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Reconsideration of Neo‐Tethys Evolution Constrained from the Nature of the Dazhuqu Ophiolitic Mantle, Southern Tibet
Author(s) -
LIU Tong,
WU Fuyuan,
LIU Chuanzhou,
ZHANG Chang,
JI Wenbin,
XU Yang
Publication year - 2020
Publication title -
acta geologica sinica ‐ english edition
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 0.444
H-Index - 61
eISSN - 1755-6724
pISSN - 1000-9515
DOI - 10.1111/1755-6724.14450
Subject(s) - ophiolite , geology , mantle (geology) , spinel , peridotite , abyssal zone , geochemistry , partial melting , tectonics , paleontology , oceanography
The nature (i.e., sub‐oceanic, sub‐arc or sub‐continental) of ophiolitic mantle peridotites from the eastern Neo‐Tethyan domain in southern Tibet has been hotly debated. This uncertainty limits our understanding of the history and evolution of the eastern Neo‐Tethys Ocean. Here we present petrological, geochemical and Re‐Os isotopic data for the mantle peridotites from the Dazhuqu ophiolite in the central segment of the Yarlung Zangbo suture zone, southern Tibet. Samples collected include both spinel lherzolites and spinel harzburgites. The lherzolites have spinel Cr # [Cr/ (Cr + Al), ∼ 0.3–0.4] comparable to those of typical abyssal peridotites. In contrast, the harzburgites have spinel Cr # (∼0.3–0.7) overlapping with the ranges of both abyssal and fore‐arc peridotites (Day et al., 2017; Parkinson and Pearce, 1998); two samples have spinel Cr # higher than 0.6, which is probably ascribed to intense melt‐rock interactions. Clinopyroxene trace element modeling indicates that the Dazhuqu mantle peridotites have experienced 0–6% garnet‐facies melting followed by 10%–18% melting in the spinel stability field. This is similar to the degree of garnet‐facies melting inferred for many abyssal peridotites (Hellebrand et al., 2002) and implies deep initial melting (> 85 km), which distinguishes the Dazhuqu mantle peridotites from fore‐arc peridotites (commonly <80 km in origin). The Dazhuqu peridotites have unradiogenic 187 Os/ 188 Os of 0.11836–0.12922, which are commonly lower than the recommended value of primitive upper mantle (PUM) (Meisel et al., 2001). All but one samples yield relatively younger Re depletion ages (T RD = 0.06–0.81 Ga) with respect to the only one sample having an older T RD age of 1.66 Ga. Re‐Os isotopes and highly siderophile element (HSE) compositions of the Dazhuqu peridotites are similar to those of abyssal peridotites (Day et al., 2017) and the Oman southern massifs (Hangh⊘j et al., 2010) but are distinct from non‐cratonic sub‐continental lithospheric mantle (SCLM) xenoliths and sub‐arc mantle. We emphasize the similarity between the Dazhuqu and Oman ophiolites, both representing Neo‐Tethyan oceanic lithosphere and implying ridge–trench collision.

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