Article ID Journal Published Year Pages File Type
4467508 Palaeogeography, Palaeoclimatology, Palaeoecology 2010 9 Pages PDF
Abstract

Magnetostratigraphic studies have established a first-order chronological framework for the Paleolithic sites in the Nihewan Basin (North China), which enabled tracking early human evolution in East Asia. However, to fully understand how well early humans were adapted to climate change, a truly precise dating of the Paleolithic sites is required. Here, we established a high-resolution astronomical timescale for the Xiantai and Donggutuo fluvio-lacustrine successions at the eastern margin of the Nihewan Basin employing low-field magnetic susceptibility (χ) as a climatic indicator, aiming to further refine the ages of the Xiantai, Donggutuo and Maliang Paleolithic sites. Starting from an initial age model constrained by geomagnetic reversals, larger-scale χ cycles were firstly tuned to orbital obliquity using an automatic orbital tuning method. This first-order tuning was followed by simultaneously tuning χ to both obliquity and precession. The finally tuned χ records can be correlated almost cycle-by-cycle with the quartz grain-size record of the Chinese loess sequence and the marine δ18O record. The astronomically estimated age of the Xiantai Paleolithic site is ca. 1.48 Ma, corresponding to paleosol layer S20 of the Chinese loess sequences or marine oxygen isotope stage (MIS) 49, an interglacial period. The astronomical estimate for the Donggutuo Paleolithic site ranges from ~ 1.06 Ma to 1.12 Ma, corresponding to paleosol/loess layers S11–S12 or MIS 31–33, spanning both interglacial and glacial periods. The astronomically estimated age of the Maliang Paleolithic site is ~ 0.79 Ma, corresponding to loess layer L8 or MIS 20, a glacial period. This astronomical finding further implies that early humans may have permanently occupied China as far north as 40oN since at least 1.1 Ma, and before this time the occupation may be intermittent.

Related Topics
Physical Sciences and Engineering Earth and Planetary Sciences Earth-Surface Processes
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