{"title":"加拿大马尼加根地区的综合遥感地貌调查:对行星撞击过程的启示","authors":"Mary-Anne Fobert, John G. Spray, Vernon Singhroy","doi":"10.1029/2025JE008982","DOIUrl":null,"url":null,"abstract":"<p>Remote sensing data were deployed to create a lineament map (LM) of central Quebec, Canada. The LM provides a first-order representation of the geological structures and is shown to co-align with 45% of the structural features previously mapped in the area. Areas displaying partial or no alignment are attributed to inconsistent structural surficial expressions, indistinguishable edge gradients, obscurity by water, and spatial offsets. Despite these challenges, the LM has extended published structural features and extracted a substantial number of new linear features. The LM allows for the distinction between pre-impact regional features from those generated by the Manicouagan impact event. Pre-impact fault systems facilitated a polygonal form to the structure, rendering Manicouagan a polygonal impact crater. Combined with field-based constraints, the LM results also reveal that the crater shows structural asymmetry, with more damage in the SW sector, expressed by enhanced concentric and radial faulting, and an elliptical collapsed transient cavity (orientated ∼70 km NE-SW and 85 km NW-SE). In addition, the central uplift is offset uprange from the geometric center to the NE and the central peak is breached, with a deeper footwall trench opening downrange to the SW. These observations indicate that Manicouagan may have been formed by a projectile traveling with a trajectory from the present-day NE at an oblique angle. The distinction of pre-impact target structures from impact-generated features on Earth has implications for better understanding these features on other solid planetary bodies, comparisons with which are made from craters on the Moon, Mars and Mercury.</p>","PeriodicalId":16101,"journal":{"name":"Journal of Geophysical Research: Planets","volume":"130 8","pages":""},"PeriodicalIF":4.0000,"publicationDate":"2025-08-08","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://agupubs.onlinelibrary.wiley.com/doi/epdf/10.1029/2025JE008982","citationCount":"0","resultStr":"{\"title\":\"An Integrated Remote Sensing Lineament Investigation of the Manicouagan Region, Canada: Implications for Planetary Cratering Processes\",\"authors\":\"Mary-Anne Fobert, John G. 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引用次数: 0
摘要
利用遥感数据绘制了加拿大魁北克省中部的线形图。LM提供了地质构造的一阶表示,并显示与该地区先前绘制的45%的构造特征共对齐。显示部分或没有对准的区域归因于不一致的结构表面表达式、无法区分的边缘梯度、水的模糊和空间偏移。尽管存在这些挑战,LM仍然扩展了已发布的结构特征,并提取了大量新的线性特征。LM允许区分撞击前的区域特征和摩尼瓦根撞击事件产生的区域特征。撞击前的断层系统促进了构造的多边形形式,使摩尼瓦根成为一个多边形撞击坑。结合基于现场的约束条件,LM结果还显示陨石坑具有结构不对称性,在西南部分受到更多破坏,表现为增强的同心和径向断裂,以及椭圆形塌陷的瞬态空洞(方向约70 km NE-SW和85 km NW-SE)。此外,中央隆起从几何中心向北东偏移,中央峰断裂,下盘沟槽向南向南打开。这些观察结果表明,摩尼瓦根可能是由一颗抛射物形成的,抛射物沿着现在东北方向的轨道以斜角飞行。撞击前目标结构与地球上撞击产生的特征之间的区别,有助于更好地理解其他固体行星体上的这些特征,并与月球、火星和水星上的陨石坑进行比较。
An Integrated Remote Sensing Lineament Investigation of the Manicouagan Region, Canada: Implications for Planetary Cratering Processes
Remote sensing data were deployed to create a lineament map (LM) of central Quebec, Canada. The LM provides a first-order representation of the geological structures and is shown to co-align with 45% of the structural features previously mapped in the area. Areas displaying partial or no alignment are attributed to inconsistent structural surficial expressions, indistinguishable edge gradients, obscurity by water, and spatial offsets. Despite these challenges, the LM has extended published structural features and extracted a substantial number of new linear features. The LM allows for the distinction between pre-impact regional features from those generated by the Manicouagan impact event. Pre-impact fault systems facilitated a polygonal form to the structure, rendering Manicouagan a polygonal impact crater. Combined with field-based constraints, the LM results also reveal that the crater shows structural asymmetry, with more damage in the SW sector, expressed by enhanced concentric and radial faulting, and an elliptical collapsed transient cavity (orientated ∼70 km NE-SW and 85 km NW-SE). In addition, the central uplift is offset uprange from the geometric center to the NE and the central peak is breached, with a deeper footwall trench opening downrange to the SW. These observations indicate that Manicouagan may have been formed by a projectile traveling with a trajectory from the present-day NE at an oblique angle. The distinction of pre-impact target structures from impact-generated features on Earth has implications for better understanding these features on other solid planetary bodies, comparisons with which are made from craters on the Moon, Mars and Mercury.
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.