Gravity and flexure models of the San Luis, Albuquerque, and Tularosa basins in the Rio Grande rift, New Mexico, and southern Colorado

C. Peterson, M. Roy
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引用次数: 11

Abstract

—The Rio Grande rift is a Cenozoic continental rift zone that trends south from central Colorado through New Mexico and merges with a broader extensional zone in west Texas and Chihuahua, Mexico. The net upper crustal extension increases southward along the rift, accompanied by a southward-widening of the rift from a narrow zone encompassing a single basin in the north to a wide zone of multiple, laterally adjacent basins to the south. In this study we model the isostatic responses of the lithosphere to extension along the Rio Grande rift, and compare and contrast this response in the San Luis and Albuquerque basins in the narrow part of rift and the Tularosa basin in the wider region of the rift. Our flexural isostatic models are based on a joint-inversion of gravity and deflection data along the footwalls of major basin-bounding faults. The main difficulty in constraining isostatic response to extension in the Rio Grande rift is a lack of constraints on footwall deflection. Our approach is to use topography as a proxy for flexural deflection, and then to compare the estimated end-loads required for plate flexure in the footwall with the end-loads estimated from hanging wall and basin geometry. Using this approach we determine the extent to which flexural isostasy could have generated elevated rift-flanks, and how this process might change along strike. Our results indicate that flexural responses to extension are consistent with rock and surface uplift in the footwalls of the Albuquerque and the Tularosa basins in the central and southern Rio Grande rift. In the San Luis basin, however, although a flexural curve may adequately fit footwall topography, the plate-end loads required for flexure are inconsistent with those inferred from the hanging wall and basin geometries. Additionally, flexure-based estimates of crustal extension agree with geologic estimates in the Albuquerque and Tularosa basins, but not in the San Luis basin. We infer therefore, that rift-flank uplift due to flexure is likely only in the central and southern parts of the Rio Grande rift; to the north, we infer an additional (perhaps pre-rift) contribution to rift-flank topography.
里奥格兰德裂谷、新墨西哥州和科罗拉多州南部的圣路易斯、阿尔伯克基和图拉罗萨盆地的重力和弯曲模型
里奥格兰德裂谷是一个新生代大陆裂谷带,从科罗拉多州中部向南穿过新墨西哥州,并与德克萨斯州西部和墨西哥奇瓦瓦州的一个更广泛的伸展带合并。上地壳净伸展沿裂谷向南增加,裂谷从北部一个包含单个盆地的狭窄地带向南扩大到南部一个包含多个横向相邻盆地的宽阔地带。在本研究中,我们模拟了沿里奥格兰德裂谷延伸的岩石圈均衡响应,并比较了裂谷狭窄部分的圣路易斯和阿尔伯克基盆地和裂谷较宽区域的图拉罗萨盆地的这种响应。我们的弯曲均衡模型是基于沿主要盆地边界断层下盘的重力和挠度数据的联合反演。制约里奥格兰德裂谷伸展的均衡响应的主要困难是缺乏对下盘挠度的制约。我们的方法是使用地形作为弯曲挠度的代表,然后将下盘弯曲所需的估计端载荷与从上盘和盆地几何形状估计的端载荷进行比较。利用这种方法,我们确定了弯曲均衡在多大程度上可以产生隆起的裂谷侧翼,以及这一过程如何沿着走向变化。研究结果表明,里奥格兰德裂谷中部和南部的Albuquerque盆地和Tularosa盆地下盘对伸展的弯曲响应与岩石和地表隆起一致。然而,在圣路易斯盆地,虽然弯曲曲线可以充分适应下盘地形,但弯曲所需的板端载荷与从上盘和盆地几何形状推断的不一致。此外,基于挠度的地壳伸展估计与Albuquerque和Tularosa盆地的地质估计一致,但在San Luis盆地则不一致。因此,我们推断,由挠曲引起的裂谷翼隆升可能只发生在里奥格兰德裂谷的中部和南部;在北部,我们推断了对裂谷翼地形的额外贡献(可能是裂谷前的)。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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