Article(id=1157393074587615306, tenantId=1146029695717560320, journalId=1146032081894723586, issueId=1157393070754025641, articleNumber=null, orderNo=9, doi=10.3981/j.issn.2097-0781.2024.01.008, pmid=null, cstr=null, oa=null, hot=null, price=null, onlineType=0, articleFormat=0, articleType=null, articleTypeStr=research-article, receivedDate=1700409600000, receivedDateStr=2023-11-20, revisedDate=1706025600000, revisedDateStr=2024-01-24, acceptedDate=null, acceptedDateStr=null, onlineDate=1753873612304, onlineDateStr=2025-07-30, pubDate=1710864000000, pubDateStr=2024-03-20, doiRegisterDate=null, doiRegisterDateStr=null, onlineIssueDate=1711468800000, onlineIssueDateStr=2024-03-27, onlineJustAcceptDate=null, onlineJustAcceptDateStr=null, onlineFirstDate=null, onlineFirstDateStr=null, sourceXml=null, magXml=null, createTime=1753873612304, creator=13701087609, updateTime=1774072493930, updator=sys-migrate, issue=Issue{id=1157393070754025641, tenantId=1146029695717560320, journalId=1146032081894723586, year='2024', volume='3', issue='1', pageStart='100', pageEnd='147', issueExtLink='null', onlineDate='null', pubDate='null', beforeIssueId=null, nextIssueId=null, price=null, status=1, issueComplete=1, articleOrder=1, issueType=-1, specialIssue=1, createTime=1753873611366, creator=13701087609, updateTime=1776075110816, updator=13041195026, preIssue=null, nextIssue=null, ext={EN=IssueExt(id=1250512908678017028, tenantId=1146029695717560320, journalId=1146032081894723586, issueId=1157393070754025641, language=EN, specialIssueTitle=Science and Technology Foresight, coverIllustrator=, specialIssueEditor=, specialIssueAbout=), CN=IssueExt(id=1250512908682211333, tenantId=1146029695717560320, journalId=1146032081894723586, issueId=1157393070754025641, language=CN, specialIssueTitle=月球及火星等地外行星科考基地建设探索专刊, coverIllustrator=, specialIssueEditor=, specialIssueAbout=)}, issueFiles=null}, startPage=100, endPage=108, ext={EN=ArticleExt(id=1157393075258703947, articleId=1157393074587615306, tenantId=1146029695717560320, journalId=1146032081894723586, language=EN, title=Research Status and Development Direction of Lunar Lava Tube Exploration, columnId=1149656489310208610, journalTitle=Science and Technology Foresight, columnName=Review and Commentary, runingTitle=null, highlight=null, articleAbstract=

The construction of scientific research stations is an important goal in current international lunar exploration, and lava tubes are one of the most important candidates for the construction of scientific research stations. This paper discusses the importance of lunar lava tubes as natural caves during the construction of lunar scientific research stations and bases, and reviews the existing understanding of lunar lava tubes in China and abroad, and focuses on the process and significance of lunar lava tube exploration and proposes future development trends for the key challenges in detecting these lava tubes. In addition, in the context of China’s lunar exploration project, this paper proposes a development strategy for China’s future lunar and deep-space exploration endeavors.

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建设月球科研站是当今国际上探月的重要目标，熔岩管是科研站的重要候选地之一。文章探讨了月球熔岩管作为天然洞穴对于建设月球科研站和月球基地的重要性，回顾了国内外月球熔岩管的现有认识，重点讨论了其探索过程和研究意义。针对月球熔岩管探测的技术难点，提出了未来发展趋势。结合中国的“嫦娥”系列探月工程，给出了相关建议。

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郑翀，博士。主要从事月球重力场及内部结构研究。电子信箱：chongz@whu.edu.cn。

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郑翀，博士。主要从事月球重力场及内部结构研究。电子信箱：chongz@whu.edu.cn。

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李斐，教授。中国绕月探测工程科学应用专家委员会委员，教育部地球物理学类专业教学指导委员会主任。主要从事月球和行星重力场及内部结构研究。获国家科技进步二等奖。发表论文180余篇。电子信箱：fli@whu.edu.cn。

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李斐，教授。中国绕月探测工程科学应用专家委员会委员，教育部地球物理学类专业教学指导委员会主任。主要从事月球和行星重力场及内部结构研究。获国家科技进步二等奖。发表论文180余篇。电子信箱：fli@whu.edu.cn。

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China lunar exploration program[J]. Journal of Deep Space Exploration, 2019, 6(5): 405-416. (in Chinese), articleTitle=China lunar exploration program, refAbstract=The Chang'E-4 probe was successfully soft landed on the far side of the moon for the first time as a human spacecraft on January 3, 2019, while the lunar rover named as "Yutu-2" leaving Chinese footprints on the Moon. So far, 125 lunar exploration activities have been carried out in the world, during which there are two important periods. During the period from 1950s to 1970s, the first round of lunar exploration culminated with the purposes of the race between the two space powers the U. S. and the former Soviet Union. After that, from the end of last century to now, many countries realize the strategic significance of the Lunar exploration, proposing their new lunar exploration plans, which culminated the second round of lunar exploration. Starting from the Chang'E-1 orbiter project in 2004, China has implemented five successful lunar missions, include Chang'E-1, 2, 3, 4, and Lunar Sample Return flight test. All five missions are successful, and great achievements have been made in space technology, space science and application, personal training, and international cooperation. China will continue lunar exploration activities mainly with unmanned Lunar Scientific Research Station.), Reference(id=1242113346472837678, tenantId=1146029695717560320, journalId=1146032081894723586, articleId=1157393074587615306, doi=10.3981/j.issn.2097-0781.2022.01.002, pmid=null, pmcid=null, year=2022, volume=1, issue=1, pageStart=17, pageEnd=27, url=null, language=null, rfNumber=[2], rfOrder=2, authorNames=于登云, 马继楠, journalName=前瞻科技, refType=null, unstructuredReference=于登云, 马继楠. 中国深空探测进展与展望[J]. 前瞻科技, 2022, 1(1): 17-27., articleTitle=中国深空探测进展与展望, refAbstract=在简要分析世界主要航天国家和新兴航天国家深空探测进展的基础上,系统梳理了中国深空探测所取得的主要技术和科学进展,对未来的深空探测任务和需要重点突破的主要关键技术提出展望,为后续深空探测发展提供参考。), Reference(id=1242113346548335151, tenantId=1146029695717560320, journalId=1146032081894723586, articleId=1157393074587615306, doi=10.3981/j.issn.2097-0781.2022.01.002, pmid=null, pmcid=null, year=2022, volume=1, issue=1, pageStart=17, pageEnd=27, url=null, language=null, rfNumber=[2], rfOrder=3, authorNames=Yu D Y, Ma J N, journalName=Science and Technology Foresight, refType=null, unstructuredReference=Yu D Y, Ma J N. 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After analyzing the progress in deep space exploration of major aerospace countries and emerging ones in the world, this paper systematically summarizes the main scientific and technological achievements regarding deep space exploration in China. Moreover, it provides an outlook on future deep space exploration and main key technologies. This review can serve as reference for the follow-up development of deep space exploration in China.

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Boston: McGraw-Hill, 2006., articleTitle=null, refAbstract=null), Reference(id=1242113346854519348, tenantId=1146029695717560320, journalId=1146032081894723586, articleId=1157393074587615306, doi=10.1007/BF00561842, pmid=null, pmcid=null, year=1971, volume=3, issue=3, pageStart=289, pageEnd=314, url=http://link.springer.com/10.1007/BF00561842, language=null, rfNumber=[6], rfOrder=8, authorNames=Greeley R, journalName=The Moon, refType=null, unstructuredReference=Greeley R. Lava tubes and channels in the lunar Marius Hills[J]. 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Geophysical Research Letters, 2017, 44(20): 10155-10161., articleTitle=Detection of intact lava tubes at Marius Hills on the Moon by SELENE (Kaguya) Lunar Radar Sounder, refAbstract=null), Reference(id=1242113347043263031, tenantId=1146029695717560320, journalId=1146032081894723586, articleId=1157393074587615306, doi=null, pmid=null, pmcid=null, year=1969, volume=1, issue=null, pageStart=75, pageEnd=80, url=null, language=null, rfNumber=[9], rfOrder=11, authorNames=Oberbeck V R, Quaide W L, Greeley R, journalName=Modern Geology, refType=null, unstructuredReference=Oberbeck V R, Quaide W L, Greeley R. On the origin of lunar sinuous rilles[J]. Modern Geology, 1969, 1: 75-80., articleTitle=On the origin of lunar sinuous rilles, refAbstract=null), Reference(id=1242113347110371896, tenantId=1146029695717560320, journalId=1146032081894723586, articleId=1157393074587615306, doi=10.1029/RG014i002p00265, pmid=null, pmcid=null, year=1976, volume=14, issue=null, pageStart=265, pageEnd=300, url=https://agupubs.onlinelibrary.wiley.com/doi/10.1029/RG014i002p00265, language=null, rfNumber=[10], rfOrder=12, authorNames=Head J, journalName=Reviews of Geophysics, refType=null, unstructuredReference=Head J. Lunar volcanism in space and time[J]. Reviews of Geophysics, 1976, 14: 265-300., articleTitle=Lunar volcanism in space and time, refAbstract=Lunar volcanic deposits are dominated by areally extensive mare units occurring in regionally low areas predominantly on the lunar near side. Data obtained from lunar orbit and earth‐based observations have been used to extend the detailed characterizations derived from Apollo and Luna sample return missions to other parts of the moon. Mare volcanism occurred over a period of about 1.3 billion years (b.y.), from about 3.8 to about 2.5 b.y. ago, although the absolute age of the youngest flows is not known. An early Ti‐rich mare phase (Apollo 11 and Apollo 17 type basalts) flooded large areas of the eastern portion of the lunar near side in the early Imbrian Period (about 3.5–3.8 b.y. ago). An intermediate age, less Ti‐rich phase (Apollo 12 and Apollo 15 type basalts) flooded widespread areas of the moon predominantly in the middle to late Imbrian Period (about 3.0–3.5 b.y. ago). Finally, a second Ti‐rich phase (unsampled by Apollo and Luna) flooded portions of Mare Imbrium and the western maria in the early Eratosthenian Period (about 2.5–3.0 b.y. ago). Features associated with mare deposits and processes include lobate scarps, sinuous rilles, domes, cones, dark halo craters, collapse craters, kipukas, lava terraces, mare ridges, and volcanic complexes. The very fluid nature of lunar lavas, their voluminous and extensive flows, and the dominance of volcanic landforms of nonexplosive origin all strongly indicate that lunar eruptions and deposits are most similar to terrestrial basaltic flood and Hawaiian eruptions. Volcanic morphologic features, deposit volumes, extrusion rates, and association of many sources with major crustal fractures all suggest that mare lavas originated at subcrustal depths and worked their way to the lunar surface through a passive but fractured lunar crust. Lavas preferentially infilled the existing low regions of the moon, apparently in a hydrostatic mode. Since lunar impact basins produce most of the topographic lows, mare deposits are concentrated in and around these features. The lunar crust acted essentially as a passive platform on which mare lavas were emplaced. Far side mare deposits are patchy but are concentrated on the floors of the largest basins. Thicker far side crust and hydrostatic emplacement of mare lavas may explain the lack of extensive far side deposits even in deep basins. Individual maria had a history of filling largely determined by the geometry and state of degradation of the basins in which they occur. Mare deposits are generally less than about 2 km in thickness but probably approach 6–8 km locally in the center of some mare basins. The process of filling took place over extensive periods of time and produced complex deposits. Although some near‐surface fractionation of mare lavas must have occurred, there is little photogeologic evidence for environments in which extensive fractionation would take place; lavas appear to have erupted at high rates, to have been very fluid, and to have spread out into thin flows; evidence is lacking for shallow magma reservoirs and for lava lakes on the scale of a mare basin. The portion of lunar mare deposits emplaced on the surface of the moon represents less than 1% of the total volume of the lunar crust. There is little unequivocal morphologic evidence for extensive highland volcanism, although intense bombardment may have erased such evidence from early lunar history. The majority of upland plains appear to be related to impact processes. Morphologic evidence for local highland volcanism is found primarily in the form of spectrally distinct domes.), Reference(id=1242113347169092153, tenantId=1146029695717560320, journalId=1146032081894723586, articleId=1157393074587615306, doi=null, pmid=null, pmcid=null, year=1973, volume=null, issue=null, pageStart=null, pageEnd=null, url=null, language=null, rfNumber=[11], rfOrder=13, authorNames=Keihm S, Langseth M, journalName=Proceedings of Lunar and Planetary Science Conference, refType=null, unstructuredReference=Keihm S, Langseth M. Surface brightness temperatures at the Apollo 17 heat flow site: Thermal conductivity of the upper 15 cm of regolith[C]// Proceedings of Lunar and Planetary Science Conference. Houston: Lunar and Planetary Institute, 1973., articleTitle=Surface brightness temperatures at the Apollo 17 heat flow site: Thermal conductivity of the upper 15 cm of regolith, refAbstract=null), Reference(id=1242113347240395322, tenantId=1146029695717560320, journalId=1146032081894723586, articleId=1157393074587615306, doi=null, pmid=null, pmcid=null, year=2021, volume=48, issue=11, pageStart=null, pageEnd=null, url=null, language=null, rfNumber=[12], rfOrder=14, authorNames=Qian Y Q, Xiao L, Head J W, journalName=Geophysical Research Letters, refType=null, unstructuredReference=Qian Y Q, Xiao L, Head J W, et al. The long sinuous rille system in Northern Oceanus Procellarum and its relation to the Chang’e‐5 returned samples[J]. 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Geophysical Research Letters, 2017, 44(1): 105-112., articleTitle=Evidence of large empty lava tubes on the Moon using GRAIL gravity, refAbstract=null), Reference(id=1242113347374613052, tenantId=1146029695717560320, journalId=1146032081894723586, articleId=1157393074587615306, doi=null, pmid=null, pmcid=null, year=2023, volume=null, issue=null, pageStart=null, pageEnd=null, url=null, language=null, rfNumber=[14], rfOrder=16, authorNames=郑翀, journalName=基于重力场的月球典型浅层结构研究, refType=null, unstructuredReference=郑翀. 基于重力场的月球典型浅层结构研究[D]. 武汉: 武汉大学, 2023., articleTitle=null, refAbstract=null), Reference(id=1242113347441721917, tenantId=1146029695717560320, journalId=1146032081894723586, articleId=1157393074587615306, doi=null, pmid=null, pmcid=null, year=2023, volume=null, issue=null, pageStart=null, pageEnd=null, url=null, language=null, rfNumber=[14], rfOrder=17, authorNames=Zheng C, journalName=A Research on lunar shallow typical structure using gravity field, refType=null, unstructuredReference=Zheng C. A Research on lunar shallow typical structure using gravity field[D]. Wuhan: Wuhan University, 2023. (in Chinese), articleTitle=null, refAbstract=null), Reference(id=1242113347504636478, tenantId=1146029695717560320, journalId=1146032081894723586, articleId=1157393074587615306, doi=10.1016/j.icarus.2016.10.008, pmid=null, pmcid=null, year=2017, volume=282, issue=null, pageStart=47, pageEnd=55, url=https://linkinghub.elsevier.com/retrieve/pii/S0019103516303566, language=null, rfNumber=[15], rfOrder=18, authorNames=Blair D M, Chappaz L, Sood R, journalName=Icarus, refType=null, unstructuredReference=Blair D M, Chappaz L, Sood R, et al. The structural stability of lunar lava tubes[J]. 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Houston: Lunar and Planetary Institute, 1976: 3143-3171., articleTitle=Revised lunar heat-flow values, refAbstract=null), Reference(id=1242113347622076992, tenantId=1146029695717560320, journalId=1146032081894723586, articleId=1157393074587615306, doi=null, pmid=null, pmcid=null, year=2018, volume=48, issue=11, pageStart=87, pageEnd=100, url=null, language=null, rfNumber=[17], rfOrder=20, authorNames=肖龙, 黄俊, 赵佳伟, journalName=中国科学: 物理学力学天文学, refType=null, unstructuredReference=肖龙, 黄俊, 赵佳伟, 等. 月面熔岩管洞穴探测的意义与初步设想[J]. 中国科学: 物理学力学天文学, 2018, 48(11): 87-100., articleTitle=月面熔岩管洞穴探测的意义与初步设想, refAbstract=null), Reference(id=1242113347680797249, tenantId=1146029695717560320, journalId=1146032081894723586, articleId=1157393074587615306, doi=null, pmid=null, pmcid=null, year=2018, volume=48, issue=11, pageStart=87, pageEnd=100, url=null, language=null, rfNumber=[17], rfOrder=21, authorNames=Xiao L, Huang J, Zhao J W, journalName=Scientia Sinica (Physica, Mechanica & Astronomica), refType=null, unstructuredReference=Xiao L, Huang J, Zhao J W, et al. Significance and preliminary proposal for exploring the lunar lava tubes[J]. Scientia Sinica (Physica, Mechanica & Astronomica), 2018, 48(11): 87-100. (in Chinese), articleTitle=Significance and preliminary proposal for exploring the lunar lava tubes, refAbstract=null), Reference(id=1242113347777266242, tenantId=1146029695717560320, journalId=1146032081894723586, articleId=1157393074587615306, doi=10.1126/science.1178658, pmid=19779151, pmcid=null, year=2009, volume=326, issue=5952, pageStart=568, pageEnd=572, url=null, language=null, rfNumber=[18], rfOrder=22, authorNames=Pieters C M, Goswami J N, Clark R N, journalName=Science, refType=null, unstructuredReference=Pieters C M, Goswami J N, Clark R N, et al. Character and spatial distribution of OH/H₂O on the surface of the Moon seen by M³ on Chandrayaan-1[J]. Science, 2009, 326(5952): 568-572., articleTitle=Character and spatial distribution of OH/H₂O on the surface of the Moon seen by M³ on Chandrayaan-1, refAbstract=The search for water on the surface of the anhydrous Moon had remained an unfulfilled quest for 40 years. However, the Moon Mineralogy Mapper (M3) on Chandrayaan-1 has recently detected absorption features near 2.8 to 3.0 micrometers on the surface of the Moon. For silicate bodies, such features are typically attributed to hydroxyl- and/or water-bearing materials. On the Moon, the feature is seen as a widely distributed absorption that appears strongest at cooler high latitudes and at several fresh feldspathic craters. The general lack of correlation of this feature in sunlit M3 data with neutron spectrometer hydrogen abundance data suggests that the formation and retention of hydroxyl and water are ongoing surficial processes. Hydroxyl/water production processes may feed polar cold traps and make the lunar regolith a candidate source of volatiles for human exploration.), Reference(id=1242113347840180803, tenantId=1146029695717560320, journalId=1146032081894723586, articleId=1157393074587615306, doi=null, pmid=null, pmcid=null, year=2012, volume=null, issue=null, pageStart=139, pageEnd=null, url=null, language=null, rfNumber=[19], rfOrder=23, authorNames=Haruyama J, Morota T, Kobayashi S, journalName=Lunar holes and lava tubes as resources for lunar science and exploration, refType=null, unstructuredReference=Haruyama J, Morota T, Kobayashi S, et al. Lunar holes and lava tubes as resources for lunar science and exploration[M]// Badescu V. Moon. Berlin, Heidelberg: Springer, 2012: 139-163., articleTitle=null, refAbstract=null), Reference(id=1242113347903095364, tenantId=1146029695717560320, journalId=1146032081894723586, articleId=1157393074587615306, doi=10.1016/j.pss.2009.06.004, pmid=null, pmcid=null, year=2010, volume=58, issue=4, pageStart=592, pageEnd=598, url=https://linkinghub.elsevier.com/retrieve/pii/S0032063309001603, language=null, rfNumber=[20], rfOrder=24, authorNames=Léveillé R J, Datta S, journalName=Planetary and Space Science, refType=null, unstructuredReference=Léveillé R J, Datta S. Lava tubes and basaltic caves as astrobiological targets on earth and Mars: A review[J]. Planetary and Space Science, 2010, 58(4): 592-598., articleTitle=Lava tubes and basaltic caves as astrobiological targets on earth and Mars: A review, refAbstract=null), Reference(id=1242113347953427013, tenantId=1146029695717560320, journalId=1146032081894723586, articleId=1157393074587615306, doi=10.11947/j.AGCS.2022.20220139, pmid=null, pmcid=null, year=2022, volume=51, issue=6, pageStart=897, pageEnd=908, url=null, language=null, rfNumber=[21], rfOrder=25, authorNames=李斐, 郑翀, 叶茂, journalName=测绘学报, refType=null, unstructuredReference=李斐, 郑翀, 叶茂, 等. 月球形状及其重力场[J]. 测绘学报, 2022, 51(6): 897-908., articleTitle=月球形状及其重力场, refAbstract=本文首先从测绘科学与技术在月球探测中的应用角度,对月球形状及重力场的研究进展、获取方法及代表性成果进行了综述;进而针对现有的月球DEM及重力场模型中存在的主要问题进行分析,并提出了解决方案;最后结合各国的探月计划和我国正在实施的“嫦娥”四期工程,对月球形状和重力场研究面临的机遇和挑战进行了展望。), Reference(id=1242113348012147270, tenantId=1146029695717560320, journalId=1146032081894723586, articleId=1157393074587615306, doi=10.11947/j.AGCS.2022.20220139, pmid=null, pmcid=null, year=2022, volume=51, issue=6, pageStart=897, pageEnd=908, url=null, language=null, rfNumber=[21], rfOrder=26, authorNames=Li F, Zheng C, Ye M, journalName=Acta Geodaetica et Cartographica Sinica, refType=null, unstructuredReference=Li F, Zheng C, Ye M, et al. 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Finally, the opportunities and challenges in lunar shape and its gravity field research are prospected in the perspective of the lunar exploration programs of other countries and the ongoing fourth step of Chang'e project in China.), Reference(id=1242113348079256135, tenantId=1146029695717560320, journalId=1146032081894723586, articleId=1157393074587615306, doi=10.1007/s11214-012-9952-7, pmid=null, pmcid=null, year=2013, volume=178, issue=1, pageStart=3, pageEnd=24, url=http://link.springer.com/10.1007/s11214-012-9952-7, language=null, rfNumber=[22], rfOrder=27, authorNames=Zuber M T, Smith D E, Lehman D H, journalName=Space Science Reviews, refType=null, unstructuredReference=Zuber M T, Smith D E, Lehman D H, et al. Gravity recovery and interior laboratory (GRAIL): Mapping the lunar interior from crust to core[J]. 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Gravity field of the Moon and gravity survey on the lunar surfac[J]. Bulletin of National Natural Science Foundation of China, 2022, 36(6): 851-858. (in Chinese), articleTitle=Gravity field of the Moon and gravity survey on the lunar surfac, refAbstract=null), Reference(id=1242113348402217548, tenantId=1146029695717560320, journalId=1146032081894723586, articleId=1157393074587615306, doi=10.1126/science.1259866, pmid=null, pmcid=null, year=2015, volume=347, issue=6227, pageStart=1226, pageEnd=1229, url=https://www.science.org/doi/10.1126/science.1259866, language=null, rfNumber=[26], rfOrder=32, authorNames=Xiao L, Zhu P M, Fang G Y, journalName=Science, refType=null, unstructuredReference=Xiao L, Zhu P M, Fang G Y, et al. A young multilayered terrane of the northern Mare Imbrium revealed by Chang’e-3 mission[J]. Science, 2015, 347(6227): 1226-1229., articleTitle=A young multilayered terrane of the northern Mare Imbrium revealed by Chang’e-3 mission, refAbstract=\n In more active periods of the Moon's history, volcanic eruptions created lava plains that formed layers of dark basalt. Without subsurface probing, we can only examine the most recent flows. After the soft landing of the Chang'E-3 spacecraft, Xiao\n et al.\n made penetrating radar measurements of the lunar crust with the Yutu rover. Several subsurface layers suggest multiple geologic processes at play throughout the crustal history, including multiple lava flows and the weathering-induced creation of dust and rocky debris.\n), Reference(id=1242113348456743501, tenantId=1146029695717560320, journalId=1146032081894723586, articleId=1157393074587615306, doi=null, pmid=17796552, pmcid=null, year=1969, volume=166, issue=3903, pageStart=384, pageEnd=385, url=null, language=null, rfNumber=[27], rfOrder=33, authorNames=Nance R L, journalName=Science, refType=null, unstructuredReference=Nance R L. Gravity: First measurement on the lunar surface[J]. Science, 1969: 166(3903): 384-385., articleTitle=Gravity: First measurement on the lunar surface, refAbstract=The gravity at the landing site of the first lunar-landing mission has been determined to be 162,821.680 milligals from data telemetered to earth by the lunar module on the lunar surface. The gravity was measured with a pulsed integrating pendulous accelerometer. These measurements were used to compute the gravity anomaly and radius at the landing site.), Reference(id=1242113348519658062, tenantId=1146029695717560320, journalId=1146032081894723586, articleId=1157393074587615306, doi=10.1016/0031-9201(71)90040-9, pmid=null, pmcid=null, year=1971, volume=4, issue=3, pageStart=193, pageEnd=196, url=https://linkinghub.elsevier.com/retrieve/pii/0031920171900409, language=null, rfNumber=[28], rfOrder=34, authorNames=Nance R L, journalName=Physics of the Earth and Planetary Interiors, refType=null, unstructuredReference=Nance R L. Gravity measured at the Apollo 12 landing site[J]. Physics of the Earth and Planetary Interiors, 1971: 4(3): 193-196., articleTitle=Gravity measured at the Apollo 12 landing site, refAbstract=null)], funds=[Fund(id=1242113344769950251, tenantId=1146029695717560320, journalId=1146032081894723586, articleId=1157393074587615306, awardId=42030110, language=CN, fundingSource=国家自然科学基金(42030110), fundOrder=null, country=null)], companyList=[AuthorCompany(id=1242113342597300739, tenantId=1146029695717560320, journalId=1146032081894723586, articleId=1157393074587615306, xref=null, ext=[AuthorCompanyExt(id=1242113342605689348, tenantId=1146029695717560320, journalId=1146032081894723586, articleId=1157393074587615306, companyId=1242113342597300739, language=EN, country=null, province=null, city=null, postcode=null, companyName=null, departmentName=null, remark=1. Chongqing Satellite Network System Co. 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State Key Laboratory of Information Engineering in Surveying, Mapping and Remote Sensing, Wuhan University, Wuhan 430079, China), AuthorCompanyExt(id=1242113342681186824, tenantId=1146029695717560320, journalId=1146032081894723586, articleId=1157393074587615306, companyId=1242113342668603910, language=CN, country=null, province=null, city=null, postcode=null, companyName=null, departmentName=null, remark=2.武汉大学测绘遥感信息工程国家重点实验室，武汉 430079)])], figs=[ArticleFig(id=1242113344161776165, tenantId=1146029695717560320, journalId=1146032081894723586, articleId=1157393074587615306, language=EN, label=Fig. 1, caption=Lunar lava tube Rima Mairan, figureFileSmall=nihsFdWcgHj8yrwxxMUw/g==, figureFileBig=l5UPrC+kOlcTEdjPj1sYAQ==, tableContent=null), ArticleFig(id=1242113344224690726, tenantId=1146029695717560320, journalId=1146032081894723586, articleId=1157393074587615306, language=CN, label=图1, caption=月球的Rima Mairan熔岩管, figureFileSmall=nihsFdWcgHj8yrwxxMUw/g==, figureFileBig=l5UPrC+kOlcTEdjPj1sYAQ==, tableContent=null), ArticleFig(id=1242113344396657191, tenantId=1146029695717560320, journalId=1146032081894723586, articleId=1157393074587615306, language=EN, label=Fig. 2, caption=Position of the moonquake meter, figureFileSmall=MQmsEJ6zAuQdCEx7E9VXnA==, figureFileBig=GWkKjPrv6dPhROPUibYEWQ==, tableContent=null), ArticleFig(id=1242113344472154664, tenantId=1146029695717560320, journalId=1146032081894723586, articleId=1157393074587615306, language=CN, label=图2, caption=月震仪部署示意图, figureFileSmall=MQmsEJ6zAuQdCEx7E9VXnA==, figureFileBig=GWkKjPrv6dPhROPUibYEWQ==, tableContent=null), ArticleFig(id=1242113344539263529, tenantId=1146029695717560320, journalId=1146032081894723586, articleId=1157393074587615306, language=EN, label=Table 1, caption=

Candidates of potential lava tubes

, figureFileSmall=null, figureFileBig=null, tableContent=

名称	经度/(°E)	纬度/(°N)	长度/km
Schröter Extension	-54.0	24.0	60
Rima Mairan	-46.0	36.0	170
Rima Marius	-54.0	17.0	50
Marius Hills Skylight	-58.0	14.0	60
Rima Aristarchus	-47.0	27.0	100
Mairan-Rumker N-S	-51.0	41.0	90
Mairan-Rumker E-W	-54.0	41.0	180
Wollaston D	-49.0	35.0	80
Hershel E	-35.5	33.5	20
Rima Delisle	128.0	31.0	50
Cavelerius E	-80.5	8.5	75

), ArticleFig(id=1242113344610566698, tenantId=1146029695717560320, journalId=1146032081894723586, articleId=1157393074587615306, language=CN, label=表1, caption=

潜在熔岩管候选

, figureFileSmall=null, figureFileBig=null, tableContent=

名称	经度/(°E)	纬度/(°N)	长度/km
Schröter Extension	-54.0	24.0	60
Rima Mairan	-46.0	36.0	170
Rima Marius	-54.0	17.0	50
Marius Hills Skylight	-58.0	14.0	60
Rima Aristarchus	-47.0	27.0	100
Mairan-Rumker N-S	-51.0	41.0	90
Mairan-Rumker E-W	-54.0	41.0	180
Wollaston D	-49.0	35.0	80
Hershel E	-35.5	33.5	20
Rima Delisle	128.0	31.0	50
Cavelerius E	-80.5	8.5	75

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