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<feed xmlns="http://www.w3.org/2005/Atom">
        <title>GCHRON - recent papers</title>


    <link rel="self" href="https://gchron.copernicus.org/articles/"/>
    <id>https://gchron.copernicus.org/articles/</id>
    <updated>2026-09-12T22:17:18+02:00</updated>
    <author>
        <name>Copernicus Publications</name>
    </author>
        <entry>
            <id>https://doi.org/10.5194/gchron-8-511-2026</id>
            <title type="html">Challenges of initial Thorium and Approaches to Robust Speleothem Age Models: A case study from the Yucat&#225;n peninsula, Mexico
            </title>
            <link href="https://doi.org/10.5194/gchron-8-511-2026"/>
            <summary type="html">
                &lt;b&gt;Challenges of initial Thorium and Approaches to Robust Speleothem Age Models: A case study from the Yucatán peninsula, Mexico&lt;/b&gt;&lt;br&gt;
                Nils Schorndorf, Sophie F. Warken, René Eichstädter, Aaron S. Mielke, Jerónimo Avilés Olguín, Frank Keppler, Dominik Hennhöfer, Fátima Tec Pool, Carlos Evia, María José Gómez, Wolfgang Stinnesbeck, and Norbert Frank&lt;br&gt;
                    Geochronology, 8, 511&#8211;528, https://doi.org/10.5194/gchron-8-511-2026, 2026&lt;br&gt;
                To accurately understand past climate change, exact chronologies are fundamental. We dated multiple stalagmites from the Yucat&amp;#225;n Peninsula covering the last 2700 years. Because these cave deposits contain high and variable amounts of contaminating elements that distort age models, we developed a multi-method approach to correct the timelines. Our corrected records now provide a reliable foundation for future studies to track ancient droughts, floods, and their links to Maya cultural evolution.
            </summary>
            <content type="html">
                &lt;b&gt;Challenges of initial Thorium and Approaches to Robust Speleothem Age Models: A case study from the Yucatán peninsula, Mexico&lt;/b&gt;&lt;br&gt;
                Nils Schorndorf, Sophie F. Warken, René Eichstädter, Aaron S. Mielke, Jerónimo Avilés Olguín, Frank Keppler, Dominik Hennhöfer, Fátima Tec Pool, Carlos Evia, María José Gómez, Wolfgang Stinnesbeck, and Norbert Frank&lt;br&gt;
                    Geochronology, 8, 511&#8211;528, https://doi.org/10.5194/gchron-8-511-2026, 2026&lt;br&gt;
                <p>Speleothems, such as stalagmites and flowstones, are invaluable archives of past environmental and climatic conditions due to their layered growth and suitability for precise <span class="inline-formula"><sup>230</sup></span><span class="inline-formula"><math xmlns="http://www.w3.org/1998/Math/MathML" id="M2" display="inline" overflow="scroll" dspmath="mathml"><mrow class="chem"><mi mathvariant="normal">Th</mi><mo>/</mo><mi mathvariant="normal">U</mi></mrow></math><span><svg:svg xmlns:svg="http://www.w3.org/2000/svg" width="29pt" height="14pt" class="svg-formula" dspmath="mathimg" md5hash="3748d82bcf905ce41a9310a5e8003313"><svg:image xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="gchron-8-511-2026-ie00001.svg" width="29pt" height="14pt" src="gchron-8-511-2026-ie00001.png"/></svg:svg></span></span&gt; dating. In tropical karst settings, however, elevated and variable detrital thorium contamination can severely compromise age accuracy, especially for young speleothems. Here, a suite of stalagmites from &amp;#193;aktun K&amp;#243;opo' Cave from the Yucat&amp;#225;n Peninsula is used as a case study to develop and evaluate a multi-method framework for constraining initial thorium and constructing robust age&amp;#8211;depth models. We combine extensive <span class="inline-formula"><sup>230</sup></span><span class="inline-formula"><math xmlns="http://www.w3.org/1998/Math/MathML" id="M4" display="inline" overflow="scroll" dspmath="mathml"><mrow class="chem"><mi mathvariant="normal">Th</mi><mo>/</mo><mi mathvariant="normal">U</mi></mrow></math><span><svg:svg xmlns:svg="http://www.w3.org/2000/svg" width="29pt" height="14pt" class="svg-formula" dspmath="mathimg" md5hash="352b718fe3ebc7fffa1ff49cd58bb731"><svg:image xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="gchron-8-511-2026-ie00002.svg" width="29pt" height="14pt" src="gchron-8-511-2026-ie00002.png"/></svg:svg></span></span&gt; dating with local isochron analysis, stratigraphic approaches, and annual <span class="inline-formula"><math xmlns="http://www.w3.org/1998/Math/MathML" id="M5" display="inline" overflow="scroll" dspmath="mathml"><mrow class="chem"><mi mathvariant="normal">Sr</mi><mo>/</mo><mi mathvariant="normal">Ca</mi></mrow></math><span><svg:svg xmlns:svg="http://www.w3.org/2000/svg" width="33pt" height="14pt" class="svg-formula" dspmath="mathimg" md5hash="b9671c4809874f370bab27d3c7829fa1"><svg:image xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="gchron-8-511-2026-ie00003.svg" width="33pt" height="14pt" src="gchron-8-511-2026-ie00003.png"/></svg:svg></span></span&gt; layer counting to constrain elevated and initial (<span class="inline-formula"><math xmlns="http://www.w3.org/1998/Math/MathML" id="M6" display="inline" overflow="scroll" dspmath="mathml"><mrow class="chem"><msup><mi/><mn mathvariant="normal">230</mn></msup><mi mathvariant="normal">Th</mi><msup><mo>/</mo><mn mathvariant="normal">232</mn></msup><mi mathvariant="normal">Th</mi></mrow></math><span><svg:svg xmlns:svg="http://www.w3.org/2000/svg" width="61pt" height="15pt" class="svg-formula" dspmath="mathimg" md5hash="9846261e3d2e0ef9487c19af7c264f88"><svg:image xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="gchron-8-511-2026-ie00004.svg" width="61pt" height="15pt" src="gchron-8-511-2026-ie00004.png"/></svg:svg></span></span>) activity ratios and resolve pronounced chronological inversions. High uranium concentrations in the speleothems (average ca. 1&amp;#8201;ppm) allow precise measurements, yet we infer a high and largely unsystematic variability of high initial (<span class="inline-formula"><math xmlns="http://www.w3.org/1998/Math/MathML" id="M7" display="inline" overflow="scroll" dspmath="mathml"><mrow class="chem"><msup><mi/><mn mathvariant="normal">230</mn></msup><mi mathvariant="normal">Th</mi><msup><mo>/</mo><mn mathvariant="normal">232</mn></msup><mi mathvariant="normal">Th</mi></mrow></math><span><svg:svg xmlns:svg="http://www.w3.org/2000/svg" width="61pt" height="15pt" class="svg-formula" dspmath="mathimg" md5hash="c9737dd2eaac67c6418a5cd8a6debca4"><svg:image xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="gchron-8-511-2026-ie00005.svg" width="61pt" height="15pt" src="gchron-8-511-2026-ie00005.png"/></svg:svg></span></span>) activity ratios in space and time, with values spanning between 4 and 68, thus far exceeding standard bulk earth values. This variability demonstrates that elevated and temporally variable initial Th may be common in tropical karst settings and that multiple, independent constraints on initial (<span class="inline-formula"><math xmlns="http://www.w3.org/1998/Math/MathML" id="M8" display="inline" overflow="scroll" dspmath="mathml"><mrow class="chem"><msup><mi/><mn mathvariant="normal">230</mn></msup><mi mathvariant="normal">Th</mi><msup><mo>/</mo><mn mathvariant="normal">232</mn></msup><mi mathvariant="normal">Th</mi></mrow></math><span><svg:svg xmlns:svg="http://www.w3.org/2000/svg" width="61pt" height="15pt" class="svg-formula" dspmath="mathimg" md5hash="262d520a87d5867cb542558adedbc58c"><svg:image xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="gchron-8-511-2026-ie00006.svg" width="61pt" height="15pt" src="gchron-8-511-2026-ie00006.png"/></svg:svg></span></span>) activity ratios are essential for reliable chronologies in such environments. Applying this framework to &amp;#193;aktun K&amp;#243;opo' Cave stalagmites yields internally consistent stalagmite age&amp;#8211;depth models spanning the past 2.7&amp;#8201;kyr, as well as evidence for earlier glacial and interglacial growth phases. These chronologies provide the basis for high-resolution, multi-proxy reconstructions of climatic and environmental changes in the northeastern Yucat&amp;#225;n Peninsula during the entire era of Maya cultural evolution, and they illustrate how robust speleothem chronologies can be obtained even in cave systems affected by elevated and highly variable initial thorium.</p>
            </content>
            <author>
                <name>Copernicus Electronic Production Support Office</name>
            </author>
            <published>2026-09-11T22:17:17+02:00</published>
            <updated>2026-09-11T22:17:17+02:00</updated>
        </entry>
        <entry>
            <id>https://doi.org/10.5194/gchron-8-495-2026</id>
            <title type="html">U-Pb dating of sub-ng&#8201;g<sup>&#8722;1</sup>&#8201;U garnet by LA-MC-ICP-MS
            </title>
            <link href="https://doi.org/10.5194/gchron-8-495-2026"/>
            <summary type="html">
                &lt;b&gt;U-Pb dating of sub-ng g−1 U garnet by LA-MC-ICP-MS&lt;/b&gt;&lt;br&gt;
                Aratz Beranoaguirre, Leo J. Millonig, Richard Albert, Horst R. Marschall, and Axel Gerdes&lt;br&gt;
                    Geochronology, 8, 495&#8211;509, https://doi.org/10.5194/gchron-8-495-2026, 2026&lt;br&gt;
                <span data-path-to-node="1,0">We present a high-sensitivity laser ablation multi-collector inductively coupled plasma mass spectrometry (LA-MC-ICP-MS) method for in-situ U&amp;#8211;Pb dating of garnet with under 1 ng g&amp;#8315;&amp;#185; U</span><span data-path-to-node="1,2">. Using ion counters, geologically meaningful ages are obtained from garnets with up to three orders of magnitude less uranium than standard in-situ U&amp;#8211;Pb dating</span><span data-path-to-node="1,4">. This expands garnet petrochronology to low-U metamorphic rocks</span><span data-path-to-node="1,6">.</span>
            </summary>
            <content type="html">
                &lt;b&gt;U-Pb dating of sub-ng g−1 U garnet by LA-MC-ICP-MS&lt;/b&gt;&lt;br&gt;
                Aratz Beranoaguirre, Leo J. Millonig, Richard Albert, Horst R. Marschall, and Axel Gerdes&lt;br&gt;
                    Geochronology, 8, 495&#8211;509, https://doi.org/10.5194/gchron-8-495-2026, 2026&lt;br&gt;
                <p>Advances in laser ablation inductively coupled plasma mass spectrometry (LA-ICP-MS) have largely focused on improving spatial resolution through progressively smaller laser spot sizes. Here, we explore the opposite end of the analytical limits by investigating the lower concentration limits of in-situ <span class="inline-formula">U&amp;#8211;Pb</span>&amp;#160;geochronology in garnet. Using a Neptune Plus multi-collector ICP-MS equipped with seven ion counters, we developed an analytical workflow specifically designed for metamorphic garnet with ultra-low <span class="inline-formula">U</span>&amp;#160;concentrations (<span class="inline-formula"><</span>&amp;#8201;10&amp;#8201;<span class="inline-formula">ng&amp;#8201;g<sup>&amp;#8722;1</sup></span>). The method was used to date garnet from a wide range of ages and geological settings, including granulites, eclogites and hydrothermal demantoids. Uranium concentrations were exceptionally low, even below&amp;#160;1&amp;#8201;<span class="inline-formula">ng&amp;#8201;g<sup>&amp;#8722;1</sup></span&gt; in some cases. At these concentrations, the total amount of&amp;#160;<span class="inline-formula">U</span&gt; ablated during a single analysis is at femtogram levels, more than three orders of magnitude lower than that of a typical in-situ analysis of zircon. Despite these extremely low signal intensities, geologically meaningful ages were obtained for the analysed samples. Analytical precision depends on the&amp;#160;<span class="inline-formula">U</span&gt; and radiogenic <span class="inline-formula">Pb</span>&amp;#160;concentrations, but we have obtained precisions of ca.&amp;#160;5&amp;#8201;%&amp;#8211;6&amp;#8201;% for garnet containing less than&amp;#160;1&amp;#8201;<span class="inline-formula">ng&amp;#8201;g<sup>&amp;#8722;1</sup>&amp;#8201;&amp;#8201;U</span>. In garnet with higher <span class="inline-formula">U</span>&amp;#160;concentrations or ages as old as the Archean, internal precision of ca.&amp;#160;1&amp;#8201;% may be achieved. These results expand the applicability of in-situ garnet <span class="inline-formula">U-Pb</span>&amp;#160;geochronology to the vast majority of metamorphic garnet, providing a powerful new tool for constraining garnet growth, prograde metamorphism, and deep crustal evolution.</p>
            </content>
            <author>
                <name>Copernicus Electronic Production Support Office</name>
            </author>
            <published>2026-09-10T22:17:17+02:00</published>
            <updated>2026-09-10T22:17:17+02:00</updated>
        </entry>
        <entry>
            <id>https://doi.org/10.5194/gchron-8-463-2026</id>
            <title type="html">Uncertainty in helium diffusion in zircon limits thermochronologic resolution: application to the Great Unconformity
            </title>
            <link href="https://doi.org/10.5194/gchron-8-463-2026"/>
            <summary type="html">
                &lt;b&gt;Uncertainty in helium diffusion in zircon limits thermochronologic resolution: application to the Great Unconformity&lt;/b&gt;&lt;br&gt;
                Matthew Fox, Adam G. G. Smith, Pieter Vermeesch, Kerry Gallagher, and Andrew Carter&lt;br&gt;
                    Geochronology, 8, 463&#8211;474, https://doi.org/10.5194/gchron-8-463-2026, 2026&lt;br&gt;
                The ability to reconstruct thermal histories from thermochronometric data is determined by kinetic parameters. The Great Unconformity represents an enormous amount of time lost from the sedimentary record and has been explored with zircon (U&amp;#8211;Th)/He ages. Here we explore the uncertainty associated with the radiation damage model and show how this limits our ability to resolve the origin of the Great Unconformity.
            </summary>
            <content type="html">
                &lt;b&gt;Uncertainty in helium diffusion in zircon limits thermochronologic resolution: application to the Great Unconformity&lt;/b&gt;&lt;br&gt;
                Matthew Fox, Adam G. G. Smith, Pieter Vermeesch, Kerry Gallagher, and Andrew Carter&lt;br&gt;
                    Geochronology, 8, 463&#8211;474, https://doi.org/10.5194/gchron-8-463-2026, 2026&lt;br&gt;
                <p>Thermochronology provides a unique perspective on the timing and magnitude of erosion during the generation of unconformities. Recently, thermochronology has been used to reinvigorate a long-standing debate about the origin of the Great Unconformity, a geological feature representing a period of missing time of almost a billion&amp;#160;years from the stratigraphic record at the end of the Precambrian. Our ability to resolve thermal histories is fundamentally limited by how well we know parameters describing the temperature sensitivity of a thermochronometric system. The <span class="inline-formula">(U-Th)</span>/<span class="inline-formula">He</span&gt; in zircon system is particularly well suited to examine the origin of the Great Unconformity because it is very sensitive to long durations of time at relatively low temperatures (<span class="inline-formula"><</span>&amp;#8201;200&amp;#8211;250&amp;#8201;<span class="inline-formula">&amp;#176;C</span>). Here we determine uncertainties in the Zircon Radiation Damage and Annealing Model (ZRDAAM, Guenthner et&amp;#160;al. 2013) that describes changes in <span class="inline-formula"><sup>4</sup>He</span>&amp;#160;diffusion kinetics as a function of radiation damage accumulation and annealing. We show that the dispersion in predicted zircon <span class="inline-formula">(U-Th)</span>/<span class="inline-formula">He</span&gt; ages for a given thermal history can be 100's of&amp;#160;<span class="inline-formula">Ma</span&gt; for a specific amount of radiation damage highlighting that thermal histories are less well resolved than previously appreciated. Additional diffusion experiments and calibration with natural laboratories would provide better constraints on diffusion kinetic parameters.</p>
            </content>
            <author>
                <name>Copernicus Electronic Production Support Office</name>
            </author>
            <published>2026-08-27T22:17:17+02:00</published>
            <updated>2026-08-27T22:17:17+02:00</updated>
        </entry>
        <entry>
            <id>https://doi.org/10.5194/gchron-8-475-2026</id>
            <title type="html">Technical note: Disentangling pre- and post-depositional thermal histories in partially reset samples
            </title>
            <link href="https://doi.org/10.5194/gchron-8-475-2026"/>
            <summary type="html">
                &lt;b&gt;Technical note: Disentangling pre- and post-depositional thermal histories in partially reset samples&lt;/b&gt;&lt;br&gt;
                Birk P. Härtel, Eva Enkelmann, and Akeek Maitra&lt;br&gt;
                    Geochronology, 8, 475&#8211;494, https://doi.org/10.5194/gchron-8-475-2026, 2026&lt;br&gt;
                We present a new strategy for extracting information on the thermal history of sedimentary samples that lost part of their radiogenic helium during sediment burial. It uses combined U/Pb and (U-Th)/He dating of zircon to find grains that formed just before deposition and use them to model the basin thermal history. The model also estimates the time when the source rock of each grain cooled. We discuss the advantages and limitations of our approach and its application to other methods.
            </summary>
            <content type="html">
                &lt;b&gt;Technical note: Disentangling pre- and post-depositional thermal histories in partially reset samples&lt;/b&gt;&lt;br&gt;
                Birk P. Härtel, Eva Enkelmann, and Akeek Maitra&lt;br&gt;
                    Geochronology, 8, 475&#8211;494, https://doi.org/10.5194/gchron-8-475-2026, 2026&lt;br&gt;
                <p>Interpreting thermochronological data of a partially reset detrital sample is challenging because its age distribution reflects a mixture of each grain's individual pre-depositional and the shared post-depositional thermal history. A promising approach to meet this challenge is combined geo- and thermochronological dating on the same grains. We present an algorithm for disentangling the pre- and post-depositional thermal histories using data from zircon <span class="inline-formula"><math xmlns="http://www.w3.org/1998/Math/MathML" id="M1" display="inline" overflow="scroll" dspmath="mathml"><mrow class="chem"><mi mathvariant="normal">U</mi><mo>/</mo><mi mathvariant="normal">Pb</mi></mrow></math><span><svg:svg xmlns:svg="http://www.w3.org/2000/svg" width="30pt" height="14pt" class="svg-formula" dspmath="mathimg" md5hash="162ad8a7dbace0ccfbe34a90b6fdeeec"><svg:image xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="gchron-8-475-2026-ie00001.svg" width="30pt" height="14pt" src="gchron-8-475-2026-ie00001.png"/></svg:svg></span></span>&amp;#8211;(U-Th)&amp;#8201;<span class="inline-formula"><math xmlns="http://www.w3.org/1998/Math/MathML" id="M2" display="inline" overflow="scroll" dspmath="mathml"><mo>/</mo></math><span><svg:svg xmlns:svg="http://www.w3.org/2000/svg" width="8pt" height="14pt" class="svg-formula" dspmath="mathimg" md5hash="527256ea34e0af356380afd605ccefc0"><svg:image xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="gchron-8-475-2026-ie00002.svg" width="8pt" height="14pt" src="gchron-8-475-2026-ie00002.png"/></svg:svg></span></span>&amp;#8201;He double-dating. It differs from previous approaches in that it doesn't make any assumptions about the pre-depositional thermal histories of the grains in their source regions. First, we determine candidate post-depositional temperature-time paths by inverse thermal-history modeling of syn-depositional grains that crystallized at or near the time of deposition. We then calculate pre-depositional (U-Th)&amp;#8201;<span class="inline-formula"><math xmlns="http://www.w3.org/1998/Math/MathML" id="M3" display="inline" overflow="scroll" dspmath="mathml"><mo>/</mo></math><span><svg:svg xmlns:svg="http://www.w3.org/2000/svg" width="8pt" height="14pt" class="svg-formula" dspmath="mathimg" md5hash="e653eaf840568ee76bb20ba3bf368ae0"><svg:image xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="gchron-8-475-2026-ie00003.svg" width="8pt" height="14pt" src="gchron-8-475-2026-ie00003.png"/></svg:svg></span></span>&amp;#8201;He model ages for each candidate thermal history representing cooling of the grains in their source regions. Subsequently, we evaluate which post-depositional thermal histories are plausible using the likelihood of their pre-depositional model ages falling in the expected interval between the <span class="inline-formula"><math xmlns="http://www.w3.org/1998/Math/MathML" id="M4" display="inline" overflow="scroll" dspmath="mathml"><mrow class="chem"><mi mathvariant="normal">U</mi><mo>/</mo><mi mathvariant="normal">Pb</mi></mrow></math><span><svg:svg xmlns:svg="http://www.w3.org/2000/svg" width="30pt" height="14pt" class="svg-formula" dspmath="mathimg" md5hash="b6df6d06d8ca6b0a57c056132a5eac7f"><svg:image xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="gchron-8-475-2026-ie00004.svg" width="30pt" height="14pt" src="gchron-8-475-2026-ie00004.png"/></svg:svg></span></span&gt; crystallization ages of each grain and the time of sediment deposition. The final result is a selection of high-likelihood pairs of post-depositional thermal histories and pre-depositional ages. We illustrate this strategy by applying it to a Devonian sandstone from the Northern Canadian Cordillera. The results show the general agreement of the modeled thermal histories and pre-depositional (U-Th)&amp;#8201;<span class="inline-formula"><math xmlns="http://www.w3.org/1998/Math/MathML" id="M5" display="inline" overflow="scroll" dspmath="mathml"><mo>/</mo></math><span><svg:svg xmlns:svg="http://www.w3.org/2000/svg" width="8pt" height="14pt" class="svg-formula" dspmath="mathimg" md5hash="93e47eb16cb371fe6916d3191efc4f1d"><svg:image xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="gchron-8-475-2026-ie00005.svg" width="8pt" height="14pt" src="gchron-8-475-2026-ie00005.png"/></svg:svg></span></span>&amp;#8201;He ages with existing thermochronological data. The post-depositional thermal histories are also consistent with additional zircon-Raman thermochronological data from the same grains. We discuss the limitations of our approach imposed by the need for syn-depositional grains, its application to other thermochronometers, and how targeting rather than avoiding partially reset samples enhances our capability to extract thermal-history information from the detrital record. Finally, we introduce <i>PaRACAS</i>, the implementation of our approach in a <i>jupyter notebook</i&gt; that calculates, plots, and evaluates the pre-depositional zircon (U-Th)&amp;#8201;<span class="inline-formula"><math xmlns="http://www.w3.org/1998/Math/MathML" id="M6" display="inline" overflow="scroll" dspmath="mathml"><mo>/</mo></math><span><svg:svg xmlns:svg="http://www.w3.org/2000/svg" width="8pt" height="14pt" class="svg-formula" dspmath="mathimg" md5hash="073414a2b77546d8d5847ae97897d626"><svg:image xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="gchron-8-475-2026-ie00006.svg" width="8pt" height="14pt" src="gchron-8-475-2026-ie00006.png"/></svg:svg></span></span>&amp;#8201;He model ages for post-depositional temperature-time paths determined in HeFTy.</p>
            </content>
            <author>
                <name>Copernicus Electronic Production Support Office</name>
            </author>
            <published>2026-08-27T22:17:17+02:00</published>
            <updated>2026-08-27T22:17:17+02:00</updated>
        </entry>
        <entry>
            <id>https://doi.org/10.5194/gchron-8-447-2026</id>
            <title type="html">Technical note: Design, construction, automation, and first-principles calibration of a low volume He measurement line
            </title>
            <link href="https://doi.org/10.5194/gchron-8-447-2026"/>
            <summary type="html">
                &lt;b&gt;Technical note: Design, construction, automation, and first-principles calibration of a low volume He measurement line&lt;/b&gt;&lt;br&gt;
                James R. Metcalf and Rebecca M. Flowers&lt;br&gt;
                    Geochronology, 8, 447&#8211;462, https://doi.org/10.5194/gchron-8-447-2026, 2026&lt;br&gt;
                (U-Th)/He chronology requires measuring the absolute amount of radiogenic He in a sample. While high-quality commercial He lines are available, these machines are not always ideal for researchers interested in developing new or emerging techniques like laser ablation (U-Th)/He chronology. This manuscript describes the design, construction, automation, and calibration of a new He analysis line in the University of Colorado Thermochronology Research and Instrumentation Lab (CU TRaIL) facility that is optimized for measuring small amounts of He.
            </summary>
            <content type="html">
                &lt;b&gt;Technical note: Design, construction, automation, and first-principles calibration of a low volume He measurement line&lt;/b&gt;&lt;br&gt;
                James R. Metcalf and Rebecca M. Flowers&lt;br&gt;
                    Geochronology, 8, 447&#8211;462, https://doi.org/10.5194/gchron-8-447-2026, 2026&lt;br&gt;
                <p>A noble-gas analysis line capable of accurate and precise measurements of small absolute amounts of <span class="inline-formula"><sup>4</sup>He</span&gt; released from crystals is a key analytical step in the production of <span class="inline-formula"><math xmlns="http://www.w3.org/1998/Math/MathML" id="M2" display="inline" overflow="scroll" dspmath="mathml"><mrow><mo>(</mo><mrow class="chem"><mi mathvariant="normal">U</mi><mtext>-</mtext><mi mathvariant="normal">Th</mi></mrow><mo>)</mo><mo>/</mo><mrow class="chem"><mi mathvariant="normal">He</mi></mrow></mrow></math><span><svg:svg xmlns:svg="http://www.w3.org/2000/svg" width="54pt" height="14pt" class="svg-formula" dspmath="mathimg" md5hash="7940423aa274e18dfb3a22834ad475f0"><svg:image xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="gchron-8-447-2026-ie00001.svg" width="54pt" height="14pt" src="gchron-8-447-2026-ie00001.png"/></svg:svg></span></span&gt; chronologic data. <span class="inline-formula">He</span>&amp;#160;analysis lines that are custom-built in-house can be optimized for specific lab needs and facilitate continued maintenance, repair, and upgrades. However, there is little information in the published literature about the methods and approaches for building a <span class="inline-formula">He</span>&amp;#160;line. Here, we describe the design, construction, automation, and metrological calibration of a custom <span class="inline-formula"><sup>4</sup>He</span>&amp;#160;extraction and analysis line as part of establishing laser-ablation <span class="inline-formula"><math xmlns="http://www.w3.org/1998/Math/MathML" id="M6" display="inline" overflow="scroll" dspmath="mathml"><mrow><mo>(</mo><mrow class="chem"><mi mathvariant="normal">U</mi><mtext>-</mtext><mi mathvariant="normal">Th</mi></mrow><mo>)</mo><mo>/</mo><mrow class="chem"><mi mathvariant="normal">He</mi></mrow></mrow></math><span><svg:svg xmlns:svg="http://www.w3.org/2000/svg" width="54pt" height="14pt" class="svg-formula" dspmath="mathimg" md5hash="4f2aa12604ee6efe6ed90d08ed7a45bb"><svg:image xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="gchron-8-447-2026-ie00002.svg" width="54pt" height="14pt" src="gchron-8-447-2026-ie00002.png"/></svg:svg></span></span&gt; methods in the University of Colorado Thermochronology Research and Instrumentation Lab (CU&amp;#160;TRaIL). The line, called the Jimbochron, is designed to precisely measure very small (<span class="inline-formula">&amp;#8764;</span>&amp;#8201;<span class="inline-formula">fmol</span>) amounts of <span class="inline-formula"><sup>4</sup>He</span&gt; while being fully automated and easily modifiable in the future. These goals are achieved by minimizing the line volume, adopting a unique double-hexagonal manifold configuration, installing a high-sensitivity quadrupole mass spectrometer, and developing editable LabView code for instrument communication and automation that is straightforward to update. We also explain the steps used to calibrate the Jimbochron metrologically from first principles with a new in-house calibration volume to ensure high-accuracy <span class="inline-formula">He</span>&amp;#160;measurements. The Jimbochron accurately and precisely measures small gas amounts (<span class="inline-formula"><</span>&amp;#8201;0.1&amp;#8201;<span class="inline-formula">fmol</span>) and now routinely generates accurate and precise <span class="inline-formula">He</span&gt; data for laser-ablation <span class="inline-formula"><math xmlns="http://www.w3.org/1998/Math/MathML" id="M14" display="inline" overflow="scroll" dspmath="mathml"><mrow><mo>(</mo><mrow class="chem"><mi mathvariant="normal">U</mi><mtext>-</mtext><mi mathvariant="normal">Th</mi></mrow><mo>)</mo><mo>/</mo><mrow class="chem"><mi mathvariant="normal">He</mi></mrow></mrow></math><span><svg:svg xmlns:svg="http://www.w3.org/2000/svg" width="54pt" height="14pt" class="svg-formula" dspmath="mathimg" md5hash="63f1c7001b7026669cd5f5586ff784af"><svg:image xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="gchron-8-447-2026-ie00003.svg" width="54pt" height="14pt" src="gchron-8-447-2026-ie00003.png"/></svg:svg></span></span&gt; applications.</p>
            </content>
            <author>
                <name>Copernicus Electronic Production Support Office</name>
            </author>
            <published>2026-08-10T22:17:17+02:00</published>
            <updated>2026-08-10T22:17:17+02:00</updated>
        </entry>
        <entry>
            <id>https://doi.org/10.5194/gchron-8-423-2026</id>
            <title type="html">Simplified modeling of the impact of lithospheric-scale geological processes on thermal histories and low-temperature thermochronometers
            </title>
            <link href="https://doi.org/10.5194/gchron-8-423-2026"/>
            <summary type="html">
                &lt;b&gt;Simplified modeling of the impact of lithospheric-scale geological processes on thermal histories and low-temperature thermochronometers&lt;/b&gt;&lt;br&gt;
                Dawn A. Kellett and David M. Whipp&lt;br&gt;
                    Geochronology, 8, 423&#8211;445, https://doi.org/10.5194/gchron-8-423-2026, 2026&lt;br&gt;
                Geological processes like erosion, burial, and faulting can influence or perturb heat conditions in the Earth's crust through time, which can complicate our interpretation of the geological significance of rock cooling histories determined from thermochronology. This 1D modeling study quantifies and illustrates the expected relationships between various lithosphere-scale geological processes and resulting thermal histories and thermochronometer ages.
            </summary>
            <content type="html">
                &lt;b&gt;Simplified modeling of the impact of lithospheric-scale geological processes on thermal histories and low-temperature thermochronometers&lt;/b&gt;&lt;br&gt;
                Dawn A. Kellett and David M. Whipp&lt;br&gt;
                    Geochronology, 8, 423&#8211;445, https://doi.org/10.5194/gchron-8-423-2026, 2026&lt;br&gt;
                <p>Many geological processes influence or perturb the thermal state of the lithosphere. This presents a challenge for relating thermal history data modeled from thermochronometers such as apatite and zircon fission-track and (U&amp;#8211;Th)<span class="inline-formula"><math xmlns="http://www.w3.org/1998/Math/MathML" id="M1" display="inline" overflow="scroll" dspmath="mathml"><mo>/</mo></math><span><svg:svg xmlns:svg="http://www.w3.org/2000/svg" width="8pt" height="14pt" class="svg-formula" dspmath="mathimg" md5hash="1b4178c77ca0d4bfee6c9ddd864f3a43"><svg:image xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="gchron-8-423-2026-ie00001.svg" width="8pt" height="14pt" src="gchron-8-423-2026-ie00001.png"/></svg:svg></span></span>He dating, to geological evolution, a primary goal of many thermochronology studies. Here we address this challenge by exploring the thermal and thermochronological evolution of tracked rock parcels for a large set of 55&amp;#8211;50&amp;#8201;<span class="inline-formula">Ma</span&gt; 1D models that simulate key lithospheric geological processes, including erosional exhumation, sedimentary burial and exhumation, dip-slip faulting and delamination of the lithospheric mantle. We compare results from common depth history scenarios in which the Moho either experiences exhumation/burial or remains at a fixed depth balanced by crustal flux and erosion. Results show that Moho depth changes have a significant effect on thermal histories and thermochronometers, though this is not often considered in thermal history studies. Further, our results show that the recorded response of rock thermal histories/thermochronometers in the upper crust and geological processes that disrupt the crustal thermal field may be disassociated in time, because of the spatial origin, time and length scales of different heat transfer mechanisms. For example, a delamination event produces younger thermochronometer ages than an identical crustal exhumation history without delamination, but those young ages do not record the timing of delamination.</p>
            </content>
            <author>
                <name>Copernicus Electronic Production Support Office</name>
            </author>
            <published>2026-08-07T22:17:17+02:00</published>
            <updated>2026-08-07T22:17:17+02:00</updated>
        </entry>
        <entry>
            <id>https://doi.org/10.5194/gchron-8-387-2026</id>
            <title type="html">Dating circulations of hydrothermal fluids in the crystalline basements of unconformity-related metal deposits using in situ Rb&#8201;&#8725;&#8201;Sr geochronology: proof of concept
            </title>
            <link href="https://doi.org/10.5194/gchron-8-387-2026"/>
            <summary type="html">
                &lt;b&gt;Dating circulations of hydrothermal fluids in the crystalline basements of unconformity-related metal deposits using in situ Rb ∕ Sr geochronology: proof of concept&lt;/b&gt;&lt;br&gt;
                Quentin Boulogne, Gaétan Milesi, Chantal Peiffert, Emmy Fischer, Christophe Ballouard, Mehdi Serdoun, Thomas Obin, Andreï Lecomte, Pierre Martz, Andrew Kaczowka, and Julien Mercadier&lt;br&gt;
                    Geochronology, 8, 387&#8211;421, https://doi.org/10.5194/gchron-8-387-2026, 2026&lt;br&gt;
                This study investigates Rb&amp;#8211;Sr system behavior in hydrothermally altered muscovite using in-situ LA-ICP-MS/MS (Laser Ablation-Inductively Coupled Plasma-Tandem Mass Spectrometry) analyses from the Athabasca Basin. Unaltered muscovite records Paleoproterozoic crystallization ages, whereas muscovite altered to illite and sudoite yields a consistent age of ~1640 Ma, corresponding to alteration halos related to unconformity-type uranium deposits. These results highlight the potential of Rb&amp;#8211;Sr dating to constrain hydrothermal processes and fluid&amp;#8211;rock interactions.
            </summary>
            <content type="html">
                &lt;b&gt;Dating circulations of hydrothermal fluids in the crystalline basements of unconformity-related metal deposits using in situ Rb ∕ Sr geochronology: proof of concept&lt;/b&gt;&lt;br&gt;
                Quentin Boulogne, Gaétan Milesi, Chantal Peiffert, Emmy Fischer, Christophe Ballouard, Mehdi Serdoun, Thomas Obin, Andreï Lecomte, Pierre Martz, Andrew Kaczowka, and Julien Mercadier&lt;br&gt;
                    Geochronology, 8, 387&#8211;421, https://doi.org/10.5194/gchron-8-387-2026, 2026&lt;br&gt;
                <p>The use of  in situ Rb&amp;#8211;Sr geochronology has boomed in recent years following its implementation using LA-ICP-MS/MS technology, which enables fast,  in situ analyses at the micron scale on selected minerals. The Rb&amp;#8211;Sr geochronometer applied to micas is now commonly used to date the crystallization or cooling of metamorphic and magmatic rocks, based on the assumptions of a closed isotope system after passing the closure temperature and of a homogeneous Sr isotopic composition at the time of crystallization. In situ Rb&amp;#8211;Sr geochronology applied to micas and related alteration products in geological contexts involving hydrothermal fluid circulation affecting micas after crystallization could provide a new way to decipher the timing and duration of fluid circulation in various settings such as mountain belts or sedimentary basins. The behavior and applicability of the Rb&amp;#8211;Sr system in such contexts are, however, poorly understood, as the system may be partially reopened with differential redistribution of Rb and Sr at the grain scale. To test this hypothesis, we selected a case study related to unconformity-related U deposits from the Athabasca Basin (Canada), which formed through intense hydrothermal fluid circulation at the interface between crystalline basement and siliciclastic sedimentary rocks and represent archetypes of unconformity-related metal deposits. Muscovite grains from metamorphic and magmatic rocks were targeted across a range of alteration states, from hydrothermally unaltered to strongly altered domains. We focused on a specific hydrothermal alteration linked to the formation of hydrothermal illite and sudoite at the expense of metamorphic or magmatic minerals. In unaltered zones, muscovite displays variable but high Rb&amp;#8201;<span class="inline-formula"><math xmlns="http://www.w3.org/1998/Math/MathML" id="M2" display="inline" overflow="scroll" dspmath="mathml"><mo>/</mo></math><span><svg:svg xmlns:svg="http://www.w3.org/2000/svg" width="8pt" height="14pt" class="svg-formula" dspmath="mathimg" md5hash="527256ea34e0af356380afd605ccefc0"><svg:image xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="gchron-8-387-2026-ie00003.svg" width="8pt" height="14pt" src="gchron-8-387-2026-ie00003.png"/></svg:svg></span></span>&amp;#8201;Sr ratios, whereas the <span class="inline-formula"><sup>87</sup></span>Sr&amp;#8201;<span class="inline-formula"><math xmlns="http://www.w3.org/1998/Math/MathML" id="M4" display="inline" overflow="scroll" dspmath="mathml"><mo>/</mo></math><span><svg:svg xmlns:svg="http://www.w3.org/2000/svg" width="8pt" height="14pt" class="svg-formula" dspmath="mathimg" md5hash="57ee8123d9c9aefcf23d9c7f6463c158"><svg:image xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="gchron-8-387-2026-ie00004.svg" width="8pt" height="14pt" src="gchron-8-387-2026-ie00004.png"/></svg:svg></span></span>&amp;#8201;<span class="inline-formula"><sup>86</sup></span>Sr intercepts derived from Rb&amp;#8211;Sr regressions are scattered and are not interpreted as meaningful initial isotopic compositions. The resulting ages range from ca.&amp;#160;1870 to ca.&amp;#160;1720&amp;#8201;Ma and are consistent with the geological context. In distal-to-proximal alteration halos of U deposits, muscovite and related alteration products yield lower <span class="inline-formula"><sup>87</sup></span>Rb&amp;#8201;<span class="inline-formula"><math xmlns="http://www.w3.org/1998/Math/MathML" id="M7" display="inline" overflow="scroll" dspmath="mathml"><mo>/</mo></math><span><svg:svg xmlns:svg="http://www.w3.org/2000/svg" width="8pt" height="14pt" class="svg-formula" dspmath="mathimg" md5hash="36bd7baae116a5efc17e692d563c2b51"><svg:image xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="gchron-8-387-2026-ie00005.svg" width="8pt" height="14pt" src="gchron-8-387-2026-ie00005.png"/></svg:svg></span></span>&amp;#8201;<span class="inline-formula"><sup>86</sup></span>Sr ratios and highly variable regression intercepts. The mean age calculated across the different samples and investigated sites clusters around <span class="inline-formula">&amp;#8764;</span>&amp;#8201;1640&amp;#8201;Ma, a value previously obtained by Ar&amp;#8211;Ar geochronology on illite and U&amp;#8211;Pb geochronology on other hydrothermal phases and proposed to correspond to a major hydrothermal event linked to a geodynamic reorganization affecting the Canadian Shield at the circum-Laurentian scale. The <span class="inline-formula">&amp;#8764;</span>&amp;#8201;1640&amp;#8201;Ma age is geologically meaningful in the studied context and is interpreted as reflecting partial, micrometric-scale resetting of the Rb&amp;#8211;Sr system in muscovite during this hydrothermal event. The wide range of regression intercept values commonly observed in disturbed Rb&amp;#8211;Sr systems is interpreted as an apparent result of open-system behavior, reflecting partial system reopening and non-conservative redistribution of Rb and Sr at the grain scale, rather than as a physically meaningful initial isotopic composition. These results demonstrate that detailed analysis of Rb&amp;#8211;Sr system perturbations in<span id="page388"/&gt; altered muscovite and related alteration products can constrain the timing of ancient hydrothermal activity and the spatial dynamics of fluid-rock interaction. This approach provides a valuable complement to conventional fluid-tracing methods and opens new perspectives for reconstructing paleo-hydrothermal systems in ancient basement terrains.</p>
            </content>
            <author>
                <name>Copernicus Electronic Production Support Office</name>
            </author>
            <published>2026-07-08T22:17:17+02:00</published>
            <updated>2026-07-08T22:17:17+02:00</updated>
        </entry>
        <entry>
            <id>https://doi.org/10.5194/gchron-8-373-2026</id>
            <title type="html">Extraction of multiple ages from <i>c</i>-axis projected fission tracks
            </title>
            <link href="https://doi.org/10.5194/gchron-8-373-2026"/>
            <summary type="html">
                &lt;b&gt;Extraction of multiple ages from c-axis projected fission tracks&lt;/b&gt;&lt;br&gt;
                Peter K. Jensen&lt;br&gt;
                    Geochronology, 8, 373&#8211;386, https://doi.org/10.5194/gchron-8-373-2026, 2026&lt;br&gt;
                Natural fission of Uranium U-238 in minerals produce tracks in the crystal lattice. The density of tracks crossing the mineral surface is traditionally used together with the uranium concentration and the decay constant to calculate the age of fast-cooling minerals. A new equation is developed which includes the track length distribution of the tracks. It is then possible to age date the tracks as a function of their length. A detailed tectonic history of the minerals can then be derived.
            </summary>
            <content type="html">
                &lt;b&gt;Extraction of multiple ages from c-axis projected fission tracks&lt;/b&gt;&lt;br&gt;
                Peter K. Jensen&lt;br&gt;
                    Geochronology, 8, 373&#8211;386, https://doi.org/10.5194/gchron-8-373-2026, 2026&lt;br&gt;
                <p>It is generally accepted that the commonly used fission track age equation accurately calculates the cooling age for apatite minerals when the cooling rate is fast. Nevertheless, it is used when the cooling rate is gradual, for example when the age of transition through the partial annealing window is to be estimated. Added age information is here obtained by inclusion of the length distribution of fully included near horizontal tracks. The tendency that the shortest tracks are the oldest ones, and the longest ones are the youngest enables the age dating of a given track by counting the number of shorter tracks, adding one, and dividing by the volumetric track generation rate. The difficulty is that the track length&amp;#8211;age relation is blurred by the spread in lengths due to the inherent spread in fission decay energies, crystallographic anisotropy and observational uncertainties. The blurring can be reduced by mathematical deconvolution in which the blurring of tracks in annealing experiments is used. A previously given equation for the oldest track in each histogram column is mathematically further reduced. This paper presents a method where deblurring is first performed by projecting the observed track lengths on the mineral <span class="inline-formula"><i>c</i></span>-axis and then by deblurring using probabilistic least squares inversion. This leads to the extraction of several track ages with deviations for each deconvolved track length histogram. This information may be used to constrain the timing of tectonic events and provide the basis for calculation of past temperature.</p>
            </content>
            <author>
                <name>Copernicus Electronic Production Support Office</name>
            </author>
            <published>2026-06-12T22:17:17+02:00</published>
            <updated>2026-06-12T22:17:17+02:00</updated>
        </entry>
        <entry>
            <id>https://doi.org/10.5194/gchron-8-351-2026</id>
            <title type="html">Atmospheric <sup>10</sup>Be from Talos Dome (East Antarctic) ice core records geomagnetic dipole intensity from 170 to 270&#8201;ka&#8201;BP
            </title>
            <link href="https://doi.org/10.5194/gchron-8-351-2026"/>
            <summary type="html">
                &lt;b&gt;Atmospheric 10Be from Talos Dome (East Antarctic) ice core records geomagnetic dipole intensity from 170 to 270 ka BP&lt;/b&gt;&lt;br&gt;
                Alexis Lamothe, Edouard Bard, Nicolas Thouveny, Ellyn Auriol, Mirko Severi, Rita Traversi, Martine De Angelis, Frank Wilhelms, Robert Mulvaney, Fawzi Zaidi, Georges Aumaitre, Karim Keddadouche, and Mélanie Baroni&lt;br&gt;
                    Geochronology, 8, 351&#8211;371, https://doi.org/10.5194/gchron-8-351-2026, 2026&lt;br&gt;
                We studied changes in Earth's magnetic field between 170 000 and 270 000 years ago using beryllium data from Antarctic ice. Our results reveal three periods when the magnetic field weakened, including one major event with a rapid fall and gradual recovery. These findings help explain how Earth's magnetic field behaves during short-term disturbances and improve the timing of past climate and geological records.
            </summary>
            <content type="html">
                &lt;b&gt;Atmospheric 10Be from Talos Dome (East Antarctic) ice core records geomagnetic dipole intensity from 170 to 270 ka BP&lt;/b&gt;&lt;br&gt;
                Alexis Lamothe, Edouard Bard, Nicolas Thouveny, Ellyn Auriol, Mirko Severi, Rita Traversi, Martine De Angelis, Frank Wilhelms, Robert Mulvaney, Fawzi Zaidi, Georges Aumaitre, Karim Keddadouche, and Mélanie Baroni&lt;br&gt;
                    Geochronology, 8, 351&#8211;371, https://doi.org/10.5194/gchron-8-351-2026, 2026&lt;br&gt;
                <p>We present high-resolution <span class="inline-formula"><sup>10</sup>Be</span&gt; concentration and flux records from the Talos Dome ice core (East Antarctica), covering the period from 170 to 270&amp;#8201;ka&amp;#8201;BP, to assess the capacity of Antarctic ice cores to capture the dipole moment reductions triggered by geomagnetic excursions of different amplitudes. Three distinct geomagnetic events are identified in the <span class="inline-formula"><sup>10</sup>Be</span&gt; flux. The dipole collapse linked to the Iceland Basin Excursion (IBE) is clearly recorded as a <span class="inline-formula"><sup>10</sup>Be</span&gt; peak flux 1.59 to 2.08 times above background between (<span class="inline-formula">192.0&amp;#177;1.4</span>)&amp;#8201;ka&amp;#8201;BP and (<span class="inline-formula">185.6&amp;#177;1.4</span>)&amp;#8201;ka&amp;#8201;BP. A clear asymmetric structure is observed, with a rapid decline of the geomagnetic dipole, followed by a three-step recovery. Two dipole decreases of lower amplitude are also resolved in relation with the Pringle Falls Excursion (PFE), lasting from (<span class="inline-formula">218.5&amp;#177;1.90</span>) to (<span class="inline-formula">206.0&amp;#177;0.8</span>)&amp;#8201;ka&amp;#8201;BP, and the Mamaku Excursion (ME), identified at (<span class="inline-formula">242.0&amp;#177;0.3</span>)&amp;#8201;ka&amp;#8201;BP, both showing an increase of the <span class="inline-formula"><sup>10</sup>Be</span&gt; flux by a factor of 1.24 to 1.63. A total of 40 short-term <span class="inline-formula"><sup>10</sup>Be</span&gt; concentration minima were also identified and are consistently associated with peaks in major ion concentrations, indicating post-depositional effects that affect concentration but not the longer-term flux signal. Comparison with Dome Fuji ice core and oceanic authigenic <span class="inline-formula"><math xmlns="http://www.w3.org/1998/Math/MathML" id="M13" display="inline" overflow="scroll" dspmath="mathml"><mrow class="chem"><msup><mi/><mn mathvariant="normal">10</mn></msup><mi mathvariant="normal">Be</mi><msup><mo>/</mo><mn mathvariant="normal">9</mn></msup><mi mathvariant="normal">Be</mi></mrow></math><span><svg:svg xmlns:svg="http://www.w3.org/2000/svg" width="49pt" height="15pt" class="svg-formula" dspmath="mathimg" md5hash="98badc90db567271d49ab9be856e290e"><svg:image xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="gchron-8-351-2026-ie00001.svg" width="49pt" height="15pt" src="gchron-8-351-2026-ie00001.png"/></svg:svg></span></span&gt; records reveals strong agreement in the timing and structure of the dipole moment collapses linked with these excursions. These results further support the use of <span class="inline-formula"><sup>10</sup>Be</span&gt; for synchronizing ice and marine archives as well as to reconstruct past geomagnetic dipole moment variations and refining age models over the Pleistocene.</p>
            </content>
            <author>
                <name>Copernicus Electronic Production Support Office</name>
            </author>
            <published>2026-06-10T22:17:17+02:00</published>
            <updated>2026-06-10T22:17:17+02:00</updated>
        </entry>
        <entry>
            <id>https://doi.org/10.5194/gchron-8-329-2026</id>
            <title type="html">Testing current estimates of the in situ cosmogenic <sup>10</sup>Be production rate in the north-western British Isles, with implications for ice sheet behaviour during Termination 1
            </title>
            <link href="https://doi.org/10.5194/gchron-8-329-2026"/>
            <summary type="html">
                &lt;b&gt;Testing current estimates of the in situ cosmogenic 10Be production rate in the north-western British Isles, with implications for ice sheet behaviour during Termination 1&lt;/b&gt;&lt;br&gt;
                Gordon R. M. Bromley, Brenda L. Hall, Aaron E. Putnam, and Thomas V. Lowell&lt;br&gt;
                    Geochronology, 8, 329&#8211;349, https://doi.org/10.5194/gchron-8-329-2026, 2026&lt;br&gt;
                Cosmogenic surface-exposure dating relies on accurate constraint of nuclide production rates. To improve dating resolution, we compare <sup>10</sup>Be concentrations in deglacial surfaces in Scotland to local <sup>14</sup>C targets to test the performance of 8 production rates. Of these, the Rannoch Moor rate from central Scotland gives the best fit with the <sup>14</sup>C; others under-predict exposure age by up to 7 %. Our <sup>10</sup>Be record also shows retreat of the last ice sheet was disrupted by a brief pause ~16 200 years ago.
            </summary>
            <content type="html">
                &lt;b&gt;Testing current estimates of the in situ cosmogenic 10Be production rate in the north-western British Isles, with implications for ice sheet behaviour during Termination 1&lt;/b&gt;&lt;br&gt;
                Gordon R. M. Bromley, Brenda L. Hall, Aaron E. Putnam, and Thomas V. Lowell&lt;br&gt;
                    Geochronology, 8, 329&#8211;349, https://doi.org/10.5194/gchron-8-329-2026, 2026&lt;br&gt;
                <p>Cosmogenic nuclide surface-exposure dating (SED) is a rapidly growing tool in geoscience owing to its unrivalled potential for directly dating rock surfaces and thus the geomorphic and climatic events they represent. Fundamental to the efficacy of the SED method is reliable constraint of the in situ production rate, which is typically calculated via calibration experiments: cosmogenic nuclide concentrations are measured in surfaces for which the true exposure age is known independently, allowing the production rate to be derived (in atoms&amp;#8201;g<span class="inline-formula"><sup>&amp;#8722;1</sup></span>&amp;#8201;yr<span class="inline-formula"><sup>&amp;#8722;1</sup></span>) for the specific calibration site. This value can then be extrapolated to distal field sites using numerical scaling methods designed to account for spatial and elevational differences in geomagnetic and atmospheric shielding. Thanks to successive and increasingly co-ordinated calibration efforts, production rate estimates for the most widely used cosmogenic nuclide, beryllium-10 (<span class="inline-formula"><sup>10</sup></span>Be), have improved in recent decades, with the majority converging on sea-level high-latitude (SLHL) values of <span class="inline-formula">&amp;#8764;</span>&amp;#8201;3.8&amp;#8211;4.1&amp;#8201;atoms&amp;#8201;g<span class="inline-formula"><sup>&amp;#8722;1</sup></span>&amp;#8201;yr<span class="inline-formula"><sup>&amp;#8722;1</sup></span&gt; (&amp;#8220;St&amp;#8221; scaling). Nonetheless, there remains sufficient variability among production rates to undermine the reliability of derived surface-exposure ages, particularly for applications to short-lived events such as the abrupt climate shifts of the last glacial termination. To help address this uncertainty, this paper reports new <span class="inline-formula"><sup>10</sup></span>Be concentrations from deglacial surfaces on the Redpoint Peninsula in north-west Scotland that were exposed during retreat of the last British ice sheet. By comparing the surface-exposure results from eight current <span class="inline-formula"><sup>10</sup></span>Be production rates to local radiocarbon constraint for deglaciation, we (1) evaluate the viability of each production rate for this site and (2) report a maximum SLHL value of 3.925&amp;#8201;<span class="inline-formula">&amp;#177;</span>&amp;#8201;0.07&amp;#8201;atoms&amp;#8201;g<span class="inline-formula"><sup>&amp;#8722;1</sup></span>&amp;#8201;yr<span class="inline-formula"><sup>&amp;#8722;1</sup></span&gt; (&amp;#8220;St&amp;#8221; scaling), above which resulting surface-exposure ages will be too young with respect to the Redpoint radiocarbon chronology. This study also demonstrates that the Rannoch Moor <span class="inline-formula"><sup>10</sup></span>Be production rate, calibrated against independently dated glacial landforms in the central Scottish Highlands, gives the best match with the <span class="inline-formula"><sup>14</sup></span>C control and thus is appropriate for Late Pleistocene applications at these geomagnetic latitudes.</p>
            </content>
            <author>
                <name>Copernicus Electronic Production Support Office</name>
            </author>
            <published>2026-06-05T22:17:18+02:00</published>
            <updated>2026-06-05T22:17:18+02:00</updated>
        </entry>
        <entry>
            <id>https://doi.org/10.5194/gchron-8-313-2026</id>
            <title type="html">Response of the Rb&#8211;Sr system in biotite during contact metamorphism in the aureole of the Makhavinekh Lake Pluton, Labrador
            </title>
            <link href="https://doi.org/10.5194/gchron-8-313-2026"/>
            <summary type="html">
                &lt;b&gt;Response of the Rb–Sr system in biotite during contact metamorphism in the aureole of the Makhavinekh Lake Pluton, Labrador&lt;/b&gt;&lt;br&gt;
                Christopher R. M. McFarlane&lt;br&gt;
                    Geochronology, 8, 313&#8211;327, https://doi.org/10.5194/gchron-8-313-2026, 2026&lt;br&gt;
                The mineral biotite is a common rock-forming mineral and notable for its ability to incorporate Rb into its structure. Microanalytical tools such a laser ablation and tandem mass spectrometry, allows Rb-Sr biotite dating with context preserved. This study reveals Sr mobility that is controlled by location in a rock. Reconstructing the timing of geological events using biotite Rb-Sr geochronology is, therefore, contingent on grain-scale evaluation of biotite textures.
            </summary>
            <content type="html">
                &lt;b&gt;Response of the Rb–Sr system in biotite during contact metamorphism in the aureole of the Makhavinekh Lake Pluton, Labrador&lt;/b&gt;&lt;br&gt;
                Christopher R. M. McFarlane&lt;br&gt;
                    Geochronology, 8, 313&#8211;327, https://doi.org/10.5194/gchron-8-313-2026, 2026&lt;br&gt;
                <p>High-temperature contact metamorphism in the aureole of the 1322&amp;#8201;Ma Makhavinekh Lake Pluton, Labrador, led to progressive consumption of 1850&amp;#8201;Ma garnet formed during upper-amphibolite facies regional metamorphism that produced migmatitic paragneiss (Tasiyuak Gneiss). Biotite Rb&amp;#8211;Sr isotope measurements were carried out in situ by laser ablation ICP-MS/MS allowing biotite in a variety of textural settings to be characterized. This natural laboratory provides important information about the nature of Rb&amp;#8211;Sr closure temperature (<span class="inline-formula"><i>T</i><sub>c</sub></span>) as a function of textural setting in high-grade metamorphic rocks. Intact biotite inclusions armoured in garnet preserved in the outer aureole (<span class="inline-formula">>4</span>&amp;#8201;km from the contact) display a range of Rb&amp;#8211;Sr isochron ages between <span class="inline-formula">&amp;#8764;1850</span&gt; and <span class="inline-formula">&amp;#8764;1322</span>&amp;#8201;Ma consistent with a zone of partial retention of Sr in biotite. Isotopic resetting in the outer aureole was controlled by microfractures in garnet that provided short-circuit diffusion pathways for redistribution of radiogenic Sr into plagioclase-bearing contact metamorphic assemblages; biotite inclusions isolated from microfractures retain 1850&amp;#8201;Ma Rb&amp;#8211;Sr isochron ages. Biotite grains falling along a <span class="inline-formula">&amp;#8764;1322</span>&amp;#8201;Ma isochron attest to efficient intra- and intercrystalline Sr diffusion at <span class="inline-formula"><i>T</i>&amp;#8805;500</span>&amp;#8201;<span class="inline-formula">&amp;#176;C</span&gt; on timescales of <span class="inline-formula">&amp;#8805;5</span>&amp;#8201;Myr. Samples in the central part of the contact aureole (3.7 to 1.1&amp;#8201;km from the contact) contain partly resorbed biotite surrounded by contact metamorphic Opx&amp;#8201;<span class="inline-formula">+</span>&amp;#8201;Crd coronal assemblages in addition to armoured inclusions in relict garnet. These display similar Rb&amp;#8211;Sr behaviour to outer aureole samples with the exception that <span class="inline-formula">&amp;#8764;1322</span>&amp;#8201;Ma biotite domains display higher <span class="inline-formula"><math xmlns="http://www.w3.org/1998/Math/MathML" id="M11" display="inline" overflow="scroll" dspmath="mathml"><mrow class="chem"><mi mathvariant="normal">Rb</mi><mo>/</mo><mi mathvariant="normal">Sr</mi></mrow></math><span><svg:svg xmlns:svg="http://www.w3.org/2000/svg" width="33pt" height="14pt" class="svg-formula" dspmath="mathimg" md5hash="d6acbcfb25563844829884b3cf6cdddf"><svg:image xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="gchron-8-313-2026-ie00001.svg" width="33pt" height="14pt" src="gchron-8-313-2026-ie00001.png"/></svg:svg></span></span&gt; due to more extreme loss of Sr. In the inner aureole, where garnet was completely consumed by contact metamorphic assemblages, a new generation of biotite neoblasts grew textural equilibrium with Opx&amp;#8201;<span class="inline-formula">+</span>&amp;#8201;Crd. This biotite preserves Rb&amp;#8211;Sr ages <span class="inline-formula">&amp;#8804;1322</span>&amp;#8201;Ma with initial <span class="inline-formula"><math xmlns="http://www.w3.org/1998/Math/MathML" id="M14" display="inline" overflow="scroll" dspmath="mathml"><mrow class="chem"><msup><mi/><mn mathvariant="normal">87</mn></msup><mi mathvariant="normal">Sr</mi><msup><mo>/</mo><mn mathvariant="normal">86</mn></msup><mi mathvariant="normal">Sr</mi></mrow></math><span><svg:svg xmlns:svg="http://www.w3.org/2000/svg" width="49pt" height="15pt" class="svg-formula" dspmath="mathimg" md5hash="b15b20bdf743f7fd52e15b626449e320"><svg:image xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="gchron-8-313-2026-ie00002.svg" width="49pt" height="15pt" src="gchron-8-313-2026-ie00002.png"/></svg:svg></span></span&gt; best interpreted as a mixture of radiogenic Sr accumulated in regional biotite and whole-rock Sr liberated from low-<span class="inline-formula"><math xmlns="http://www.w3.org/1998/Math/MathML" id="M15" display="inline" overflow="scroll" dspmath="mathml"><mrow class="chem"><mi mathvariant="normal">Rb</mi><mo>/</mo><mi mathvariant="normal">Sr</mi></mrow></math><span><svg:svg xmlns:svg="http://www.w3.org/2000/svg" width="33pt" height="14pt" class="svg-formula" dspmath="mathimg" md5hash="d95450951ff259f3fe6ec539c7983b44"><svg:image xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="gchron-8-313-2026-ie00003.svg" width="33pt" height="14pt" src="gchron-8-313-2026-ie00003.png"/></svg:svg></span></span&gt; regional metamorphic garnet, apatite, and plagioclase. This study reveals how the exact textural setting of biotite in high-grade metamorphic rocks influences the preservation of Rb&amp;#8211;Sr ages and demonstrates that there is no universal closure temperature for biotite Rb&amp;#8211;Sr. It also reveals that in situ Rb&amp;#8211;Sr dating of granulite-facies rocks might provide robust chronometric data if grains isolated from intergranular diffusion are systematically evaluated to reveal zones of partial retention.</p>
            </content>
            <author>
                <name>Copernicus Electronic Production Support Office</name>
            </author>
            <published>2026-05-28T22:17:18+02:00</published>
            <updated>2026-05-28T22:17:18+02:00</updated>
        </entry>
        <entry>
            <id>https://doi.org/10.5194/gchron-8-297-2026</id>
            <title type="html">Novel insights into the post-IR IRSL<sub>200</sub> signal bleachability of single-grain K-feldspars in fluvial modern analogues  from the Southern Central Andes, Chile
            </title>
            <link href="https://doi.org/10.5194/gchron-8-297-2026"/>
            <summary type="html">
                &lt;b&gt;Novel insights into the post-IR IRSL200 signal bleachability of single-grain K-feldspars in fluvial modern analogues  from the Southern Central Andes, Chile&lt;/b&gt;&lt;br&gt;
                Arindam Biswas, Svenja Riedesel, Louise Karman-Besson, Max Hellers, Anne Guyez, Stéphane Bonnet, and Tony Reimann&lt;br&gt;
                    Geochronology, 8, 297&#8211;312, https://doi.org/10.5194/gchron-8-297-2026, 2026&lt;br&gt;
                We evaluate luminescence signal resetting in single-grain K-feldspar from modern fluvial analogues in Chile. Our results show a uniform sample-average bleaching trend but strong grain-scale variability. Residual doses are independent of feldspar geochemistry and catchment lithology but scale with natural dose. Taken together, these findings refine palaeodose correction strategies and support defining sample&amp;#8209;specific bleaching thresholds for luminescence&amp;#8209;based sediment tracing.
            </summary>
            <content type="html">
                &lt;b&gt;Novel insights into the post-IR IRSL200 signal bleachability of single-grain K-feldspars in fluvial modern analogues  from the Southern Central Andes, Chile&lt;/b&gt;&lt;br&gt;
                Arindam Biswas, Svenja Riedesel, Louise Karman-Besson, Max Hellers, Anne Guyez, Stéphane Bonnet, and Tony Reimann&lt;br&gt;
                    Geochronology, 8, 297&#8211;312, https://doi.org/10.5194/gchron-8-297-2026, 2026&lt;br&gt;
                <p>Post-infrared infrared stimulated luminescence (post-IR IRSL) signals from potassium feldspars are gaining prominence in both luminescence dating and luminescence-based sediment tracing techniques. To enhance the accuracy and reliability of these applications, it is essential to develop a comprehensive understanding of how post-IR IRSL signals undergo bleaching. While previous studies have explored post-IR IRSL bleachability using multi-grain approaches, a systematic single-grain investigation on modern analogues has not been conducted. In this study, we examined the bleaching behaviour of the post-infrared infrared stimulated luminescence signal measured at 200&amp;#8201;&amp;#176;C (post-IR IRSL<span class="inline-formula"><sub>200</sub></span>) at the single-grain level in eleven modern floodplain samples from the tectonically active Southern Central Andes. Our study demonstrated considerable variation in the residual doses following 2&amp;#8201;d of laboratory solar simulator bleaching across the sample set. This variability was evident not only between different samples but also among individual grains within the same sample. Thus, we evaluated the influence of bleaching duration, grain-specific geochemical composition, catchment-scale lithological variability, and the size of the natural dose on the laboratory-measured residual doses.</p&gt;        <p>Our laboratory bleaching experiments in which single grains were given a fixed regenerated dose of 30&amp;#8201;Gy  prior to solar simulator exposure showed similar post-IR IRSL<span class="inline-formula"><sub>200</sub></span&gt; signal bleaching behaviour across four different samples, reaching a plateau based on normalised luminescence signal after 2&amp;#8201;d of exposure to solar simulator light. While individual grains exhibited a wide range of bleaching rates, this variability did not account for the spread in residual dose values. Notably, extended light exposure reduced variability in signal intensity, underscoring its role in dose homogenisation. Geochemical analysis of major oxides showed no significant correlation with either residual dose magnitude or bleaching rate, suggesting that mineral composition (including K-concentration) does not influence bleaching efficiency at the individual grain level. Furthermore, bleaching behaviour remained consistent across samples regardless of catchment lithology, with no discernible relationship between lithological units and remnant dose (defined as the natural dose remaining at the time of deposition and burial) or residual dose values. Most importantly, we identified a strong positive linear correlation (<span class="inline-formula"><i>R</i><sup>2</sup>=</span>&amp;#8201;0.89) between residual dose and natural remnant dose, revealing dose-dependent bleaching efficiency and the presence of a negligible unbleachable component at the time of deposition. This relationship between residual dose and natural remnant dose also suggests that while the youngest samples (with low natural remnant dose) could reach zero residual dose, the relatively older samples (with more than 10&amp;#8201;Gy of natural remnant dose) could show a significant amount of residual dose. By integrating insights on bleachability with the information on the unbleachable component and remnant doses derived from modern analogues, we highlight the limitations of correcting palaeodoses by directly using either residual or remnant doses and evaluate three context-sensitive correction strategies. Finally,<span id="page298"/&gt; we discuss how residual doses can be leveraged to more reliably identify well-bleached grains, enhancing the accuracy of luminescence-based sediment tracing applications.</p>
            </content>
            <author>
                <name>Copernicus Electronic Production Support Office</name>
            </author>
            <published>2026-05-27T22:17:18+02:00</published>
            <updated>2026-05-27T22:17:18+02:00</updated>
        </entry>
        <entry>
            <id>https://doi.org/10.5194/gchron-8-279-2026</id>
            <title type="html"><sup>40</sup>Ar&#8201;&#8725;&#8201;<sup>39</sup>Ar constraints on the eruption history of the Christiana Volcano of the Christiana-Santorini-Kolumbo volcanic field, Greece
            </title>
            <link href="https://doi.org/10.5194/gchron-8-279-2026"/>
            <summary type="html">
                &lt;b&gt;40Ar ∕ 39Ar constraints on the eruption history of the Christiana Volcano of the Christiana-Santorini-Kolumbo volcanic field, Greece&lt;/b&gt;&lt;br&gt;
                Pieter Z. Vroon, Teun Beemster, Xiaolong Zhou, Paraskevi Nomikou, Martijn Klaver, Jan R. Wijbrans, and Klaudia F. Kuiper&lt;br&gt;
                    Geochronology, 8, 279&#8211;295, https://doi.org/10.5194/gchron-8-279-2026, 2026&lt;br&gt;
                The Christiana Islands represents the oldest subaerial volcanism in the Christiana-Santorini-Kolombo volcanic field, but the exact age of this volcano has been unknown. This study reports new <sup>40</sup>Ar/<sup>39</sup>Ar ages of ten volcanic samples from Christiana Island that cluster between 2.5&amp;#8211;2.7 Ma with small uncertainties (0.02&amp;#8211;0.14 Ma). One sample dated much younger: 133 ka; this is most likely derived from the Middle Pumice Plinian eruption of Santorini.
            </summary>
            <content type="html">
                &lt;b&gt;40Ar ∕ 39Ar constraints on the eruption history of the Christiana Volcano of the Christiana-Santorini-Kolumbo volcanic field, Greece&lt;/b&gt;&lt;br&gt;
                Pieter Z. Vroon, Teun Beemster, Xiaolong Zhou, Paraskevi Nomikou, Martijn Klaver, Jan R. Wijbrans, and Klaudia F. Kuiper&lt;br&gt;
                    Geochronology, 8, 279&#8211;295, https://doi.org/10.5194/gchron-8-279-2026, 2026&lt;br&gt;
                <p>The Christiana Islands group consists of three at present uninhabited islands 20&amp;#8201;km SW of Santorini, Aegean Sea, Greece, that are the subaerial remnants of the Christiana volcano. The age of the Christiana Islands has been unclear and has been previously assumed to have started around the same time as the emergence of Santorini (600&amp;#8201;ka). Other studies, based on seismic reflection, have correlated volcanic deposits of the Christiana archipelago to Pliocene sedimentary layers. Five subaerial Christiana volcanic rocks of the Upper Lava formation cluster tightly between  2.57&amp;#8211;2.69&amp;#8201;Ma with relatively small uncertainties (0.02&amp;#8211;0.03&amp;#8201;Ma). One sample dated much younger: 133&amp;#8201;ka; this obsidian from a pyroclastic deposit is most likely derived from the Middle Pumice Plinian eruption of Santorini. The 2.5&amp;#8211;2.7&amp;#8201;Ma age for Christiana volcano shows that all volcanic fields of the South Aegean Volcanic Arc (SAVA) were active around 3&amp;#8201;Ma ago and started when oceanic crust arrived at 100&amp;#8201;km depth below the SAVA volcanic fields after a long period of continental lithosphere subduction. The Christiana volcano was constructed when the local stress field showed NNE-SSW extension. During the transition from NNE-SSW to NW-SE extension the Christiana volcano became extinct and a period of <span class="inline-formula">>1.0</span>&amp;#8201;Ma with volcanic quiescence and/or low volcanic output followed until the start of submarine volcano Poseidon and present-day volcanic centres Santorini and Kolumbo.</p>
            </content>
            <author>
                <name>Copernicus Electronic Production Support Office</name>
            </author>
            <published>2026-05-27T22:17:18+02:00</published>
            <updated>2026-05-27T22:17:18+02:00</updated>
        </entry>
        <entry>
            <id>https://doi.org/10.5194/gchron-8-255-2026</id>
            <title type="html">Paired <sup>14</sup>C&#8211;<sup>10</sup>Be exposure ages from Mount Murphy, West Antarctica: Implications for accurate and precise deglacial chronologies
            </title>
            <link href="https://doi.org/10.5194/gchron-8-255-2026"/>
            <summary type="html">
                &lt;b&gt;Paired 14C–10Be exposure ages from Mount Murphy, West Antarctica: Implications for accurate and precise deglacial chronologies&lt;/b&gt;&lt;br&gt;
                Jonathan R. Adams, Dylan H. Rood, Klaus Wilcken, Stephen J. Roberts, and Joanne S. Johnson&lt;br&gt;
                    Geochronology, 8, 255&#8211;277, https://doi.org/10.5194/gchron-8-255-2026, 2026&lt;br&gt;
                Ice sheet mass loss is adding to sea-level rise, and is expected to increase, but by how much and how fast remains uncertain. Isotopes produced in rock at the Earth&amp;#8217;s surface provide records of past ice sheet thinning which help predict future change but are more effective if they are precise enough to determine past changes to the nearest thousand years. Carbon-14 is a unique isotope that provides an accurate record of past change since the last ice age, however, its precision can be improved.
            </summary>
            <content type="html">
                &lt;b&gt;Paired 14C–10Be exposure ages from Mount Murphy, West Antarctica: Implications for accurate and precise deglacial chronologies&lt;/b&gt;&lt;br&gt;
                Jonathan R. Adams, Dylan H. Rood, Klaus Wilcken, Stephen J. Roberts, and Joanne S. Johnson&lt;br&gt;
                    Geochronology, 8, 255&#8211;277, https://doi.org/10.5194/gchron-8-255-2026, 2026&lt;br&gt;
                <p>Cosmogenic-nuclide surface exposure ages provide empirical data for validating models simulating the timing and pace of ice-sheet response to a warming climate. Increasing emphasis is being placed on obtaining exposure ages that both accurately constrain Holocene deglaciation and are precise enough to capture ice sheet change at the sub-millennial scale. However, longer-lived nuclides such as <span class="inline-formula"><sup>10</sup>Be</span&gt; are susceptible to cosmogenic nuclide inheritance often persisting through multiple periods of exposure and burial, which can impact the accuracy of the most recent Holocene exposure history. Shorter-lived in situ cosmogenic <span class="inline-formula"><sup>14</sup>C</span&gt; (in situ <span class="inline-formula"><sup>14</sup>C</span>) is largely insensitive to nuclide inheritance pre-dating the last glacial maximum (LGM), and when combined with longer-lived nuclides can be used to constrain complex ice sheet histories over Holocene timescales. Here, we present new in situ <span class="inline-formula"><sup>14</sup>C</span&gt; exposure ages from nine erratic cobbles from Mount Murphy, West Antarctica. Six of these suggest Mt Murphy deglaciated from 5&amp;#8211;3&amp;#8201;ka; this is inconsistent with previously measured <span class="inline-formula"><sup>10</sup>Be</span&gt; ages of the same samples that place deglaciation from 8&amp;#8211;6&amp;#8201;ka. We investigate potential explanations for the conflicting exposure histories by analysing paired <span class="inline-formula"><sup>14</sup>C</span>&amp;#8211;<span class="inline-formula"><sup>10</sup>Be</span&gt; data of Holocene age presently archived in the informal cosmogenic-nuclide exposure-age database (ICE-D, <span class="uri">https://version2.ice-d.org/</span>,  last access: 29&amp;#160;March&amp;#160;2024). Our analysis reveals that neither variations in geologic setting nor modelled scenarios of subsurface nuclide production can explain the conflicting Mt Murphy ages. However, replicate in situ <span class="inline-formula"><sup>14</sup>C</span&gt; measurements indicate that initial in situ <span class="inline-formula"><sup>14</sup>C</span&gt; concentrations used to calculate the youngest exposure ages (5&amp;#8211;3&amp;#8201;ka) do not reproduce within stated <span class="inline-formula">2<i>&amp;#963;</i></span&gt; uncertainty, whereas measurements used to calculate the older ages (8&amp;#8211;6&amp;#8201;ka) are reproducible. Furthermore, we observe that in situ <span class="inline-formula"><sup>14</sup>C</span&gt; concentrations measured in 15 of 31 samples taken from ICE-D do not replicate within their nominal <span class="inline-formula">2<i>&amp;#963;</i></span&gt; analytical uncertainty. Together, these results suggest that analytical uncertainty for in situ <span class="inline-formula"><sup>14</sup>C</span&gt; measurements may currently be underestimated. We provide recommendations for improving measurement precision that will benefit future Holocene deglaciation studies, including analysis and publication of more replicate measurements and the continuation of efforts to quantify and minimise sources of scatter in blank measurements.</p>
            </content>
            <author>
                <name>Copernicus Electronic Production Support Office</name>
            </author>
            <published>2026-05-05T22:17:18+02:00</published>
            <updated>2026-05-05T22:17:18+02:00</updated>
        </entry>
        <entry>
            <id>https://doi.org/10.5194/gchron-8-223-2026</id>
            <title type="html">Dating Late Pleistocene pluvial lake shorelines in the Great Basin, USA using rock surface luminescence dating techniques: developing new approaches for challenging lithologies
            </title>
            <link href="https://doi.org/10.5194/gchron-8-223-2026"/>
            <summary type="html">
                &lt;b&gt;Dating Late Pleistocene pluvial lake shorelines in the Great Basin, USA using rock surface luminescence dating techniques: developing new approaches for challenging lithologies&lt;/b&gt;&lt;br&gt;
                Christina M. Neudorf, Teresa Wriston, Geraint T. H. Jenkins, and Sebastien Huot&lt;br&gt;
                    Geochronology, 8, 223&#8211;253, https://doi.org/10.5194/gchron-8-223-2026, 2026&lt;br&gt;
                This study examines the feasibility of dating beach ridges associated with pluvial lake highstands in the Great Basin, USA, using rock surface luminescence dating techniques. Limestone and volcanic rock lithologies prominent in this region pose challenges, but preliminary measurements show promise. We show that ages derived from beach ridge gravel rocks record the timing of lake highstands as well as climatically driven soil formation processes.
            </summary>
            <content type="html">
                &lt;b&gt;Dating Late Pleistocene pluvial lake shorelines in the Great Basin, USA using rock surface luminescence dating techniques: developing new approaches for challenging lithologies&lt;/b&gt;&lt;br&gt;
                Christina M. Neudorf, Teresa Wriston, Geraint T. H. Jenkins, and Sebastien Huot&lt;br&gt;
                    Geochronology, 8, 223&#8211;253, https://doi.org/10.5194/gchron-8-223-2026, 2026&lt;br&gt;
                <p>This study examines the feasibility of dating pluvial lake beach ridges using rock surface luminescence dating techniques. Dating pluvial lake highstands in the internally drained Great Basin of the United States helps us understand the timing of changes in precipitation and temperature patterns in western North America during the Late Pleistocene. The majority of highstand ages have relied on few radiocarbon ages of shell and/or charcoal sometimes coupled with luminescence dating of sand. Within our study area in the south-central Great Basin, luminescence ages of sand-size particles have successfully dated aeolian influxes of sand during arid intervals, but have not successfully dated the highstand beach ridges, the best preserved of which are largely gravel.</p&gt;        <p>Directly dating when these gravel clasts were last exposed to sunlight via luminescence is ideal but their limestone and volcanic lithologies prove challenging. Initial measurements from these lithologies show that feldspar luminescence signals are suited to single-aliquot regenerative (SAR) dose measurement protocols and show evidence for heterogeneous bleaching of rock surfaces. Polymineral extracts from dissolved limestone clast surfaces from Coal Valley that contain sufficient detrital sediment exhibit infrared signals measured at 50&amp;#8201;&amp;#176;C (IR<span class="inline-formula"><sub>50</sub></span>) with low to moderate fading rates. Single-grain ages from detrital sediment from three clasts, calculated using the central dose model, are statistically consistent with the radiocarbon age estimate of the Pluvial Lake Coal highstand.</p&gt;        <p>Crushed slices from volcanic clasts from Cave Valley could be dated using a high-temperature (290&amp;#8201;&amp;#176;C) post-infrared infrared stimulated luminescence (pIRIR) signal with a correction for fading. Many ages obtained from volcanic clast surfaces are observed to be several thousand years younger than the expected age of the <span class="inline-formula">&amp;#8764;</span>&amp;#8201;18&amp;#8211;20&amp;#8201;ka beach ridge. This suggests that the volcanic rocks have been exposed to light long after the pluvial lake highstand, likely because of bioturbation, and that their most recent burial occurred in response to climatically driven soil formation processes. Comparisons between age-depth profile plateau ages from inside volcanic rocks and independent age control suggest that gravel-sized volcanic rocks were small enough to have been bleached throughout their entire thickness in the pluvial lake beach environment and that pIRIR signals that record the time of beach ridge formation and subsequent soil formation during the Pleistocene-Holocene transition may be preserved within the rock sub-surface.</p&gt;        <p>This study develops novel dating approaches for challenging rock lithologies. Rock surface dating techniques for pluvial lake beach ridges in the Great Basin should be further developed with consideration of local bedrock type(s), clast size, sample collection and preparation methods, gravel bleaching processes in pluvial lake environments and the impact of soil development and bioturbation on study sites.</p>
            </content>
            <author>
                <name>Copernicus Electronic Production Support Office</name>
            </author>
            <published>2026-04-07T22:17:18+02:00</published>
            <updated>2026-04-07T22:17:18+02:00</updated>
        </entry>
        <entry>
            <id>https://doi.org/10.5194/gchron-8-209-2026</id>
            <title type="html">Technical note: Geodynamic Thermochronology (GDTchron) &#8211; A Python package to calculate low-temperature thermochronometric ages from geodynamic numerical models
            </title>
            <link href="https://doi.org/10.5194/gchron-8-209-2026"/>
            <summary type="html">
                &lt;b&gt;Technical note: Geodynamic Thermochronology (GDTchron) – A Python package to calculate low-temperature thermochronometric ages from geodynamic numerical models&lt;/b&gt;&lt;br&gt;
                Dylan A. Vasey, Peter M. Scully, John B. Naliboff, and Sascha Brune&lt;br&gt;
                    Geochronology, 8, 209&#8211;222, https://doi.org/10.5194/gchron-8-209-2026, 2026&lt;br&gt;
                We present an open-access Python package (GDTchron) designed to forward model apatite (U-Th)/He, apatite fission track, and zircon (U-Th)/He ages using temperatures output by geodynamic numerical models. The software can be used in a parallelized workflow to calculate large numbers of ages. We present two examples of potential applications of GDTchron: a simple model of exhumation and a complex model of continental rifting followed by mountain building.
            </summary>
            <content type="html">
                &lt;b&gt;Technical note: Geodynamic Thermochronology (GDTchron) – A Python package to calculate low-temperature thermochronometric ages from geodynamic numerical models&lt;/b&gt;&lt;br&gt;
                Dylan A. Vasey, Peter M. Scully, John B. Naliboff, and Sascha Brune&lt;br&gt;
                    Geochronology, 8, 209&#8211;222, https://doi.org/10.5194/gchron-8-209-2026, 2026&lt;br&gt;
                <p>Low-temperature thermochronology provides a powerful means of extracting quantitative information on the thermal evolution of different tectonic settings from rocks exposed at the surface of the Earth. Geodynamic numerical models enable tracking the entire thermal structure of simulated tectonic settings throughout their evolution. Despite the highly complementary nature of these two approaches, few geodynamic modeling studies have used the thermal information in models to predict thermochronometric ages as a means of comparing model results with observational data. Here, we present Geodynamic Thermochronology (GDTchron): an open-source Python package designed to forward model large numbers of low-temperature thermochronometric ages from time&amp;#8211;temperature paths output by geodynamic numerical models. This package uses existing techniques to estimate apatite <span class="inline-formula"><math xmlns="http://www.w3.org/1998/Math/MathML" id="M1" display="inline" overflow="scroll" dspmath="mathml"><mrow class="chem"><mo>(</mo><mi mathvariant="normal">U</mi><mtext>-</mtext><mi mathvariant="normal">Th</mi><mo>)</mo><mo>/</mo><mi mathvariant="normal">He</mi></mrow></math><span><svg:svg xmlns:svg="http://www.w3.org/2000/svg" width="54pt" height="14pt" class="svg-formula" dspmath="mathimg" md5hash="765a9d5e53367702b431ab9c157dbbb8"><svg:image xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="gchron-8-209-2026-ie00001.svg" width="54pt" height="14pt" src="gchron-8-209-2026-ie00001.png"/></svg:svg></span></span>, apatite fission track, and zircon <span class="inline-formula"><math xmlns="http://www.w3.org/1998/Math/MathML" id="M2" display="inline" overflow="scroll" dspmath="mathml"><mrow class="chem"><mo>(</mo><mi mathvariant="normal">U</mi><mtext>-</mtext><mi mathvariant="normal">Th</mi><mo>)</mo><mo>/</mo><mi mathvariant="normal">He</mi></mrow></math><span><svg:svg xmlns:svg="http://www.w3.org/2000/svg" width="54pt" height="14pt" class="svg-formula" dspmath="mathimg" md5hash="9d24790ca0043a794668902e1949e0af"><svg:image xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="gchron-8-209-2026-ie00002.svg" width="54pt" height="14pt" src="gchron-8-209-2026-ie00002.png"/></svg:svg></span></span&gt; ages from time&amp;#8211;temperature paths in a parallelized workflow that enables faster computation on multicore processors and high-performance computing systems.  The workflow is built on typical output files from geodynamic models containing particle location, time, and temperature, and we use an interpolation scheme to allow new particles to inherit the thermal histories of their nearest neighbors. GDTchron can be applied to any tectonic setting, though for results to be comparable to nature, geodynamic models should carefully account for erosion and sedimentation. We demonstrate the functionality of this software with a highly simplified geodynamic model of exhumation and a more complicated model of rift-inversion orogenesis with the aim of encouraging community participation in broadening future development.</p>
            </content>
            <author>
                <name>Copernicus Electronic Production Support Office</name>
            </author>
            <published>2026-04-01T22:17:18+02:00</published>
            <updated>2026-04-01T22:17:18+02:00</updated>
        </entry>
        <entry>
            <id>https://doi.org/10.5194/gchron-8-191-2026</id>
            <title type="html">The conflict between sampling resolution and stratigraphic constraints from a Bayesian perspective: OSL and  radiocarbon case studies
            </title>
            <link href="https://doi.org/10.5194/gchron-8-191-2026"/>
            <summary type="html">
                &lt;b&gt;The conflict between sampling resolution and stratigraphic constraints from a Bayesian perspective: OSL and  radiocarbon case studies&lt;/b&gt;&lt;br&gt;
                Guillaume Guérin, Pierre Guitton-Boussion, Imène Bouafia, and Anne Philippe&lt;br&gt;
                    Geochronology, 8, 191&#8211;207, https://doi.org/10.5194/gchron-8-191-2026, 2026&lt;br&gt;
                Bayesian modelling is often used to refine numerically dated chronological sequences, e.g., by making use of stratigraphic constraints. First, a high-resolution dataset based on luminescence dating is modelled with the dedicated R package BayLum. Then, three Bayesian modelling tools &amp;#8211; namely BayLum, Chronomodel and OxCal &amp;#8211; are compared using a high-resolution, radiocarbon dataset. Modelling artefacts are identified; the strengths and weaknesses of the models are discussed.
            </summary>
            <content type="html">
                &lt;b&gt;The conflict between sampling resolution and stratigraphic constraints from a Bayesian perspective: OSL and  radiocarbon case studies&lt;/b&gt;&lt;br&gt;
                Guillaume Guérin, Pierre Guitton-Boussion, Imène Bouafia, and Anne Philippe&lt;br&gt;
                    Geochronology, 8, 191&#8211;207, https://doi.org/10.5194/gchron-8-191-2026, 2026&lt;br&gt;
                <p>Bayesian modelling is often implemented in geochronology and its applications to geomorphology, archaeology, etc. The rationale behind such practices is the aim to improve robustness, precision and accuracy thanks to the use of prior knowledge regarding the studied sites, and in particular the order of samples constrained by stratigraphy. All chronological models tested in this study (OxCal, Chronomodel and BayLum) use the same mathematical model to handle stratigraphic constraints. However, this model has been shown to lead to estimation biases. First, this bias is illustrated with BayLum modelling on a high-resolution OSL dataset. Then, this paper compares statistical inferences obtained with the three above-mentioned modelling software on the Neolithic East mound of &amp;#199;atalh&amp;#246;y&amp;#252;k (Turkey). For this site, 49 radiocarbon ages were obtained with the aim to determine the start of occupations at this locality. Interestingly, age uncertainties are rather large, because of calibration curve plateaus. Therefore, the conditions for estimation biases are met. We discuss the behaviour of the different models and show that caution must be taken when modelling results are at odds with measurements. While OxCal, Chronomodel and BayLum are all affected by a spread in ages resulting from their common model of stratigraphic errors, Chronomodel suffers from a great loss of precision and OxCal, through the phase model, concentrates ages undesirably. We also conclude that the onset of occupations at &amp;#199;atalh&amp;#246;y&amp;#252;k was probably earlier than previously thought based on the OxCal model.</p>
            </content>
            <author>
                <name>Copernicus Electronic Production Support Office</name>
            </author>
            <published>2026-03-30T22:17:18+02:00</published>
            <updated>2026-03-30T22:17:18+02:00</updated>
        </entry>
        <entry>
            <id>https://doi.org/10.5194/gchron-8-165-2026</id>
            <title type="html">Analytical and modelling strategies for thermal histories from in situ (U-Th-Sm)&#8201;&#8725;&#8201;He data of single apatites
            </title>
            <link href="https://doi.org/10.5194/gchron-8-165-2026"/>
            <summary type="html">
                &lt;b&gt;Analytical and modelling strategies for thermal histories from in situ (U-Th-Sm) ∕ He data of single apatites&lt;/b&gt;&lt;br&gt;
                Ann-Kathrin Maier, Christoph Glotzbach, and Sarah Falkowski&lt;br&gt;
                    Geochronology, 8, 165&#8211;189, https://doi.org/10.5194/gchron-8-165-2026, 2026&lt;br&gt;
                (U-Th-Sm)/He dating is a tool to investigate when and how rocks cooled through the upper Earth&amp;#8217;s crust. We explore strategies to reconstruct thermal histories of individual apatite crystals by direct measurement of their helium concentration profile and radionuclide distribution. This approach allows for the inclusion of inhomogeneous grains in thermal modelling, which is often problematic in traditional (U-Th-Sm)/He methods.
            </summary>
            <content type="html">
                &lt;b&gt;Analytical and modelling strategies for thermal histories from in situ (U-Th-Sm) ∕ He data of single apatites&lt;/b&gt;&lt;br&gt;
                Ann-Kathrin Maier, Christoph Glotzbach, and Sarah Falkowski&lt;br&gt;
                    Geochronology, 8, 165&#8211;189, https://doi.org/10.5194/gchron-8-165-2026, 2026&lt;br&gt;
                <p>(U-Th-Sm)&amp;#8201;<span class="inline-formula"><math xmlns="http://www.w3.org/1998/Math/MathML" id="M2" display="inline" overflow="scroll" dspmath="mathml"><mo>/</mo></math><span><svg:svg xmlns:svg="http://www.w3.org/2000/svg" width="8pt" height="14pt" class="svg-formula" dspmath="mathimg" md5hash="527256ea34e0af356380afd605ccefc0"><svg:image xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="gchron-8-165-2026-ie00003.svg" width="8pt" height="14pt" src="gchron-8-165-2026-ie00003.png"/></svg:svg></span></span>&amp;#8201;He is a thermochronometric method used to reconstruct the rates and timing of geological processes. Recent developments in analytical approaches, specifically laser ablation (in situ) measurements, allow quantifying the distribution of parent isotopes (U, Th, and, in apatites, Sm) and decay products (<span class="inline-formula"><sup>4</sup></span>He) within individual mineral grains. This is particularly important to understand potential date over-dispersion, which can arise from the heterogeneous distribution of parent isotopes, and to develop thermal history modelling for single-grain (U-Th-Sm)&amp;#8201;<span class="inline-formula"><math xmlns="http://www.w3.org/1998/Math/MathML" id="M4" display="inline" overflow="scroll" dspmath="mathml"><mo>/</mo></math><span><svg:svg xmlns:svg="http://www.w3.org/2000/svg" width="8pt" height="14pt" class="svg-formula" dspmath="mathimg" md5hash="57ee8123d9c9aefcf23d9c7f6463c158"><svg:image xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="gchron-8-165-2026-ie00004.svg" width="8pt" height="14pt" src="gchron-8-165-2026-ie00004.png"/></svg:svg></span></span>&amp;#8201;He techniques.</p&gt;        <p>We build on previous studies and combine in situ <span class="inline-formula"><sup>4</sup></span>He concentration profile measurements with parent nuclide distribution mapping in natural apatites to explore analytical and modelling strategies for single-grain thermal history reconstructions. Specifically, we investigate the effects of laser ablation spot size, the number and location of ablation spots in a grain, and grain size on data resolution and suitability for thermal history modelling. In doing so, we introduce the calculation of <span class="inline-formula"><i>C</i><sub>aw</sub></span>, which is the concentration of parent nuclides at each ablation site weighted by alpha-particle stopping distances to account for the redistribution of <span class="inline-formula"><sup>4</sup></span>He in the crystal from high-energy alpha decay. We present stacked U, Th, and Sm maps measured at different ablation depths in two apatite grains from South Germany (one with homogeneous and one with zoned parent isotope distribution) and one apatite from the McClure Mountain Syenite age standard. Furthermore, we show in situ <span class="inline-formula"><sup>4</sup></span>He profiles of the two South German apatites and inversions for thermal histories. Our results indicate that, for our study and instrument set-up (a RESOchron system (Applied Spectra) consisting of a He-line and an excimer laser), four to six spot measurements at various distances from the grain rim enable measuring an in situ <span class="inline-formula"><sup>4</sup></span>He profile. We tested different laser ablation spot sizes (10&amp;#8211;30&amp;#8201;<span class="inline-formula">&amp;#181;</span>m) in grains with a range of <span class="inline-formula"><sup>4</sup></span>He concentrations and (U-Th-Sm)&amp;#8201;<span class="inline-formula"><math xmlns="http://www.w3.org/1998/Math/MathML" id="M12" display="inline" overflow="scroll" dspmath="mathml"><mo>/</mo></math><span><svg:svg xmlns:svg="http://www.w3.org/2000/svg" width="8pt" height="14pt" class="svg-formula" dspmath="mathimg" md5hash="6bfc4ae3491d603d986b6e1d0e6866cf"><svg:image xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="gchron-8-165-2026-ie00005.svg" width="8pt" height="14pt" src="gchron-8-165-2026-ie00005.png"/></svg:svg></span></span>&amp;#8201;He dates (16 to <span class="inline-formula">&amp;#8764;</span>&amp;#8201;200&amp;#8201;Ma) and determined that the optimal spot diameter for in situ <span class="inline-formula"><sup>4</sup></span>He profile measurements for apatite grains with (U-Th-Sm)&amp;#8201;<span class="inline-formula"><math xmlns="http://www.w3.org/1998/Math/MathML" id="M15" display="inline" overflow="scroll" dspmath="mathml"><mo>/</mo></math><span><svg:svg xmlns:svg="http://www.w3.org/2000/svg" width="8pt" height="14pt" class="svg-formula" dspmath="mathimg" md5hash="7572a9d7afeaa92ba0e8bb6f686362bd"><svg:image xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="gchron-8-165-2026-ie00006.svg" width="8pt" height="14pt" src="gchron-8-165-2026-ie00006.png"/></svg:svg></span></span>&amp;#8201;He dates as young as 16&amp;#8201;Ma is 20&amp;#8211;30&amp;#8201;<span class="inline-formula">&amp;#181;</span>m. Additionally, with an ablation spot diameter of 20&amp;#8201;<span class="inline-formula">&amp;#181;</span>m, a six-spot in situ <span class="inline-formula"><sup>4</sup></span>He profile requires a minimum grain diameter (measured perpendicular to the <span class="inline-formula"><i>c</i></span>-axis) of 145&amp;#8201;<span class="inline-formula">&amp;#181;</span>m. Combined with information from detailed parent nuclide maps, the in situ <span class="inline-formula"><sup>4</sup></span>He profiles offer a possibility to reconstruct the thermal histories of single grains, potentially including zoned and irregularly shaped crystals.</p>
            </content>
            <author>
                <name>Copernicus Electronic Production Support Office</name>
            </author>
            <published>2026-03-27T22:17:18+01:00</published>
            <updated>2026-03-27T22:17:18+01:00</updated>
        </entry>
        <entry>
            <id>https://doi.org/10.5194/gchron-8-143-2026</id>
            <title type="html">U-Pb dating of chrysocolla from supergene copper deposits in the Coastal Cordillera of northern Chile, Atacama Desert
            </title>
            <link href="https://doi.org/10.5194/gchron-8-143-2026"/>
            <summary type="html">
                &lt;b&gt;U-Pb dating of chrysocolla from supergene copper deposits in the Coastal Cordillera of northern Chile, Atacama Desert&lt;/b&gt;&lt;br&gt;
                Juan Ríos-Contesse, Richard Albert, Benedikt Ritter-Prinz, Axel Gerdes, Tibor Dunai, and Eduardo Campos&lt;br&gt;
                    Geochronology, 8, 143&#8211;164, https://doi.org/10.5194/gchron-8-143-2026, 2026&lt;br&gt;
                This study dated chrysocolla, a supergene copper mineral, from copper deposits hosted in the Coastal Cordillera of northern Chile, with ages between 8.0 and 0.045 million years. Results show that from the Late Miocene to the Pleistocene, short periods of moisture triggered mineral formation despite the hyperarid climate. These wetter periods were likely caused by occasional rainfall or stronger coastal fog, causing repeated pulses of supergene activity in the Coastal Cordillera.
            </summary>
            <content type="html">
                &lt;b&gt;U-Pb dating of chrysocolla from supergene copper deposits in the Coastal Cordillera of northern Chile, Atacama Desert&lt;/b&gt;&lt;br&gt;
                Juan Ríos-Contesse, Richard Albert, Benedikt Ritter-Prinz, Axel Gerdes, Tibor Dunai, and Eduardo Campos&lt;br&gt;
                    Geochronology, 8, 143&#8211;164, https://doi.org/10.5194/gchron-8-143-2026, 2026&lt;br&gt;
                <p>The dating of supergene copper minerals has been widely used as a proxy to investigate the evolution and onset of hyperaridity in the Atacama Desert. However, investigation of supergene copper mineralisation in the Atacama Desert has been restricted to two physiographic units favourable for the industrial extraction of copper: the Central Depression and the Precordillera. Furthermore, these studies dated the timing of supergene mineralisation by secondary non-copper minerals like alunite. In this study, we present new results of LA-ICP-MS U-Pb dating of chrysocolla from supergene deposits hosted in the western part of the Coastal Cordillera of northern Chile. The obtained U-Pb ages range from <span class="inline-formula">8.0&amp;#177;1.2</span&gt; to <span class="inline-formula">0.045&amp;#177;0.027</span>&amp;#8201;Ma. Supergene mineralisation ages point to significantly reduced precipitation, necessary for leaching and mineral precipitation process, since the Late Miocene to Pleistocene in the Coastal Cordillera, later than the secondary supergene mineralisation ages from the Precordillera. The data point to repeated phases of sufficient moisture along the Coastal Cordillera that promoted chrysocolla mineralisation during the Pliocene and Pleistocene. We propose that due to the position of the study areas near the coastal escarpment, and the predominant hyperarid environment in this part of the Coastal Cordillera since at least the Mid-Miocene, pluvial periods and/or intensification of coastal fog events caused alternating phases of supergene activity.</p>
            </content>
            <author>
                <name>Copernicus Electronic Production Support Office</name>
            </author>
            <published>2026-03-11T22:17:18+01:00</published>
            <updated>2026-03-11T22:17:18+01:00</updated>
        </entry>
        <entry>
            <id>https://doi.org/10.5194/gchron-8-119-2026</id>
            <title type="html">In situ cosmogenic <sup>10</sup>Be and <sup>26</sup>Al reveal the complex exposure and erosion history of the landscape once covered by the Quebec-Labrador Ice Dome
            </title>
            <link href="https://doi.org/10.5194/gchron-8-119-2026"/>
            <summary type="html">
                &lt;b&gt;In situ cosmogenic 10Be and 26Al reveal the complex exposure and erosion history of the landscape once covered by the Quebec-Labrador Ice Dome&lt;/b&gt;&lt;br&gt;
                Peyton M. Cavnar, Paul R. Bierman, Jeremy D. Shakun, Lee B. Corbett, Danielle LeBlanc, Gillian L. Galford, Pierre-Olivier Couette, Jean-Francois Ghienne, Patrick Lajeunesse, Jérôme van der Woerd, and Marc Caffee&lt;br&gt;
                    Geochronology, 8, 119&#8211;141, https://doi.org/10.5194/gchron-8-119-2026, 2026&lt;br&gt;
                To investigate the Laurentide Ice Sheet&amp;#8217;s erosivity before and during the Last Glacial Maximum, we sampled sand deposited by ice in eastern Canada before final deglaciation. We also sampled modern river sand. The <sup>26</sup>Al and <sup>10</sup>Be measured in glacial deposited sediments suggests that ice remained during some Pleistocene warm periods and was an inefficient eroder. Similar concentrations of <sup>26</sup>Al and <sup>10</sup>Be in modern sand suggests that most modern river sediment is sourced from glacial deposits.&amp;#160;
            </summary>
            <content type="html">
                &lt;b&gt;In situ cosmogenic 10Be and 26Al reveal the complex exposure and erosion history of the landscape once covered by the Quebec-Labrador Ice Dome&lt;/b&gt;&lt;br&gt;
                Peyton M. Cavnar, Paul R. Bierman, Jeremy D. Shakun, Lee B. Corbett, Danielle LeBlanc, Gillian L. Galford, Pierre-Olivier Couette, Jean-Francois Ghienne, Patrick Lajeunesse, Jérôme van der Woerd, and Marc Caffee&lt;br&gt;
                    Geochronology, 8, 119&#8211;141, https://doi.org/10.5194/gchron-8-119-2026, 2026&lt;br&gt;
                <p>The rate at which ice sheets erode rock and produce sediment is poorly known. Here, we use paired cosmogenic nuclides in both deglacial and modern sediment to understand better the efficacy with which the Quebec-Labrador Ice Dome (QLID) of the Laurentide Ice Sheet eroded bedrock and generated sand and boulders across the landscape of eastern Canada. We sampled deglacial sediment (esker and delta sand, <span class="inline-formula"><i>n</i>=</span>&amp;#8201;10), sediment from modern streams (<span class="inline-formula"><i>n</i>=</span>&amp;#8201;11), one bedrock outcrop, and a bedrock depth profile (<span class="inline-formula"><i>n</i>=</span>&amp;#8201;7), measuring concentrations of <span class="inline-formula"><sup>10</sup></span>Be and <span class="inline-formula"><sup>26</sup></span>Al in quartz isolated from all samples. We also collated published cosmogenic nuclide measurements of boulders and bedrock from eastern Canada (<span class="inline-formula"><i>n</i>=</span>&amp;#8201;237 samples), and using independent estimates of deglaciation timing, calculated initial nuclide concentrations when the material was exposed by the most recent deglaciation, between 6.3 to 15.2&amp;#8201;ka.</p&gt;        <p>At the time of deposition, all 10 deglacial sand samples contained <span class="inline-formula"><sup>10</sup></span>Be and <span class="inline-formula"><sup>26</sup></span>Al, on average equivalent to several thousand years of surface exposure. The ubiquitous presence of <span class="inline-formula"><sup>10</sup></span>Be and <span class="inline-formula"><sup>26</sup></span>Al in eastern Quebec deglacial sediment is consistent with older-than-expected exposure ages for bedrock outcrops (<span class="inline-formula"><i>n</i>=</span>&amp;#8201;26 of 46 samples) and boulders (<span class="inline-formula"><i>n</i>=</span>&amp;#8201;65 of 192 samples) once covered by the QLID. Error-weighted averages of <span class="inline-formula"><sup>26</sup></span>Al&amp;#8201;<span class="inline-formula"><math xmlns="http://www.w3.org/1998/Math/MathML" id="M18" display="inline" overflow="scroll" dspmath="mathml"><mo>/</mo></math><span><svg:svg xmlns:svg="http://www.w3.org/2000/svg" width="8pt" height="14pt" class="svg-formula" dspmath="mathimg" md5hash="62d2c8208bbdf49afb8db19c9f7b6b50"><svg:image xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="gchron-8-119-2026-ie00001.svg" width="8pt" height="14pt" src="gchron-8-119-2026-ie00001.png"/></svg:svg></span></span>&amp;#8201;<span class="inline-formula"><sup>10</sup></span>Be ratios for both deglacial (6.1&amp;#8201;<span class="inline-formula">&amp;#177;</span>&amp;#8201;0.3, all uncertainties 1&amp;#160;SD) and modern sediment samples (6.6&amp;#8201;<span class="inline-formula">&amp;#177;</span>&amp;#8201;0.5) are lower than the measured production ratio at high latitudes (Greenland, 7.3&amp;#8201;<span class="inline-formula">&amp;#177;</span>&amp;#8201;0.3), suggesting cumulative burial of at least some sediment grains for at least hundreds of thousands of years.</p&gt;        <p>This burial history suggests that ice at the middle of the QLID either survived some interglacials and/or that the average sediment residence time on the landscape is several times longer than a 100&amp;#8201;kyr glacial cycle, allowing storage and burial of sediment over multiple glacial cycles, either under ice and/or in thick deposits such as deltas and moraines. Modern river sand contains on average only slightly higher nuclide concentrations than deglacial sediment, suggesting that  contemporary river sand is predominately recycled from glacial deposits. Together, the new sediment data (which amalgamate across large areas of the landscape), and our compilation of bedrock and boulder point data, suggest that the average depth of bedrock erosion by ice and the speed of glacial sediment transport in eastern Canada were insufficient to remove material containing cosmogenic nuclides produced during prior interglacial(s).</p>
            </content>
            <author>
                <name>Copernicus Electronic Production Support Office</name>
            </author>
            <published>2026-03-03T22:17:18+01:00</published>
            <updated>2026-03-03T22:17:18+01:00</updated>
        </entry>
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