Abstract. Here, we present cosmogenic-10Be and cosmogenic-3He data
from Ferrar dolerite pyroxenes in surficial rock samples and a bedrock core
from the McMurdo Dry Valleys, Antarctica, with the goal of refining the
laboratory methods for extracting beryllium from pyroxene, further
estimating the 10Be production rate in pyroxene and demonstrating the
applicability of 10Be–3He in mafic rock. The ability to routinely
measure cosmogenic 10Be in pyroxene will open new opportunities for
quantifying exposure durations and Earth surface processes in mafic rocks.
We describe scalable laboratory methods for isolating beryllium from
pyroxene, which include a simple hydrofluoric acid leaching procedure for
removing meteoric 10Be and the addition of a pH 8 precipitation step
to reduce the cation load prior to ion exchange chromatography. 10Be
measurements in pyroxene from the surface samples have apparent 3He
exposure ages of 1–6 Myr. We estimate a spallation production rate for
10Be in pyroxene, referenced to 3He, of 3.6 ± 0.2 atoms g−1 yr−1. 10Be and 3He measurements in the bedrock core
yield initial estimates for parameters associated with 10Be and
3He production by negative-muon capture (f10∗=0.00183
and f3∗fCfD=0.00337). Next, we demonstrate that the 10Be–3He pair in pyroxene can be
used to simultaneously resolve erosion rates and exposure ages, finding that
the measured cosmogenic-nuclide concentrations in our surface samples are
best explained by 2–8 Myr of exposure at erosion rates of 0–35 cm Myr−1. Finally, given the low 10Be in our laboratory blanks
(average of 5.7 × 103 atoms), the reported measurement precision, and
our estimated production rate, it should be possible to measure 2 g samples
with 10Be concentrations of 6 × 104 and 1.5 × 104 atoms g−1 with 5 % and 15 % uncertainty, respectively. With
this level of precision, Last Glacial Maximum to Late Holocene surfaces can
now be dated with 10Be in pyroxene. Application of 10Be in
pyroxene, alone or in combination with 3He, will expand possibilities
for investigating glacial histories and landscape change in mafic rock.