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	<title>cosmic-ray isotope analysis &#8211; Science</title>
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	<title>cosmic-ray isotope analysis &#8211; Science</title>
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		<title>Ancient peat was meters thicker in Belgium, cosmic-ray clocks reveal</title>
		<link>https://scienmag.com/ancient-peat-was-meters-thicker-in-belgium-cosmic-ray-clocks-reveal/</link>
		
		<dc:creator><![CDATA[Violet Maxwell]]></dc:creator>
		<pubDate>Thu, 08 Oct 2026 12:44:05 +0000</pubDate>
				<category><![CDATA[Earth Science]]></category>
		<category><![CDATA[aluminum-26]]></category>
		<category><![CDATA[ancient peat thickness measurement]]></category>
		<category><![CDATA[Belgian Ardennes]]></category>
		<category><![CDATA[Belgian Ardennes peatland study]]></category>
		<category><![CDATA[beryllium-10]]></category>
		<category><![CDATA[carbon cycle]]></category>
		<category><![CDATA[cosmic radiation in geology]]></category>
		<category><![CDATA[cosmic-ray clocks and Earth history]]></category>
		<category><![CDATA[cosmic-ray exposure dating techniques]]></category>
		<category><![CDATA[cosmic-ray isotope analysis]]></category>
		<category><![CDATA[cosmogenic nuclides]]></category>
		<category><![CDATA[denudation rates]]></category>
		<category><![CDATA[Earth Surface Dynamics]]></category>
		<category><![CDATA[geochronology using cosmic-ray produced isotopes]]></category>
		<category><![CDATA[Hautes Fagnes]]></category>
		<category><![CDATA[Holocene climate and carbon reservoirs]]></category>
		<category><![CDATA[impact of peatland expansion on Holocene climate]]></category>
		<category><![CDATA[land use history]]></category>
		<category><![CDATA[mid-Pleistocene uplift]]></category>
		<category><![CDATA[peat degradation]]></category>
		<category><![CDATA[peatland historical reconstruction]]></category>
		<category><![CDATA[peatlands]]></category>
		<category><![CDATA[quartz isotopes in peat dating]]></category>
		<category><![CDATA[role of peatlands in atmospheric greenhouse gases]]></category>
		<guid isPermaLink="false">https://scienmag.com/?p=247722</guid>

					<description><![CDATA[Cosmogenic aluminum-26 and beryllium-10 in bedrock beneath Belgian peat bogs reveal that the Hautes Fagnes blanket was once 1.8 to 3.4 meters thicker, with historical land use driving the loss.]]></description>
										<content:encoded><![CDATA[<p>Buried beneath the mist-soaked plateau of the Hautes Fagnes in the Belgian Ardennes, a quiet archive of cosmic radiation has just rewritten the history of one of Europe&#8217;s most iconic peatlands. A team of Earth scientists led by Angus Moore of the Earth and Life Institute at Université catholique de Louvain and the Institute of Geophysics of the Czech Academy of Sciences has shown that the blanket of peat covering these upland bogs was once roughly two to three meters thicker than it is today. The evidence comes not from the peat itself, which decays and vanishes over geological time, but from rare isotopes forged by cosmic rays in the quartz-rich bedrock hidden underneath. The findings, published in the journal Earth Surface Dynamics, offer the first direct way to measure how thick a peatland was averaged over hundreds of thousands of years, a window that no other technique can open.</p>
<p>The problem the researchers set out to solve is a stubborn one. Peatlands are among the largest terrestrial carbon reservoirs on the planet, and their expansion after the last ice age helped shape the concentration of methane and carbon dioxide in the Holocene atmosphere. Yet peat is perishable. Radiocarbon dating, the workhorse of peatland science, reaches back less than 50,000 years, and in formerly glaciated northern landscapes, ice sheets destroyed nearly all peat that formed before the Last Glacial Maximum. In old, undisturbed bogs, decomposition eventually balances the input of fresh plant litter, so the modern peat column no longer records the full history of peat on the landscape. Everything scientists believe about peatlands before the last glacial cycle therefore rests on a handful of exceptionally well-preserved deposits and on computer models.</p>
<p>The Belgian team&#8217;s solution exploits a property of quartz that has become one of geomorphology&#8217;s most powerful tools. Cosmic rays striking the uppermost meters of the Earth&#8217;s surface produce rare isotopes, including beryllium-10 and aluminum-26, inside mineral grains. The deeper a grain sits beneath overlying material, the fewer cosmic rays reach it, so the concentration of these cosmogenic nuclides in a sample carries a memory of how much mass, in this case peat, shielded it over its exposure history. Crucially, the two isotopes decay at different rates: aluminum-26 has a half-life of about 717,000 years while beryllium-10 persists for about 1.39 million years. When a landscape erodes slowly enough, the mismatch between these clocks becomes measurable, and the ratio of the two isotopes can be unpicked to yield both the rate of landscape lowering and the average thickness of the blanket above it simultaneously.</p>
<p>The Hautes Fagnes turned out to be an almost ideal natural laboratory. Perched on the highest ground in the Belgian Ardennes, the plateau receives about 1,440 millimeters of rain per year while mean annual temperatures hover near 6.7 degrees Celsius, and persistent orographic cloud keeps evapotranspiration low, conditions that favor peat accumulation. The study hillslope sits upstream of a mid-Pleistocene knickzone on the Hoëgne river, in a landscape so sluggish that it has barely responded to the uplift that rejuvenated rivers elsewhere in the Ardennes. The team cored through the modern peat blanket, which ranges from 0.2 to 2.1 meters deep along the transect, to collect saprolite, the rotted bedrock beneath, at six positions from the interfluve down to the channel. They also gathered stream sediment at the base of the slope and spent a full year gauging discharge and sampling stream water for dissolved silicon.</p>
<p>The measurements delivered a surprise. In quartz formed at the surface, aluminum-26 and beryllium-10 accumulate in a characteristic production ratio, about 7.2 at this site. Every sample the team analyzed fell below that ratio, from 3.29 at the summit to 6.06 at the toe-slope, and all plotted below the steady-state denudation line on a two-nuclide diagram by more than the modern peat cover could explain. Because the site sits near a local topographic high in a region never overridden by ice, deep burial by sediment or glaciers could not account for the deficit. The only plausible interpretation was that the samples had spent their exposure histories under substantially more shielding than the present-day peat provides, in other words, that the peat used to be much thicker.</p>
<p>To turn that qualitative signal into numbers, the researchers built a sophisticated inverse model. They accounted for the fact that saturated peat, which is roughly 90 percent water, attenuates cosmic radiation differently from mineral rock, adopting a shorter absorption mean free path of about 110 grams per square centimeter in peat compared with 160 in saprolite. They also modeled muon-induced production, which matters greatly under thick cover because muons penetrate far deeper than ordinary cosmic-ray nucleons. A Markov Chain Monte Carlo inversion then explored millions of parameter combinations to find those consistent with the measured isotope concentrations, yielding probability distributions rather than single answers. The results were cross-checked against an entirely independent estimate of the watershed-scale denudation rate, about 7.2 tons per square kilometer per year, derived from dissolved silicon fluxes and the weathering intensity of the regolith, which agreed in order of magnitude with the cosmogenic values.</p>
<p>The modeled denudation rates were astonishingly low, between 0.3 and 4.9 tons per square kilometer per year, equivalent to a landscape lowering of roughly 0.1 to 1.9 meters per million years, placing the Ardennes plateau among the slowest-eroding landscapes on Earth, comparable to ancient surfaces in Brazil, Australia, and South Africa. Because erosion is so slow, the isotope signal integrates over 0.7 to 1.8 million years, spanning every glacial-interglacial cycle since the mid-Pleistocene. Against that long baseline, the median long-term overburden thicknesses exceeded modern values by 190 to 350 grams per square centimeter along the transect, equivalent to roughly 1.8 to 3.4 meters of saturated peat. The inferred thicknesses, between about 2.5 and 4.2 meters, are physically sensible: they fall below the roughly 8.5-meter maximum observed in plateau raised bogs such as Misten, and their relationship to hillslope gradient obeys the classic groundwater-mound physics that governs steady-state bog morphology.</p>
<p>So where did the missing meters of peat go? The team systematically ruled out alternatives. Snow cover, even at persistent winter maxima, would add only a few grams per square centimeter of shielding on average, two orders of magnitude too little. A continuous loess blanket thick enough to explain the signal would have to exceed a meter and a half, yet no loess survives at the site and the geochemistry of the saprolite shows it formed in place from the underlying bedrock. Ground ice during periglacial episodes was too local and too short-lived. That leaves human activity. Peat cutting for fuel is documented in the Hautes Fagnes since the sixteenth century and intensified dramatically in the nineteenth, when records show nearly 200,000 cubic meters extracted annually. Medieval mowing, grazing, slash-and-burn cultivation, and wildfires shifted the bogs into negative mass balance, and drainage ditches plus spruce plantations in the early twentieth century accelerated subsidence at rates of one to two centimeters per year reported for comparable bogs. Together, the authors calculate, these pressures could account for more than two meters of peat loss, explaining most of the gap between the long-term average and today&#8217;s thin blanket.</p>
<p>The summit sample held one final revelation. Its model clearly resolved a step-change in overburden thickness, a thickening event with peak probability between 0.8 and 1.4 million years ago, which the authors interpret as the onset of the peat blanket itself. Remarkably, that timing coincides with a well-documented pulse of tectonic uplift in the Ardennes, recorded by the abandonment of the Younger main terrace of the Meuse and Rhine rivers around 0.7 million years ago. Before that uplift, the summit stood near 530 meters elevation, just below the threshold where orographic cooling and cloudiness begin to create the cool, wet conditions peat requires. As the massif rose roughly 100 meters, the site crossed into peat-forming territory, tying the birth of this carbon-rich ecosystem directly to the slow breathing of the Earth&#8217;s crust.</p>
<p>Beyond its local story, the study carries a warning for anyone estimating erosion rates in peatland terrain. If the beryllium-10 concentration in the stream sediment were interpreted the conventional way, assuming the modern peat cover represents long-term steady state, the resulting erosion rate would overestimate landscape lowering by an order of magnitude, because depressed aluminum-26 to beryllium-10 ratios masquerade as deep burial rather than thick organic cover. The paired-nuclide approach demonstrated here should work in any slowly eroding, unglaciated landscape with peat, from the moorlands of southwestern Britain to tropical cratonic peatlands in Amazonia and the Congo basin. And pairing beryllium-10 with cosmogenic carbon-14, whose short half-life suits faster-eroding and formerly glaciated terrain, could soon extend the method to peatlands worldwide. At a moment when drained and degraded peatlands are recognized as ticking carbon bombs, the Hautes Fagnes offer a sobering baseline: what we see today is not what these landscapes once were, and the atmosphere remembers the difference.</p>
<p><strong>Subject of Research:</strong> Using paired cosmogenic 26Al and 10Be nuclides to reconstruct long-term peat thickness and denudation rates in the Hautes Fagnes upland peatland, Belgian Ardennes</p>
<p><strong>Article Title:</strong> Long-term peat thickness from cosmogenic 26Al and 10Be, Hautes Fagnes, Belgian Ardennes</p>
<p><strong>Article References:</strong> Moore, A., Henrion, M., Li, Y., du Bois d&#x27;Aische, E., Gautschi, P., Christl, M., Jonard, F., Lambot, S., Van Oost, K., Opfergelt, S., &amp; Vanacker, V. (2026). Long-term peat thickness from cosmogenic 26 Al and 10 Be, Hautes Fagnes, Belgian Ardennes. <em>Earth Surface Dynamics, 14</em>(5), 763-780. <a href="https://doi.org/10.5194/esurf-14-763-2026" rel="noopener noreferrer">https://doi.org/10.5194/esurf-14-763-2026</a></p>
<p><strong>Image Credits:</strong> AI Generated</p>
<p><strong>DOI:</strong> <a href="https://doi.org/10.5194/esurf-14-763-2026" rel="noopener noreferrer">10.5194/esurf-14-763-2026</a></p>
<p><strong>Keywords:</strong> cosmogenic nuclides, peatlands, beryllium-10, aluminum-26, Hautes Fagnes, Belgian Ardennes, denudation rates, carbon cycle, peat degradation, land use history, mid-Pleistocene uplift, Earth Surface Dynamics</p>
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