Zircon as the best mineral for P– T–time history of UHP metamorphism: A review on mineral inclusions and U–Pb SHRIMP ages of zircons from the Dabie–Sulu UHP rocks

• Published in: Journal of Asian earth sciences Vol. 40; no. 1; pp. 1 - 39
• Main Authors: Liu, F.L., Liou, J.G.
• Format: Journal Article
• Language: English
• Published: Elsevier Ltd 04-01-2011
• Subjects: Cathodoluminescence image; Dabie–Sulu UHP terrane; Mineral inclusion; P– T– t path; SHRIMP U–Pb dating; Zircon; Cathodoluminescence image; Mineral inclusion; SHRIMP U–Pb dating; Dabie–Sulu UHP terrane; Zircon; P– T– t path
• ISSN: 1367-9120; 1878-5786
• DOI: 10.1016/j.jseaes.2010.08.007

► Zircon is the best mineral to record the metamorphic history of UHP rocks. ► UHP mineral inclusions in zircons can be easily identified by Laser Raman. ► Discrete and meaningful ages are recorded in zoned zircon. ► New UHP metamorphic belts will be found by mineral inclusions in zircon.
Zircon is the best mineral to record the complex evolution history of ultrahigh-pressure (UHP) metamorphic rocks as mineralogical and geochemical tracers of UHP metamorphism are almost obliterated in matrix assemblages resulted from subsequent retrogression during exhumation. Zircons from Dabie–Sulu UHP rocks, including outcrop and core samples from drill holes ranging from 432 to 5158
m in depth contain abundant mineral inclusions of protolith, prograde, peak (UHP) and retrograde minerals in different domains; these minute inclusions were identified by laser Raman spectroscopy and/or electronic microprobe analysis. Systematic studies on inclusions in zircons from previous and present studies indicate that the Dabie–Sulu UHP terrane extends for >2000
km, is about 50
km wide, and has at least 10
km thick, probably the largest UHP terrane recognized in the world thus far. The internal structure of zircon revealed by cathodoluminescence (CL) imaging displays a distinct zonation, which comprises an inherited (magmatic or detrital) core, prograde, peak (UHP), and outmost retrograde domains, each with distinctive mineral inclusion assemblages. Low-pressure, igneous mineral inclusions are common in the inherited (magmatic or detrital) zircon cores. In contrast, quartz eclogite-facies inclusion assemblages occur in prograde domains, coesite eclogite-facies inclusion assemblages are preserved in UHP domains, and amphibolite-facies inclusion assemblages are enclosed in outmost retrograde rims. Parageneses and compositions of inclusion minerals preserved in distinct zircon domains were used to constrain the metamorphic
P–
T path of many Dabie–Sulu UHP rocks. The results indicate that Neoproterozoic supracrustal rocks together with minor mafic-ultramafic rocks were subjected to a prograde subduction-zone metamorphism at 570–690
°C and 1.7–2.1
GPa, and UHP metamorphism at 750–850
°C and 3.4–4.0
GPa, following by rapid decompression to amphibolite-facies retrograde metamorphism at 550–650
°C and 0.7–1.05
GPa. Sensitive high-resolution ion microprobe (SHRIMP) U–Pb spot analyses of the zoned zircons show four discrete and meaningful ages of the Dabie–Sulu metamorphic evolution: (1) Neoproterozoic protolith ages (800–750
Ma); (2) 246–244
Ma for early-stage quartz eclogite-facies prograde metamorphism; (3) 235–225
Ma for UHP metamorphism; and (4) 215–208
Ma for late-stage amphibolite-facies retrogression. This indicates that Neoproterozoic voluminous igneous protoliths of orthogneiss in response to the breakup of Rodinia supercontinent, together with various sedimentary rocks, and minor mafic-ultramafic intrusive and extrusive rocks, were subjected to coeval Triassic subduction to mantle depths and exhumation during the collision between the South China Block and North China Block. The estimated subduction and exhumation rates for the Dabie–Sulu UHP terrane would be up to 4.7–9.3
km
Myr
−1 and 5.0–11.3
km
Myr
−1, respectively. The zonal distribution of mineral inclusions and the preservation of index UHP minerals such as coesite imply that zircon is the best mineral container for each metamorphic stage, particular for supracrustal rocks as their metamorphic evolution and UHP evidence have been almost or completely obliterated. Similar conclusions have been documented elsewhere for other UHP terranes.