Technical note: Studying lithium metaborate fluxes and extraction protocols with a new, fully automated in situ cosmogenic 14C processing system at PRIME Lab
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Published:2023-09-20
Issue:2
Volume:5
Page:361-375
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ISSN:2628-3719
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Container-title:Geochronology
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language:en
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Short-container-title:Geochronology
Author:
Lifton NathanielORCID, Wilson JimORCID, Koester AllieORCID
Abstract
Abstract. Extraction procedures for in situ cosmogenic 14C (in situ 14C) from
quartz require quantitative isotopic yields while maintaining scrupulous
isolation from atmospheric and organic 14C. These time- and labor-intensive
procedures are ripe for automation; unfortunately, our original automated
in situ 14C extraction and purification systems, reconfigured and retrofitted
from our original systems at the University of Arizona, proved less reliable
than hoped. We therefore installed a fully automated stainless-steel system
(except for specific borosilicate glass or fused-silica components)
incorporating more reliable valves and improved actuator designs, along with
a more robust liquid nitrogen distribution system. As with earlier versions,
the new system uses a degassed lithium metaborate (LiBO2) flux to dissolve
the quartz sample in an ultra-high-purity oxygen atmosphere, after a
lower-temperature combustion step to remove atmospheric and organic 14C. We compared single-use high-purity Al2O3 against reusable
90 %Pt / 10 %Rh (Pt/Rh) sample combustion boats. The Pt/Rh boats heat more
evenly than the Al2O3, reducing procedural blank levels and
variability for a given LiBO2 flux. This lower blank variability also
allowed us to trace progressively increasing blanks to specific batches of
fluxes from our original manufacturer. Switching to a new manufacturer
returned our blanks to consistently low levels on the order of (3.4 ± 0.9) × 104 14C atoms. We also analyzed the CRONUS-A intercomparison material to investigate
sensitivity of extracted 14C concentrations to the temperature and
duration of the combustion and extraction steps. Results indicate that 1 h
combustion steps at either 500 or 600 ∘C yield results consistent
with the consensus value of Jull et al. (2015), while 2 h
at 600 ∘C results in loss of ca. 9 % of the high-temperature
14C inventory. Results for 3 h extractions at temperatures ranging
from 1050 to 1120 ∘C and 4.5 h at 1000 ∘C
yielded similar results that agreed with the nominal value and
published results from most laboratories. On the other hand, an extraction
for 3 h at 1000 ∘C was judged to be incomplete due to a
significantly lower measured concentration. Based on these results, our
preferred technique is now combustion for 1 h at 500 ∘C followed
by a 3 h extraction at 1050 ∘C. Initial analyses of the CoQtz-N
intercomparison material at our lab yielded concentrations ca. 60 % lower
than those of CRONUS-A, but more analyses of this material from this and
other labs are clearly needed to establish a consensus value.
Funder
National Science Foundation
Publisher
Copernicus GmbH
Subject
Paleontology,Stratigraphy,Geology
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