Antarctic permafrost processes and antiphase dynamics of cold-based glaciers in the McMurdo Dry Valleys inferred from 10Be and 26Al cosmogenic nuclides

Jacob T. H. Anderson, T. Fujioka, David Fink, A. Hidy, Gary S. Wilson, K. Wilcken, Andrey Abramov, Nikita Demidov
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Abstract

Abstract. Soil and sediment mixing and associated permafrost processes are not widely studied or understood in the McMurdo Dry Valleys of Antarctica. In this study, we investigate the stability and depositional history of near-surface permafrost sediments to ∼ 3 m depth in the Pearse and lower Wright valleys using measured cosmogenic 10Be and 26Al depth profiles. In Pearse Valley, we estimate a minimum depositional age of ∼ 74 ka for the active layer and paleoactive-layer sediments (< 0.65 m). Combined depth profile modelling of 10Be and 26Al gives a depositional age for near-surface (< 1.65 m) permafrost in Pearse Valley of 180 +20/-40 ka, implying that the deposition of permafrost sediments predates MIS 5 advances of Taylor Glacier. Deeper permafrost sediments (> 2.09 m) in Pearse Valley are thus inferred to have a depositional age of > 180 ka. At a coastal, lower-elevation site in neighbouring lower Wright Valley, 10Be and 26Al depth profiles from a second permafrost core exhibit near-constant concentrations with depth and indicate the sediments are either vertically mixed after deposition or sufficiently young so that post-depositional nuclide production is negligible relative to inheritance. 26Al/10Be concentration ratios for both depth profiles range between 4.0 and 5.2 and are all lower than the nominal surface production rate ratio of 6.75, indicating that prior to deposition, these sediments experienced complex, yet similar, exposure–burial histories. Assuming a single-cycle exposure–burial scenario, the observed 26Al/10Be ratios are equivalent to a total minimum exposure–burial history of ∼ 1.2 Myr. In proximity to the depth profile core site, we measured cosmogenic 10Be and 26Al in three granite cobbles from thin, patchy drift (Taylor 2 Drift) in Pearse Valley to constrain the timing of retreat of Taylor Glacier. Assuming simple continuous exposure, our minimum, zero-erosion exposure ages suggest Taylor Glacier partially retreated from Pearse Valley no later than 65–74 ka. The timing of retreat after 65 ka and until the Last Glacial Maximum (LGM) when Taylor Glacier was at a minimum position remains unresolved. The surface cobble ages and permafrost processes reveal Taylor Glacier advances during MIS 5 were non-erosive or mildly erosive, preserving the underlying permafrost sediments and peppering boulders and cobbles upon an older, relict surface. Our results are consistent with U/Th ages from central Taylor Valley and suggest changes in moisture delivery over Taylor Dome during MIS 5e, 5c, and 5a appear to be associated with the extent of the Ross Ice Shelf and sea ice in the Ross Sea. These data provide further evidence of antiphase behaviour through retreat of a peripheral lobe of Taylor Glacier in Pearse Valley, a region that was glaciated during MIS 5. We suggest a causal relationship of cold-based glacier advance and retreat that is controlled by an increase in moisture availability during retreat of sea ice and perhaps the Ross Ice Shelf, as well as, conversely, a decrease during times of sea ice and Ross Ice Shelf expansion in the Ross Sea.
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从 10Be 和 26Al 宇宙成因核素推断南极永久冻土过程和麦克默多干谷冷基冰川的反相动力学
摘要在南极洲的麦克默多干谷,土壤和沉积物的混合以及相关的永久冻土过程还没有得到广泛的研究和了解。在这项研究中,我们利用测量到的宇宙成因 10Be 和 26Al 深度剖面图,研究了皮尔斯谷和赖特谷下部深度为 3 米的近地表永久冻土沉积物的稳定性和沉积历史。在皮尔斯谷,我们估计活动层的最小沉积年龄为 74 ka,因此推断皮尔斯谷的古活动层沉积物(2.09 米)的沉积年龄大于 180 ka。在邻近下莱特河谷的一个海拔较低的沿海地点,第二个永久冻土岩芯的 10Be 和 26Al 深度剖面显示出随深度变化的近乎恒定的浓度,表明沉积物要么是沉积后垂直混合的,要么是足够年轻的,因此沉积后的核素生成相对于继承来说可以忽略不计。两个深度剖面的 26Al/10Be 浓度比介于 4.0 和 5.2 之间,均低于 6.75 的名义地表生产率比,表明这些沉积物在沉积之前经历了复杂但相似的暴露-埋藏历史。假设是单循环暴露-埋藏,观测到的 26Al/10Be 比率相当于总的最低暴露-埋藏历史为 1.2 Myr。在深度剖面岩心点附近,我们测量了皮尔斯谷薄层、成片漂移(泰勒2漂移)的三块花岗岩鹅卵石中的宇宙成因10Be和26Al,以确定泰勒冰川退缩的时间。假设只是简单的连续出露,我们的最小零侵蚀出露年龄表明泰勒冰川从皮尔斯谷部分后退的时间不会晚于 65-74 ka。65 ka之后直至末次冰川极盛时期(LGM)泰勒冰川处于最小位置时的退缩时间仍未确定。地表鹅卵石的年龄和永久冻土过程显示,泰勒冰川在MIS 5期间的推进是非侵蚀性或轻度侵蚀性的,保留了下层的永久冻土沉积物,并在较古老的遗迹表面撒上了巨石和鹅卵石。我们的研究结果与泰勒谷中部的U/Th年龄一致,表明在MIS 5e、5c和5a期间,泰勒穹顶的水分输送变化似乎与罗斯冰架和罗斯海海冰的范围有关。这些数据进一步证明了通过皮尔斯谷泰勒冰川外围叶片的后退而产生的反相行为,该地区在 MIS 5 期间曾有冰川形成。 我们提出了基于寒冷的冰川前进和后退的因果关系,这种因果关系是由海冰和罗斯冰架后退期间水分供应量的增加以及罗斯海海冰和罗斯冰架扩张期间水分供应量的减少所控制的。
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