Geochemical features and geodynamic significance of the southern Tyrrhenian backarc basin
Geochemical features and geodynamic significance of the southern Tyrrhenian backarc basin
复制标题
第勒尼安弧后盆地南部地球化学特征及地球动力学意义
DOI:
10.1130/2007.2418(11
复制
发表时间:
2007
影响因子:
--
通讯作者:
M. Marani
中科院分区:
文献类型:
--
作者:
T. Trua;G. Serri;M. Marani
The southern Tyrrhenian region represents a rare case of an active backarc basin where island-arc basalt (IAB)–type and ocean-island basalt (OIB)–type magmas coexist. IAB-type magmatism is the most common, whereas OIB-type magmas are restricted to a few areas. Geochemical and isotopic characteristics of southern Tyrrhenian submarine volcanic samples are summarized herein, with special attention to samples recovered during recent seafl oor sampling. Samples derived from Marsili volcano, the biggest seamount in the Tyrrhenian Sea, together with those of the Prometeo submarine lava fi eld and Palinuro seamount, give a comprehensive picture of the mantle sources of southern Tyrrhenian magmatism. Most of these samples are relatively high-magnesian basalts that approximate primary magma compositions, thus providing insight into petrogenesis of IABand OIB-type magmas of this area. Petrological data, integrated with new bathymetric data, allow the geodynamic evolution of the southern Tyrrhenian backarc basin to be reconstructed. We suggest that the transition from IABto OIB-type magmas recorded in the southern Tyrrhenian backarc basin is related to the propagation of asthenospheric mantle from beneath Africa around the edges of the Ionian slab. The data suggest that the infl ow of asthenosphere from beneath Africa has been important since the early Neogene evolution of the southern Tyrrhenian region.