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Amphitheater-headed canyons formed by megaflooding at Malad Gorge, Idaho

机译:在爱达荷州的马拉德峡谷(Malad Gorge)进行的特大洪水形成的圆形露天剧场峡谷

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摘要

Many bedrock canyons on Earth and Mars were eroded by upstream propagating headwalls, and a prominent goal in geomorphology and planetary science is to determine formation processes from canyon morphology. A diagnostic link between process and form remains highly controversial, however, and field investigations that isolate controls on canyon morphology are needed. Here we investigate the origin of Malad Gorge, Idaho, a canyon system cut into basalt with three remarkably distinct heads: two with amphitheater headwalls and the third housing the active Wood River and ending in a 7% grade knickzone. Scoured rims of the headwalls, relict plunge pools, sediment-transport constraints, and cosmogenic (^3He) exposure ages indicate formation of the amphitheater-headed canyons by large-scale flooding ∼46 ka, coeval with formation of Box Canyon 18 km to the south as well as the eruption of McKinney Butte Basalt, suggesting widespread canyon formation following lava-flow diversion of the paleo-Wood River. Exposure ages within the knickzone-headed canyon indicate progressive upstream younging of strath terraces and a knickzone propagation rate of 2.5 cm/y over at least the past 33 ka. Results point to a potential diagnostic link between vertical amphitheater headwalls in basalt and rapid erosion during megaflooding due to the onset of block toppling, rather than previous interpretations of seepage erosion, with implications for quantifying the early hydrosphere of Mars.
机译:地球和火星上的许多基岩峡谷都被上游传播的顶壁侵蚀,地貌学和行星科学的一个重要目标是根据峡谷的形态确定形成过程。然而,过程与形式之间的诊断联系仍然存在很大争议,因此需要对峡谷形态进行控制隔离的野外调查。在这里,我们研究了爱达荷州Malad Gorge的起源,该峡谷系统被切割成具有三个截然不同的头部的玄武岩:两个具有圆形露天剧场的顶壁,而第三个则容纳了活跃的伍德河,并以7%等级的尼克斯区结束。顶壁的冲刷边缘,残渣冲刷池,泥沙输送约束和成矿作用(^ 3He)暴露年龄表明,大洪水〜46 ka形成了圆形露天剧场为首的峡谷,与距峡谷18公里的Box Canyon形成同期南部以及麦金尼比尤特玄武岩的喷发,表明古伍德河的熔岩流改道后形成了广泛的峡谷形成。在以尼克斯为首的峡谷内的暴露年龄表明,阶地阶地的上游逐渐年轻化,并且至少在过去的33 ka内,尼克斯的传播速率为2.5 cm / y。结果表明,玄武岩中的垂直圆形剧场端壁与大洪水期间的快速侵蚀之间存在潜在的诊断联系,这是由于块体倾覆的发生,而不是先前对渗漏侵蚀的解释,这对量化火星的早期水圈意义重大。

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