POLYMETAMORPHIC EVOLUTION OF THE WESTERN BLUE RIDGE TERRANE THROUGH ACADIAN AND ALLEGHANIAN OROGENIES
The protolith of the MHHS has an OIB-type chemical signature and crystallized at ca. 435 Ma, as revealed through our new zircon U-Pb geochronology. Whole-rock and zircon trace element systematics indicate that the source of the protolith was likely basalt with enriched mantle chemical characteristics, potentially part of a seamount.
Hornblende 39Ar-40Ar geochronology of the MHHS, including both multi- and single-crystal step heating results revealed plateau ages of ca. 340-385 Ma. The Ar release spectra also display the effect of extraneous 40Ar in hornblende, causing the apparently older ages for some of the samples analyzed. However, results are Devonian to early-Carboniferous. Furthermore, rutile grains were observed cross-cutting the hornblendes in thin-sections, representing a younger phase. This observation was supported by the ca. 320 Ma U-Pb ages obtained from the rutile grains. We interpret these ages to indicate a partial overprint during the late-Carboniferous.
These new results help to better constrain the tectonic evolution of the MHHS and the timing of the amphibolite facies metamorphism of WBR. Results are consistent with OIB-like ocean floor magmatism at the Laurentian margin during the Silurian, followed by previously proposed successor basin development supported by palaeontologic evidence from the Murphy Synclinorium. New U-Pb and Ar-Ar ages indicate a Devonian (Acadian Orogeny) tectonothermal event with a partial overprint in Carboniferous (Alleghanian Orogeny).