U‐Pb Geochronological and Thermochronological Time–Temperature Constraints of 40Ar/39Ar Hornblende Reference Material HB 3gr
Terrence Blackburn, Noah M. McLean, Samuel A. Bowring
Abstract
Terrence Blackburn, Noah M. McLean, Samuel A. Bowring
Abstract
Hornblende from the Lone Grove Pluton, Llano Uplift, Texas, has served as an irradiation reference material in 40Ar/39Ar studies for decades. In order to evaluate the apparent age bias that currently exists between the U‐Pb and 40Ar/39Ar systems, zircon and titanite were dated by isotope dilution‐thermal ionisation mass spectrometry (ID‐TIMS) from the same rock from which the hornblende 40Ar/39Ar reference material HB3gr is derived. Zircon U‐Pb data indicate initial crystallisation at 1090.10 ± 0.16 Ma (2s), a date that is 1.7% older than the accepted K‐Ar date (1072 ± 14 Ma, 2s) for HB3gr; an offset that exceeds the typical 0.5–1% bias between the two systems, though remaining within uncertainty due to the large uncertainties in the 40K decay constant. Zircon data are presented using both EARTHTIME tracers ET535 and ET2535 and are statistically indistinguishable. Single grain titanite analyses range between 1082 ± 0.75 and 1086 ± 0.81 Ma (2s) and are interpreted to record the subsequent cooling following crystallisation at rates between 30 and 50 °C Ma−1. This is supported by the observation that hornblende 40Ar/39Ar dates corrected for decay constant bias are resolvably younger than the zircon U‐Pb date and in good agreement with titanite U‐Pb dates, permitting the conclusion that both titanite U‐Pb and hornblende 40Ar/39Ar systems provide a record of cooling.
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Hornblende from the Lone Grove Pluton, Llano Uplift, Texas, has served as an irradiation reference material in 40Ar/39Ar studies for decades. In order to evaluate the apparent age bias that currently exists between the U‐Pb and 40Ar/39Ar systems, zircon and titanite were dated by isotope dilution‐thermal ionisation mass spectrometry (ID‐TIMS) from the same rock from which the hornblende 40Ar/39Ar reference material HB3gr is derived. Zircon U‐Pb data indicate initial crystallisation at 1090.10 ± 0.16 Ma (2s), a date that is 1.7% older than the accepted K‐Ar date (1072 ± 14 Ma, 2s) for HB3gr; an offset that exceeds the typical 0.5–1% bias between the two systems, though remaining within uncertainty due to the large uncertainties in the 40K decay constant. Zircon data are presented using both EARTHTIME tracers ET535 and ET2535 and are statistically indistinguishable. Single grain titanite analyses range between 1082 ± 0.75 and 1086 ± 0.81 Ma (2s) and are interpreted to record the subsequent cooling following crystallisation at rates between 30 and 50 °C Ma−1. This is supported by the observation that hornblende 40Ar/39Ar dates corrected for decay constant bias are resolvably younger than the zircon U‐Pb date and in good agreement with titanite U‐Pb dates, permitting the conclusion that both titanite U‐Pb and hornblende 40Ar/39Ar systems provide a record of cooling.
Key concepts: Titanite, Zircon, Hornblende, Geology, Pluton, Isotope dilution, Thermochronology, Isotopes of argon