{"title":"Wavelet Multi-Scale Analysis of the Linear Gravity Anomalies of the Moon","authors":"Yan Wan, Bo Chen, Changyi Xu, Jinsong Du","doi":"10.1029/2024JE008427","DOIUrl":null,"url":null,"abstract":"<p>The history of the thermal and dynamic evolution of the Moon is partly recorded by lunar linear structures. Identification and analysis of subsurface linear structures and their associated gravity anomalies provide insights into the early evolution of the Moon. However, the current understanding of their deep extensions is limited. In this study, we employ gravity data and the 2D continuous wavelet transform technique to analyze the subsurface extension of linear structures. Four significant linear gravity anomalies (LGAs) are studied, including the north (FN) and south (FS) anomalies located in the lunar farside and the northwest (NNW) and northeast (NNE) anomalies in the nearside. Our results indicate that the top depths and widths of the mass sources associated with these linear structures can be determined. The intrusion depths of all four LGAs vary along their strike, with the shallowest intrusion depth reaching 8–10 km. For the FN anomaly, the top depths of the intrusive body range from 8 to 20 km, while intrusion widths vary between 30 and 50 km. Wavelet analysis for the FS anomaly indicates an intrusive source with a top width and depth of ∼30 and 10 km. For the NNW anomaly, the source body has top depths of 10–20 km with varying top widths at different sections (25∼50 km). As for the NNE structure, our results suggest substantial top widths between 75 and 150 km alongside relatively shallow top depths of 8–15 km. These LGAs are likely attributed to vertical magma intrusions connected at their bases to the crust-mantle interface.</p>","PeriodicalId":16101,"journal":{"name":"Journal of Geophysical Research: Planets","volume":"130 2","pages":""},"PeriodicalIF":3.9000,"publicationDate":"2025-02-20","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"Journal of Geophysical Research: Planets","FirstCategoryId":"89","ListUrlMain":"https://onlinelibrary.wiley.com/doi/10.1029/2024JE008427","RegionNum":1,"RegionCategory":"地球科学","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q1","JCRName":"GEOCHEMISTRY & GEOPHYSICS","Score":null,"Total":0}
引用次数: 0
Abstract
The history of the thermal and dynamic evolution of the Moon is partly recorded by lunar linear structures. Identification and analysis of subsurface linear structures and their associated gravity anomalies provide insights into the early evolution of the Moon. However, the current understanding of their deep extensions is limited. In this study, we employ gravity data and the 2D continuous wavelet transform technique to analyze the subsurface extension of linear structures. Four significant linear gravity anomalies (LGAs) are studied, including the north (FN) and south (FS) anomalies located in the lunar farside and the northwest (NNW) and northeast (NNE) anomalies in the nearside. Our results indicate that the top depths and widths of the mass sources associated with these linear structures can be determined. The intrusion depths of all four LGAs vary along their strike, with the shallowest intrusion depth reaching 8–10 km. For the FN anomaly, the top depths of the intrusive body range from 8 to 20 km, while intrusion widths vary between 30 and 50 km. Wavelet analysis for the FS anomaly indicates an intrusive source with a top width and depth of ∼30 and 10 km. For the NNW anomaly, the source body has top depths of 10–20 km with varying top widths at different sections (25∼50 km). As for the NNE structure, our results suggest substantial top widths between 75 and 150 km alongside relatively shallow top depths of 8–15 km. These LGAs are likely attributed to vertical magma intrusions connected at their bases to the crust-mantle interface.
期刊介绍:
The Journal of Geophysical Research Planets is dedicated to the publication of new and original research in the broad field of planetary science. Manuscripts concerning planetary geology, geophysics, geochemistry, atmospheres, and dynamics are appropriate for the journal when they increase knowledge about the processes that affect Solar System objects. Manuscripts concerning other planetary systems, exoplanets or Earth are welcome when presented in a comparative planetology perspective. Studies in the field of astrobiology will be considered when they have immediate consequences for the interpretation of planetary data. JGR: Planets does not publish manuscripts that deal with future missions and instrumentation, nor those that are primarily of an engineering interest. Instrument, calibration or data processing papers may be appropriate for the journal, but only when accompanied by scientific analysis and interpretation that increases understanding of the studied object. A manuscript that describes a new method or technique would be acceptable for JGR: Planets if it contained new and relevant scientific results obtained using the method. Review articles are generally not appropriate for JGR: Planets, but they may be considered if they form an integral part of a special issue.