z-logo
open-access-imgOpen Access
The peopling of Europe and the cautionary tale of Y chromosome lineage R-M269
Author(s) -
George B. J. Busby,
Francesca Brisighelli,
Paula SánchezDiz,
Eva RamosLuis,
Conrado MartinezCadenas,
Mark Thomas,
Daniel G. Bradley,
Leonor Gusmão,
Bruce Winney,
Walter F. Bodmer,
Marielle Vennemann,
Valentina Coia,
Francesca Scarnicci,
Sergio Tofanelli,
Giuseppe Vona,
Rafał Płoski,
Carla Vecchiotti,
Tatijana Zemunik,
Igor Rudan,
Sena Karachanak-Yankova,
Драга Тончева,
Paolo Anagnostou,
Gianmarco Ferri,
Cesare Rapone,
Tor Hervig,
Torolf Moen,
James F. Wilson,
Cristian Capelli
Publication year - 2011
Publication title -
proceedings of the royal society b biological sciences
Language(s) - English
Resource type - Journals
eISSN - 1471-2954
pISSN - 0962-8452
DOI - 10.1098/rspb.2011.1044
Subject(s) - cline (biology) , haplogroup , biological dispersal , lineage (genetic) , diversity (politics) , evolutionary biology , geography , ancestor , genealogy , biology , demography , history , haplotype , genetics , sociology , archaeology , allele , population , anthropology , gene
Recently, the debate on the origins of the major European Y chromosome haplogroup R1b1b2-M269 has reignited, and opinion has moved away from Palaeolithic origins to the notion of a younger Neolithic spread of these chromosomes from the Near East. Here, we address this debate by investigating frequency patterns and diversity in the largest collection of R1b1b2-M269 chromosomes yet assembled. Our analysis reveals no geographical trends in diversity, in contradiction to expectation under the Neolithic hypothesis, and suggests an alternative explanation for the apparent cline in diversity recently described. We further investigate the young, STR-based time to the most recent common ancestor estimates proposed so far for R-M269-related lineages and find evidence for an appreciable effect of microsatellite choice on age estimates. As a consequence, the existing data and tools are insufficient to make credible estimates for the age of this haplogroup, and conclusions about the timing of its origin and dispersal should be viewed with a large degree of caution.

The content you want is available to Zendy users.

Already have an account? Click here to sign in.
Having issues? You can contact us here
Accelerating Research

Address

John Eccles House
Robert Robinson Avenue,
Oxford Science Park, Oxford
OX4 4GP, United Kingdom