Research Article| May 01, 2005 Dating offset fans along the Mojave section of the San Andreas fault using cosmogenic 26Al and 10Be A. Matmon; A. Matmon 1U.S. Geological Survey, 345 Middlefield Rd., Menlo Park, California 94025, USA Search for other works by this author on: GSW Google Scholar D.P. Schwartz; D.P. Schwartz 1U.S. Geological Survey, 345 Middlefield Rd., Menlo Park, California 94025, USA Search for other works by this author on: GSW Google Scholar R. Finkel; R. Finkel 2Lawrence Livermore National Laboratory, Livermore, California 94550, USA Search for other works by this author on: GSW Google Scholar S. Clemmens; S. Clemmens 2Lawrence Livermore National Laboratory, Livermore, California 94550, USA Search for other works by this author on: GSW Google Scholar T. Hanks T. Hanks 3U.S. Geological Survey, 345 Middlefield Rd., Menlo Park, California 94025, USA Search for other works by this author on: GSW Google Scholar Author and Article Information A. Matmon 1U.S. Geological Survey, 345 Middlefield Rd., Menlo Park, California 94025, USA D.P. Schwartz 1U.S. Geological Survey, 345 Middlefield Rd., Menlo Park, California 94025, USA R. Finkel 2Lawrence Livermore National Laboratory, Livermore, California 94550, USA S. Clemmens 2Lawrence Livermore National Laboratory, Livermore, California 94550, USA T. Hanks 3U.S. Geological Survey, 345 Middlefield Rd., Menlo Park, California 94025, USA Publisher: Geological Society of America Received: 13 Feb 2004 Revision Received: 06 Jul 2004 Accepted: 27 Jul 2004 First Online: 02 Mar 2017 Online ISSN: 1943-2674 Print ISSN: 0016-7606 Geological Society of America GSA Bulletin (2005) 117 (5-6): 795–807. https://doi.org/10.1130/B25590.1 Article history Received: 13 Feb 2004 Revision Received: 06 Jul 2004 Accepted: 27 Jul 2004 First Online: 02 Mar 2017 Cite View This Citation Add to Citation Manager Share Icon Share Facebook Twitter LinkedIn MailTo Tools Icon Tools Get Permissions Search Site Citation A. Matmon, D.P. Schwartz, R. Finkel, S. Clemmens, T. Hanks; Dating offset fans along the Mojave section of the San Andreas fault using cosmogenic 26Al and 10Be. GSA Bulletin 2005;; 117 (5-6): 795–807. doi: https://doi.org/10.1130/B25590.1 Download citation file: Ris (Zotero) Refmanager EasyBib Bookends Mendeley Papers EndNote RefWorks BibTex toolbar search Search Dropdown Menu toolbar search search input Search input auto suggest filter your search All ContentBy SocietyGSA Bulletin Search Advanced Search Abstract Analysis of cosmogenic 10Be and 26Al in samples collected from exposed boulders (n = 20) and from buried sediment (n = 3) from offset fans along the San Andreas fault near Little Rock, California, yielded ages, ranging from 16 to 413 ka, which increase with distance from their source at the mouth of Little Rock Creek. In order to determine the age of the relatively younger fans, the erosion rate of the boulders and the cosmogenic nuclide inheritance from exposure prior to deposition in the fan were established. Cosmogenic nuclide inheritance values that range between 8.5 × 103 and 196 × 103 atoms 10Be g−1 quartz were determined by measuring the concentrations and ratios of 10Be and 26Al in boulders (n = 10) and fine sediment (n = 7) at the outlet of the present active stream. Boulder erosion rate, ranging between 17 and 160 mm k.y.−1, was estimated by measuring 10Be and 26Al concentrations in nearby bedrock outcrops (n = 8). Since the boulders on the fans represent the most resistant rocks in this environment, we used the lowest rate for the age calculations. Monte Carlo simulations were used to determine ages of 16 ± 5 and 29 ± 7 ka for the two younger fan surfaces.Older fans (older than 100 ka) were dated by analyzing 10Be and 26Al concentrations in buried sand samples. The ages of the three oldest fans range between 227 ± 242 and 413 ± 185 ka. Although fan age determinations are accompanied by large uncertainties, the results of this study show a clear trend of increasing fan ages with increasing distance from the source near Little Rock Creek and provide a long-term slip rate along this section of the San Andreas fault.Slip rate along the Mojave section of the San Andreas fault for the past 413 k.y. can be determined in several ways. The average slip rate calculated from the individual fan ages is 4.2 ± 0.9 cm yr−1. A linear regression through the data points implies a slip rate of 3.7 ± 1.0 cm yr−1. A most probable slip rate of 3.0 ± 1.0 cm yr−1 is determined by using a χ2 test. These rates suggest that the average slip along the Mojave section of the San Andreas fault has been relatively constant over this time period. The slip rate along the Mojave section of the San Andreas fault, determined in this study, agrees well with previous slip rate calculations for the Quaternary. You do not have access to this content, please speak to your institutional administrator if you feel you should have access.
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