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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 The rapidly retreating Thwaites and Pine Island glaciers together dominate present-day ice loss from the West Antarctic Ice Sheet and are implicated in runaway deglaciation scenarios. Knowledge of whether these glaciers were substantially smaller in the mid-Holocene and subsequently recovered to their present extents is important for assessing whether current ice recession is irreversible. Here we reconstruct relative sea-level change from radiocarbon-dated raised beaches at sites immediately seawards of these glaciers, allowing us to examine the response of the earth to loading and unloading of ice in the Amundsen Sea region. We find that relative sea level fell steadily over the past 5.5 kyr without rate changes that would characterize large-scale ice re-expansion. Moreover, current bedrock uplift rates are an order of magnitude greater than the rate of long-term relative sea-level fall, suggesting a change in regional crustal unloading and implying that the present deglaciation may be unprecedented in the past ~5.5 kyr. While we cannot preclude minor grounding-line fluctuations, our data are explained most easily by early Holocene deglaciation followed by relatively stable ice positions until recent times and imply that Thwaites and Pine Island glaciers have not been substantially smaller than present during the past 5.5 kyr. 

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. 

Abstract. Widespread existing geological records from above the modern ice sheet surface and outboard of the current ice margin show that the Antarctic IceSheet (AIS) was much more extensive at the Last Glacial Maximum (∼ 20 ka) than at present. However, whether it was ever smaller thanpresent during the last few millennia, and (if so) by how much, is known only for a few locations because direct evidence lies within or beneath theice sheet, which is challenging to access. Here, we describe how retreat and readvance (henceforth “readvance”) of AIS grounding lines during theHolocene could be detected and quantified using subglacial bedrock, subglacial sediments, marine sediment cores, relative sea-level (RSL) records,geodetic observations, radar data, and ice cores. Of these, only subglacial bedrock and subglacial sediments can provide direct evidence forreadvance. Marine archives are of limited utility because readvance commonly covers evidence of earlier retreat. Nevertheless, stratigraphictransitions documenting change in environment may provide support for direct evidence from subglacial records, as can the presence of transgressionsin RSL records, and isostatic subsidence. With independent age control, ice structure revealed by radar can be used to infer past changes in iceflow and geometry, and therefore potential readvance. Since ice cores capture changes in surface mass balance, elevation, and atmosphericand oceanic circulation that are known to drive grounding line migration, they also have potential for identifying readvance. A multidisciplinaryapproach is likely to provide the strongest evidence for or against a smaller-than-present AIS in the Holocene.