Geology 114 Lecture Notes
Introduction
Read Chapter 1 of Nesse
atoms → molecules → crystals → rocks → Earth
see http://darkwing.uoregon.edu/~cashman/GEO311/311pages/L1-Intro_pic_files/image014.gif
Strategic Minerals and Metals
Atoms and Elements
Read Chapter 3 of Nesse
Element: A form of matter
than cannot be broken down by conventional heating or cooling
Common mineral-forming elements
Elemental composition of the whole Earth and the crust (the
outermost solid layer):
|
element |
whole Earth |
crust |
mineral |
|
O |
29% |
46% |
most
minerals |
|
Si |
15% |
28% |
silicates |
|
Al |
1% |
8% |
feldspar |
|
Fe |
35% |
6% |
pyroxene,
amphibole |
|
Ca |
1% |
4% |
plagioclase |
|
Na |
<1% |
2% |
feldspar |
|
Mg |
11% |
2% |
olivine |
|
K |
<1% |
2% |
K-feldspar |
|
S |
<3% |
<1% |
pyrite |
|
Ni |
2% |
<1% |
olivine |
composition of Earth’s crust
the arrangement of elements in columns relates to the similarities in
their chemical behavior:
noble gases
halogens
metals
alkaline earth metals
alkali metals
Atoms
nucleus
Atom: The smallest particle
that retains the chemical properties of an element; composed of (isotopes are
atoms, but every isotope is not an element)
proton: electric charge +1, 1.00728 amu
neutron: electric charge 0, 1.00867 amu
electron: electric charge –1, 0.00055 amu
(insignificant)
For
example, Li has an atomic number of 3, meaning 3 protons (and 3
electrons, if neutral); if it is 7Li, it has a mass of 7 and thus 4 neutrons
electrons fill orbital levels around the nucleus: 2 in the first level,
8 in the second, and so on
the position of an element in the periodic table relates to the number of
electrons in the outer orbital
Structure of Atoms
The
four electron shells surrounding the nucleus are named—with increasing distance
and energy—K, L, M, and N shells. Each shell is split into subshells, labeled s, p, d, and f. An s subshell consists
of one s orbital (with 2 electrons),
a p subshell consists of up to 3 p orbitals (6 electrons), and a d subshell consists of up to 5 d orbitals (10 electrons).
shell
(±) K L L M M M N N
Z element 1s 2s 2p 3s 3p 3d 4s 4p
1 H 1
2 He 2 (1 shell is full)
3 Li 2 1
4 Be 2 2
5 B 2 2 1
6 C 2 2 2
7 N 2 2 3
8 O 2 2 4
9 F 2 2 5
10 Ne 2 2 6 (2
shell is full)
11 Na 2 2 6 1
12 Mg 2 2 6 2
13 Al 2 2 6 2 1
14 Si 2 2 6 2 2
15 P 2 2 6 2 3
16 S 2 2 6 2 4
17 Cl 2 2 6 2 5
18 Ar 2 2 6 2 6 (3 shell is full)
19 K 2 2 6 2 6 1
20 Ca 2 2 6 2 6 2
21 Sc 2 2 6 2 6 1 2
22 Ti 2 2 6 2 6 2 2
23 V 2 2 6 2 6 3 2
24 Cr 2 2 6 2 6 4 2
25 Mn 2 2 6 2 6 5 2
26 Fe 2 2 6 2 6 6 2
27 Co 2 2 6 2 6 7 2
28 Ni 2 2 6 2 6 8 2
29 Cu 2 2 6 2 6 9 2
30 Zn 2 2 6 2 6 10 2
31 Ga 2 2 6 2 6 10 2 1
32 Ge 2 2 6 2 6 10 2 2
33 As 2 2 6 2 6 10 2 3
34 Se 2 2 6 2 6 10 2 4
35 Br 2 2 6 2 6 10 2 5
36 Kr 2 2 6 2 6 10 2 6 (4
shell is full)
Ions
elements tend to gain or lose
electrons to acquire the configuration of a noble gas
cation: ion w/ excess + charge
anion: ion w/ excess — charge
typical oxidation states: http://www.wsu.edu/~wherland/#Radii or http://en.wikipedia.org/wiki/Ionic_bond
this propensity was termed electronegativity by Linus Pauling; e.g., Li has an electronegativity of 1 and F is 4
Cosmochemistry and the production of elements
(for more see http://en.wikipedia.org/wiki/Stellar_nucleosynthesis)
The birth of matter in the universe
began about 13.7 Ga, judged by tracing expanding galaxies (groups of stars)
back to a common origin in the Big Bang.
After 1 m.y., the universe had cooled sufficiently (3000K) for H and He to form
from subatomic particles.
These elements aggregated to form stars
via gravitational attraction after 200 Myr; stars are 75 wt% H, 22 wt% He, and
3% heavier elements.
Carbon burning
12C + 12C –> 20Ne or 23Na or 23Mg
or 24Mg or 16O
carbon is consumed and a core of product elements builds up; gravity builds
up and the new core collapses sufficiently to burn heavier elements
Oxygen burning
16O + 16O –> 28Si or 31P or 31S
or 30Si or 30P or 32S or 24Mg
O, Ne, Mg, Si, S burning takes a star 6 months, reaching
3E9 Kelvin
The heat of star aggregation caused
particles and elements to accelerate and collide, forming elements as heavy as
Fe (atomic number 26).
Silicon burning
lasts one day, reaching 5E9 Kelvin. This causes a gravitational collapse,
forming either a neutron star or a black hole, with the outer layers being
blown off in a supernova whose neutron burst forms elements heavier than Fe
28Si + 4He –> 32S
32S + 4He –> 36Ar
36Ar + 4He –> 40Ca
40Ca + 4He –> 44Ti
44Ti + 4 He –>48Cr
48Cr + 4He –> 52Fe
52Fe + 4He –> 56Ni
Elements heavier than Fe are
produced by during supernovae explosions,
which occur when the gravitational force of the outer layers of a star
overcomes the thermal pressure of the fusing inner layers.
Further accretion formed solar systems,
meteorites, and planets by about 4.5 Ga
Differentiation of the Earth occurred by gravitational separation of the lightest elements into the
atmosphere and the densest elements into the core.
Chemical Bonds
What is a molecule?
Molecule: group of bonded atoms; e.g., H2O, SiO2, NaCl
What is a mineral?
Mineral: a solid of specific composition with a regular arrangement of
atoms
How do atoms bond together to form
minerals?
Elements bond by sharing or transferring electrons
Why don't elements prefer to remain alone,
unbonded?
Elements like to have their outer electron orbital full of electrons, so
elements with full orbitals are very stable (e.g., the noble gases He, Ar, Kr, Xe)
elements near the left side of the periodic table (e.g., K+, Mg2+)
like to give up electrons (the next lower orbital becomes full), while those
near the right side like to gain electrons to become full (e.g., S2–,
Cl–)
ionic bond: electrostatic attraction between cations and anions; charge balanced
covalent bond: sharing of electrons when orbitals overlap
metallic bond: special type of covalent bond in which electrons are freer to migrate around crystals
hydrogen bond: weak electrostatic attraction among individual polar molecules (e.g., H2O)
hydrogen bonding in ice
van der Waals bond: weak electrostatic attraction between molecular sheets
geckos may climb using van der Waals forces
van der Waals forces hold sheets of C together
bond length: separation between atoms that are bonded
effective radius of an atom is its size within a crystal lattice
effective radius is affected by oxidation state, with cations smaller than the neutral atom and anions larger:
effective radius is affected by density
of packing/coordination:
mineral formula
e.g., Ca2+Mg4+Si4+2O2—6
charge balance
Crystal Structure
Read Chapter 4 of Nesse
If Si and O are the most common elements
in Earth’s crust, what are common minerals made of?
silicates are the most common minerals because O is the most common
anion and Si is the most common cation
How do Si and O bond together to form 3-D
structures?
Is SiO4 a stable compound?
SiO4 has a net negative charge of 4–; this must be balanced by
cations
What structure can be formed from pure Si
and O?
Quartz: SiO2 in a 3-D array of tetrahedra,
each of which is joined to other tetrahedra at all 4 corners; quartz is 100% SiO2
and has a density of 2.65 g/cm3
the minimum coordination number for
an element that is part of a 3D mineral is IV, thus SiO4, (cannot form 3-D
structures from 3-coordinated things like CO3)
coordination number: number of atoms surrounding another
3-fold, III, planar only
4-fold IV tetrahedral
5-fold, V (L) trigonal bipyramid or (R) pentagonal bipyramid
6-fold VI octahedral
7-fold VII
8-fold VIII (see BCC below)
10-fold X
12-fold XII (see FCC and HCP below)
real example, diopside
VIIICa2+VIMg4+IVSi4+2O2—6
close packing
because metals share electrons freely, they can attain close packing
Here’s a helpful animation to see how cannonballs stack
to make tetrahedra: http://upload.wikimedia.org/wikipedia/en/3/32/Animated-HCP-Lattice.gif
hexagonal closest packing 12 neighboring atoms
cubic closest packing (face-centered cubic packing) 12 neighboring atoms
body-centered cubic packing
8 neighboring atoms
based on a square, rather than triangular, plane lattice
Lattices, Symmetry, Point Groups, Space Groups
Read Chapter 2 of Nesse
plane lattice: a 2D pattern of atoms that extends infinitely
(from
http://www.emat.ua.ac.be/Images/WebNovCerBulk.jpg)
space lattice: a 3D pattern of atoms that extends infinitely
crystal axes: vectors defined by the unit cell
unit cell: minimum portion of space lattice required to describe crystal (may be more than once choice)
There are six types of unit cell:
|
isometric |
a = b= c |
a
= b = g = 90° |
|
hexagonal |
a ≠ c |
a = 90° g = 60° |
|
tetragonal |
a = b ≠ c |
a = b = g = 90° |
|
orthorhombic |
a ≠ b ≠ c |
a = b = g = 90° |
|
monoclinic |
a ≠ b ≠ c |
a = g = 90° ≠ b |
|
triclinic |
a ≠ b ≠ c |
a ≠ b ≠ g |
You may find the movies here helpful:
http://www.gly.uga.edu/schroeder/geol3010/3010lecture05.html
cubic example: garnet
cubic example: fluorite
tetragonal example: rutile
tetragonal example: zircon
hexagonal example: quartz
hexagonal example: calcite
(from
www.mineralminers.com/.../mins/perm111.jpg)
orthorhombic example: olivine
(from http://www.telefonica.net/web2/barahonamicros/0100_Diopside_Jumilla_Murci.jpg)
monoclinic example: diopside
(from http://eps.berkeley.edu/~wenk/EPS100A/P5-2-Amazonite.jpg)
triclinic example: albite
see http://www.uwsp.edu/geo/projects/geoweb/participants/dutch/symmetry/unitcell.htm for some nice examples of how crystal forms are made up of unit cells
The distribution of atoms in the unit cell (P, primitive; F, face centered; I, body centered or Innenzentrierte) gives rise to the 14 Bravais lattices (above)
Crystal Faces
crystal faces tend to be close-packed planes of atoms
prism
set of faces parallel to one direction
rhombohedron
6 rhomb-shaped faces like a stretched or squashed cube
tetrahedron
4 triangular faces
If you like, for more crystal forms, see http://www.uwsp.edu/geo/projects/geoweb/participants/dutch/symmetry/xlforms.htm
octahedron
Point symmetry and Point Groups
Point symmetry operations in 2D are
reflection
like a mirror
rotation
around an axis
reflection and rotation produce the 10 2D point groups
Adding a 3rd dimension permits a 3rd symmetry operation:
rotoinversion: rotation + inversion
rotoinversion axes have a bar over the top of the number to distinguish them from ordinary rotation axes
note that
after Bloss (1971)
and leads to the 32 space groups, with their Hermann–Mauguin symbols (the first symbol of each stereonet below)
|
crystal system |
1st symbol |
2nd symbol |
3rd symbol |
|
cubic |
4, 4/m, |
3, |
2, 2/m, m |
|
hexagonal |
6, 6/m, |
2/m, m |
2, 2/m, m |
|
tetragonal |
4, 4/m, |
2, 2/m, m |
2, 2/m, m |
|
orthorhombic |
2, 2/m, m |
2, 2/m, m |
2, 2/m, m |
|
monoclinic |
2, 2m, m |
|
|
|
triclinic |
1, |
|
|
example: 6 2/m 2/m
Miller indices
are used to describe crystal faces and directions
Directions
Miller indices for directions are integers that describe the vector representation of the direction;
e.g., [104] is the direction that points 1 unit cell in the a direction and 4 unit cells in the c direction and is parallel to the b axis.
[uvw] describes a specific direction; <uvw> is a family of crystallographically equivalent directions
Planes
Miller indices for planes are integers that are the reciprocal of the intersection with each axis;
e.g., (104) is the plane that intersects the a axis at 1 unit-cell spacing and the c axis at 1/4 unit-cell spacing and is parallel to the b axis.
(hkl) describes a specific plane; {hkl} is a family of crystallographically equivalent planes
somewhat more painful in the hexagonal system
[uvtw] describes a specific direction; <uvtw> is a family of crystallographically equivalent directions
t = – (u+v)
(hkil) describes a specific plane; {hkil} is a family of crystallographically equivalent planes
i = – (h+k)
Phase Transformations
Read Chapter 4 of Nesse
Isostructural transformation: same structure, different composition (e.g., carbonates, MCO3)
Polymorphism: same composition, different structure (e.g., C, SiO2)
reconstructive polymorphism: bonds must be broken and reformed
(e.g., C, graphite, diamond)
(from http://www.prettyrock.com/php/mineraldetail.php?f=&n=Diamond)
graphite = hexagonal 6/m 2/m 2/m, H = 1–2, density = 2.1 g/cm3
diamond = cubic 4/m
(from http://www.emporia.edu/earthsci/amber/go336/salley/pics/carbon.gif)
(from http://fixedreference.org/2006-Wikipedia-CD-Selection/images/65/6506.png)
graphite structure: click for
animation
diamond structure: click for animation
(from http://www.eos.ubc.ca/research/diamonds/kopylova/pics/Maar_xsect1.gif) (from
http://www.min.tu-clausthal.de/www/lager/Exc2005/bilder/klein/sa041_b.htm)
displacive polymorphism: bonds rotate, change length (e.g., a quartz, b quartz)
(from
http://www.auburn.edu/~hameswe/Quartzpage.html)
See the following nice discussion of silica polymorphs: http://www.uwsp.edu/geo/projects/geoweb/participants/dutch/PETROLGY/Silica%20Poly.HTM
Here’s an animated gif of the a–b transition: http://www.rocksandminerals.org/suppl_nd06.php
See the following nice discussion of ice polymorphs: http://www.uwsp.edu/geo/projects/geoweb/participants/dutch/PETROLGY/Ice%20Structure.HTM
Phase Transformation Textures and Rates
http://www.geol.ucsb.edu/faculty/hacker/geo102C/lectures/part10.html
Mineral Chemistry
Read Chapter 9 of Nesse
How mineral compositions are measured with an electron microprobe http://www.geol.ucsb.edu/faculty/hacker/geo102C/lectures/part9.html
How to calculate a mineral formula
Table 9.3; see p. 173
Mineral Growth
Read Chapter 5 of Nesse
solid solutions
|
mineral |
end members |
exchange vector |
|
olivine |
forsterite
Mg2SiO4 <—> fayalite Fe2SiO4 |
Fe2+
<—> Mg2+ |
|
plagioclase |
albite
NaAlSi3O8 <—> anorthite CaAl2Si2O8 |
Na+
Si4+ <—> Ca2+ Al3+ |
|
amphibole |
tremolite
Ca2Mg5Si8O22(OH)2
<—> tschermakite Ca2(Mg3Al2)(Al2Si6)O22(OH)2 |
VIMg2+
IVSi4+ <—>VIAl3+ IVAl3+
(tschermak exchange) |
|
mica |
muscovite
KAl2(AlSi3)O10(OH)2 <—>
phengite KMgAlSi4O10(OH)2 |
VIAl3+
IVAl3+ <—> VIMg2+ IVSi4+(inverse
tschermak exchange) |
Mineral growth, diffusion, zoning
Diffusion is the transfer of mass via the motion
of individual atoms or molecules.
Diffusion within crystals is often discussed in terms of point defects,
which are missing atoms (vacancies) or extra atoms in the crystal lattice.
Every crystal has an equilibrium number of vacancies that allows the crystal to
be in a lower free energy state than if it were perfect crystal-this is
important because it means that crystals are always "ready to go"
when it comes to diffusion.
(from http://www.union.edu/PUBLIC/GEODEPT/COURSES/petrology/met_minerals.htm#Al-silicates)
Crystal Structures
Read Chapter 20, Chapters 11–19 of Nesse
Oxides
Ice H2O hexagonal
(see phase diagram that we looked at earlier in class)
Hydroxides
|
‘bauxite’ |
Al hydroxide |
Al foil |
|
MnO·OH |
Mn hydroxide |
pigment |
XO2 group
tetrahedral
|
rutile |
TiO2 |
source of Ti |
|
uraninite |
UO2 |
source of U |
(from
http://www.hgs-model.com/gallery/img/photo_Rutile02.gif)
rutile structure
rutile uraninite
X2O3 group
cubic
|
hematite |
Fe3+2O3 |
|
|
corundum |
Al3+2O3 |
source of Cr (ruby) |
|
ilmenite |
Fe2+Ti4+O3 |
source of Fe |
hematite corundum ilmenite
hematite structure
crystal structure movie: http://ist-socrates.berkeley.edu/~eps2/wisc/geo360/hem.mov
Spinel
XY2O4 cubic
|
spinel |
MgAl2O4 |
|
|
chromite |
FeCr2O4 |
source of Cr |
|
magnetite |
Fe2+Fe3+2O4 |
source of Fe |
spinel chromite magnetite
(from
http://www.tf.uni-kiel.de/matwis/amat/def_en/kap_2/illustr/spinel.gif)
Carbonate Minerals
|
calcite |
CaCO3 |
hexagonal |
2.71 g/cm3 |
|
aragonite |
CaCO3 |
orthorhombic |
2.94 g/cm3 |
|
magnesite |
MgCO3 |
|
|
|
dolomite |
CaMg(CO3)2 |
|
|
calcite structure
Sulfate Minerals
|
gypsum |
hydrous CaSO4 |
evaporites |
wallboard |
|
anhydrite |
CaSO4 |
evaporites |
|
|
barite |
BaSO4 |
Ba source |
dense additive |
alabaster anhydrite
barite structure
Phosphate Minerals
apatite hydrous calcium phosphate
Tungstate Minerals
scheelite CaWO4
(from
http://www.wrightsrockshop.com/gallery/wulfenitemimetite/wulfenitemimetitemiscellaimages/scheelite022504.JPG)
source of W
Pine Creek Mine near Bishop
Borate Minerals
borax hydrous Na borate
source of B
Halide Minerals
|
halite |
NaCl |
cubic |
|
fluorite |
CaF2 |
cubic |
halite; Na+ (green) coordinated with six Cl–
(orange)
fluorite; Ca2+ (grey) coordinated with eight F– (yellow)
Sulfide Minerals
|
sphalerite |
ZnS |
cubic |
|
galena |
PbS |
cubic |
|
pyrite |
FeS |
cubic |
|
molybdenite |
MoS2 |
hexagonal |
sphalerite galena pyrite
pyrite; (Fe2+ yellow, S2– gray)
Silicate Minerals
|
|
|
no of O shared per tetrahedron |
|
orthosilicates |
nesosilicates |
0 |
|
disilicates |
sorosilicates |
1 |
|
ring silicates |
cyclosilicates |
2 |
|
chain silicates |
inosilicates |
2 or 3 |
|
sheet silicates |
phyllosilicates |
3 |
|
framework silicates |
tectosilicates |
4 |
nesosilicate (from http://classes.colgate.edu/rapril/geol201/summaries/silicates/neso.htm)
sorosilicate (from http://classes.colgate.edu/rapril/geol201/summaries/silicates/soro.htm)
cyclosilicate (from http://classes.colgate.edu/rapril/geol201/summaries/silicates/cyclo.htm)
single-chain inosilicate (from http://classes.colgate.edu/rapril/geol201/summaries/silicates/ino.htm)
double-chain inosilicate (from http://classes.colgate.edu/rapril/geol201/summaries/silicates/amphib.htm)
phyllosilicate (from http://classes.colgate.edu/rapril/geol201/summaries/silicates/phyllo.htm)
tectosilicate (from http://classes.colgate.edu/rapril/geol201/summaries/silicates/tecto.htm)
Framework Silicates (Tectosilicates)
Quartz etc.
SiO2 vs SiO4
SiO2 phase diagram: http://darkwing.uoregon.edu/~cashman/GEO311/311pages/L5_crystallization_files/image001.gif
ab
plane of beta quartz, showing heights of SiO2 tetrahedra arranged in hexagonal array to form framework in
which each tetrahedron shares four corners (after Putnis,
1992)
Feldspar
monoclinic and triclinic
K-feldspar KAlSi3O8
crystal structure movie:http://ist-socrates.berkeley.edu/~eps2/wisc/geo360/Sanidine.mov (SiO4 and AlO4 tetrahedra blue, K 9-fold sites red)
|
sanidine |
monoclinic |
high T, rapid cooling |
complete Al/Si disorder |
|
orthoclase |
monoclinic |
moderate T, cooling |
partial Al/Si order |
|
microcline |
triclinic |
low T, slow cooling |
complete Al/Si order |
(from http://www.union.edu/PUBLIC/GEODEPT/COURSES/petrology/met_minerals.htm#Al-silicates)
perthite: albite exsolution lamellae in K-feldspar host
plagioclase NaAlSi3O8–CaAl2Si2O8
amazonite (albite)
|
high albite |
triclinic |
high T, rapid cooling |
complete Al/Si disorder |
|
intermediate albite |
triclinic |
moderate T, cooling |
partial Al/Si order |
|
low albite |
triclinic |
low T, slow cooling |
complete Al/Si order |
crystal structure movie: http://ist-socrates.berkeley.edu/~eps2/wisc/geo360/Albitem.mov (SiO4 and AlO4 tetrahedra blue, Na 9-fold sites red)
http://ist-socrates.berkeley.edu/~eps2/wisc/geo360/Anorthite.mov (SiO4 tetrahedra blue, AlO4 tetrahedra grey, Ca 9-fold sites red)
albite–anorthite
albite–An10–oligoclase–An30–andesine–An50–labradorite–An70–bytownite–An90–anorthite
(from http://www.union.edu/PUBLIC/GEODEPT/COURSES/petrology/met_minerals.htm#Al-silicates)
feldspar twinning
(from http://www.geo.auth.gr/212/6_tekto/fds_twin.htm)
Carlsbad [001](010) Albite ┴(010)(010) Pericline [010](h0l) Albite
and Pericline
Zeolites
‘(Na, K)(Ca, Mg)(AlSiO)’·mH2O
important filtering agents
crystal structure movie: http://ist-socrates.berkeley.edu/~eps2/wisc/geo360/Analcime.mov
(SiO4 tetrahedra blue, AlO4 tetrahedra purple, Na pink, H2O yellow)
analcime NaAlSi2O6•H2O
laumontite CaAl2Si4O12•4H2O
Orthosilicates (Nesosilicates)
SiO4 + cations
olivine
(from http://www.union.edu/PUBLIC/GEODEPT/COURSES/petrology/met_minerals.htm#Al-silicates)
orthorhombic
forsterite Mg2SiO4
in ultramafic rocks
fayalite Fe2SiO4
crystal structure movie: http://ist-socrates.berkeley.edu/~eps2/wisc/geo360/olivine.mov
(SiO4 tetrahedra blue, Fe & Mg distorted
octahedral sites yellow, Fe & Mg octahedral sites orange)
Garnet X3Y2Si3O12
almandine Fe
pyrope Mg
grossular Ca
spesssartine Mn
laser Y3Al2Si3O12
(from http://www.geo.uni-potsdam.de/Mitarbeiter/OBrien/obrien/Atoll/index.html)
crystal structure movie: http://ist-socrates.berkeley.edu/~eps2/wisc/geo360/garnet.mov
(SiO4 tetrahedra blue, Al octahedra red, M2+ distorted 8-fold sites cyan)
Aluminumsilicates
Al2SiO5
|
sillimanite VIAlIVAl |
orthorhombic |
high temperature |
|
andalusite VIAlVAl |
orthorhombic |
low pressure |
|
kyanite VIAlVIAl |
triclinic |
high pressure |
andalusite sillimanite
kyanite (after Putnis, 1992)
crystal structure movies:
http://ist-socrates.berkeley.edu/~eps2/wisc/geo360/andalusite.mov
(SiO4 tetrahedra blue, VIAl
pale blue, VAl green)
http://ist-socrates.berkeley.edu/~eps2/wisc/geo360/sillimanite.mov
(SiO4 tetrahedra blue, VIAl
pale blue, IVAl yellow)
kyanite (from http://www.union.edu/PUBLIC/GEODEPT/COURSES/petrology/met_minerals.htm#Al-silicates)
sillimanite (fibrolite) (from http://www.union.edu/PUBLIC/GEODEPT/COURSES/petrology/met_minerals.htm#Al-silicates)
zircon
ZrSiO4
(from http://www.union.edu/PUBLIC/GEODEPT/COURSES/petrology/met_minerals.htm#Al-silicates)
crystal structure movie: http://ist-socrates.berkeley.edu/~eps2/wisc/geo360/zircon.mov (SiO4 tetrahedra blue, Zr4+ 8-fold sites green)
sphene
CaTiSiO4(OH,Cl,F)4
staurolite
(Mg,Fe)2Al9Si4O22(OH)2
(from http://www.union.edu/PUBLIC/GEODEPT/COURSES/petrology/met_minerals.htm#Al-silicates)
Disilicates (Sorosilicates)
paired SiO4 tetrahedra, Si2O7
epidote hydrous Ca-Al silicate
Ca2(Al,Fe+3)Al2Si3O12(OH)
monoclinic
has 7 and 11-fold coordinated sites
crystal structure movie: http://ist-socrates.berkeley.edu/~eps2/wisc/geo360/epidote.mov
(Ca 7- and 11-fold sites green, Si tetrahedra chains
blue, Al M2 octahedral site cyan, Al–Fe M1 octahedral site yellow)
(from http://www.union.edu/PUBLIC/GEODEPT/COURSES/petrology/met_minerals.htm#Al-silicates)
zoisite hydrous Ca-Al silicate
orthorhombic
Ca2Al3Si3O12(OH)
lawsonite hydrous Ca-Al silicate
indicates high pressure
Ring Silicates (Cyclosilicates)
beryl Be silicate
Be3Al2Si6O18
emerald Cr-beryl
(SiO4 tetrahedra yellow, Al 6-fold sites gray, Be
4-fold sites green)
crystal structure movie: http://ist-socrates.berkeley.edu/~eps2/wisc/geo360/beryl.mov
(SiO4 tetrahedra blue, Al 6-fold sites green, Be
4-fold sites pale green; ignore the yellow and pink)
tourmaline Li–B silicate
Na(Mg,Fe,Mn,Li,Al)3Al6Si6O18(BO3)3(OH)4
crystal structure movie: http://ist-socrates.berkeley.edu/~eps2/wisc/geo360/tourmaline.mov (SiO4 tetrahedra cyan, Na+ or OH– yellow, Al cyan, Li & Mg and Al purple, BO3 pale green)
Chain Silicates (Inosilicates)
Pyroxene
crystal structure movies:
orthopyroxene, showing tetrahedral chains: http://ist-socrates.berkeley.edu/~eps2/wisc/geo360/diopibeam.mov (SiO4 tetrahedra blue, Mg & Ca octahedra yellow)
http://ist-socrates.berkeley.edu/~eps2/wisc/geo360/opx.mov (SiO4 tetrahedra blue, Mg & Ca octahedra yellow)
http://ist-socrates.berkeley.edu/~eps2/wisc/geo360/diopside.mov (SiO4 tetrahedra blue, Mg octahedra yellow, Ca octahedra orange)
orthorhombic and monoclinic
VIII or VIXVIYIVZ2O6
VIII or VIM2VIM1IVT2O6
(from http://www.tulane.edu/~sanelson/eens212/olivines&pyroxenes.htm)
(from http://www.nature.com/nature/journal/v406/n6791/fig_tab/406059a0_F2.html
)
enstatite
MgSiO3
ferrosilite
FeSiO3
wollastonite
CaSiO3 common in skarns
diopside
CaMgSi2O6
hedenbergite
CaFeMgSi2O6
jadeite
NaAlSi2O6 indicates high pressure
(from http://www.tulane.edu/~sanelson/eens212/olivines&pyroxenes.htm)
augite (Na,Ca,Fe,Mg)(Al,Ti,Si)2O6
Amphibole
orthorhombic and monoclinic
XW0–1VIII or VIX2VIY5IVZ8O22(OH)2
XA0–1VIII or VIM42VI(M1, M2, M3)5IVT8O22(OH)2
http://ist-socrates.berkeley.edu/~eps2/wisc/geo360/tremolite.mov
(SiO4 tetrahedra blue, Mg octahedra
yellow, Ca 8- or 6-fold sites pale blue, Na 10-fold site green)
http://ist-socrates.berkeley.edu/~eps2/wisc/geo360/glaucophane.mov (SiO4 tetrahedra
blue, Mg octahedra yellow, Al 8- or 6-fold sites pale
blue, Na 10-fold site green)
anthophyllite []Mg2Mg5Si8O22(OH)2
Mg–Fe orthoamphibole
Mg–Fe rich rocks: ultramafic
tremolite–actinolite []Ca2Mg5Si8O22(OH)2
Ca–Mg–Fe clinoamphibole
tremolite is Mg endmember; actinolite is Fe endmember
blackwall rinds
glaucophane []Na2(Mg3Al2)Si8O22(OH)2
Na clinoamphibole
indicates high pressure
(from http://www.union.edu/PUBLIC/GEODEPT/COURSES/petrology/met_minerals.htm#Al-silicates)
hornblende (Na, K)Ca2(Mg, Fe2+, Fe3+,
Al, Ti) 5Si8O22(OH)2
K, Na, K, Mg, Fe, Al clinoamphibole
(from http://www.union.edu/PUBLIC/GEODEPT/COURSES/petrology/met_minerals.htm#Al-silicates)
Sheet Silicates (Phyllosilicates)
made of interlayered octahedral (two planes of OH– with interlayer 2+ or 3+ cations) and tetrahedral sheets
(from
http://classes.colgate.edu/rapril/geol201/summaries/silicates/phyllo.htm)
brucite: Mg(OH)2 single di-octahedral sheet
di-octahedral sheet contains 3+ cations; the 6– charge of the anions is satisfied by two 3+ cations, so two or every three sites is vacant; each O or OH is bonded to two cations
gibbsite: Al(OH)3 single tri-octahedral sheet
tri-octahedral sheet contains 2+ cations; the 6– charge of the anions is satisfied by three 2+ cations, so no sites are vacant; each O or OH is bonded to three cations
serpentine: Mg3Si2O5(OH)2
TO structure (from
http://classes.colgate.edu/rapril/geol201/summaries/silicates/phyllo.htm)
lizardite, chrysotile, antigorite
lizardite crystals are small because of mismatch between octahedral and tetrahedral layers
asbestos, including crocidolite amphibole
(after Nesse, 2000)
talc: Mg3Si4O10(OH)2
TOT structure (from
http://classes.colgate.edu/rapril/geol201/summaries/silicates/phyllo.htm)
crystal structure movie: http://ist-socrates.berkeley.edu/~eps2/wisc/geo360/talc.mov
muscovite: KAl2(AlSi3O10)(OH)2
(from http://www.union.edu/PUBLIC/GEODEPT/COURSES/petrology/met_minerals.htm#Al-silicates)
TOT + interlayer cation
crystal structure movie: http://ist-socrates.berkeley.edu/~eps2/wisc/geo360/muscovite.mov
biotite: K(Mg, Fe)3(AlSi3O10)(OH)2
phlogopite is Mg endmember; found in mantle
TOT + interlayer cation like muscovite
crystal structure movie:http://ist-socrates.berkeley.edu/~eps2/wisc/geo360/phlogopite.mov
chlorite: (Mg, Fe)3(Al,
Si)4O10(OH)2
crystal structure movie: http://ist-socrates.berkeley.edu/~eps2/wisc/geo360/chlorite.mov
TOT + interlayer cation = talc + brucite
(from http://www.union.edu/PUBLIC/GEODEPT/COURSES/petrology/met_minerals.htm#Al-silicates)
clay minerals
kaolinite
smectite
illite
drilling mud, ceramics, cosmetics, absorbents, food