2019
DOI: 10.1016/j.geomorph.2019.03.019
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Rock glaciers in Pearse Valley, Antarctica record outlet and alpine glacier advance from MIS 5 through the Holocene

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Cited by 6 publications
(17 citation statements)
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“…Based on the GPR data and field investigations, the South Fork rock glacier contains ice-rich sediments (30–50% porosity if ice-filled, with isolated centimetre-scale ice lenses). This talus-derived model of formation distinguishes the rock glacier of South Fork from many of the other rock glaciers and viscous flow lobes in Taylor Valley, which have been shown to contain > 10 m-thick lenses of clean ice of glacial origin overlain by talus and fluvial sediments (Swanger et al 2010, 2019). The demonstrated variation in the ice content and origin for viscous flow features in the McMurdo Dry Valleys provides a compelling analogue for the large viscous flow features on Mars, especially given recent insights into the possibility that some Martian features contain clean ice lenses at depth while others might not (Petersen et al 2018, Brough et al 2019).…”
Section: Discussionmentioning
confidence: 96%
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“…Based on the GPR data and field investigations, the South Fork rock glacier contains ice-rich sediments (30–50% porosity if ice-filled, with isolated centimetre-scale ice lenses). This talus-derived model of formation distinguishes the rock glacier of South Fork from many of the other rock glaciers and viscous flow lobes in Taylor Valley, which have been shown to contain > 10 m-thick lenses of clean ice of glacial origin overlain by talus and fluvial sediments (Swanger et al 2010, 2019). The demonstrated variation in the ice content and origin for viscous flow features in the McMurdo Dry Valleys provides a compelling analogue for the large viscous flow features on Mars, especially given recent insights into the possibility that some Martian features contain clean ice lenses at depth while others might not (Petersen et al 2018, Brough et al 2019).…”
Section: Discussionmentioning
confidence: 96%
“…Rock glaciers are numerous in this cold, hyper-arid region (Hassinger & Mayewski 1983, Bockheim 2014). Despite regional snowfall precipitation of ~10–100 mm water equivalent per year (Fountain et al 2010), rock glaciers and debris-covered ice are able to form and survive, possibly for timescales of 10 5 –10 6 years (Mackay et al 2014, Swanger et al 2019). The mechanism of rock glacier formation probably varies within the McMurdo Dry Valleys (Bockheim 2014).…”
Section: Introductionmentioning
confidence: 99%
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“…Besides the burial of glacier ice (e.g. Lacelle et al, 2011, Marchant et al, 2002, Swanger et al, 2010, Swanger, 2017, Swanger et al, 2019, different hypotheses have been advanced to explain the emplacement of ground ice in the permafrost of the upper MDV. For example, in places where ground temperatures remain < 0°C, ground ice was likely emplaced by vapour-diffusion, whereas in places where ground surface temperatures rise > 0°C, it was likely emplaced by vapour-diffusion as well as by the freezing of evaporated snowmelt (e.g.…”
Section: Cryostratigraphy Of Mid-miocene Permafrost At Friis Hills Upper Mcmurdo Dry Valleys Of Antarcticamentioning
confidence: 99%