Effect of Intense Weathering and Postdepositional Degradation of Organic Matter on Hg/TOC Proxy in Organic‐rich Sediments and its Implicationsfor Deep‐Time Investigations

American Geophysical Union (AGU) - Tập 21 Số 2 - 2020
Guillaume Charbonnier1, Thierry Adatte1, Karl B. Föllmi1, Guillaume Suan2
1Institute of Earth Sciences, Géopolis, University of Lausanne, Lausanne, Switzerland
2Université de Lyon, UCBL, ENSL, CNRS, LGL‐TPE Villeurbanne France

Tóm tắt

AbstractMercury (Hg) enrichments in sediments are increasingly used as tracer for distal volcanism in deep‐time investigations. The impact of changes in organic‐matter deposition and preservation on sedimentary Hg sequestration is, however, poorly understood. In this study, we evaluate the potential role of intense weathering and postdepositional organic‐matter degradation on the Hg/TOC proxy in sediments. For this, we investigate weathering profiles in organic‐rich sediments from lowermost Toarcian sediments (T‐OAE; Lafarge cement quarry, France) and organic‐rich deposits from the uppermost Cenomanian‐lowermost Turonian Bonarelli level (OAE2; Furlo and Monte Velo, Italy; Manilva and El Chorro, Spain). The comparison of Hg data along weathering profiles in lowermost Toarcian sediments indicates that recent intense oxidation of the originally organic‐rich deposits has removed up to 89% of the Hg signal. The organic‐rich sediments of the Furlo and Manilva sections are characterized by lower Hg/total organic carbon (TOC) ratios, which suggest important Hg scavenging by organic matter (OM) deposition. At the opposite, in equivalent successions, three significant positive Hg/TOC excursions persist at El Chorro and Monte Velo. These samples exhibit low Hydrogen Index (HI) values, which plot in the field of type‐III OM. This resulted from postdepositional degradation of marine OM type II to type III, which largely modified the amount and the quality of OM. Consequently, the recorded Hg/TOC ratios do not reflect original Hg drawdown but postdepositional oxidation, suggesting that extreme care is needed in the evaluation of the history of OM preservation when using Hg as a proxy for volcanic activity.

Từ khóa


Tài liệu tham khảo

Arthur M., 1982, Nature and origin of Cretaceous carbon‐rich facies, 7

10.1006/cres.1998.0126

10.2516/ogst:2001013

10.1073/pnas.1709070114

10.1016/0037-0738(93)90133-P

10.1146/annurev-earth-050212-124107

10.1016/0037-0738(70)90019-9

10.1016/0025-3227(81)90113-4

10.1130/G38207.1

10.1016/j.palaeo.2018.06.013

10.1038/srep40808

Coccioni R.(1996).The Cretaceous of the Umbria‐Marche Apennines (central Italy) Wiedmann symposium cretaceous stratigraphy paleobiology and paleobiogeography the Umbria–Marche Apennines (Central Italy).Tübingen 7‐10.

Dercourt J., 1993, Atlas Tethys Paleoenvironmental maps

10.1021/es305071v

10.1016/S0016-6995(09)90011-0

10.2516/ogst:1985035

10.1016/j.earscirev.2019.102932

10.1128/AEM.72.1.457-464.2006

10.1130/G37451.1

10.1016/j.gca.2008.12.012

10.1038/s41598-017-05524-5

Grasby S. E., 2015, Mercury anomalies associated with three extinction events (Capitanian crisis, latest Permian extinction and the Smithian/Spathian extinction) in NW Pangea, Geological Magazine, 13

10.1016/j.chemgeo.2013.05.022

10.1130/G38487.1

10.1021/es2010072

10.1039/9781849730822-00365

Hunt J. M., 1995, Petroleum Geochemistry and Geology, 408

10.1029/2009GC002788

10.1130/G38940.1

10.1016/j.gr.2017.12.002

10.1016/0009-2541(88)90045-9

10.2516/ogst:1998036

Leythäuser D., 1973, Effects of weathering on organic matter in shales, Geochimica et Cosmochimica Acta, 37, 120

Lin C.‐C., 2012, Environmental chemistry and toxicology of mercury, 155

10.1016/0016-7037(91)90494-P

10.1006/cres.1999.0146

Martín‐Algarra A.(1987).Evolución geológica alpina del contacto entre las Zonas Internas y las Zonas Externas de la Cordillera Bética. PhD Thesis Universidad de Granada Spain 1171 pp.

10.1029/2007PA001435

10.1016/j.cretres.2006.09.003

10.1130/G23475A.1

10.1021/es070408x

10.1126/science.1230667

10.1130/G37997.1

10.2475/08.2018.01

Percival L. M. E. Ruhl M. Hesselbo S. P. Jenkyns H. C. Mather T. A. &Whiteside J. H.(2017).Mercury evidence for pulsed volcanism during the end‐Triassic mass extinction.PNAS.https://doi.org/10.1073/pnas.1705378114

10.1016/j.epsl.2015.06.064

10.1016/S0146-6380(00)00014-0

10.5194/acpd-10-4719-2010

10.1016/j.atmosenv.2003.07.011

10.1130/G40233.1

10.1016/j.palaeo.2018.01.008

10.1130/G32596.1

10.3989/egeol.96523-4260

10.1002/2017GC007153

Selin N. E., 2008, Global 3‐D land‐ocean‐atmosphere model for mercury: Present‐day versus preindustrial cycles and anthropogenic enrichment factors for deposition, Global Biogeochemical Cycles, 22, 1

10.1016/j.epsl.2019.01.028

10.1016/j.cretres.2016.05.006

10.1016/j.palaeo.2014.08.013

10.1016/j.palaeo.2013.07.019

10.1130/G37683C.1

10.1021/es902186s

10.1017/S0016756812000970

10.1016/j.epsl.2018.11.029

10.1038/ncomms11147

10.1007/978-3-642-87813-8

10.1016/j.epsl.2019.02.026

Winterer E. L., 1981, Subsidence and sedimentdtion on a Jurassic passive continental margin, southern Alps, Italy, American Association of Petroleum Geologists Bulletin, 65, 3944421

10.1038/220173a0

10.1016/j.chemgeo.2012.06.001