月球佩塔维厄斯幅(LQ-21)数字地质填图与区域地质演化特征

doi:10.13745/j.esf.sf.2021.3.11

地学前缘 ›› 2022, Vol. 29 ›› Issue (2): 354-369.DOI: 10.13745/j.esf.sf.2021.3.11

• 月球地质与基础地质数据更新 • 上一篇下一篇

月球佩塔维厄斯幅(LQ-21)数字地质填图与区域地质演化特征

许可娟¹^,²(), 丁孝忠¹^,²^,^*(), 韩坤英¹^,², 刘敬稳³, 凌宗成⁴, 庞健峰¹^,², 王颖¹^,²

1.中国地质科学院地质研究所, 北京 100037
2.中国地质调查局全国地质编图研究中心, 北京 100037
3.中国科学院地球化学研究所月球与行星科学研究中心, 贵州贵阳 550002
4.山东大学空间科学院研究学院, 山东威海 264209

收稿日期:2020-12-28 修回日期:2021-03-06 出版日期:2022-03-25 发布日期:2022-03-31
通信作者: 丁孝忠
作者简介:许可娟(1987—),女,博士,主要从事区域地质编图及GIS应用的研究。E-mail: 867807379@qq.com
基金资助:
科学技术部科技基础性工作专项项目“月球数字地质图编研”(2015FY210500);国家自然科学基金专项项目(41941003);中国科学院前沿科学重点研究项目(QYZDY-SSW-DQC028)

Compilation of the geological map of the Petavius quadrangle of the Moon (LQ-21) and study on the regional geological evolution

XU Kejuan¹^,²(), DING Xiaozhong¹^,²^,^*(), HAN Kunying¹^,², LIU Jingwen³, LING Zongcheng⁴, PANG Jianfeng¹^,², WANG Ying¹^,²

1. Institute of Geology, Chinese Academy of Geological Sciences, Beijing 100037, China
2. National Research Center of Geological Mapping, China Geological Survey, Beijing 100037, China
3. Lunar and Planetary Science Research Center, Institute of Geochemistry, Chinese Academy of Sciences, Guiyang 550002, China
4. Institute of Space Sciences, Shandong University, Weihai 264209, China

Received:2020-12-28 Revised:2021-03-06 Online:2022-03-25 Published:2022-03-31
Contact: DING Xiaozhong

摘要/Abstract

摘要：

佩塔维厄斯幅月球地质图(LQ-21)位于近月面与远月面交接位置,又处于月海和月陆的过渡区,周边邻近酒海、丰富海、史密斯海等大型撞击盆地,是月球数字地质填图工作中的一个典型区域。研究该地区的地质发育概况有助于了解月球的发展演化历史。本文利用中国探月工程所获得的“嫦娥一号”(CE-1)CCD影像数据、干涉成像光谱仪(IIM)数据、激光高度计(LAM)数据和“嫦娥二号”(CE-2)CCD影像数据以及其他已有的月球地质资料,应用ArcGIS平台,开展月表物质成分、构造要素、地质时代信息的研究和数字填图工作,编制了1: 2 500 000佩塔维厄斯幅(LQ-21)数字月球地质图,总结了该地区区域地质演化历史并建立地质图空间数据库。

关键词: 月球, 佩塔维厄斯, 朗伦努斯, 地质演化, 数字地质填图

Abstract:

The Petavius quadrangle (LQ-21) is located at the junction of the near and far sides of the Moon in the transition zone between the mare and highland terrain. Large impact basins such as Nectaris, Foecunditatis, and Smythii basins are developed around this region. Understanding the geological development of this area is helpful for understanding the development and evolutionary history of the Moon. Accordingly, this area is a key area in the digital geological mapping of the Moon. This work combines the Chang’E-1(CE-1) CCD image data, interference imaging spectrometer(IIM) data, laser altimeter (LAM) data, Chang’E-2(CE-2) CCD image data, as well as other lunar geological data, to study the material composition, structural elements, and geochronology of the lunar surface, and to compile the lunar geological map using the ArcGIS platform. So far, we have completed the geological map of the Petavius quadrangle at 1: 2.5 million scale, summarized the regional geological evolutionary history, and established a spatial database for the geological map of this region.

Key words: Moon, Petavius, Langrenus, geological evolution, digital geological mapping

中图分类号:

许可娟, 丁孝忠, 韩坤英, 刘敬稳, 凌宗成, 庞健峰, 王颖. 月球佩塔维厄斯幅(LQ-21)数字地质填图与区域地质演化特征[J]. 地学前缘, 2022, 29(2): 354-369.

XU Kejuan, DING Xiaozhong, HAN Kunying, LIU Jingwen, LING Zongcheng, PANG Jianfeng, WANG Ying. Compilation of the geological map of the Petavius quadrangle of the Moon (LQ-21) and study on the regional geological evolution[J]. Earth Science Frontiers, 2022, 29(2): 354-369.

图/表 13

图1 1∶2 500 000佩塔维厄斯幅(LQ-21)月球地质图位置图(底图为CE-1 CCD影像数据)

Fig.1 Lunar geological overview map of the Petavius quadrangle (LQ-21) at 1∶2.5 million scale (with CE-1 CCD data overlay)

图2 1∶2 500 000佩塔维厄斯幅(LQ-21)地形地貌图(LOLA数据叠加山体阴影)

Fig.2 Topographic map of the Petavius quadrangle (LQ-21) (a shaded relief map with LOLA topographical data overlay)

图3 月球地质要素分类体系及图式图例

Fig.3 Classification system of lunar geological elements and map legends

图4 佩塔维厄斯幅(LQ-21)岩石分布概略图图例详见图3。

Fig.4 Distribution map of rock formations within LQ-21

表1 月球地质年代划分表(据文献[11,12]修改)

Table 1 Geological time scale of the Moon. Modified after [11-12].

地层年代	地质年代单元		年龄/Ga
新月宙(Neolunarisian, NL)	哥白尼纪(Copernican, C)		0.8~0.0
新月宙(Neolunarisian, NL)	爱拉托逊纪(Eratothenian, E)		3.16~0.8
古月宙(Paleolunarisian, PL)	雨海纪(Imbrian, I)	晚雨海世	3.8~3.16
	雨海纪(Imbrian, I)	早雨海世	3.85~3.8
	酒海纪(Nectarian, N)		3.92~3.85
	艾肯纪(Aitkenian, A)		4.2~3.92
冥月宙(Eolunarisian, EL)	前艾肯纪(pre-Aitkenian, pA)		4.52~4.2

图5 佩塔维厄斯幅(LQ-21)撞击盆地分布概略图图例详见图3。

Fig.5 Distribution map of impact basins within LQ-21

表2 佩塔维厄斯幅(LQ-21)地质图主要撞击盆地数据(据文献[18,32-33,35,45,50]修改)

Table 2 Basic information on impact basins within the Petavius quadrangle (LQ-21). Modified after [18,32-33,35,45,50].

盆地名称	直径/km	盆地模式年龄/Ga	样品年龄/Ga	岩浆活动年龄/Ga	盆地序列^[18]	地质年代单元
丰富海	690	4.30		3.69~3.36	7	艾肯纪
巴尔末-卡普坦	500				10	艾肯纪
史密斯海	740	4.26		3.48~3.14	21	艾肯纪
酒海	860	4.17	3.85±0.01 3.92±0.03 4.22±0.01		53	酒海纪
危海	740	4.07	3.93~3.89	3.2~2.5	55	酒海纪
洪堡	199			3.50	74	晚雨海世

图6 史密斯海盆地建造解译 a—LRO WAC影像图;b—LOLA DEM数据,单位为m;c—史密斯海盆地物质划分图(叠加山体阴影);d—峰环盆地物质类型划分(艾肯纪);e—地质剖面示意图(剖面线由图b中切线AB生成)。图例详见图3。

Fig.6 Interpretation of Smythii basin maping results

图7 洪堡盆地物质解译 a—LRO WAC影像图;b—CE1 CCD影像图;c—坡度图(LOLA DEM数据制作,z因子为3.30E-5); d—LOLA DEM数据;e—OMAT数据;f—朗伦努斯撞击坑物质划分图(叠加山体阴影)。图例详见图3。

Fig.7 Interpretation of Humboldt basin mapping results

图8 佩塔维厄斯幅内撞击坑分布概略图

Fig.8 Distribution map of craters within LQ-21

图9 佩塔维厄斯撞击坑坑物质解译 a—LRO WAC影像图;b—CE1 CCD影像图;c—坡度图(LOLA DEM数据制作,z因子为3.30E-5); d—LOLA DEM数据,单位为m;e—撞击坑物质类型划分图(早雨海世);f—佩塔维厄斯撞击坑物质划分图(叠加山体阴影);g—地质剖面示意图(剖面线由图d中切线CD生成)。图例详见图3。

Fig.9 Interpretation of Petavius crater mapping results

图10 朗伦努斯撞击坑坑物质解译 a—LRO WAC影像图;b—CE1 CCD影像图;c—坡度图(LOLA DEM数据制作,z因子为3.30E-5); d—LOLA DEM数据,单位为m;e—OMAT数据;f—朗伦努斯撞击坑物质划分图(叠加山体阴影)。图例详见图3。

Fig.10 The interpretation of Crater Langrenus Materials

图11 佩塔维厄斯幅(LQ-21)月球地质图图例详见图3。

Fig.11 The geological map of Petavius quadrangle (LQ-21) of the Moon

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月球佩塔维厄斯幅(LQ-21)数字地质填图与区域地质演化特征

Compilation of the geological map of the Petavius quadrangle of the Moon (LQ-21) and study on the regional geological evolution

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