Preprints
https://doi.org/10.5194/egusphere-2026-4455
https://doi.org/10.5194/egusphere-2026-4455
23 Sep 2026
 | 23 Sep 2026
Status: this preprint is open for discussion and under review for The Cryosphere (TC).

Evaporitic carbonates record surface melting in Antarctica

Noah Brigham, Jesper L. Giardino, Gavin Piccione, Jessica Gagliardi, Samuel T. Kodama, Slawek Tulaczyk, Christine Siddoway, and Terrence Blackburn

Abstract. Changes in Pleistocene Antarctic temperatures often coincide with variations in Northern Hemisphere summer insolation. While models invoking global CO₂ changes and shifts in oceanic and atmospheric circulation explain the temperature coherence between the poles, the role of Southern Hemisphere insolation in local Antarctic temperatures remain unclear. Here we present a temporal and geochemical record of Antarctic surface melting recorded by evaporitic carbonate formation from eight sites spanning the Amundsen Sea to the Ross Sea and 365m - 2000m in elevation. Isotopic data indicate water sourced from surface melt that weathers local rock and saturates carbonate through evaporation. U–Th dates restrict carbonate formation to three of the five most recent periods of high Southern Hemisphere summer insolation. These observations calibrate the effective albedo of darkened surfaces near nunataks and identify a Southern Hemisphere summer insolation threshold at which surface melt can occur under polar conditions.

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Noah Brigham, Jesper L. Giardino, Gavin Piccione, Jessica Gagliardi, Samuel T. Kodama, Slawek Tulaczyk, Christine Siddoway, and Terrence Blackburn

Status: open (until 04 Nov 2026)

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Noah Brigham, Jesper L. Giardino, Gavin Piccione, Jessica Gagliardi, Samuel T. Kodama, Slawek Tulaczyk, Christine Siddoway, and Terrence Blackburn
Noah Brigham, Jesper L. Giardino, Gavin Piccione, Jessica Gagliardi, Samuel T. Kodama, Slawek Tulaczyk, Christine Siddoway, and Terrence Blackburn
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Latest update: 23 Sep 2026
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Short summary
We present a record of carbonate mineral crusts found on Antarctic nunataks that form when snow melts and the resulting water evaporates. By dating these crusts with uranium-series methods, we show that surface melting happened during three of the last five peaks in Southern Hemisphere summer radiation (insolation). The results provide insight into how intense solar radiation can trigger snow melting on darkened rock surfaces even when temperatures are well below freezing.
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