The age and origin of the South Mountain Batholith (Nova Scotia, Canada) as constrained by zircon U–Pb geochronology, geochemistry, and O–Hf isotopes

Author:

Bickerton Luke1,Kontak Daniel J.1,Murphy J. Brendan2ORCID,Kellett Dawn A.3ORCID,Samson Iain M.14,Marsh Jeffrey H.15,Dunning Greg6,Stern Richard7

Affiliation:

1. Harquail School of Earth Sciences, Laurentian University, Sudbury, ON P3E 2C6, Canada

2. Department of Earth Sciences, St. Francis Xavier University, Antigonish, NS B2G 2W5, Canada

3. Geological Survey of Canada, 1 Challenger Drive, Dartmouth, NS B2Y 4A2, Canada

4. School of the Environment, University of Windsor, Windsor, ON N9B 3P4, Canada

5. Mineral Exploration Research Centre Isotope Geochemistry Lab, Laurentian University, Sudbury, ON P3E 2C6, Canada

6. Department of Earth Sciences, Memorial University, St. John's, NL A1B 3X5, Canada

7. Department of Earth and Atmospheric Sciences, University of Alberta, Edmonton, AB T6G 2R3, Canada

Abstract

The South Mountain Batholith (SMB; Nova Scotia, Canada) is the largest composite batholith exposed in the Appalachians and lies entirely within the most outboard Meguma terrane. In situ and CA–TIMS U–Pb dating and in situ isotopes (Lu–Hf, O) and geochemistry for zircon from all phases of the SMB constrain its source as well as its evolution. CA–ID–TIMS for zircon yields emplacement (autocryst) ages, indicating a transition from granodiorite (378.7 ± 1.2 to 375.4 ± 0.8 Ma) to leucogranite (375.4 to 371.8 ± 0.8 Ma) over several million years. Furthermore, in situ SHRIMP, LA–MC–ICP–MS, and SIMS analyses of distinct zircon domains reveal: (1) abundant ancient xenocrysts (∼420 Ma to 2.2 Ga); (2) antecryst ages ca. 3–15 million years older than SMB emplacement; (3) autocryst δ18O values between +7.3‰ and +9.1‰ (V-SMOW); (4) similar isotopes, REE signatures, and derived fO2 values among antecrysts and autocrysts; and (5) εHf values from the 371.8 ± 0.8 Ma Davis Lake Pluton (DLP) autocrysts that are higher (+1.74 to +4.38) than the rest of the SMB (−2.99 to +1.68). Collectively, these data suggest a protracted magmatic evolution for the SMB with melt generation and assembly from ∼390 to 370 Ma via melting of a metasomatized mantle source followed by contamination, first from the structurally underlying Avalonian terrane and later by metasedimentary wall rocks of the Meguma terrane. The most southwesterly part of the SMB (i.e., DLP) represents a petrogenetically distinct magmatic phase that underwent less overall contamination than the rest of the SMB.

Publisher

Canadian Science Publishing

Subject

General Earth and Planetary Sciences

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