New research documents erosion rates in the Andes Mountains.
Every second, Earth is bombarded by vast amounts of cosmic rays—invisible sub-atomic particles that originate from things like the sun and supernova explosions. These high-energy, far-traveled cosmic rays collide with atoms as they enter Earth’s atmosphere and set off cascades of secondary cosmic rays.
When secondary cosmic rays penetrate the upper meters of Earth’s surface, they turn elements in minerals, like oxygen, into rare radioisotopes (or “cosmogenic radionuclides”) including beryllium-10 (Be-10) and carbon-14 (C-14).
Scientists can then study the variations in concentrations of these cosmogenic nuclides to estimate how long rocks have been exposed at the Earth’s surface. This in turn allows researchers to gain a better understanding of planetary processes, such as rates of erosion—from nothing more than a kilogram of river sand.
Gregory Hoke, professor and department chair of earth and environmental sciences at Syracuse University, J.R. Slosson, a postdoctoral researcher at the University of Massachusetts Amherst, and Nat Lifton, associate professor of earth, atmospheric, and planetary sciences at Purdue University, analyzed cosmogenic radionuclides in samples from the Argentine Andes. Their findings appear in the journal Geophysical Research Letters.
Their goal was to document the amount of time material resides on the hillslopes in the Andes Mountains relative to the overall erosion rate of the river basin. This information is critical to helping scientists identify landslide risks and understand how climate change will affect the dynamics of material transport on hillslopes as regions get wetter or drier.
To determine erosion rates, the team obtained samples of river sand collected at the foot of the eastern flank of the Andes Mountains in the Mendoza and San Juan provinces, located in west-central Argentina. The river sand should be a representative, well-mixed sample of the entire catchment (or runoff area) upstream of where the sample was collected.
In Hoke’s lab, the sand was treated to isolate pure quartz from the other minerals in the sample. The researchers use pure quartz because it is an optimal source for Be-10 and C-14. Splits of pure quartz were sent to Lifton’s lab where beryllium and carbon were extracted. Subsequent measurements of C-14 took place at Purdue’s PRIME Lab and Be-10 was analyzed at Lawrence Livermore National laboratory to figure out concentrations of each radionuclide.
The highest non-volcanic peaks in the Andes are located between Santiago, Chile and Mendoza, Argentina. The river basins that drain the high Andes span 5,000 meters (16,500 feet) in elevation and their hillslopes are lined with accumulations of rocky debris known as talus and scree.
Because Be-10 and C-14 are produced proportionally but decay at vastly different rates, the cosmogenic radionuclide concentrations within a sample reveal the rate at which sediment is produced from bare rock surfaces (Be-10) and the time it takes to travel down hillslopes through landslides (C-14). As sediment is mobilized and buried through landsliding, the rate of production of both isotopes diminishes, but because C-14 decays 1,000 times faster than Be-10, their proportionality changes rapidly. This change in proportionally allowed the authors to apply a statistical model to determine the average duration of time it takes material to travel down talus slopes.
According to Hoke, this is one of the first studies to use the combination of Be-10 and C-14 to show the long-term average rate of sediment generation and the time and process it takes to move down to and through the rivers, giving a broader picture of the factors involved.
“Previously, we’ve relied nearly exclusively on Be-10 and sediment concentration measurements made at river gauge stations to estimate average erosion rates,” notes Hoke. “What attracted us to study these catchments with C-14 was the agreement of gauge and Be-10 data. We expected to see the two isotopes and gauge data yield the same rates and demonstrate that mountain erosion was occurring at a steady state.”
While the concentration of Be-10 came back as anticipated over the long timescale, they found that C-14 was much lower than anticipated, meaning that sediments eroded from the high mountain watersheds were shielded from cosmic rays for at least 7,000 to 15,0000 years. The authors explain that temporary storage in talus slopes best explains the lower concentration of C-14 relative to Be-10.
“This study shows that it is possible to fill an important gap in the observational timescale using the C-14/Be-10 pair that brings to life what really happens on the hillslopes,” says Hoke.
With the risk that landslides pose to humans and infrastructure, Slosson says their results indicate that C-14 can be significant in unraveling sediment transport dynamics going forward, and potentially help predict where future landslides might occur. He explains, “utilizing C-14 along with Be-10 provides a new window into the complexity of sediment transport in mountain settings and can provide a backdrop for evaluating contemporary changes in earth surface processes.”
The project had funding from the National Science Foundation, the Geological Society of America, and Syracuse University.
Source: Syracuse University
