HR: 08:55h
AN: GP31A-04 [PDF]
TI: Magnetite dissolution in siliceous sediments
AU: * Florindo, F
EM: florindo@ingv.it
AF: Istituto Nazionale di Geofisica Vulcanologia, Via di Vigna Murata 605, Rome, 00143
Italy
AU: * Florindo, F
EM: florindo@ingv.it
AF: Southampton Oceanography Centre, University of Southampton, European Way, Southampton, S014 3ZH
United Kingdom
AU: Roberts, A P
EM: arob@soc.soton.ac.uk
AF: Southampton Oceanography Centre, University of Southampton, European Way, Southampton, S014 3ZH
United Kingdom
AU: Palmer, M R
EM: martin.r.palmer@soc.soton.ac.uk
AF: Southampton Oceanography Centre, University of Southampton, European Way, Southampton, S014 3ZH
United Kingdom
AB:
Magnetite dissolution, and consequent loss of magnetization, is widely observed in reducing sedimentary environments, where
the decrease in Eh-pH values with depth is driven by bacterially mediated degradation of organic carbon. We have observed low
magnetizations in sediments with elevated porewater silica concentrations that arise from diagenesis of biogenic silica
and/or silicic volcanic ash. These depletions in magnetization are greater than can be accounted for by dilution with
magnetite-poor sediments and suggest that post-depositional destruction of magnetite has occurred. Biosiliceous sediments
usually also contain elevated concentrations of organic carbon, which makes it difficult to separate organic-carbon-related
magnetite dissolution from other possible mechanisms for magnetite dissolution. However, the extent of magnetite dissolution
in the sedimentary sequences that we have studied is not obviously related to the redox-state of the environment. This
suggests that other mechanisms might have given rise to magnetite dissolution in these siliceous sediments. Thermodynamic
calculations indicate that magnetite is unstable under conditions of elevated dissolved silica concentrations (and
appropriate Eh-pH conditions) and predict that magnetite will break down to produce iron-bearing smectite. A survey of
magnetic susceptibility and pore water geochemical data from widely distributed Ocean Drilling Program sites supports this
observed link between high dissolved silica concentrations and low magnetic susceptibilities. This observed link also holds
for environments with low biogenic silica productivity (and low organic carbon content), but with high interstitial silica
concentrations due to dissolution of silicic volcanic ashes. Dissolution of magnetite is therefore predicted to be a common
feature of siliceous sedimentary environments.
DE: 1045 Low-temperature geochemistry
DE: 1050 Marine geochemistry (4835, 4850)
DE: 1512 Environmental magnetism
DE: 1519 Magnetic mineralogy and petrology
DE: 1540 Rock and mineral magnetism
SC: Geomagnetism and Paleomagnetism [GP]
MN: 2003 Fall Meeting