4.7 Article

Mid-Holocene drying of the US Great Basin recorded in Nevada speleothems

期刊

QUATERNARY SCIENCE REVIEWS
卷 127, 期 -, 页码 174-185

出版社

PERGAMON-ELSEVIER SCIENCE LTD
DOI: 10.1016/j.quascirev.2015.04.011

关键词

Great Basin; Holocene; Speleothems; U-Th dating; Paleoclimate

资金

  1. NSF [EAR-1103379]
  2. MIT EAPS Student Research Fund
  3. Comer Science and Education foundation

向作者/读者索取更多资源

Lake level records point to dramatic changes in Great Basin water balance over the last 25 ka, but the timing and pace of Holocene drying in the region remains poorly documented. Here we present stable isotope and trace metal data from two Lehman Caves, NV speleothems that provide a well-dated record of latest Pleistocene to mid-Holocene hydroclimate in the U.S. Great Basin. Together the stalagmites span the interval between 16.4 ka and 3.8 ka, with a hiatus from 15.0 ka to 12.7 ka. Mg/Ca and delta C-13 covary throughout the records, consistent with control by the extent of degassing and prior calcite precipitation (PCP); measurements of modern cave and soil waters support PCP as the primary control on drip-water trace-element composition. We therefore interpret Mg/Ca and delta C-13 as reflecting infiltration rates, with higher values corresponding to drier periods. Both Mg/Ca and delta C-13 indicate a wet period at the beginning of the record (12.7-8.2 ka) followed by pronounced drying after 8.2 ka. This mid-Holocene drying is consistent with records from around the western United States, including a new compilation of Great Basin lake-level records. The strong temporal correspondence with the collapse of the Laurentide ice sheet over Hudson Bay suggests that this drying may have been triggered by northward movement of the winter storm track as a result of ice sheet retreat. However, we cannot rule out an alternative hypothesis that wet early Holocene conditions are related to equatorial Pacific sea-surface temperature. Regardless, our results suggest that Great Basin water balance in the early Holocene was driven by factors other than orbital changes. (C) 2015 Elsevier Ltd. All rights reserved.

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