Optically stimulated luminescence (OSL) geochronology yields the time from the last light or heat exposure after sediment erosion, deposition and burial; and further exposure to light or heat. Thus, natural sedimentary processes or heating events (>300 °C) reduces the previously inherited luminescence signal to a consistently low level. In the past two decades, there have been substantial advances in luminescence dating, such as single aliquot and grain analysis of specific mineral grains, like quartz. These experiment-based dating protocols with blue or green diodes can compensate effectively for sensitivity changes induced in the laboratory, rendering OSL ages for the past ca. 500 ka1,2,3.
Silicate minerals such as quartz and potassium feldspar have varying crystal lattice-charge defects; some formed at the time of mineral crystallization and others due to subsequent exposure to ionizing radiation, resulting in geochronometric potential. These defects are probable locations of electron storage with trap-depth energies of ~1.3-3 eV. A subpopulation of contained electrons in lattice-charge defects of quartz grains is a source for time-diagnostic luminescence emissions with excitation by blue light. Thus, this luminescence emission increases with time, above the solar or heat reset level with exposure to ionizing radiation during the burial period. This signal is reduced to a low, definable level ("zeroed") with subsequent sunlight exposure with sediment erosion, transport, and deposition. This luminescence "cycle" occurs in most depositional environments on Earth and other planets. Thus, OSL dating of sedimentary quartz grains provides a depositional age, reflecting the time elapsed since the last light exposure with deposition and burial (Figure 1).
Luminescence dating is a dosimetric-based technique that yields age estimates for selected mineral grains, like quartz, from eolian, fluvial, lacustrine, marine, and colluvial sediments associated with enumerable contexts for geomorphic, tectonic, paleontologic, paleoclimatic, and archaeologic research2,4,5,6,7. OSL dating is also being evaluated to constrain surface processes on other planets, particularly on Mars8,9. Often, the most used mineral in OSL dating on Earth is quartz, reflecting its natural abundance, an inherent sensitivity as a geochronometer, signal stability, and rapid resetting with sunlight exposure (seconds to minutes)4,10,11,12. However, the accuracy of OSL dating is compromised if the quartz extract is impure, particularly if contaminated by potassium and other feldspars, which can have luminescence emissions ten to hundred-fold brighter than quartz and can yield age underestimates13. Therefore, the absolute (>99%) purity for extracts of quartz grains from sediment is pivotal for accurate OSL dating. Thus, the focus of this contribution is to provide detailed procedures for isolating highly purified quartz grain separates from a variety of polymineral sediments. This requires integration of knowledge of mineralogy, crystal chemistry; optical and Raman imaging, to effectively apply laboratory protocols, to render OSL ages on quartz grains from carefully sampled strata from retrieved sediment cores. The sediment cores were collected by a push and percussion coring method, which retrieved intact sediment down to a depth of 20-25 m.
The OSL time-sensitive signal is reset relatively rapidly with minutes to hours of sunlight exposure. The geological OSL signal accumulates from this solar reset level. Although, the OSL emissions of quartz are considerably variable, reflecting original crystalline structure, lattice impurities, sensitization with luminescence resetting cycles14 (Figure 1). Thus, there is inherent variability in the dose sensitivity of quartz, and dating protocols need to be devised for specific mineralogic and sedimentary provenance. Fortunately, the emergence of single aliquot regenerative (SAR) dose protocols for quartz1,2 yielded systematics to redress variability in the OSL emissions and metrics to evaluate laboratory changes in apparent OSL sensitivity. Sediment grains function as long-term radiation dosimeters when concealed from further light exposure, with the luminescence signal serving as a measure of radiation exposure during the burial period. The radiation dose that is equivalent to the natural luminescence emission of isolated quartz grains is referred to as the equivalent dose (De: in grays, Gy), which is the numerator of the OSL age equation (Equation 1). The denominator is the Dose rate (Dr: Grays/yr.), defined by contributing α, β, and γ radiation, originating from the radioactive decay of daughter isotopes in the 235U, 238U, 232Th decay series, 40K, and with lesser contributions from the decay of 85Rb and cosmic and galactic sources.
OSL age (yr) =
(Equation 1)
Where, Dα = alpha dose Dβ = beta dose Dγ = gamma dose Dc = cosmic dose and w=water attenuation factor.
Another method for U and Th determinations in the laboratory or the field is gamma spectrometry, with the Germanium variant able to quantify U and Th isotopic disequilibrium with suitable adjustments to the dose rate. The beta and gamma components of the environmental dose rate need to be modified for mass attenuation15. However, there is an effectively insignificant alpha dose for grains >50 µm with the outer 10-20 µm of grains removed by treatment with undiluted HF during preparation. A critical component in dose rate assessment is the quantification of the cosmic and galactic dose during the burial period, which is calculated for specific points on Earth with adjustments for longitude, latitude, elevation, burial depth, and density of overlying sediment16,17.
Sediments that contain >15% quartz are usually relatively straightforward for separating out a high purity quartz fraction. However, sediments with <15% quartz often require added time to ensure needed mineralogic purity for OSL dating. Approximately 500-1000 quartz grains are needed for this analysis, but often thousands of grains are separated for duplicate analyses, archiving to expand a calibration library, and future advancements. The mineralogic composition of sediment samples is initially assessed, grain by grain, by petrographic analysis through a binocular microscopic (10-20x) and associated imagine analysis. The mineralogy of individual grains is tested further by Raman spectroscopy to measure grain spectra using an excitation laser (455 nm, 532 nm, 633 nm, or 785 nm) and statistically compare grain emissions to known mineral spectra from the RRUFF System Database18.
Once the visual and spectral inspection is satisfactory, the purity of the OSL signal is further checked, utilizing an automated luminescence reader system. Three to five aliquots of the sample are exposed to infrared excitation (IR = 1.08 watts at 845 nm ± 4 nm), which preferentially stimulates feldspar minerals, and this emission is compared to emissions by blue light excitation (Bl = 470 nm ± 20 nm), which preferentially stimulates quartz. If the ratio IR/Bl ≥ 5%, the test indicates feldspar contamination and acid digestions are repeated. If the ratio IR/Bl <5%, then the samples are deemed quartz fraction satisfactorily for dating.
Single aliquot regeneration (SAR) protocols on quartz grains is an often-used approach in OSL dating sediments with procedures tailored for a specific sample, a study site, or an area. The reproducibility of these protocols is determined by giving quartz grains a known beta dose (e.g., 30 Gy) and evaluating what heat pretreatment recovers this known dose (Figure 2). In practice, determining a De with the SAR protocols involves the calculation of a ratio between the natural luminescence and the luminescence from a known test dose (Ln/Tn ratio), which is compared to the luminescence emissions for regenerative doses divided by the luminescence from the same test dose (Lx/Tx) (Figure 2). A correction, a consistently applied test-dose (e.g., 5 Gy), has been devised to compensate for quartz grain(s) sensitivity changes with measurement through SAR cycles. Often the OSL emissions increase by >5% with each successive SAR cycle, though given the same dose (e.g., 5 Gy)7.
At least forty aliquots of quartz or 500 grains are analyzed with TL/OSL reader system, with blue light excitation. The luminescence data generated is analyzed by software associated with the Risø TL/OSL-DA-20 reader system. The De and Dr values and age estimates are calculated using the Luminescence Dose and Age Calculator (LDAC)17. This platform applies statistical models to determine equivalent dose (De) values and render corresponding OSL age with constrained errors.
The extracted light-shielded sample from a core is prepared for two reasons: 1) To obtain a mineralogic fraction of quartz grains with a purity of >99%, and 2) To isolate grains of specific size fraction, e.g., 150-250 µm, for assessment of the environmental Dr for OSL dating17. In many sedimentary settings, quartz grains are common; but mixed with other silicate and non-silicate minerals, rock fragments, and organic matter. Previously, procedures were briefly outlined, indicating some specific steps and reagents needed to isolate pure quartz grains in the context of OSL dating 13,19,20,21,22,23. This contribution has benefited greatly from these previous approaches. This paper outlines revised, and more detailed protocols using petrographic imaging and Raman technology to monitor grain mineralogy and render highly pure (>99%) quartz extracts for luminescence dating. These quartz isolation protocols have been developed after preparing hundreds of samples from diverse geological environments in the Americas, Eurasia, China, and Africain, the Baylor Geoluminescence Dating Research Laboratory, reflecting analytical experience over thirty years, and are not definitive methods, with suitable variations used by other labs. These are not static protocols, and modifications and additions for improvement are welcomed.