Thermal studies on the lower Carboniferous basins of Khenifra and Qasbat-Tadla, Morocco: What do they teach us about the pre-Variscan stages in NW Africa?

IF 2.2 4区 地球科学 Q2 GEOSCIENCES, MULTIDISCIPLINARY Journal of African Earth Sciences Pub Date : 2024-09-01 DOI:10.1016/j.jafrearsci.2024.105406
R. Leprêtre , M. El Houicha , A. Schito , R. Ouchaou , F. Chopin , P. Cózar
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Abstract

Within the Variscan Belt of Morocco, the Central Massif preserves Early Carboniferous rift basins. The Lower Carboniferous Khenifra and Qasbat-Tadla basins are aborted rifts, developed just before the Variscan orogenesis in Morocco that occurred during the Pennsylvanian-Cisuralian in NW Africa. Due to both weak inversion of these basins during the Variscan orogeny and limited burial afterwards, these basins offer the opportunity to study the Early Carboniferous pre-orogenic thermal regimes. In the Khenifra basin, 77 samples collected across the basin and its basement's boundaries, allowed the determination of the maximal temperature reached during the rocks burial by means of Raman spectroscopic analyses. The Ordovician basement shows mean temperatures between 230 and 300 °C whereas the upper Visean/Serpukhovian infill has a wide range, from temperatures <160 °C to 250–260 °C. This thermal variation within the basinal series has been evidenced from west to east and cannot have been acquired during the Variscan events. The acquisition of these maximal temperatures occurred between Late Devonian to Upper Visean/Serpukhovian and is thought to result from the formation of an extended rift. In the Qasbat-Tadla basin, Rock-Eval data from Ordovician to Devonian source-rocks indicate significantly lower maximal temperatures reached by pre-Carboniferous samples that are within the oil window. Our results are in favor of a heterodox model for the Variscan belt in Morocco and NW African in general, suggesting that no pre-Variscan compressional events are needed. Instead, the development of the intraplate Variscan belt in NW Africa was permitted through the development of hot and weak Lower Carboniferous basins, subsequently inverted in a far-field stress field. The striking thermal differences between the Khenifra and Qasbat-Tadla basins suggest that important tectonic segmentation must have shaped the area during the Early Carboniferous extensional phase.

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对摩洛哥 Khenifra 和 Qasbat-Tadla 下石炭纪盆地的热研究:它们对西北非洲的前瓦利斯坎阶段有何启示?
在摩洛哥的瓦利斯坎带,中央丘保留了早石炭世裂谷盆地。下石炭统 Khenifra 和 Qasbat-Tadla 盆地是中止的裂谷,是在西北非宾夕法尼亚-志留纪期间发生的摩洛哥瓦里斯坎造山运动之前形成的。由于这些盆地在瓦里肯造山运动期间的反转作用较弱,而造山运动之后的埋藏作用有限,因此这些盆地为研究早石炭世前造山运动的热机制提供了机会。在 Khenifra 盆地,通过对盆地及其基底边界采集的 77 个样本进行拉曼光谱分析,确定了岩石埋藏期间达到的最高温度。奥陶纪基底的平均温度在 230 ° C 到 300 ° C 之间,而上维谢安/塞普霍夫页岩的填充温度范围很广,从 160 ° C 到 250-260 ° C 不等。基底系列内的这种热量变化是自西向东的,不可能是在瓦利斯坎时期获得的。这些最高温度的获得发生在晚泥盆世至上维西期/上塞普霍夫期,被认为是延伸裂谷形成的结果。在卡斯巴特-塔德拉盆地,来自奥陶纪至泥盆纪源岩的岩石-评价数据表明,石炭纪以前的样本所达到的最高温度要低得多,而这些样本都在石油窗口之内。我们的研究结果表明,摩洛哥和整个西北非洲的瓦利斯坎带采用的是一种非正统模型,即不需要发生瓦利斯坎前的压缩事件。相反,西北非洲板内瓦里斯坎带的发展是通过下石炭纪热而弱的盆地的发展实现的,这些盆地随后在远场应力场中发生了倒转。Khenifra盆地和Qasbat-Tadla盆地之间显著的热差异表明,在早石炭世的伸展阶段,该地区一定发生了重要的构造分段。
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来源期刊
Journal of African Earth Sciences
Journal of African Earth Sciences 地学-地球科学综合
CiteScore
4.70
自引率
4.30%
发文量
240
审稿时长
12 months
期刊介绍: The Journal of African Earth Sciences sees itself as the prime geological journal for all aspects of the Earth Sciences about the African plate. Papers dealing with peripheral areas are welcome if they demonstrate a tight link with Africa. The Journal publishes high quality, peer-reviewed scientific papers. It is devoted primarily to research papers but short communications relating to new developments of broad interest, reviews and book reviews will also be considered. Papers must have international appeal and should present work of more regional than local significance and dealing with well identified and justified scientific questions. Specialised technical papers, analytical or exploration reports must be avoided. Papers on applied geology should preferably be linked to such core disciplines and must be addressed to a more general geoscientific audience.
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