Search for: All records

During the last deglaciation, collapse of the saddle between the North American Cordilleran and Laurentide ice sheets led to rapid ice-sheet mass loss and separation, with meltwater discharge contributing to deglacial sea level rise. We directly date ice-sheet separation at the end of the saddle collapse using 64 10Be exposure ages along an ~1200-km transect of the ice-sheet suture zone. Collapse began in the south by 15.4 ± 0.4 ka and ended by 13.8 ± 0.1 ka at ~56◦N. Ice-sheet model simulations consistent with the 10Be ages find that the saddle collapse contributed 6.2–7.2 m to global mean sea-level rise from ~15.5 ka to ~14.0 ka, or approximately one third of global mean sea-level rise over this period. We determine 3.1–3.6 m of the saddle collapse meltwater was released during Meltwater Pulse 1A ~14.6-14.3 ka, constituting 20–40% of this meltwater pulse’s volume. Because the separation of the Cordilleran and Laurentide ice sheets occurred over 1–2 millennia, the associated release of meltwater during the saddle collapse supplied a smaller contribution to the magnitude of Meltwater Pulse 1A than has been recently proposed. 

Abstract Pine Island Glacier, West Antarctica, is the largest Antarctic contributor to global sea-level rise and is vulnerable to rapid retreat, yet our knowledge of its deglacial history since the Last Glacial Maximum is based largely on marine sediments that record a retreat history ending in the early Holocene. Using a suite of 10Be exposure ages from onshore glacial deposits directly adjacent to Pine Island Glacier, we show that this major glacier thinned rapidly in the early to mid-Holocene. Our results indicate that Pine Island Glacier was at least 690 m thicker than present prior to ca. 8 ka. We infer that the rapid thinning detected at the site farthest downstream records the arrival and stabilization of the retreating grounding line at that site by 8–6 ka. By combining our exposure ages and the marine record, we extend knowledge of Pine Island Glacier retreat both spatially and temporally: to 50 km from the modern grounding line and to the mid-Holocene, providing a data set that is important for future numerical ice-sheet model validation. 

Abstract Constraining past West Antarctic Ice Sheet (WAIS) change helps validate numerical models simulating future ice sheet dynamics. Following rapid deglaciation during the mid‐Holocene, ice near Thwaites Glacier was ∼35 m thinner than present; however, the timing of ice regrowth to its present configuration remains unknown. To fill this knowledge gap, we present cosmogenic nuclide exposure ages of cobbles from the surface of a moraine situated between Thwaites and Pope glaciers. We infer that the moraine formed and stabilized in the Late Holocene (∼1.4 ka) when a small glacier thickened. We also present a novel reconstruction of WAIS volume constrained by sea‐level data, which demonstrates that moraine formation coincided with a large‐scale WAIS readvance. Our new geologic constraints will help inform models of the solid Earth response to surface mass loading, improving our understanding of ice sheet dynamics in a vulnerable part of WAIS. 

Abstract. Cosmogenic-nuclide concentrations in subglacial bedrock cores show that the West Antarctic Ice Sheet (WAIS) at a site between Thwaites and Pope glaciers was at least 35 m thinner than present in the past several thousand years and then subsequently thickened. This is important because of concern that present thinning and grounding line retreat at these and nearby glaciers in the Amundsen Sea Embayment may irreversibly lead to deglaciation of significant portions of the WAIS, with decimeter- to meter-scale sea level rise within decades to centuries. A past episode of ice sheet thinning that took place in a similar, although not identical, climate was not irreversible. We propose that the past thinning–thickening cycle was due to a glacioisostatic rebound feedback, similar to that invoked as a possible stabilizing mechanism for current grounding line retreat, in which isostatic uplift caused by Early Holocene thinning led to relative sea level fall favoring grounding line advance. 

Abstract. Evidence for the timing and pace of past grounding lineretreat of the Thwaites Glacier system in the Amundsen Sea embayment (ASE)of Antarctica provides constraints for models that are used to predict thefuture trajectory of the West Antarctic Ice Sheet (WAIS). Existingcosmogenic nuclide surface exposure ages suggest that Pope Glacier, a formertributary of Thwaites Glacier, experienced rapid thinning in the early tomid-Holocene. There are relatively few exposure ages from the lower ice-freesections of Mt. Murphy (<300 m a.s.l.; metres above sea level) that are uncomplicated byeither nuclide inheritance or scatter due to localised topographiccomplexities; this makes the trajectory for the latter stages ofdeglaciation uncertain. This paper presents 12 new 10Be exposure agesfrom erratic cobbles collected from the western flank of Mt. Murphy, within160 m of the modern ice surface and 1 km from the present grounding line.The ages comprise two tightly clustered populations with mean deglaciationages of 7.1 ± 0.1 and 6.4 ± 0.1 ka (1 SE). Linear regressionanalysis applied to the age–elevation array of all available exposure agesfrom Mt. Murphy indicates that the median rate of thinning of Pope Glacierwas 0.27 m yr−1 between 8.1–6.3 ka, occurring 1.5 times faster thanpreviously thought. Furthermore, this analysis better constrains theuncertainty (95 % confidence interval) in the timing of deglaciation atthe base of the Mt. Murphy vertical profile (∼ 80 m above themodern ice surface), shifting it to earlier in the Holocene (from 5.2 ± 0.7 to 6.3 ± 0.4 ka). Taken together, the results presentedhere suggest that early- to mid-Holocene thinning of Pope Glacier occurredover a shorter interval than previously assumed and permit a longer durationover which subsequent late Holocene re-thickening could have occurred.