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The Cryosphere· 2026Q1

Rate-induced tipping of ice sheets due to visco-elastic Earth response under idealized conditions

Johannes Feldmann, Ann Kristin Klose, Torsten Albrecht, Ricarda Winkelmann

Short summary

Ice sheet tipping points are reached up to 80% faster (rate-induced tipping) than predicted by static models when considering the Earth's visco-elastic response to melting, especially for weaker Earth structures.

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Key points

  • The Earth's visco-elastic response can cause rate-induced tipping (R-tipping) in ice sheets, triggering instability faster than static models predict.
  • For weaker Earth structures (West-Antarctic type), the R-tipping threshold is more than an order of magnitude lower than for a fixed bed.
  • Bed uplift is insufficient to halt a marine ice sheet instability (MISI) once initiated due to rapid grounding-line retreat.
  • Simulations show self-sustaining oscillations between advanced and collapsed ice-sheet states driven by internal ice-flow and Earth dynamics.

AI-generated from the title and abstract; the full text is not read.

Abstract

Abstract. The future evolution of the West Antarctic Ice Sheet may be characterized by self-reinforcing and irreversible retreat due to the unfolding of a marine ice sheet instability (MISI). How the stabilizing mechanism of glacial isostatic adjustment (GIA) does influence the timing and spatial extent of West Antarctica's present and potential future destabilization is highly uncertain and thus increasingly subject of numerical modeling studies that are based on observational data, striving for a most realistic representation of the Antarctic Ice Sheet. Here we employ an ensemble of idealized simulations in a synthetic model setup to systematically investigate how the interaction between ice-sheet dynamics and the visco-elastic response of the solid Earth affect the tipping dynamics of an inherently buttressed, Antarctic-type ice-sheet-shelf system that is perturbed by basal ice-shelf melting. Exploring a wide range of solid Earth structures we find that the threshold of bifurcation-induced tipping (B-tipping), i.e., the critical meltrate magnitude inferred for the ice sheet in quasi equilibrium, strongly depends on the timescale and the spatial extent of the solid-Earth response. Compared to the case of a fixed bed (no bed deformation), the B-tipping threshold increases for the strongest (East-Antarctic type) Earth structures by at least 80 % (from 0.8 to 1.5 m yr−1) whereas for the weakest (West-Antarctic type) Earth structures the increase is more than one order of magnitude larger. Due to the different timescales involved in the interplay between the dynamics of the ice sheet and the solid Earth, we find that for half of the ensemble members rate-induced tipping (R-tipping) occurs. That is, a sufficiently fast ramp-up of the basal meltrates triggers a MISI even before the critical forcing threshold of B-tipping would be crossed. In fact, due to R-tipping the effective critical tipping threshold reduces by up to 80 % for high upper-mantle viscosities and thin lithospheres. In none of our simulations bed uplift can stop a MISI once it is triggered, due to the very fast timescale of self-reinforcing grounding-line retreat. Furthermore, we highlight the occurrence of grounding-line overshoots and demonstrate cases of self-sustaining oscillations between advanced and collapsed ice-sheet states. Once triggered, these oscillations continue perpetually just due to the internal, non-linear interaction between ice-flow and solid-Earth dynamics. Our findings highlight that the character of the solid-Earth structure underlying a MISI-prone ice sheet can strongly affect its tipping dynamics mediated by the strength and timescale of the GIA feedback that counteracts MISI. In the context of Antarctic ice-sheet stability under global warming, our results particularly underscore that besides the magnitude also the rate of future anthropogenic greenhouse gas emissions are likely to play a crucial role.

The authors' abstract, as published at the source. The Cryosphere, 2026 · DOI ↗

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Field: Atmospheric Science

Atmospheric ScienceEarth and Planetary Sciences