2007 GSA Denver Annual Meeting (28–31 October 2007)

Paper No. 5
Presentation Time: 2:40 PM

CONSTRAINTS ON THE TIMING OF FAN DEPOSITION IN DEATH VALLEY, CALIFORNIA, USING COSMOGENIC 10BE AND 26AL


DÜHNFORTH, Miriam, Dept. of Earth and Environmental Sciences, Ludwig- Maximilians-University, Munich, 80333 munich, Germany, IVY-OCHS, Susan, Particle Physics/Institute of Geography, ETH Zurich/University of Zurich, Hoenggerberg, HPK, Zurich, 8093, Switzerland, DENSMORE, Alexander L., Department of Geography, Durham University, South Road, Durham, DH1 3LE, United Kingdom and KUBIK, Peter W., Paul Scherrer Institute c/o Institute of Particle Physics, HPH H30, ETH Hoenggerberg, Zurich, CH-8093, Switzerland, miriam.duehnforth@iaag.geo.uni-muenchen.de

Cosmogenic dating of fan surfaces potentially provides a unique opportunity to study the long-term controls on fan evolution, particularly on fans with long depositional surface chronologies over a few 105 yrs. However, cosmogenic ages obtained from fan surfaces only reflect the true depositional timing if the inheritance is negligible.

Fans such as the Warm Springs fan on the western side of Death Valley, California, are ideal for the reconstruction of a long-term depositional history. The Warm Springs fan is characterized by ~25 m of incision at the fan head, which has led to a subsequent basinward shift of the active depositional lobe. Based on morphologic criteria such as the depth of fan surface dissection, we mapped three distinct fan lobes and dated these fan surfaces using cosmogenic exposure dating with the isotopes 10Be and 26Al. For the fan surface dating, we measured 18 amalgamated clast samples from pavements, each containing 30-40 quartzite clasts of 5-10 cm in diameter. For the estimation of present-day inheritance, we took a total of 10 amalgamated samples from different locations within the incised, active channel.

Cosmogenic measurements on the Warm Springs fan reveal 10Be ages between ~60 and 860 ka assuming zero erosion. The oldest, deeply dissected fan surfaces on the proximal fan record deposition during ~860 and 390 10Be ka. On the distal, undissected surfaces, depositional 10Be ages are younger and reflect depositional timing between 320 and 160 ka. The 10Be and 26Al nuclide concentrations furthermore show that the fan surfaces generally underwent a simple exposure history and were not affected by complex histories of long burial and re-exposure. The cosmogenic samples from the incised channel show that present-day inheritance varies between 0.4 x 106 and 1.0 x 106 10Be atoms g-1 at the fan head and between 0.5 x 106 and 1.1 x 106 10Be atoms g-1 at the distal fan, which corresponds, depending on the production rate at the different sampling sites in the channel, to an exposure time of ~60 to 160 kyr and ~110 to 240 kyr, respectively. Although the influence of inheritance on the depositional ages diminishes with fan surface age, our results show that, assuming that inheritance in this setting did not significantly change through time, the inheritance component complicates efforts to resolve the true depositional timing.