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Scientific objectives and payload configuration of the Chang'E-7 mission

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National Science Review 2024年第2期11卷 285-300页

作者： Chi Wang Yingzhuo Jia Changbin Xue yangting lin Jianzhong Liu Xiaohui Fu lin Xu Yun Huang Yufen Zhao Yigang Xu Rui Gao Yong Wei Yuhua Tang Dengyun Yu Yongliao Zou State Key Laboratory of Space Weather National Space Science Center Chinese Academy of Sciences National Space Science Center Chinese Academy of Sciences Institute of Geology and Geophysics Chinese Academy of Sciences Institute of Geochemistry Chinese Academy of Sciences Shandong Provincial Key Laboratory of Optical Astronomy and Solar-Terrestrial Environment School of Space Science and Physics Institute of Space SciencesShandong University Institute of Drug Discovery Technology Ningbo University State Key Laboratory of Isotope Geochemistry Guangzhou Institute of Geochemistry Chinese Academy of Sciences School of Earth Science and Engineering Sun Yat-sen University Lunar Exploration and Space Engineering Center China Aerospace Science and Technology Corporation

As the cornerstone mission of the fourth phase of the Chinese Lunar Exploration Program, Chang'E-7(CE-7) was officially approved, and implementation started in 2022, including a main probe and a communication relay satellite. The main probe, consisting of an orbiter, a lander, a rover and a mini-flying probe, is scheduled to be launched in 2026. The lander will land on Shackleton crater's illuminated rim near the lunar south pole, along with the rover and mini-flying probe. The relay satellite(named Queqiao-2) will be launched in February 2024 as an independent mission to support relay communication during scientific exploration undertaken by Chang'E-4, the upcoming Chang'E-6 in 2024 and subsequent lunar *** CE-7 mission is mainly aimed at scientific and resource exploration of the lunar south pole. We present CE-7's scientific objectives, the scientific payloads configuration and the main functions for each scientific payload with its key technical specifications.

关键词： Chang’ E-7 scientific objectives scientific payloads

Return to the Moon:New perspectives on lunar exploration

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Science Bulletin 2024年第13期69卷 2136-2148页

作者： yangting lin Wei Yang Hui Zhang Hejiu Hui Sen Hu Long Xiao Jianzhong Liu Zhiyong Xiao Zongyu Yue Jinhai Zhang Yang Liu Jing Yang Honglei lin Aicheng Zhang Dijun Guo Sheng Gou lin Xu Yuyang He Xianguo Zhang Liping Qin Zongcheng ling Xiongyao Li Aimin Du Huaiyu He Peng Zhang Jinbin Cao Xianhua Li Key Laboratory of Earth and Planetary Physics Institute of Geology and GeophysicsChinese Academy of SciencesBeijing 100029China State Key Laboratory for Mineral Deposits Research and School of Earth Sciences and Engineering Nanjing UniversityNanjing 210023China State Key Laboratory of Geological Processes and Mineral Resources School of Earth SciencesChina University of GeosciencesWuhan 430074China Institute of Geochemistry Chinese Academy of SciencesGuiyang 550002China Planetary Environmental and Astrobiological Research Laboratory School of Atmospheric SciencesSun Yat-sen UniversityZhuhai 519082China National Space Science Center Chinese Academy of SciencesBeijing 100190China Deep Space Exploration Laboratory/CAS Key Laboratory of Crust-Mantle Materials and Environments University of Science and Technology of ChinaHefei 230026China Shandong Key Laboratory of Optical Astronomy and Solar-Terrestrial Environment Institute of Space SciencesShandong UniversityWeihai 264209China Technology and Engineering Center for Space Utilization Chinese Academy of SciencesBeijing 100094China School of Space and Environment Beihang UniversityBeijing 100191China

Lunar exploration is deemed crucial for uncovering the origins of the Earth-Moon system and is the first step for advancing humanity’s exploration of deep *** the past decade,the Chinese Lunar Exploration Program(CLEP),also known as the Chang’e(CE)Project,has achieved remarkable *** has successfully developed and demonstrated the engineering capability required to reach and return from the lunar ***,the CE Project has made historic firsts with the landing and on-site exploration of the far side of the Moon,along with the collection of the youngest volcanic samples from the Procellarum KREEP *** achievements have significantly enhanced our understanding of lunar *** on this success,China has proposed an ambitious crewed lunar exploration strategy,aiming to return to the Moon for scientific exploration and *** plan encompasses two primary phases:the first crewed lunar landing and exploration,followed by a thousand-kilometer scale scientific expedition to construct a geological cross-section across the lunar *** the limitations of current lunar exploration efforts and China’s engineering and technical capabilities,this paper explores the benefits of crewed lunar exploration while leveraging synergies with robotic *** study refines fundamental lunar scientific questions that could lead to significant breakthroughs,considering the respective engineering and technological *** research lays a crucial foundation for defining the objectives of future lunar exploration,emphasizing the importance of crewed missions and offering insights into potential advancements in lunar science.

关键词： Crewed lunar exploration Water and volatiles Composition and structure of lunar interior Volcanic activity and evolution of lunar mantle Space weathering and radiation environments Exploration technology

矿物微-纳尺度硫同位素分析及在东营凹陷油气成藏的应用示范

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岩石学报 2024年第1期40卷 313-322页

作者：郝佳龙张刘平李照阳杨蔚林杨挺中国科学院地质与地球物理研究所地球与行星物理院重点实验室北京100029 中国科学院地质与地球物理研究所油气资源研究院重点实验室北京100029 防灾科技学院三河市065201

黄铁矿等硫化物离子探针硫同位素分析已经广泛应用在成矿机理、古环境重建、大气环境硫源示踪及行星演化等研究中。纳米离子探针(CAMECA Nano SIMS 50L)的使用将硫化物硫同位素分析空间分辨率提升到微纳尺度(1μm~100nm),实现了分辨率1~... 详细信息

黄铁矿等硫化物离子探针硫同位素分析已经广泛应用在成矿机理、古环境重建、大气环境硫源示踪及行星演化等研究中。纳米离子探针(CAMECA Nano SIMS 50L)的使用将硫化物硫同位素分析空间分辨率提升到微纳尺度(1μm~100nm),实现了分辨率1~2μm、精度0.5‰(1SD)的硫同位素点分析方法,分辨率100nm、精度1‰的硫同位素图像分析方法。为了进一步优化分析流程拓展纳米离子探针硫同位素的应用,本文系统比较了纳米离子探针微纳尺度硫同位素点分析方法、图像分析方法的各自特点及分析流程;并以东营凹陷北带沙四段黄铁矿为研究对象,联合采用了纳米离子探针硫同位素点分析和硫同位素图像分析手段,对黄铁矿微细结构进行分析,从而揭示了储层中黄铁矿成因及其油气成藏的指示意义。

关键词：纳米离子探针硫同位素空间分辨率东营凹陷同位素图像

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首次在嫦娥五号月壤中鉴定出铁陨石碎片类型

Science Bulletin 2024年第4期69卷 554-561页

作者：刘小莹谷立新田恒次李静唐旭胡森林杨挺 Key Laboratory of Earth and Planetary Physics Institute of Geology and GeophysicsChinese Academy of SciencesBeijing 100029China College of Earth and Planetary Sciences University of Chinese Academy of SciencesBeijing 100049China

Lunar soil preserves numerous fragments of meteorites impacting on the Moon,providing a unique opportunity to investigate the distribution of the types of projectiles over billions of *** we report the first discovery of an iron meteorite fragment from the Chang’e-5 lunar soil,which consists mainly of martensite(quenched from taenite),kamacite,and schreibersite,with a trace of *** meteorite fragment is Ni-and P-rich,S-poor,and based on its mineral chemistry and bulk composition,can be classified into the IID-group,a rare and carbonaceous group of iron meteorite originating in the outer Solar *** meteorite fragment experienced only limited partial melting followed by fast cooling,suggestive of efficient preservation of intact remnants of iron meteorites impacting on the porous lunar ***,it is a relic of a low-velocity impact of submillimeter-sized metal grains originated from an IID-like iron *** observations demonstrate that it is feasible to achieve the type distribution of meteorites impacting on the Moon via systematically analyzing a large number of metal grains separated from lunar soils,thus shedding light on the dynamic evolution of the Solar System.

关键词： Chang’e-5 lunar soils Metal clast Iron meteorite Schreibersite Impact event

Analysis of platinum-group elements in drill core samples from the Meishan Permian-Triassic boundary section, China

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Chinese Journal Of Geochemistry 2014年第4期33卷 365-373页

作者： XU lin lin yangting Key Laboratory of Lunar and Deep Space Exploration National Astronomical Observatories Chinese Academy of Sciences State Key Laboratory of Lithospheric Evolution Institute of Geology and Geophysics Chinese Academy of Sciences

There is a long-standing controversy of what triggered the extinction at the Permian-Triassic boundary, the most severe mass extinction in the geologic record, including flood basaltic volcanism and/or bolide impact hypothesis. In order to clarify various pieces of evidence for the mass extinction event at the Permian-Triassic boundary, some researchers from some laboratories throughout the world have made a comprehensive study on a group of samples from the Meishan area of China. Some fresh core samples from the Permian-Triassic boundary in the Meishan area were analyzed in this study. The results showed that there is no Ir anomaly. Moreover, the PGEs patterns of those samples show obvious differentiation characteristics, that is different from the case encountered in meteorites. So no evidence supports the hypothesis of extraterrestrial impact. In contrast, the PGEs patterns are similar to those of Siberian and Emeishan basalts, which indicates that those PGEs are derived mainly from the basalts, lending a support to the correlation between mass extinction at the Permian-Triassic boundary and flood basaltic volcanism. This study has also confirmed the results for samples from section C prior to the analysis of the samples.

关键词：界线剖面铂族元素岩芯样品三叠系元素分析中国峨眉山玄武岩灭绝事件

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小行星探测历史及启示

空间科学学报 2024年第1期44卷 19-50页

作者：魏思佳何雨旸刘天宇杨蔚林杨挺中国科学院地质与地球物理研究所地球与行星物理重点实验室北京100029 中国科学院大学地球与行星科学学院北京100049 中国科学院地质与地球物理研究所矿产资源研究重点实验室北京100029

自1989年美国Galileo探测器在探测木星的途中顺访了小行星951 Gaspra和243 Ida起,小行星探测已经逐渐成为各主要航天国家深空探测的重点目标之一.过去30年,小行星探测任务从飞掠探测到专访探测再到采样返回,探测类型愈加丰富,并逐步从... 详细信息

自1989年美国Galileo探测器在探测木星的途中顺访了小行星951 Gaspra和243 Ida起,小行星探测已经逐渐成为各主要航天国家深空探测的重点目标之一.过去30年,小行星探测任务从飞掠探测到专访探测再到采样返回,探测类型愈加丰富,并逐步从单纯的科学探测发展到小行星防御与资源利用.中国预计在2025年发射天问二号,同时计划开展首次小行星防御任务.在此背景之下,本文详细分析了迄今为止小行星探测任务的历程、科学目标、科学载荷配置以及主要研究成果,并重点研究了日本Hayabusa和Hayabusa 2任务及美国OSIRISREx任务的样品储存管理、分配经验和返回样品实验室初步分析流程,以期对中国未来小行星探测任务的设计和实施提供参考.设计低成本、多频次采样返回任务;统筹任务规划,注重加强任务之间的配合;加强科学团队建设是更好地规划中国未来小行星探测任务的要点.

关键词：探测任务采样返回地外样品储存管理与分配分析流程

Bulk Chemical Composition of the Ningqiang Carbonaceous Chondrite:An Issue of Classification

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Acta Geologica Sinica(English Edition) 2007年第1期81卷 141-147页

作者： WANG Guiqin lin yangting Key Laboratory of Isotope Geochronology and Geochemistry Guangzhou Institute of Geochemistry Chinese Academy of Sciences Guangzhou Guangdong 510640 Graduate School Chinese Academy of Sciences Beijing 100049 State Key Laboratory of Lithosphere Tectonic Evolution Institute of Geology and Geophysics Chinese Academy of Sciences Beijing 100029

The Ningqiang meteorite is a fall carbonaceous chondrite, containing various Ca-, Al-rich inclusions that usually escaped from secondary events such as high-temperature heating and low- temperature alteration. However, it has not yet been classified into any known chemical group. In order to address this issue, 41 elements of the bulk Ningqiang meteorite were analyzed using inductively coupled plasma mass spectrometry （ICP-MS） and inductively coupled plasma atom emission spectrometry （ICP-AES） in this study. The Allende （CV3） carbonaceous chondrite and the Jilin （H5） ordinary chondrite were also measured as references, and our analyses are consistent with the previous results. Rare earth and other refractory lithophile elements are depleted in Ningqiang relative to both Allende and mean CK chondrites. In addition, the REE pattern of Ningqiang is nearly flat, while that of Allende shows slight enrichment of LREE relative to HREE. Siderophile elements of Ningqiang are close to those of mean CK chondrites, but lower than those of Allende. Our new analyses indicate that Ningqiang cannot be classified into any known group of carbonaceous chondrites, consistent with previous reports.

关键词： meteorite carbonaceous chondrite classification bulk composition ICP-MS

Space weathering simulation and spectrum decoding

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Chinese Journal Of Geochemistry 2012年第2期31卷 128-135页

作者： HU Sen lin yangting Key Laboratory of the Earth＇s Deep Interior Institute of Geology and Geophysics Chinese Academy of Science Beijing 100029 China Graduate University of Chinese Academy of Sciences Beijing 100049 China

Visible and near-infrared spectra are routinely used to achieve mineral abundances and mineral chemistry of the global surfaces of the Moon and ***,these spectra can be significantly modified by space weathering,including micrometeorite impacting,solar wind implanting and cosmic ray *** this paper we report results of laser-bombarding experiments on the Jilin ordinary chondrite,simulating micrometeorite impacting on the surface of *** laser bombardment,the spectra became significantly redder and moderately darker. With the Modified Gaussian Model(MGM)method,the absorption band positions of olivine can be decoded from the modified spectra,which are correlated with their fayalite *** addition,a continuum of the modified spectra can be decoded,and its slope may be used to depict the degree of space ***,relative strengths of the absorption sub-bands of olivine and pyroxenes show significant variant after the bombardment, hence they cannot be used to estimate the relative abundances of high-Ca to low-Ca pyroxenes of the lunar surface and other matured surfaces of asteroids.

关键词：解码风化近红外光谱月球表面频谱仿真太空普通球粒陨石

SHARAD study on the structures and permittivity of a buried impact crater in Martian Central Elysium Planitia

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Science China Earth Sciences 2023年第11期66卷 2452-2462页

作者： Peng FANG Wenzhe FA Jinhai ZHANG yangting lin Key Laboratory of Earth and Planetary Physics Institute of Geology and GeophysicsChinese Academy of SciencesBeijing 100029China Engineering Laboratory for Deep Resources Equipment and Technology Institute of Geology and GeophysicsChinese Academy of SciencesBeijing 100029China College of Earth and Planetary Sciences University of Chinese Academy of SciencesBeijing 100029China Institute of Remote Sensing and Geographical Information System School of Earth and Space SciencesPeking UniversityBeijing 100871China

The Elysium Planitia,located in the transition zone between the northern and southern hemispheres,is one of the key areas for studying the stratigraphic structure and geological history of *** studies have shown that this plain has undergone complex surface modification processes including fluvial and volcanic processes,and systematic progress has been made in the study of macro-geological ***,there are relatively few studies on the regional structure of the plain,which restricts our understanding of the regional geological processes.A buried impact crater in the central part of the Elysium Planitia could have recorded the surface modification process since the formation of the impact crater,however,it is difficult to distinguish the subsurface stratigraphy due to the weak orbital radar reflection *** this study,we denoised Shallow Radar data and obtained a radargram with clear subsurface *** estimated the permittivity of subsurface materials via a multilayer reflection *** results show that two subsurface reflectors divide the structure of the buried impact crater into three layers(overlying layer,underlying layer,and bottom layer).The shallow subsurface reflector covers almost the whole impact crater,while the deep subsurface reflector covers only the southwest part of the impact *** the permittivity inversion results with the geological background of lava activity in the Elysium Planitia area,we argue that the overlying layer may be a mixture of regolith and lava flow with low density,while the underlying layer and bottom layer are dense lava *** reflector between the underlying layer and bottom layer is probably a thin deposit derived from weathering between two lava activities,and its possible formation mechanism is as follows:the crater rim and peripheral ejecta has undergone relatively strong wind erosion and the eroded material was transport to the southwestern part of the impact crater,forming

关键词： Mars Elysium Planitia SHARAD Buried crater Permittivity inversion