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

中国高校优秀科技期刊

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

“嫦娥五号”采样点周缘穹窿形貌特征及成因研究

吴文慧 任鑫 帕丽古力·杰恩斯 陈媛 孙国洋

吴文慧, 任鑫, 帕丽古力·杰恩斯, 陈媛, 孙国洋. “嫦娥五号”采样点周缘穹窿形貌特征及成因研究[J]. 深空探测学报(中英文). doi: 10.15982/j.issn.2096-9287.2022.20210068
引用本文: 吴文慧, 任鑫, 帕丽古力·杰恩斯, 陈媛, 孙国洋. “嫦娥五号”采样点周缘穹窿形貌特征及成因研究[J]. 深空探测学报(中英文). doi: 10.15982/j.issn.2096-9287.2022.20210068
WU Wenhui, Paliguli·JIEENSI, REN Xin, CHEN Yuan, SUN Guoyang. Study on the Morphological Characteristics and Genesis of Dome Around Chang'e 5 Sampling Point[J]. Journal of Deep Space Exploration. doi: 10.15982/j.issn.2096-9287.2022.20210068
Citation: WU Wenhui, Paliguli·JIEENSI, REN Xin, CHEN Yuan, SUN Guoyang. Study on the Morphological Characteristics and Genesis of Dome Around Chang'e 5 Sampling Point[J]. Journal of Deep Space Exploration. doi: 10.15982/j.issn.2096-9287.2022.20210068

“嫦娥五号”采样点周缘穹窿形貌特征及成因研究

doi: 10.15982/j.issn.2096-9287.2022.20210068
详细信息
    作者简介:

    吴文慧(2001– ),女,硕士研究生,主要研究方向:资源勘查工程(固体矿产)。通讯地址:中国地质大学(北京)地球科学与资源学院(100083)E-mail:wenhuiwu@163.com

    任鑫(1978– ),男,副研究员,主要研究方向:行星遥感。本文通讯作者。通讯地址:中国科学院国家天文台月球与深空探测实验室(100012)E-mail:renx@nao.cas.cn

  • ● Using Chang'e image data, 17 volcanic domes around Chang'e 5 sampling point are delineated, of which the newly discovered dome is No. 11. ● Based on the morphological and rheological characteristics, the characteristics of Rümker mare domes and Mairan non- mare domes around Chang'e 5 sampling point are compared. ● The division of lunar mare domes and non-mare domes should be determined in combination with its morphological parameters, geographical location, rheological parameters, material composition and other parameters.
  • 中图分类号: V412.41

Study on the Morphological Characteristics and Genesis of Dome Around Chang'e 5 Sampling Point

  • 摘要: “嫦娥五号”采样点周缘区域分布有吕姆克山(Mons Rümker)和Mairan火山穹窿构造。通过“嫦娥”影像和地形数据对两类穹窿的形貌特征和形成因素展开对比研究,讨论穹窿的划分标准。共计圈定了吕姆克山13个月海穹窿和Mairan所在的4个非月海穹窿,并计算了穹窿形成过程中的岩浆流变学参数。研究结果表明:吕姆克山月海穹窿较为低缓,按照坡度和高度划分为吕姆克山第一类月海穹窿(坡度均< 5°,高度200~400 m)和吕姆克山第二类月海穹窿(坡度5°~7°,高度300~600 m),其中第二类较高陡的月海穹隆具有较高的粘度和更低的喷发速率。 Mairan非月海穹窿更为高陡,其岩浆喷发速率低于吕姆克山月海穹窿,岩浆粘度较高,流动性较差,喷发周期较长;在空间上,Mairan所在的4个非月海穹窿呈线性展布,其物质成分和形成时间相近,表明彼此关联的可能性很大。
    Highlights
    ● Using Chang'e image data, 17 volcanic domes around Chang'e 5 sampling point are delineated, of which the newly discovered dome is No. 11. ● Based on the morphological and rheological characteristics, the characteristics of Rümker mare domes and Mairan non- mare domes around Chang'e 5 sampling point are compared. ● The division of lunar mare domes and non-mare domes should be determined in combination with its morphological parameters, geographical location, rheological parameters, material composition and other parameters.
  • 图  1  风暴洋东北部穹窿LRO_WAC影像特征和Clemetine UVVIS 假彩色合成图特征

      注:1-Mairan中央穹顶,2-Mairan T穹顶,3-Mairan 南部穹顶,4-Mairan西北部穹顶(a)吕姆克山穹窿LRO_WAC影像特征 (b)吕姆克山穹窿Clemetine UVVIS 假彩色合成图特征(c)Mairan穹窿LRO_WAC影像特征1 (d)Mairan穹窿Clemetine UVVIS 假彩色合成图1特征 (e)Mairan穹窿LRO_WAC影像特征2 (f)Mairan穹窿Clemetine UVVIS 假彩色合成图特征2

    Fig.  1  Northern Oceanus Procellarum domes CE2 LRO_ WAC and Clemetine UVVIS false color composite image features

    图  2  穹窿参数表示

    Fig.  2  Dome parameter representation

    图  3  风暴洋北部穹窿分布图

    Fig.  3  Distribution of northern Oceanus Procellarum domes

    表  1  月球喷出型穹窿划分表

    Table  1  Division of lunar extrusive domes

    类别R415/R750坡度/(°)直径/km体积/km3喷发速率/(m3·s–1喷发时间/a年粘度/(Pa·s)
    A>0.640.3~15~13<3100~6200.05~0.3102~103
    B10.55~0.642~5.46~155~3230~2003~18106~107
    B20.55~0.641.3~1.98~152~2180~1700.7~1.2104~105
    C10.55~0.60.6~1.813~287~50200~2 0000.06~7104~105
    C20.6~0.641~2.58~174~17100~3000.5~7104~105
    D>0.641.3~1.5≈2540~67
    E10.58~0.622~4<60.5~0.8≈251.0~1.7105~106
    E20.58~0.62<2<60.5~0.8100~3000.05~0.3103
    G0.55~0.6>67~3020~40048~12012.8~42108~109
    H10.62~0.68<5<5<210~100≈2≈106
    H20.62~0.682~55~151~4310~100≈4≈106
    H30.62~0.685~95~137~3710~100≈10≈107
      注:根据文献[13]修改。
    下载: 导出CSV

    表  2  本研究中所使用的数据[14--15]

    Table  2  Data used in this study[14--15]

    数据名称探测任务空间分辨率/
    (m·pixel–1
    本文作用
    LRO WAC(GLD100)月球勘测轨道飞行器(Lunar Reconnaissance Orbiter,LRO),2008年100确定穹窿的边界和位置
    CE2_TMap2015_50m 的
    DEM数据产品
    嫦娥二号,2010年50提取形貌参数
    CE2_TMap2015_50 m
    的DOM数据产品
    嫦娥二号,2010年50给WAC图像、UVVIS图像几何配准提供基准底图
    Clementine UVVIS假彩色
    合成图像
    “克莱门汀号”( Clementine),1994年200做物质成分参考
    下载: 导出CSV

    表  3  穹窿定量刻画参数

    Table  3  Quantitative characterization parameters of dome(Formula quoted from[17][18]

    参数名称参数定义提取方法其它说明
    穹窿基底面积A/km2轮廓线以内穹窿的表面面积由轮廓限定的像素来确定假设穹窿为标准圆形
    (见图2
    直径D/m穹体基底圆所在圆周过圆心任意两点的连线D = 2 $ \sqrt{A/\mathrm{\pi }} $
    高度H/m穹窿顶点与穹窿轮廓中最低点的差值通过裁剪每个穹窿的DEM数据,提取穹窿高程数据,将最高点与最低点高程作差
    坡度Slope/(°)穹窿高度与穹体基底直径一半比值的反函数Slope=tan−1( 2H/Dg为月球重力加速度,取1.63 m/s2cf2为熔岩流动有效真厚度;
    κ为熔岩的热扩散率,κ ≈ 10−6 m2/s;SV为穹窿表面体积
    屈服强度τ/Pa抵抗微量塑性变形的应力τ=$ \frac{0.323{H}^{2}\rho g}{D/2} $
    塑性粘度
    η(τ)/(Pa·S)
    当流体微团内微团之间发生相对滑移时,内部产生的剪切应力(切向阻力)ητ) = 6 × 10−4 τ 2.4
    喷发速率
    E(m3.s-1
    从喷口喷出单位体积岩浆所花的时间E=$ \frac{{0.323}^{1/2}300\kappa {(\frac{D}{2})}^{2}}{{0.65}^{5/2}{{c}_{\mathrm{f}}}^{2}H} $
    喷发持续
    时间Te (s)
    熔岩喷发持续时间Te = $ \frac{SV}{E} $
    注:表中公式引自文献[17-18]。
    下载: 导出CSV

    表  4  研究区穹窿形貌学参数和流变学特征参数提取结果

    Table  4  Extraction results of dome morphological parameters and rheological characteristic parameters in the study area

    穹窿
    编号
    经度/
    (°W)
    纬度/
    (°N)
    基底面积A/
    km2
    穹窿高
    H/m
    穹窿直径D/
    km
    坡度S/
    (°)
    表面体积SV/
    km3
    屈服
    强度τ/Pa
    塑性粘度
    ητ)/(Pa·s)
    喷发速率
    E/(m3·s-1
    喷发持续
    时间Te/ s
    其它
    说明
    147.741.4146.9902.213.77.560.61.3×1051.0×10936.01.7×109
    非月海
    穹窿
    248.441.848.2845.47.812.220.41.9×1052.9×10912.61.6×109
    347.740.822.6492.15.410.43.59.5×1045.3×10810.23.4×108
    449.943.711.6266.33.87.92.33.9×1046.2×1079.72.4×108
    558.439.954.0371.98.35.118.13.5×1044.9×10732.15.6×108


    月海穹窿
    658.740.161.1318.58.84.110.92.4×1042.0×10742.52.6×108
    758.439.982.9300.410.33.311.51.8×1041.0×10761.11.9×108
    858.240.175.2324.59.83.818.72.3×1041.7×10751.33.6×108
    958.540.380.0581.310.16.631.07.1×1042.6×10830.51.0×109
    1058.840.6227.7493.617.03.386.63.0×1043.4×107102.18.5×108
    1159.540.863.5281.89.03.615.21.9×1041.1×10749.93.0×108
    1259.541.130.4390.36.27.29.75.2×1041.2×10817.25.7×108
    1359.341.325.2321.55.76.56.93.8×1046.0×10717.44.0×108
    1458.741.197.2363.011.13.728.32.5×1042.1×10759.24.8×108
    1558.541.474.9457.19.85.358.64.5×1048.9×10736.31.6E+09
    1657.941.295.9305.711.03.225.71.8×1049.5×10669.43.7×108
    1757.440.834.7224.26.73.97.81.6×1047.3×10634.32.3×108
    下载: 导出CSV
  • [1] HEAD J W,GIFFORD A. Lunar mare domes:classification and modes of origin[J]. The moon and the planets,1980,22(2):235-258. doi:  10.1007/BF00898434
    [2] HEAD J W,McCORD T B. Imbrian-age highland volcanism on the Moon:the Gruithuisen and Mairan domes[J]. Science,1978,199(4336):1433-1436. doi:  10.1126/science.199.4336.1433
    [3] 何姝珺. 月表静海地区地质构造分布特征及其演化分析[D]. 北京: 中国地质大学(北京), 2014.

    HE S J. Distribution characteristics and evolution analysis of geological structures in the l unar surface Jinghai area [D]. China University of Geosciences (Beijing), 2014.
    [4] KUSUMA K N,SEBASTIAN N,MURTY S V S. Geochemical and mineralogical analysis of Gruithuisen region on Moon using M3 and DIVINER images[J]. Planetary and Space Science,2012,67(1):46-56. doi:  10.1016/j.pss.2012.02.012
    [5] WHITFORD-STARK,JAMES L,HEAD J W. The Procellarum volcanic complexes-contrasting styles of volcanism[J]. Lunar and Planetary Science Conference Proceedings,1977:2705-2724.
    [6] WEITZ,CATHERINE M,HEAD III,et al. Spectral properties of the Marius Hills volcanic complex and implications for the formation of lunar domes and cones[J]. Journal of Geophysical Research:Planets,1999,104(E8):18933-18956. doi:  10.1029/1998JE000630
    [7] ZHAO J,XIAO L,QIAO L,et al. The Mons Rümker volcanic complex of the Moon:a candidate landing site for the Chang'E-5 mission[J]. Journal of Geophysical Research:Planets,2017,122(7):1419-1442.
    [8] SCOTT D H,EGGLETON R E SMITH E I. Geologic map of the Rumker quadrangle of the Moon[J]. US Geological Survey Report,1973:805.
    [9] GLOTCH, TIMOTHY D , LUCEY P, et al. The Mairan domes: silicic volcanic constructs on the Moon[J]. Geophysical Research Letters, 2011, 38(21).
    [10] LUCEY,PAUL G,BLEWETT,et al. Lunar iron and titanium abundance algorithms based on final processing of Clementine ultraviolet‐visible images[J]. Journal of Geophysical Research:Planets,2000,105(E8):20297-20305. doi:  10.1029/1999JE001117
    [11] WÖHLER,CHRIETIAN,LENA R et al. A combined spectrophotometric and morphometric study of the lunar mare dome fields near Cauchy,Arago,Hortensius,and Milichius[J]. Icarus,2006,183(2):237-264. doi:  10.1016/j.icarus.2006.03.003
    [12] WÖHLER,CHRIETIAN,LENA R,et al. Formation of lunar mare domes along crustal fractures:Rheologic conditions,dimensions of feeder dikes,and the role of magma evolution[J]. Icarus,2007,189(2):279-307. doi:  10.1016/j.icarus.2007.01.011
    [13] LENA R, WÖHLER C, PHILLIPS J, et al. Lunar domes: properties and formation processes[M]. Italia: Springer Science & Business Media, 2013: 59-65.
    [14] 李春来,刘建军,任鑫,等. 基于嫦娥二号立体影像的全月高精度地形重建[J]. 武汉大学学报(信息科学版),2018,43(4):485-495.

    LI C L,LIU J,REN X,et al. Full month high-precision terrain reconstruction based on Chang'e-2 stereo image[J]. Journal of Wuhan University (Information Science Edition),2018,43(4):485-495.
    [15] REN X,LIU J,LI C,et al. A global adjustment method for photogrammetric processing of Chang’E-2 stereo images[J]. IEEE Transactions on Geoscience and Remote Sensing,2019,57(9):6832-6843. doi:  10.1109/TGRS.2019.2908813
    [16] CHEN Y,HUANG Q,ZHAO J,et al. Unsupervised machine learning on domes in the lunar gardner region:implications for dome classification and local magmatic activities on the Moon[J]. Remote Sensing,2021,13(5):845. doi:  10.3390/rs13050845
    [17] LIONE W,HEAD J W,et al. Lunar gruithuisen and mairan domes:rheology and mode of emplacement[J]. Journal of Geophysical Research:Planets,2003,108(E2):5012.
    [18] BLAKE S. Viscoplastic models of lava domes[M]//Lava Flows and Domes. Berlin: Springer, 1990.
    [19] BOYCE J M,GIGUERE T,MOUGINIS-MARK P,et al. Geology of Mairan middle dome:its implication to silicic volcanism on the Moon[J]. Planetary and Space Science,2018,162:62-72. doi:  10.1016/j.pss.2017.12.009
    [20] WIECZOREK M A,ZUBER M T,PHILLIPS R J,et al. The role of magma buoyancy on the eruption of lunar basalts[J]. Earth and Planetary Science Letters,2001,185(1-2):71-83. doi:  10.1016/S0012-821X(00)00355-1
    [21] WAGNER R,HEAD J,WOLF U,et al. Stratigraphic sequence and ages of volcanic units in the Gruithuisen region of the Moon[J]. Journal of Geophysical Research:Planets,2002,107(E11):14-1-14-15.
  • [1] 李海涛, 程承, 黄磊, 陈少伍, 李宇波, 强立, 康凯.  “嫦娥五号”发射及入轨段X频段测控任务设计 . 深空探测学报(中英文), doi: 10.15982/j.issn.2096-9287.2022.20210099
    [2] 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),
    [3] 周昌义, 王赤, 李慧军, 孙辉先, 江源源, 何志平, 周斌, 杨建峰, 周维佳, 胡永富, 范开春, 徐欣锋, 周晴, 王雷, 张宝明.  “嫦娥五号”探测器有效载荷分系统设计 . 深空探测学报(中英文), doi: 10.15982/j.issn.2096-9287.2021.20200050
    [4] 刘志强, 赵晨, 曹彦, 陈建岳, 杨敏, 李天义.  “嫦娥五号”轨道器供配电系统高比能设计 . 深空探测学报(中英文), doi: 10.15982/j.issn.2096-9287.2021.20210007
    [5] 李轶, 黎藜, 郭明姝, 王同磊, 张国峰, 李晓锋.  “嫦娥五号”探测器GNC应用软件高可信研制技术 . 深空探测学报(中英文), doi: 10.15982/j.issn.2096-9287.2021.20200065
    [6] 裴照宇, 任俊杰, 彭兢, 王琼, 胡震宇, 李海涛, 黄磊, 耿光有.  “嫦娥五号”任务总体方案权衡设计 . 深空探测学报(中英文), doi: 10.15982/j.issn.2096-9287.2021.20210028
    [7] 刘攀, 王志国, 刘建峰, 闵康磊, 游红俊.  “嫦娥五号”载荷数据存储管理方法 . 深空探测学报(中英文), doi: 10.15982/j.issn.2096-9287.2021.20210001
    [8] 任天鹏, 路伟涛, 孔静, 谢剑锋, 韩松涛, 王美, 满海钧, 牛东文, 刘河山, 周之金.  “嫦娥五号”深空干涉测量性能分析 . 深空探测学报(中英文), doi: 10.15982/j.issn.2096-9287.2021.20210055
    [9] 胡晓东, 张宽, 谢圆, 张辉, 卢皓, 刘传凯, 陈翔, 赵焕洲, 谢剑锋.  “嫦娥五号”月面采样机械臂路径规划 . 深空探测学报(中英文), doi: 10.15982/j.issn.2096-9287.2021.20210095
    [10] 孟占峰, 高珊, 彭兢.  基于轨道任务几何的“嫦娥五号”采样区选择 . 深空探测学报(中英文), doi: 10.15982/j.issn.2096-9287.2021.20210023
    [11] 李海涛, 陈少伍, 李赞, 樊敏, 程承.  “嫦娥五号”任务再入返回段测控布站区域确定方法 . 深空探测学报(中英文), doi: 10.15982/j.issn.2096-9287.2021.20200053
    [12] 王亚林, 刘鹏, 吴辉阳, 黎衡, 赵巍.  碎石堆构造小行星表面地形分析与仿真验证 . 深空探测学报(中英文), doi: 10.15982/j.issn.2095-7777.2019.05.009
    [13] 郭弟均, 刘建忠, HEADW.James, 李帅, POTTERW.K.Ross, 林红磊.  月球阿波罗盆地区域月壳结构及光谱特征 . 深空探测学报(中英文), doi: 10.15982/j.issn.2095-7777.2018.05.013
    [14] 连懿, 何龙, 孟治国, 平劲松, 胡硕, 曾晓明.  基于场理论的“嫦娥4号”着陆区亮温时空分布特征研究 . 深空探测学报(中英文), doi: 10.15982/j.issn.2095-7777.2018.01.004
    [15] 黄倩, 王太茂, 赵健楠, 孟治国.  “嫦娥4号”月球背面着陆区月壳及深部结构特征 . 深空探测学报(中英文), doi: 10.15982/j.issn.2095-7777.2018.01.006
    [16] 徐青, 王栋, 邢帅, 蓝朝桢.  小行星形貌测绘与表征技术 . 深空探测学报(中英文), doi: 10.15982/j.issn.2095-7777.2016.04.007
    [17] 刘建忠, 郭弟均, 籍进柱, 刘敬稳, 王庆龙.  月球的构造格架及其演化差异 . 深空探测学报(中英文), doi: 10.15982/j.issn.2095-7777.2015.01.011
    [18] 王栋, 徐青, 邢帅, 刘衷瑞.  小行星形貌特征的分析与描述 . 深空探测学报(中英文), doi: 10.15982/j.issn.2095-7777.2015.04.010
    [19] 魏若岩, 阮晓钢, 庞涛, OuattaraSIE, 武旋, 肖尧.  小天体软着陆中的地面特征区域提取与跟踪算法 . 深空探测学报(中英文), doi: 10.15982/j.issn.2095-7777.2014.04.011
    [20] CliveNEAL, 平劲松.  月球仍然活跃的构造、火成和内部特征等证据 . 深空探测学报(中英文), doi: 10.15982/j.issn.2095-7777.2014.03.001
  • 加载中
计量
  • 文章访问数:  112
  • 被引次数: 0
出版历程
  • 网络出版日期:  2022-03-08

“嫦娥五号”采样点周缘穹窿形貌特征及成因研究

doi: 10.15982/j.issn.2096-9287.2022.20210068
    作者简介:

    吴文慧(2001– ),女,硕士研究生,主要研究方向:资源勘查工程(固体矿产)。通讯地址:中国地质大学(北京)地球科学与资源学院(100083)E-mail:wenhuiwu@163.com

    任鑫(1978– ),男,副研究员,主要研究方向:行星遥感。本文通讯作者。通讯地址:中国科学院国家天文台月球与深空探测实验室(100012)E-mail:renx@nao.cas.cn

  • ● Using Chang'e image data, 17 volcanic domes around Chang'e 5 sampling point are delineated, of which the newly discovered dome is No. 11. ● Based on the morphological and rheological characteristics, the characteristics of Rümker mare domes and Mairan non- mare domes around Chang'e 5 sampling point are compared. ● The division of lunar mare domes and non-mare domes should be determined in combination with its morphological parameters, geographical location, rheological parameters, material composition and other parameters.
  • 中图分类号: V412.41

摘要: “嫦娥五号”采样点周缘区域分布有吕姆克山(Mons Rümker)和Mairan火山穹窿构造。通过“嫦娥”影像和地形数据对两类穹窿的形貌特征和形成因素展开对比研究,讨论穹窿的划分标准。共计圈定了吕姆克山13个月海穹窿和Mairan所在的4个非月海穹窿,并计算了穹窿形成过程中的岩浆流变学参数。研究结果表明:吕姆克山月海穹窿较为低缓,按照坡度和高度划分为吕姆克山第一类月海穹窿(坡度均< 5°,高度200~400 m)和吕姆克山第二类月海穹窿(坡度5°~7°,高度300~600 m),其中第二类较高陡的月海穹隆具有较高的粘度和更低的喷发速率。 Mairan非月海穹窿更为高陡,其岩浆喷发速率低于吕姆克山月海穹窿,岩浆粘度较高,流动性较差,喷发周期较长;在空间上,Mairan所在的4个非月海穹窿呈线性展布,其物质成分和形成时间相近,表明彼此关联的可能性很大。

注释:
1)  ● Using Chang'e image data, 17 volcanic domes around Chang'e 5 sampling point are delineated, of which the newly discovered dome is No. 11. ● Based on the morphological and rheological characteristics, the characteristics of Rümker mare domes and Mairan non- mare domes around Chang'e 5 sampling point are compared. ● The division of lunar mare domes and non-mare domes should be determined in combination with its morphological parameters, geographical location, rheological parameters, material composition and other parameters.

English Abstract

吴文慧, 任鑫, 帕丽古力·杰恩斯, 陈媛, 孙国洋. “嫦娥五号”采样点周缘穹窿形貌特征及成因研究[J]. 深空探测学报(中英文). doi: 10.15982/j.issn.2096-9287.2022.20210068
引用本文: 吴文慧, 任鑫, 帕丽古力·杰恩斯, 陈媛, 孙国洋. “嫦娥五号”采样点周缘穹窿形貌特征及成因研究[J]. 深空探测学报(中英文). doi: 10.15982/j.issn.2096-9287.2022.20210068
WU Wenhui, Paliguli·JIEENSI, REN Xin, CHEN Yuan, SUN Guoyang. Study on the Morphological Characteristics and Genesis of Dome Around Chang'e 5 Sampling Point[J]. Journal of Deep Space Exploration. doi: 10.15982/j.issn.2096-9287.2022.20210068
Citation: WU Wenhui, Paliguli·JIEENSI, REN Xin, CHEN Yuan, SUN Guoyang. Study on the Morphological Characteristics and Genesis of Dome Around Chang'e 5 Sampling Point[J]. Journal of Deep Space Exploration. doi: 10.15982/j.issn.2096-9287.2022.20210068
参考文献 (21)

返回顶部

目录

    /

    返回文章
    返回