DOI: 10.1029/2017JE005463
Scopus记录号: 2-s2.0-85049825700
论文题名: Formation of Simple Impact Craters in Layered Targets: Implications for Lunar Crater Morphology and Regolith Thickness
作者: Prieur N.C. ; Rolf T. ; Wünnemann K. ; Werner S.C.
刊名: Journal of Geophysical Research: Planets
ISSN: 21699097
出版年: 2018
卷: 123, 期: 6 起始页码: 1555
结束页码: 1578
语种: 英语
英文关键词: crater morphology
; impact crater modeling
; layering
; Moon
; regolith thickness
; simple impact craters
Scopus关键词: crater
; Moon
; numerical model
; regolith
英文摘要: Impact crater morphologies vary significantly across the lunar maria. Craters with diameter less than 400 m are closely related to variations in target properties (rock strength, porosity, and layering) as well as the impact velocity. Here we investigate target and impact conditions feasible for reproducing crater morphologies, such as normal, central-mound, flat-bottomed, and concentric craters, using numerical models of impact crater formation in two-layer targets under lunar conditions (i.e., average-impact velocity and gravity). Based on more than 1,000 numerical models, we observe that concentric craters can form with a strength contrast as low as factor of 2 between the layers as long as the difference in cohesion is larger than a value between 50 and 450 kPa (for an impact velocity of 12.7 km/s). Because of this small contrast, concentric craters do not serve as a good indication for the lunar regolith-mare interface. Crater morphology changes with crater diameter according to three different scenarios depending on layers' strengths and the impact velocity. For high-impact velocity or/and moderate material strength, normal crater morphology transitions directly to concentric morphology, while with large material strengths and/or low-impact velocity, craters change with size from normal to flat-bottomed and then to concentric morphology; only this latter pathway is consistent with previous laboratory results. Lunar regolith thicknesses estimated from crater morphologies can differ by up to 80% from previously inferred thicknesses. The transition from normal to flat-bottomed craters is found to be the most robust transition to infer the thickness of the surficial target layer. ©2018. American Geophysical Union. All Rights Reserved. Citation statistics:
资源类型: 期刊论文
标识符: http://119.78.100.158/handle/2HF3EXSE/113823
Appears in Collections: 气候减缓与适应
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作者单位: Centre for Earth Evolution and Dynamics, University of Oslo, Oslo, Norway; Museum für Naturkunde, Leibniz-Institute for Evolution and Biodiversity Science, Berlin, Germany; Institute of Geological Sciences, Planetary Sciences and Remote Sensing, Freie Universität Berlin, Berlin, Germany
Recommended Citation:
Prieur N.C.,Rolf T.,Wünnemann K.,et al. Formation of Simple Impact Craters in Layered Targets: Implications for Lunar Crater Morphology and Regolith Thickness[J]. Journal of Geophysical Research: Planets,2018-01-01,123(6)