Abstract
The so-called “Gran Dolina site” (Atapuerca mountain range, N Spain) is a karstic cavity filled by sediments during the Pleistocene, some of which contain a rich ensemble of archaeological and paleontological records. These sediments have contributed significantly to our understanding of early human dispersal in Europe but, in contrast, older, interior facies deposits have received much less of attention. The stratigraphy of Gran Dolina reveals an abrupt sedimentary change of interior to entrance facies from bottom to top, reflecting a significant paleoenvironmental change that promoted the accumulation of sediments transported from the vicinity of the cave by water or “en masse”. Since the major magnetic polarity reversal known as the Matuyama-Brunhes boundary (0.78 Ma) was detected within the TD7 unit in the middle of the stratigraphic section, we carried out a new combined paleomagnetic, radiometric (U-Pb), and electron spin resonance (ESR) dating study of the lower part of the sequence in order to constrain the chronology of the interior facies at Gran Dolina. U-Pb analysis of speleothems did not produce age information as the samples proved to be extremely unradiogenic. The magnetic stratigraphy of the cave interior sediments reveals a dominant reverse magnetic polarity, coherent with a Matuyama age, and interrupted by a normal polarity magnetozone interpreted as the Jaramillo Subchron (1.0–1.1 Ma). ESR ages on quartz grains from the upper part of the interior facies sediments are coherent with such an interpretation. We conclude that the fluvial deposits (interior facies) that constitute the cave floor began accumulating before 1.2 Ma. The development of large cave entrances at Gran Dolina occurred shortly after the Jaramillo Subchron but before ca 900 ka ago.
Original language | English |
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Pages (from-to) | 1-16 |
Number of pages | 16 |
Journal | Quaternary Science Reviews |
Volume | 186 |
DOIs | |
Publication status | Published - 15 Apr 2018 |
Funding
Access and permission to collect samples in Atapuerca was granted by Junta de Castilla y León. The authors are deeply indebted to the Atapuerca Research Team (EIA) and the Fundación Atapuerca for continuous support of this research. We are thankful to Miguel Ángel Martín for preparing field photographs (Fig. 2). Financial support for this work was obtained from Junta de Castilla y León and from MINECO Grants CGL2010-16821 and CGL2015-65387-C3-3-P . M. Duval's research is currently funded by an Australian Research Council Future Fellowship ( FT150100215 ). U-Pb dating at Melbourne was conducted with funding from the Australian Research Council . MJS was funded by the Netherlands Organisation for Scientific Research grants NWO-ALW 823.01.003 . We thank the three anonymous reviewers for their helpful constructive comments and suggestions.
Keywords
- ESR
- Interior facies
- Karstic cave
- Paleomagnetism
- Pleistocene
- Spain
- U/Pb dating