Timing of the local last glacial maximum in Terra Nova Bay, Antarctica defined by cosmogenic dating

Authors
Rhee, Hyun HeeLee, Min KyungSeong, Yeong BaeHong, SeongchanLee, Jae IlYoo, Kyu-CheulYu, Byung Yong
Issue Date
2019-10
Publisher
PERGAMON-ELSEVIER SCIENCE LTD
Citation
QUATERNARY SCIENCE REVIEWS, v.221
Abstract
The Jangbogo Hills are erratic-covered landforms consisting of a series of benches that are parallel to the length of Campbell Glacier, northern Victoria Land, Antarctica. We sampled 41 erratic cobbles from six benches to reveal the exposure times of glacier erratics using in situ Be-10 and Al-26. The erratics from the upper three benches yield exposure ages older than Marine Isotope Stage (MIS) 4, with most exposed since MIS 5. However, the lower three benches exhibit tight clusters of exposure ages that range from MIS 3 to the Holocene. Campbell Glacier underwent rapid downwasting during MIS 5, centered at 98.3 ka from its maximum position at the penultimate glacial maximum (PGM). This downwasting continued throughout the last glacial period, with a potential minor stagnation around a bench (similar to 90 m asl) between 35.4 and 17.0 ka. Our cosmogenic nuclides surface exposure dating results highlight three important points concerning the glacial history of Terra Nova Bay since the penultimate glacial maximum (PGM) in northern Victoria Land, Antarctica: 1) Campbell Glacier was thicker at the PGM than at the global last glacial maximum (LGM); 2) the local LGM occurred during MIS 4; and 3) the extent of Campbell Glacier during the global LGM (90 m) was much smaller than previously assumed (300-400 m). Hence, the previous view that the local LGM (MIS 4) in Victoria Land, Antarctica was synchronous with the global LGM (MIS 2) should be treated with caution. (C) 2019 Elsevier Ltd. All rights reserved.
Keywords
NORTHERN VICTORIA LAND; SURFACE EXPOSURE AGES; ICE-SHEET; ROSS-SEA; NUCLIDES DOCUMENT; DRY-VALLEYS; BE-10; RETREAT; HISTORY; RANGE
ISSN
0277-3791
URI
https://pubs.kist.re.kr/handle/201004/119485
DOI
10.1016/j.quascirev.2019.105897
Appears in Collections:
KIST Article > 2019
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