Late-glacial and Holocene history of the northeast Mediterranean mountain glaciers - New insights from in situ-produced 36Cl-based cosmic ray exposure dating of paleo-glacier deposits on Mount Olympus, Greece. (1st August 2018)

• Record Type: Journal Article
• Authors: Aumaître, Georges; Bourlès, Didier; Keddadouche, Karim; Styllas, Michael N.; Schimmelpfennig, Irene; Benedetti, Lucilla; Ghilardi, Mathieu
• Is Part Of: Quaternary science reviews. Volume 193(2018)
• Page Start: 244
• Page End: 265
• Publication Date: 2018-08-01
• Subjects: Small cirque glaciers -- In situ produced cosmogenic 36Cl -- Surface exposure dating (SED) -- Glacial phases -- Late-glacial -- Holocene -- Northeast Mediterranean -- Mount Olympus -- Greece; Geology, Stratigraphic -- Quaternary -- Periodicals; Stratigraphie -- Quaternaire -- Périodiques; 551.79
• DOI: 10.1016/j.quascirev.2018.06.020
• Languages: English
• ISSNs: 0277-3791

Abstract

Abstract: In this study, we present a new glacial chronology based on 20 in situ -produced 36 Cl-based cosmic ray exposure datings from moraine boulders and bedrock from the Throne of Zeus (TZ) and Megala Kazania (MK) cirques on Mount Olympus. The 36 Cl derived ages of glacial landforms range from 15.6 ± 2.0 to 0.64 ± 0.08 ka, spanning the Late-glacial and the Holocene. The Late-glacial, recorded in both cirques, is partitioned in three distinct phases (LG1-3): an initial phase of moraine stabilization at 15.5 ± 2.0 ka with subsequent deglaciation starting at ∼14 ka (LG1), followed by a shift to marginal conditions for glaciation at 13.5 ± 2.0 ka (LG2), sustained by large amounts of wind-blown snow, despite regional warming. Glacial conditions returned at 12.5 ± 1.5 ka (LG3) and were characterized by low air temperatures and glacier shrinking. The Holocene glacial phases (HOL1-3) are recorded only in the MK cirque, likely due to its topographic attributes. An early Holocene glacier stillstand (HOL1) at 9.6 ± 1.1 ka follows the regional temperatures recovery. No glacier activity is observed during the mid-Holocene. The Late Holocene glacier expansions, include a moraine stabilization phase (HOL2) at 2.5 ± 0.3 ka, during wet conditions and solar insolation minima, while (HOL3) corresponds to the early part of the Little Ice Age (0.64 ± 0.08ka). Our glacial chronology is coherent with glacial chronologies from several cirques along the northeast Mediterranean mountains and in pace with numerous proxies from terrestrial and marine systems from the north Aegean Sea. Highlights: The first 15ka-long glacial chronology of the southern Balkans, based on 20 36 Cl-based cosmic ray exposure datings from Mount Olympus, Greece. Three Late-glacial (LG1:15.5-14.0 ka, LG2:13.5ka, LG3:12.5ka) and three Holocene (HOL1: 9.6ka, HOL2: 2.5ka, HOL3: 0.64ka) glacial phases. HOL1-3 glacial phases occur only in the NW-oriented Megala Kazania cirque emphasizing the role of the local topography on Mediterranean glaciations. Glacial variability and solar insolation exhibit an out-of-phase behavior during the Late-glacial, but are synchronized during the Holocene. The new glacial record provides additional evidence for a seesaw Mediterraean climatic pattern during the Younger Dryas and the Little Ice Age.