Friday 10 August 2012

Principles of Crystal Chemistry


Principles of Crystal Chemistry


Our discussion of bonding led us to conclude that the bond character is determined primarily by the electronic configurations and electronegativity values of the combining elements, whereas the crystal structure (which controls the shape and system of the crystal) is a function of the plane lattice and the coordination number(s) (C.N.).

I- Coordination Number

1-      Is the number of nearest neighbors in a crystal structure. It depends on the radius ratio + type of hybridization in covalent ones (Table 1) and the radius ratio in ionic structures (Table 2).
2-      Whereas the C.N. is strongly controlled by the radius ratio, the radius of an ion (or atom) may (and usually does) change as a function of the C.N. (Fig. 1; Table 3). Other factors influencing the size of an ion are its charge, the atomic number of its element, and the “shielding” effect of some electrons, especially those of the penultimate shell. Of particular interest is the “lanthanide contraction”.
3-      Coordination numbers are usually 2, 3, 4, 6, 8, or 12. C.N.’s of 5, 7, 9, 10, or 11 are much less common, but can occur in some cases!

Some Examples of C.N. (Fig. 2)
Halite: NaCl
Na : Cl = 6 : 6

Sphalerite: ZnS

Zn : S = 4 : 4

Fluorite: CaF2

Ca : F = 8 : 4

II- Structure Controls for minerals with metallic bonding:
·         Bonding takes place between electropositive elements of similar electronegativities.
·         Radii of the combining elements are also similar; radius ratio (rA/rB) @ 1.
·         Three types of packing (Fig. 3):
1.      Hexagonal close packing “HCP”: layers arranged in the pattern: ABAB. C.N. = 12.
2.      Cubic close packing “CCP”: layers arranged in the pattern: ABCABC. C.N. = 12.
3.      Body centered cubic packing: lower density structure; C.N. is always 8.
·     Close packing results in the high density observed for metals and alloys.

III- Structure controls for minerals with covalent bonding:
·         Hybridization of the orbitals forces this type of bonding to have a strong directional character.
·         Because of hybridization, the covalent radius of an element will be different from its ionic or metallic radii.
·         The structure of the mineral will be controlled by (i) the covalent radii of the elements; (ii) the type of hybrid resulting (Table 1); same factors that affect the C.N.!


IV- Structure controls for minerals with ionic bonding:

Pauling’s Rules for ionic compounds:

Rule 1:-

Cation – anion distance in a structure determined by radius sums, C.N.’s determined from r+/r- (Table 1).

For this rule, the following points are very important:
1-      The r+/r- limiting values for the different coordination numbers are derived by simple rules of geometry and trigonometry (Figs 4 & 5).
2-      If the r+/r- falls very close to one of the limiting values (e.g. 0.414), then the same compound may have two different structures (in this case, one with a C.N. of 4; the other with 6). This may result in polymorphism.
3-      Because Oxygen is the most abundant element in the Earth’s crust, and because it is strongly electronegative, most of the common rock-forming minerals have a significant ionic character. Accordingly, relative to Oxygen, elements will have a fairly predictable size and coordination number. Common coordination numbers for some cations are listed in Table 3. Please make a strong effort to remember these!

Rule 2:

Electrostatic valency principle: The total strength of the valency bonds that reach an anion from all the neighboring cations is equal to the charge of the anion (Fig. 6).

Electrostatic valency = Z/C.N.                       (Where Z is the charge of the cation).
Strength of bond = sum of its electrostatic valencies.

This rule is useful for constraining the types of polyhedra in a crystal structure.

Example: Find the # of Ca2+ ions bonded to O in the structure of calcite, knowing that the C.N. of Ca2+ (to O) = 6. Use Pauling’s second rule knowing that the carbonate radical has a trigonal planar structure.

e.s.v. for CO3-2 = Z (for C)/ C.N. = 4/3
e.s.v. for Ca 2+ = 2/6 = 1/3
Let x be the # of Ca2+ linked to O in Calcite,
\x . 1/3 + 4/3 = 2
Þ x = 2.

Example 2:
e.s.v for Si – O = 4/4 = 1
            = ½ of 2 Þ (2 Si can link to one O)
\2 or more tetrahedra can become linked at their apex by sharing one of their oxygens.

This process, by which different tetrahedra are linked to each other, results in the formation of rings, chains, sheets or frameworks, and is known as polymerization.

Types of ionic compounds according to electrostatic bond strength:

1-      Isodesmic compounds: Crystals or compounds in which all bonds are of equal strength are known as isodesmic (Example: the Spinel group (MgAl2O4)). In the case of the spinels, there are 2 polyhedra. The contribution of oxygen to each of these two polyhedra is 2, which makes the mineral isodesmic. Isodesmic compounds are characterized by high symmetries, crystallizing in the cubic, tetragonal or hexagonal systems. Oxides, halides, and hydroxides are isodesmic.

2-      Anisodesmic compounds: Are ones that have different bonds with different bond strengths. Sulfates and carbonates are anisodesmic. Carbonates, phosphates and sulfates fall into this group.

3-      Mesodesmic compounds: Are ones in which one particular cation always accounts for half of the total bond strengths in the compound. Silicates are mesodesmic.

Rule 3:
Polyhedra are usually joined at their corners; joining at their edges is much less common, whereas joining by sharing faces is rare (Fig. 7). Sharing of faces among polyhedra generally decreases the stability of the structure, especially if the centers of these polyhedra are occupied by cations with high valency and small coordination numbers. This effect is especially large when the radius ratio approaches the lower stability limit of the polyhedron.

Rule 4:
In a crystal with different cations, those cations with high valency and small C.N. tend not to share polyhedral elements with each other. However, if they do, the polyhedra become distorted. This is necessary to minimize cation – cation repulsion.

Rule 5:
The number of essential sites in a crystal structure that are substantially different (i.e. with differences in size and coordination) tends to be small. On the other hand, many of these sites may be occupied by different ions, leading to the phenomenon of “isomorphism”. This is known as the “principle of parsimony”.

Example: Amphiboles are minerals that often contain 13 different elements (or more!), and are characterized by the formula:
A0-1B2C5T8O22(OH,F,Cl)2
Although this group of minerals has a large # of different sites (relative to most other minerals), there are only 5 such “different” sites:
A: occupied by K or Na in 8 or 12 coordination
B sites: filled with Na, Li, Ca, Fe2+, Mg and Mn2+ in six or 8 coordination
C sites: filled with Mg, Fe2+, Mn, Al, Fe3+, or Ti all in six coordination
T sites: filled with Si or Al, in 4 coordination; and finally,
Hydroxyl sites: where F and Cl may substitute.


IV- Calculation of the number of formula units per unit cell “f”:
Density of mineral = weight of unit cell/volume of unit cell (V)
Weight of the unit cell = molecular weight . # of formula units in the cell (f)/ # of formula units in 1 mole.
The # of formula units in 1 mole is Avogadro’s # (A = 6.023 . 1023).

D = Mol. Wt . f/A. V
f = D . A . V/Mol. Wt.

V- Isostructuralism and Isotypism:
Isotypes: Two minerals are considered isotypes if they have the same structures (arising from similar C.N.’s and r+/r- values), but otherwise have no chemical relations between them. Examples: Galena and Halite, NaNO3 and CaCO3, Stishovite and Rutile.

Isostructural groups: Minerals are considered isostructural if they have the same structures (same C.N.’s), and same anionic group (but obviously different cations, and hence different r+/r- values. Examples are members of the aragonite group (aragonite, strontianite, witherite, and cerussite).

VI- Some important crystal structures

1-      Diamond (covalent): F 41/d  2/m; C.N = 4 (Fig. 8)
2-      Graphite (covalent): P 63/m m c; C.N. = 3 (Fig. 9)
3-      Sphalerite: F  3 m, C.N. = 4 (Fig. 10)
4-      Halite (ionic): F 4/m  2/m, C.N. = 6 (Fig. 11)
5-      Pyrite (ionic/metallic): P 2/m , C.N. = 12:6 (Fig. 12)
6-      CsCl (ionic): P 4/m  2/m, C.N. = 8 (Fig. 13)
7-      Fluorite (ionic): F 4/m  2/m, C.N. = 8:4 (Fig. 14)
8-      Calcite: P  2 m, C.N. = 6:6:2 (Fig. 15).
9-      Spinel: F 41/d  2/m, C.N.: Mg:O = 4:1, Al:O = 6:3, Mg:Al = 4:2 (Fig. 16)
10-    Perovskite: P 21/c 21/m 21/n, C.N.: Ca:O = 12:4, Ti:O = 6:2, Ca:Ti = 8:8 (Fig. 17)

VII- Structure of Silicates

·         The bond between Si and O has a mixed character, and is approximately 50% ionic and 50% covalent.
·         Remember, silicate structures are mesodesmic.
·         Si is tetravalent, whereas O is divalent. Therefore, if both elements are to form an electrically neutral compound, it would be SiO2 (equivalent mineral would be quartz or one of its polymorphs).
·         A Si atom may also combine with two more oxygens to form a negatively charged group (SiO4)-4. This group will always be tetrahedral as dictated by the radius ratio of Si to O. This is the basic building block of all silicate structures.
·         For this group to form an electrically neutral mineral, it needs to combine with two divalent cations, one monovalent and one trivalent cation, or four monovalent cations, of a specific size or size range. The most common minerals with this structure are olivines: (Fe,Mg)2SiO4 formed of single tetrahedra. Separate tetrahedra that are adjacent to one another may polymerize by sharing Oxygens, giving rise to more complex structures or networks of tetrahedra with different charges.
·         The reason for polymerization of tetrahedra can be understood from applying Pauling’s second rule; the e.s.v. between Si and O = 4/4 =1, which is equivalent to ½ the bonding strength of O-2. Two tetrahedra may therefore be linked through a bridging or shared oxygen.
·         The degree of polymerization will depend on the conditions of formation or crystallization of the silicate mineral, and may be used to subdivide silicates into six groups (Fig. 18; Table 4).

Types of silicate structures:

(1) Nesosilicates (orthosilicates): with isolated tetrahedra linked by bonds sharing oxygen through cations. Example: olivine.

(2) Sorosilicates: consisting of two tetrahedra sharing one oxygen (Si2O7)-6. Example: hemimorphite Zn4Si2O7(OH)2.H2O

(3) Cyclosilicates: more polymerized, consisting of closed rings of 3, 4 or 6 tetrahedra each sharing 2 oxygens (Si3O9)-6, (Si4O12)-8, (Si6O18)-12. Example: tourmaline

(4) Inosilicates: consisting of single chains of tetrahedra, each sharing two oxygens (Si2O6)-4 (e.g. pyroxenes), or double chains of tetrahedra in which each tetrahedron shares three oxygens (Si4O11)-6 (e.g. amphiboles).

(5) Phyllosilicates: Continuous sheets of hexagonal networks of tetrahedra formed by sharing three oxygens (Si4O10)-4. Individual sheets are bonded to each other by the "interlayer cations", resulting in the minerals developing excellent cleavage which separates it into individual sheets. Example: micas.

(6) Tectosilicates: Three-dimensional networks of tetrahedra, each sharing all four of its oxygens (e.g. Feldspars).

It should be noted that Al+3 may substitute for Si+4 in many of the above structures, as both cations are of comparable sizes. This substitution increases the negative charge of the overall structural group, and must be compensated for in any mineral by another substitution that will increase the total number of positive charges to maintain electrical neutrality.




X-Ray Fluorescence (XRF)


X-Ray Fluorescence (XRF)
Karl Wirth, Macalester College and Andy Barth, Indiana University~Purdue University, Indianapolis
What is X-Ray Fluorescence (XRF)
An X-ray fluorescence (XRF) spectrometer is an x-ray instrument used for routine, relatively non-destructive chemical analyses of rocks, minerals, sediments and fluids. It works on wavelength-dispersive spectroscopic principles that are similar to an electron microprobe (EPMA). However, an XRF cannot generally make analyses at the small spot sizes typical of EPMA work (2-5 microns), so it is typically used for bulk analyses of larger fractions of geological materials. The relative ease and low cost of sample preparation, and the stability and ease of use of x-ray spectrometers make this one of the most widely used methods for analysis of major and trace elements in rocks, minerals, and sediment.
Fundamental Principles of X-Ray Fluorescence (XRF)
The XRF method depends on fundamental principles that are common to several other instrumental methods involving interactions between electron beams and x-rays with samples, including: X-ray spectroscopy (e.g., SEM - EDS), X-ray diffraction (XRD), and wavelength dispersive spectroscopy (microprobe WDS).

The analysis of major and trace elements in geological materials by x-ray fluorescence is made possible by the behavior of atoms when they interact with radiation. When materials are excited with high-energy, short wavelength radiation (e.g., X-rays), they can become ionized. If the energy of the radiation is sufficient to dislodge a tightly-held inner electron, the atom becomes unstable and an outer electron replaces the missing inner electron. When this happens, energy is released due to the decreased binding energy of the inner electron orbital compared with an outer one. The emitted radiation is of lower energy than the primary incident X-rays and is termed fluorescent radiation. Because the energy of the emitted photon is characteristic of a transition between specific electron orbitals in a particular element, the resulting fluorescent X-rays can be used to detect the abundances of elements that are present in the sample.
X-Ray Fluorescence (XRF) Instrumentation - How Does It Work?
The analysis of major and trace elements in geological materials by XRF is made possible by the behavior of atoms when they interact with X-radiation. An XRF spectrometer works because if a sample is illuminated by an intense X-ray beam, known as the incident beam, some of the energy is scattered, but some is also absorbed within the sample in a manner that depends on its chemistry. The incident X-ray beam is typically produced from a Rh target, although W, Mo, Cr and others can also be used, depending on the application.
When this primary X-ray beam illuminates the sample, it is said to be excited. The excited sample in turn emits X-rays along a spectrum of wavelengths characteristic of the types of atoms present in the sample. How does this happen? The atoms in the sample absorb X-ray energy by ionizing, ejecting electrons from the lower (usually K and L) energy levels. The ejected electrons are replaced by electrons from an outer, higher energy orbital. When this happens, energy is released due to the decreased binding energy of the inner electron orbital compared with an outer one. This energy release is in the form of emission of characteristic X-rays indicating the type of atom present. If a sample has many elements present, as is typical for most minerals and rocks, the use of a Wavelength Dispersive Spectrometer much like that in an EPMA allows the separation of a complex emitted X-ray spectrum into characteristic wavelengths for each element present. Various types of detectors (gas flow proportional and scintillation) are used to measure the intensity of the emitted beam. The flow counter is commonly utilized for measuring long wavelength (>0.15 nm) X-rays that are typical of K spectra from elements lighter than Zn. The scintillation detector is commonly used to analyze shorter wavelengths in the X-ray spectrum (K spectra of element from Nb to I; L spectra of Th and U). X-rays of intermediate wavelength (K spectra produced from Zn to Zr and L spectra from Ba and the rare earth elements) are generally measured by using both detectors in tandem. The intensity of the energy measured by these detectors is proportional to the abundance of the element in the sample. The exact value of this proportionality for each element is derived by comparison to mineral or rock standards whose composition is known from prior analyses by other techniques.
Applications
X-Ray fluorescence is used in a wide range of applications, including
  • research in igneous, sedimentary, and metamorphic petrology
  • soil surveys
  • mining (e.g., measuring the grade of ore)
  • cement production
  • ceramic and glass manufacturing
  • metallurgy (e.g., quality control)
  • environmental studies (e.g., analyses of particulate matter on air filters)
  • petroleum industry (e.g., sulfur content of crude oils and petroleum products)
  • field analysis in geological and environmental studies (using portable, hand-held XRF spectrometers)
X-Ray fluorescence is particularly well-suited for investigations that involve
  • bulk chemical analyses of major elements (Si, Ti, Al, Fe, Mn, Mg, Ca, Na, K, P) in rock and sediment
  • bulk chemical analyses of trace elements (in abundances >1 ppm; Ba, Ce, Co, Cr, Cu, Ga, La, Nb, Ni, Rb, Sc, Sr, Rh, U, V, Y, Zr, Zn) in rock and sediment - detection limits for trace elements are typically on the order of a few parts per million
X-ray fluorescence is limited to analysis of
  • relatively large samples, typically > 1 gram
  • materials that can be prepared in powder form and effectively homogenized
  • materials for which compositionally similar, well-characterized standards are available
  • materials containing high abundances of elements for which absorption and fluorescence effects are reasonably well understood
In most cases for rocks, ores, sediments and minerals, the sample is ground to a fine powder. At this point it may be analyzed directly, especially in the case of trace element analyses. However, the very wide range in abundances of different elements, especially iron, and the wide range of sizes of grains in a powdered sample, makes the proportionality comparison to the standards particularly troublesome. For this reason, it is common practice to mix the powdered sample with a chemical flux and use a furnace or gas burner to melt the powdered sample. Melting creates a homogenous glass that can be analyzed and the abundances of the (now somewhat diluted) elements calculated.
Strengths and Limitations of X-Ray Fluorescence (XRF)?
Strengths
X-Ray fluorescence is particularly well-suited for investigations that involve:
  • bulk chemical analyses of major elements (Si, Ti, Al, Fe, Mn, Mg, Ca, Na, K, P) in rock and sediment
  • bulk chemical analyses of trace elements (>1 ppm; Ba, Ce, Co, Cr, Cu, Ga, La, Nb, Ni, Rb, Sc, Sr, Rh, U, V, Y, Zr, Zn) in rock and sediment
Limitations
In theory the XRF has the ability to detect X-ray emission from virtually all elements, depending on the wavelength and intensity of incident x-rays. However...
  • In practice, most commercially available instruments are very limited in their ability to precisely and accurately measure the abundances of elements with Z<11 in most natural earth materials.
  • XRF analyses cannot distinguish variations among isotopes of an element, so these analyses are routinely done with other instruments (see TIMS and SIMS).
  • XRF analyses cannot distinguish ions of the same element in different valence states, so these analyses of rocks and minerals are done with techniques such as wet chemical analysis or Mossbauer spectroscopy.
User's Guide - Sample Collection and Preparation
Virtually any solid or liquid material can be analyzed, if adequate standards are available. For rocks and minerals, typical commercial instruments require a sample constituting at least several grams of material, although the sample collected may be much larger. For XRF chemical analyses of rocks, samples are collected that are several times larger than the largest size grain or particle in the rock. This initial sample then suffers a series of crushing steps to reduce it to an average grain size of a few millimeters to a centimeter, when it can be reduced by splitting to a small representative sample of a few tens to hundreds of grams. This small sample split is then ground into a fine powder by any of a variety of techniques to create the XRF sample. Care must be taken particularly at this step to be aware of the composition of the crushing implements, which will inevitably contaminate the sample to some extent.
Data Collection, Results and Presentation
  • X-Ray spectrum
  • Data table
  • Detection limits
  • Precision
  • Accuracy
  • Database and Plotting
  • Evaluation of Data Quality (flyers, trends, discriminant fields)
  • Geochemical Plots
Literature
The following literature can be used to further explore X-Ray Fluorescence (XRF)
The following literature can be used to further explore the XRF technique and uses of XRF data.
  • Fitton, G., 1997, X-Ray fluorescence spectrometry, in Gill, R. (ed.), Modern Analytical Geochemistry: An Introduction to Quantitative Chemical Analysis for Earth, Environmental and Material Scientists: Addison Wesley Longman, UK.
  • Potts, P.J., 1987, A Handbook of Silicate Rock Analysis: Chapman and Hall.
  • Rollinson, H., 1993, Using Geochemical Data: Evaluation, Presentation, Interpretation: John Wiley, NY.
Related Links
For more information about X-Ray Fluorescence (XRF) follow the links below.
General information about XRF principles and applications:

For more information about XRF laboratories follow the links below:
For information on the availability of standards follow the links below:
Sources of Geochemical Data
  • EarthChem - an international database that combines the assets of PetDB, NavDat, and GeoRoc. Search the database for analyses according to location, rock type, chemical parameters, or references in the literature.
  • Geochemical Earth Reference Model (GERM) contains several databases, geochemistry of all reservoirs in the Earth, modern paleo, rock and geomagnetic data
Teaching Activities and Resources
Teaching activities, labs, and resources pertaining to X-Ray Fluorescence (XRF).
For examples of the use of XRF data in teaching activities, check out:
Other Resources for Teaching Whole Rock Geochemistry (major and trace elements)

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