制导控制研究现状与趋势. 深空探测学报(中英文）, 2016, 3(4): 345-355.doi:10.15982/j.issn.2095-7777.2016.04.006
    [17] 饶炜, 孙泽洲, 孟林智, 王闯, 吉龙.火星着陆探测任务关键环节技术途径分析. 深空探测学报(中英文）, 2016, 3(2): 121-128.doi:10.15982/j.issn.2095-7777.2016.02.004
    [18] 孟林智, 董捷, 许映乔, 王硕.无人火星取样返回任务关键环节分析. 深空探测学报(中英文）, 2016, 3(2): 114-120,128.doi:10.15982/j.issn.2095-7777.2016.02.003
    [19] 丁萌, 李海波, 曹云峰, 庄丽葵.基于光学图像的撞击坑识别研究综述. 深空探测学报(中英文）, 2015, 2(3): 195-202.doi:10.15982/j.issn.2095-7777.2015.03.001
    [20] 徐青, 耿迅, 蓝朝祯, 邢帅.火星地形测绘研究综述. 深空探测学报(中英文）, 2014, 1(1): 28-35.
  • 加载中
WeChat 点击查看大图
计量
  • 文章访问数:4617
  • HTML全文浏览量:171
  • PDF下载量:1133
  • 被引次数:0
出版历程
  • 收稿日期:2015-09-28
  • 修回日期:2015-11-04

利用CRISM数据探测火星表面含水矿物及其演化

doi:10.15982/j.issn.2095-7777.2016.02.015
  • 1. 中国科学院 上海天文台, 上海 200030;中国科学院大学, 北京 100049
  • 2. 中国科学院 上海天文台, 上海 200030
  • 收稿日期:2015-09-28
  • 修回日期:2015-11-04

摘要:火星表层矿物识别是了解火星大气环境变化、表层地质环境的关键因素。通过确定火星表层矿物,分析矿物特性,了解火星的环境状态、地质演化以及火星的未来适居性。火星勘测轨道器(Mars reconnaissance orbiter,MRO)上搭载的紧凑型侦察成像仪(compact reconnaissance imaging spectrometer for Mars,CRISM)是针对火星矿物探测的最新的高光谱成像仪,以很高的光谱分辨率覆盖可见光至近红外波段,为火星表面的矿物分布及区域填图提供了可能。通过光谱匹配及计算CRISM光谱参数综合产品,分析了火星Jezero以及Holden撞击坑内的矿物成分及其演化。Jezero与Holden因其复杂而关键的地质特征,被列为火星2020登陆任务的备选登陆点。对这两个地点的矿物探测与填图分析不仅可进一步分析火星典型地质特征以及演化,而且还可以为未来的火星登陆点分析提供现实意义。在研究区域已检测到与水成蚀变相关的含水硅酸盐类以及碳酸盐类与含水硫酸盐类。水合矿物增加了这些区域曾经含水的可能性,且矿物的多样性表明研究区地质环境经历了不同的变化,其中Jezero地区不同于火星的绝大多数地区从中性环境到酸性环境的演化,有可能经历了从中性环境到碱性环境的演化。

English Abstract

杨懿, 金双根, 薛岩松. 利用CRISM数据探测火星表面含水矿物及其演化[J]. 深空探测学报(中英文）, 2016, 3(2): 187-194. doi: 10.15982/j.issn.2095-7777.2016.02.015
引用本文: 杨懿, 金双根, 薛岩松. 利用CRISM数据探测火星表面含水矿物及其演化[J]. 深空探测学报(中英文）, 2016, 3(2): 187-194.doi:10.15982/j.issn.2095-7777.2016.02.015
shu
YANG Yi, JIN Shuanggen, XUE Yansong. Identification and Geological Evolution of Hydrated Minerals at Holden and Jezero Impact Craters Mars Using MRO CRISM Hyperspectral Data[J]. Journal of Deep Space Exploration, 2016, 3(2): 187-194. doi: 10.15982/j.issn.2095-7777.2016.02.015
Citation: YANG Yi, JIN Shuanggen, XUE Yansong. Identification and Geological Evolution of Hydrated Minerals at Holden and Jezero Impact Craters Mars Using MRO CRISM Hyperspectral Data[J].Journal of Deep Space Exploration, 2016, 3(2): 187-194.doi:10.15982/j.issn.2095-7777.2016.02.015
shu

    全文HTML

参考文献 (26)

目录

    /

      返回文章
      返回

        您是第976321位访问者

        版权所有: 《深空探测学报》（中英文）编辑部编辑部地址: 中关村南大街5号邮编: 100081电话: （010）81384397

        本系统由北京仁和汇智信息技术有限公司开发 百度统计

        Baidu
        map