Authigenic 10Be/9Be ratio signature of the Matuyama–Brunhes boundary in the Montalbano Jonico marine succession

Type Article
Date 2017-02
Language English
Author(s) Simon QuentinORCID1, 2, Bourles Didier L.1, Bassinot Franck3, 4, Nomade Sebastien3, 4, Marino Maria5, Ciaranfi Neri5, Girone Angela5, Maiorano Patrizia5, Thouveny Nicolas1, Choy Sandrine1, 2, Dewilde Fabien3, 4, Scao Vincent3, 4, Isguder Gulay3, 4, Blamart Dominique3, 4, Aster Team
Affiliation(s) 1 : Aix Marseille Univ, Coll France, CNRS, IRD,CEREGE UM34, Aix En Provence, France.
2 : Univ Paris Diderot, Sorbonne Paris Cite, IPGP, UMR 7154 CNRS, F-75238 Paris, France.
3 : UVSQ, CNRS, CEA, Lab Sci Climat & Environm, UMR8212, LSCE IPSL, Gif Sur Yvette, France.
4 : Univ Paris Saclay, Gif Sur Yvette, France.
5 : Univ Bari Aldo Moro, Dept Earth & Geoenvironm Sci, E Orabona 4, I-70125 Bari, Italy.
Source Earth And Planetary Science Letters (0012-821X) (Elsevier Science Bv), 2017-02 , Vol. 460 , P. 255-267
DOI 10.1016/j.epsl.2016.11.052
WOS© Times Cited 32
Keyword(s) Be-10 cosmogenic nuclide, authigenic Be-10/Be-9 ratio, Matuyama Brunhes Boundary (MBB), high-resolution oxygen isotope stratigraphy, MIS 19, GSSP stratotype
Abstract

Geomagnetic dipole moment (GDM) lows associated with polarity reversals or geomagnetic excursions induce significant modulation of the cosmogenic nuclide Beryllium-10 (Be-10) production. Hence, the reconstruction of atmospheric Be-10 production rates from natural archives such as marine sedimentary sequences or ice cores constitutes a complementary approach, independent from paleomagnetic measurements, to decipher past GDM fluctuations. This is particularly important in the Montalbano Jonico succession (South Italy) since it is candidate to host the Global Stratotype Section and Point of the Middle Pleistocene Stage but where the magnetostratigraphic positioning of the Matuyama-Brunhes boundary (MBB) has not been available up to now. This study presents (1) original authigenic Be-10 cosmogenic nuclide and Be stable isotope results, and (2) new high-resolution benthic oxygen isotope record covering termination IX and Marine Isotope Stage (MIS) 19. A robust chronological framework is established on the basis of (i) our oxygen isotope stratigraphy, using the strong analogies between MIS 1 and MIS 19c in terms of orbital forcing and CO2 level, and (ii) one precise Ar-40/Ar-39 date obtained in the tephra layer V4. The authigenic Be-10/Be-9 ratio record marks the atmospheric Be-10 overproduction linked to the dipole low accompanying the MBB transition, with a characteristic twofold increase of the Be-10 production at the end of MIS 19c and early MIS 19b. This signature is similar to those described in both marine and ice core records. The detailed chronostratigraphy constrained by a radiometrically-dated tephra layer (773.9 +/- 1.3 ka) within the MBB interval, makes it possible to discuss the structure and to assess the timing of the Be-10-production changes, and thus the MBB geomagnetic variations, with an unprecedented accuracy for a marine archive (sedimentation rates similar to 80 cm/ka). These new cosmogenic nuclide production signatures provide the only missing constraint required for retaining the Montalbano Jonico succession as a global-scale correlation reference section for the Early-Middle Pleistocene boundary.

Full Text
File Pages Size Access
Publisher's official version 13 1 MB Open access
Table S1. Stable isotopic oxygen results. 52 KB Open access
Table S2. Correlation matrix between authigenic Be results versus environmental proxies. 41 KB Open access
Table S3. Test of all calibrations in use for the 40Ar/39Ar dating method. 44 KB Open access
Top of the page

How to cite 

Simon Quentin, Bourles Didier L., Bassinot Franck, Nomade Sebastien, Marino Maria, Ciaranfi Neri, Girone Angela, Maiorano Patrizia, Thouveny Nicolas, Choy Sandrine, Dewilde Fabien, Scao Vincent, Isguder Gulay, Blamart Dominique, Aster Team (2017). Authigenic 10Be/9Be ratio signature of the Matuyama–Brunhes boundary in the Montalbano Jonico marine succession. Earth And Planetary Science Letters, 460, 255-267. Publisher's official version : https://doi.org/10.1016/j.epsl.2016.11.052 , Open Access version : https://archimer.ifremer.fr/doc/00420/53183/