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Nanoscale characterization of the ‘critical zone’ of<br />
naturally weathered minerals by FIB and TEM<br />
David Brown, Mark Hodson, Maureen MacKenzie,<br />
Roland Hellmann, Caroline Smith & Martin Lee
Outline<br />
• The critical zone: models for feldspar weathering<br />
• Materials<br />
• Focused Ion Beam (FIB) technique<br />
• Results<br />
• Integration with XPS<br />
Aim<br />
• FIB-TEM investigation of mineral weathering:<br />
– Grain surface topography; structure; composition;<br />
reaction products<br />
– How do feldspars weather in natural systems?
Models for feldspar weathering
Models for feldspar weathering
Models are difficult to test:<br />
• Reactive sites at the bottom of etch pits<br />
• Beneath reaction products or organic/inorganic debris.
Advantages of FIB<br />
• Previous techniques for TEM foil preparation destructive:<br />
– (e.g. microtome, Ar ion milling)<br />
• FIB allows site specific cross sectional slices to be<br />
prepared, through the critical zone<br />
• Direct observation of layers?
Materials<br />
• Naturally weathered alkali feldspars from post-glacial<br />
soils<br />
• Shap (north-west England)<br />
– Acidic (pH 3.4) & waterlogged peat.<br />
Grain surfaces free of weathering<br />
products.<br />
• Glen Feshie (Cairngorm, Scotland)<br />
– Soil chronosequence (80 yr-1 kyr).<br />
Grain surfaces have abundant<br />
weathering products.
FIB Technique
Beam Damage<br />
• Sample can be damaged by<br />
the beam<br />
– 1 µm Pt strip<br />
• Au coating essential<br />
– Amorphisation of the<br />
sample<br />
• >85 nm of Au required<br />
• Supported by SRIM<br />
modelling (
Amorphous layers?<br />
• No amorphous layers recognised on pH1 laboratory<br />
dissolution experiments and on naturally weathered<br />
samples<br />
• Previous experiments – 10’s of nm, where are the layers?
• Can Au coating<br />
(by sputtering)<br />
damage sample?<br />
• Grains partially<br />
covered by resin<br />
• No amorphous<br />
material<br />
• Evaporated Au<br />
• No amorphous<br />
material<br />
Sputtering Damage?<br />
Pt<br />
Au<br />
Resin<br />
Au<br />
Crystalline<br />
feldspar<br />
Pt
How are the feldspars<br />
weathering?
Shap alkali feldspars: microtopography<br />
(001)<br />
Coherent<br />
albite<br />
lamellae<br />
• Free of reaction products, but pitted<br />
• Corrugations at sites of coherent albite lamellae
Shap alkali feldspars: microtopography<br />
• Albite dissolves more rapidly<br />
– Composition or magnitude of elastic coherency strain<br />
– Higher strain on albite; dissolves faster
Shap alkali feldspars: etch pit networks<br />
• Pits extend into grain interiors;<br />
• “Etch tubes” - fluids exploit nanotunnels (Fitz Gerald et al. 2006)
Shap alkali feldspars: microstructure of pit walls<br />
• Pits extend along former albite lamellae into the grain interior
Shap alkali feldspars: microstructure of pit walls<br />
• Pit walls crystalline throughout; no amorphous layers
Glen Feshie<br />
• Microbes, reaction products<br />
• Pits dug in river terraces
Glen Feshie feldspars: weathering products<br />
• Some amorphous weathering products; others 1.0 nm<br />
Fe-aluminosilicate clays
Glen Feshie (80 yr): clay-feldspar interface<br />
• Poorly crystalline material occurs between clays and<br />
grain surface; little evidence for feldspar recrystallization:
Glen Feshie (1.1 kyr): reconstruction at grain surfaces<br />
• Reaction products may have a gradational interface with<br />
feldspar, possible interaction?
Glen Feshie (1.1 kyr): crystallization of clays<br />
• Reaction products have crystallised K-aluminosilicates (illite)
Conclusions<br />
• Shap weathers by stoichiometric<br />
dissolution<br />
– Centred on reactive sites<br />
controlled by composition and/or<br />
strain<br />
– Leached layers must be < ~2 nm<br />
• Glen Feshie weathering products<br />
grow passively on grains from bulk<br />
waters<br />
– Some amorphous<br />
– Crystallises to form clays
XPS on Shap feldspars<br />
• 15°, 45°and 90°= 2.5, 6 and 9 nm<br />
• Si enriched, K and Na depleted<br />
~1-2 nm<br />
• Surface chemistry modified<br />
without destroying feldspar<br />
framework (leaching of alkalis)<br />
• Layer is present (1-2 nm) but<br />
difficult to resolve on TEM.<br />
XPS data represents “dilution<br />
of result” with depth
TEM layers: a cautionary tale<br />
• Previous TEM layers (tens of nm thick):<br />
– Probable beam damage!<br />
Amorphous<br />
Au & Pt Au & Pt<br />
50 nm 50 nm