GSTDTAP  > 气候变化
DOI10.1029/2018GL078150
Magma Ascent and Eruption Triggered by Cratering on the Moon
Michaut, Chloe1; Pinel, Virginie2
2018-07-16
发表期刊GEOPHYSICAL RESEARCH LETTERS
ISSN0094-8276
EISSN1944-8007
出版年2018
卷号45期号:13页码:6408-6416
文章类型Article
语种英语
国家France
英文摘要

On the Moon, the low-density crust exerts a strong filter to magma ascent. Many lunar craters are filled with mare, and evidence of pyroclastic activity and shallow magmatism is often located within craters called floor-fractured craters (FFCs). Interpreting quantitative observations on mare-filled craters and FFCs based on mechanical models, we show that a surface unloading caused by an impact crater provides a driving overpressure to the magma stalling at depth. This overpressure counterbalances the melt negative buoyancy, favoring its ascent through the crust. Providing a large unloading and a thin crust, magma can ascend up to the crater floor. FFC characteristics are consistent with a magma denser than the crust by 200-300 kg/m(3) and an elastic lithosphere thickness larger than 70 km. Our study suggests that small impact cratering likely induced magmatism and thereby crustal evolution in the early times of terrestrial planets.


Plain Language Summary On the terrestrial planets showing particularly old surfaces, such as on the Moon, volcanic deposits and evidence of magma intrusions are often found on the floors of relatively small impact craters, too small for the melt to have formed because of the impact itself. Why then is the process of magma ascent and eruption linked to that of cratering? Here we show that the unloading associated to an impact crater decompresses the elastic medium situated beneath. If magma is stalling at depth, it becomes pressurized relatively to its encasing rocks, which allows for its ascent in the crust. Magma might erupt at the surface if the unloading is sufficiently large and the crust relatively thin. Our model well explains observations on evidence of magma eruption versus intrusion at different craters varying by their sizes and by the crustal thickness at their locations on the Moon. We suggest that, in the early times of planets where magmatism and cratering were dominant, magma ascent caused by crater unloading might have modified the initial crustal composition and structure.


英文关键词magma intrusion Moon impact craters floor-fractured crater mare-filled crater magma ascent
领域气候变化
收录类别SCI-E
WOS记录号WOS:000439784300010
WOS关键词FLOOR-FRACTURED CRATERS ; EXPLOSIVE VOLCANISM ; LUNAR CRATERS ; CRUST ; MERCURY ; BASINS ; GENERATION ; INTRUSION ; INSIGHTS ; GRAIL
WOS类目Geosciences, Multidisciplinary
WOS研究方向Geology
引用统计
文献类型期刊论文
条目标识符http://119.78.100.173/C666/handle/2XK7JSWQ/26448
专题气候变化
作者单位1.Univ Lyon, CNRS, Ecole Normale Super Lyon, Labo Geol Lyon Terre,Planetes,Environm,UCBL, Lyon, France;
2.Univ Savoie Mt Blanc, Univ Grenoble Alpes, CNRS, IRD,IFSTTAR,ISTerre, Grenoble, France
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GB/T 7714
Michaut, Chloe,Pinel, Virginie. Magma Ascent and Eruption Triggered by Cratering on the Moon[J]. GEOPHYSICAL RESEARCH LETTERS,2018,45(13):6408-6416.
APA Michaut, Chloe,&Pinel, Virginie.(2018).Magma Ascent and Eruption Triggered by Cratering on the Moon.GEOPHYSICAL RESEARCH LETTERS,45(13),6408-6416.
MLA Michaut, Chloe,et al."Magma Ascent and Eruption Triggered by Cratering on the Moon".GEOPHYSICAL RESEARCH LETTERS 45.13(2018):6408-6416.
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