The Bosumtwi meteorite impact structure, Ghana: A magnetic model

被引:50
作者
Plado, J
Pesonen, LJ
Koeberl, C
Elo, S
机构
[1] Univ Tartu, Inst Geol, EE-51014 Tartu, Estonia
[2] Univ Helsinki, Dept Geophys, FIN-00014 Helsinki, Finland
[3] Geol Survey Finland, FIN-02151 Espoo, Finland
[4] Univ Vienna, Inst Geochem, A-1090 Vienna, Austria
来源
METEORITICS & PLANETARY SCIENCE | 2000年 / 35卷 / 04期
关键词
D O I
10.1111/j.1945-5100.2000.tb01456.x
中图分类号
P3 [地球物理学]; P59 [地球化学];
学科分类号
0708 ; 070902 ;
摘要
A magnetic model is proposed for the Bosumtwi meteorite impact structure in Ghana, Africa. This relatively young (similar to 1.07 Ma) structure with a diameter of similar to 10.5 km is exposed within early Proterozoic Birimian-Tarkwaian rocks. The central part of the structure is buried under postimpact lake sediments, and because of lack of drill cores, geophysics is the only way to reveal its internal structure. To study the structure below and beyond the lake, a high-resolution, low altitude (similar to 70 m) airborne geophysical survey across the structure was conducted, which included measurements of the total magnetic field, electromagnetic data, and gamma radiation. The magnetic data show a circumferential magnetic halo outside the lakeshore, similar to 12 km in diameter. The central-north part of the lake reveals a central negative magnetic anomaly with smaller positive side-anomalies north and south of it, which is typical for magnetized bodies at shallow latitudes. A few weaker negative magnetic anomalies exist in the eastern and western part of the lake. Together with the northern one, they seem to encircle a central uplift. Our model shows that the magnetic anomaly of the structure is presumably produced by one or several relatively strongly remanently magnetized impact-melt rock or melt-rich suevite bodies. Petrophysical measurements show a clear difference between the physical properties of preimpact target rocks and impactites. Suevites have a higher magnetization and have low densities and high porosities compared to the target rocks. In suevites, the remanent magnetization dominates over induced magnetization (Koenigsberger ratio > 3). Preliminary palaeomagnetic results reveal that the normally magnetized remanence component in suevites was acquired during the Jaramillo normal polarity epoch. This interpretation is consistent with the modelling results that also require a normal polarity magnetization for the magnetic body beneath the lake. The reverse polarity remanence component, superimposed on the normal component, is probably acquired during subsequent reverse polarity events.
引用
收藏
页码:723 / 732
页数:10
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