Article

Cosmogenic 3He in Himalayan garnets indicating an altitude dependence of the 3He/10Be production ratio

Centre de Recherches Pétrographiques et Géochimiques, CRPG, CNRS-UPR 2300, BP 20, 54 501 Vandoeuvre-Lès-Nancy Cedex, France; Laboratoire de Géodynamique des Chaines Alpines, LGCA-UMR 5025, Maison des Géosciences, BP 53, 38041 Grenoble, France; CEREGE, UMR 6635 CNRS-Université Aix-Marseille III, BP 80, 13545 Aix-en-Provence Cedex 04, France; Ecole Nationale Supérieure de Géologie, ENSG, rue du Doyen Marcel Roubault, BP 40, 54501 Vandoeuvre-Lès-Nancy Cedex, France
Earth and Planetary Science Letters DOI:10.1016/j.epsl.2004.10.009

ABSTRACT To investigate the potential of using cosmogenic helium in garnet as a dating tool, 3Hec and 10Bec have been measured within garnets and coexisting quartz, respectively, sampled in the Himalayan range at various elevations. Comparison and correlation of 3Hec and 10Bec concentrations demonstrate that cosmogenic 3He is well retained in Himalayan garnets and can thus be used in this mineral to quantify precisely earth's surface processes. This, in the case of recently cooled orogenic samples which contain limited amounts of non-cosmogenic helium. For these high-elevation samples, the exposure ages derived from 3Hec using classical scaling factors lead however to an overestimation of 3Hec ages, compared to 10Bec ages (0.1 to 28 ky), by up to a factor of 2. Additionally, over the samples altitude range (3000–4622 m), the theoretically invariant polar 3Hec/10Bec production ratio (∼22.5), increases with increasing elevation, challenging classical models of production rate evolution. To explain this observation, we propose a new 3Hec production mechanism, based on the altitudinal dependence of the energy spectrum of cosmic rays, and according to which neutrons or protons resulting from a first spallation reaction within the rock (tertiary particles) may have sufficient energy to induce an additional in situ spallation reaction producing a second 3H or 3He, but insufficient energy to produce 10Be, the probability of such a mechanism increasing with altitude. According to these observations, we propose for future and ongoing studies to use the empirically determined attenuation length of 121 g/cm2 for helium production at high altitude.

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Keywords

10Bec concentrations
 
classical models
 
classical scaling factors lead
 
coexisting quartz
 
contain limited amounts
 
earth's surface processes
 
exposure ages
 
first spallation reaction
 
helium production
 
high-elevation samples
 
insufficient energy
 
new 3Hec production mechanism
 
non-cosmogenic helium
 
orogenic samples
 
production rate evolution
 
samples altitude range
 
situ spallation reaction
 
tertiary particles
 
theoretically invariant polar 3Hec/10Bec production ratio
 
various elevations