Organic carbon burial forcing of the carbon cycle from Himalayan erosion

• Published in: Nature
• Main Authors: France-Lanord, Christian, Derry, Louis
• Other Authors: Centre de Recherches Pétrographiques et Géochimiques (CRPG), Université de Lorraine (UL)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), Centre National de la Recherche Scientifique (CNRS), Department of Earth and Atmospheric Sciences Ithaca) (EAS), Cornell University New York
• Format: Article in Journal/Newspaper
• Language: English
• Published: HAL CCSD 1997
• Subjects: [SDU]Sciences of the Universe [physics]; [SDU.STU]Sciences of the Universe [physics]/Earth Sciences; [SDU.OCEAN]Sciences of the Universe [physics]/Ocean; Atmosphere; Carbonic acid
• Online Access: https://hal.archives-ouvertes.fr/hal-02149397; https://hal.archives-ouvertes.fr/hal-02149397/document; https://hal.archives-ouvertes.fr/hal-02149397/file/CFL%20Derry.pdf; https://doi.org/10.1038/36324

International audience Weathering and erosion can affect the long-term ocean-atmosphere budget of carbon dioxide both through the consumption of carbonic acid during silicate weathering and through changes in the weathering and burial rates of organic carbon 1-4. Recent attention has focused on increased silicate weathering of tectoni-cally uplifted areas in the India-Asia collision zone as a possible cause for falling atmospheric CO 2 levels in the Cenozoic era 5-7. The chemistry of Neogene sediments from the main locus of sedimentary deposition for Himalayan detritus, the Bengal Fan, can be used to estimate the sinks of CO 2 from silicate weathering and from the weathering and burial of organic carbon resulting from Himalayan uplift. Here we show that Neogene CO 2 consumption from the net burial of organic carbon during Himala-yan sediment deposition was 2-3 times that resulting from the weathering of Himalayan silicates. Thus the dominant effect of Neogene Himalayan erosion on the carbon cycle is an increase in the amount of organic carbon in the sedimentary reservoir, not an increase in silicate weathering fluxes. Silicate weathering is typically incongruent, yielding both a solute and a secondary mineral phase, so direct evidence of chemical weathering can be found in the record of secondary minerals in sedimentary basins. The Bengal Fan and Ganges-Brahmaputra (GB) delta contain a huge volume of sediment derived from erosion of the India-Asia collision zone, with 6 X 10 6 km 3 deposited in the past 20 Myr (ref. 8). Isotopic data for Nd, Sr and O from Bengal Fan sediments show that the source for over 80% of the detritus since 20 Myr ago has been the high-grade metasedimentary rocks of the High Himalayan crystalline (HHC) sequence 9. Clastic and carbo-nate sediments of the Precambrian Lesser Himalaya (LH) and Palaeozoic-Mesozoic Tethyan Himalaya (TH) are the other important sources of sediment to the Bengal Fan during the Neogene.