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Chapter I: Introduction to Extractive Metallurgy

3. Natural Resources

There are four main regions or "spheres" from which raw materials are taken (Figure 3.1). These are the lithosphere (crust), the biosphere (plants, animals, bacteria), the hydrosphere (oceans and freshwater) and the atmosphere. Metals extraction relies almost entirely on the lithosphere for metal bearing raw materials. However, the industry also relies heavily upon each of the other spheres: the hydrosphere for water; the atmosphere for air, or oxygen (concentrated from the air), and; the biosphere, e.g. animal proteins and carbohydrates as additives in metal processing and bacteria used in biological leaching of sulfide ores. It is intriguing to ponder the astounding differentiation between metal compounds in the earth's crust and the oceans. Only three metal ions are found in the oceans at any appreciable concentration: Na+, 0.47%; Mg+2 0.053%, and; Ca+2, 0.010%. Some very valuable metals occur at very low concentrations in the oceans, e.g. gold at ~1 μg/L (~1 part per billion), but as yet there are no economic methods of extracting these. Note too that the lithosphere includes that roughly ¾ of the Earth’s surface which is covered by the oceans. This is largely unexplored. There is interest in this, but land-based mineral resources are still plentiful enough and economically much more viable. Oil and gas are notable exceptions.

Diagram of Earth’s spheres as sources of raw materials: atmosphere (O₂, N₂, CO₂, noble gases), hydrosphere (water, salts), lithosphere (metals, fuels, helium), and biosphere (cellulose, fats, enzymes, bacteria).
Figure 3.1 - Main terrestrial sources of raw materials.

How minerals are distributed in the earth's crust is crucially important in the business of metal extraction. There are three aspects to this. One is the natural abundance of the element in the Earth’s crust. This is the average concentration in the lithosphere. A second is the occurrence of mineral deposits of the elements. Often these contain the pertinent minerals at considerably higher concentration than the average in the crust overall. It is fortunate that the elements are often not uniformly distributed. (Some elements are more evenly dispersed on average.) The third factor is that the mineral deposits must be able to be economically produced. The metals need to be present at suitable concentrations and in mineral forms that can be processed. Numerous factors go into the economic viability of a mineral deposit. To illustrate, copper has a natural abundance of 0.0068% by weight (68 g Cu per tonne of rock). But an economically producible copper mineral deposit would have contained around 1.8% Cu 100 years ago, whereas today a deposit with as little as 0.5% Cu could be economic to produce.

Table 3.1 shows the natural abundances of many commercially important metals and elements in the lithosphere. Most of the Earth’s crust is composed of oxygen (45.5%), silicon (27.2%), aluminum (8.3%), iron (6.2%), calcium, magnesium, sodium and potassium; these 8 elements comprise about 99% of the earth's crust! Most of the transition metals and the other heavier metals are either rare or very rare, with a few exceptions (iron, titanium and manganese - among the earlier of the transition metals). Natural abundances are also illustrated in the form of a periodic table in Figure 3.2. Note that often the lighter elements are the more common, while the heaviest transition metals are relatively rare. Indeed the platinum group metals, gold and silver are among the very rarest elements. There are exceptions to the general rule. The lanthanides (also called the rare earths) are not actually all that rare, compared to some of the less abundant transition metals.

As mentioned previously, many elements are concentrated in mineral deposits. The major types of minerals are listed in Table 3.2. Where a mineral is a compound, it is commonly thought of as formally a combination of cations and anions. However, the nature of the bonds between the atoms is often a lot more complex than this. Components of ionic, covalent and metallic bonds, as well as weaker bonding interactions, like hydrogen bonding, may be involved. Hence one usually cannot regard minerals as actually being salts. PbS, for example, is formally comprised of Pb+2 and S2-, but in reality it is not composed of discrete cations and anions.

Table 3.1 - Natural Abundances in Percent by Weight of Many Commercially Important Metals and Some Non-metals in the Earth’s Crust
Li Alkali Metals Ni 0.099 Transition Metals
Na Pd 1.5x10-6
K Pt 1x10-6
Be Alkaline Earths Cu 0.0068
Mg Ag 8x10-6
Ca Au 4x10-7
Sc Transition Metals Zn 0.0076
Y Cd 1.6x10-5
La Hg 8x10-6
Ti Al 8.3 Groups III-VI
Zr Ga 0.0019
Hf In 2.4x10-5
V Tl 7x10-5
Nb Sn 0.00021
Ta Pb 0.0013
Cr Bi 8x10-7
Mo Lanthanides 8-660x10-5
W Th 0.00081 Actinides
Mn U 0.00023
Re Si 27.2 Semiconductors
Fe Ge 0.00015
Ru As 0.00018
Os Sb 2x10-5
Co Te 1x10-7
Rh Se 5x10-6
Ir S 0.034 Non-metals

Diagram of human body elements grouped by abundance: major (O, C, H, N, Ca, P, K, S, Na, Cl, Mg, Fe), trace (Cu, Zn, Cr, Mn, Ni, Se, I, F, Mo, Co, Si), and ultratrace/nonessential (Li, B, V, Sn, Cd, Pb, Hg, As, others).
Figure 3.2 - Natural abundances of elements in the lithosphere.

Table 3.2 - Classification of Minerals According to their Formally Anionic components.
Anion
Sulfides S2-, S22- (i.e. a polysulfide)
Selenides, tellurides Se2-, Te2- (rarer than sulfides)
Oxides/hydroxides O2-/OH-(common)
Halides Cl-, F-; rarely Br-, I-
Carbonates CO32-
Sulfates SO42-
Nitrates NO3-
Phosphates PO43-
Arsenates AsO43-
Silicates SiO44-, Si2O76-, many others (common)
Aluminosilicates [Alw(OH)xSiyOz]n- (numerous)
Chromates CrO42-
Molybdates MoO42-
Tungstates WO42-
Vanadates VO43-
Borates B(OH)4-, B4O5(OH)42-, etc. )others


The formalism is useful for classification purposes and for understanding the chemistry. Minerals are usually classified by the formally anionic components since there are many metals that form precipitates with the same anion, for instance there are many metal sulfides, such as Cu2S, CuFeS2, PbS, ZnS, etc. In many cases the metal values reside in the formally cationic parts of the minerals, e.g. CuS (Cu+2/S2-), AlO(OH) (Al+3/O2-,OH-), and PbCO3 (Pb+2/CO32-). But in some cases the metal of interest resides in the formally anionic part as complex ions, e.g. CaWO4 (Ca+2/WO42-). Oxides/hydroxides, silicates/aluminosilicates and sulfides are the most commonly mined minerals. (There are also other classes of minerals which, in the context of metal production, are not commonly produced.)

A sample list of some of the more important minerals is shown below in Table 3.3. Some rare and valuable metals may be disseminated in a variety of mineral matrices, for example gold may be hosted in quartz or pyrite or arsenopyrite etc. In some instances there are now few available ores of some metals (e.g. silver). In such cases the main means of production is as a by-product of another metal’s production. A partial list of applicable leaching systems for treating the mineral, or conditions under which it may at least partially be dissolved are also indicated in the table. Note the preponderance of acid, most often sulfuric acid (the cheapest of the “mineral acids”).

There are vastly more minerals than listed here, but this gives an indication of some of the more important ones. New minerals are still being discovered. Natural deposits may contain a diverse mixture of minerals, some at very low concentrations, which may have an impact on the extraction process. Thorough study of the mineralogy of an ore is crucial to a successful process. Many a plant has been doomed due to inattention to mineralogy.

In addition to minerals that contain metals of interest, ores inevitably contain gangue minerals. These have no commercial value in the context of the metal extraction process of interest. Very often the gangue constitutes by far the major fraction of an ore. This does not mean that some of the associated metals are not valuable. But, they cannot be economically processed from the given ore. For example, pyrite contains iron, the basis for steel, but there is not economically viable means to make iron from pyrite processed in the context of hydrometallurgy. Common gangue minerals and their reactivity are listed in Table 3.4.

Gangue minerals require careful attention. They may cause excessive consumption of costly reagents. They may host valuable minerals (e.g. fine crystals within gangue minerals, or chemical substituted within the gangue crystals, e.g. Ni in nickeliferrous limonite, Table 3.3). Gangue minerals may cause solid-liquid separation problems, e.g. clay minerals.

Table 3.3. - Common and important minerals of various metals.
Metal Mineral Formula Principal leaching chemistry
Al Gibbsite Al(OH)3 Caustic (NaOH)
Boehmite AlO(OH) NaOH; less reactive than diaspore
Diaspore AlO(OH) NaOH; less reactive than gibbsite
Bauxite Mixtures of above 3
Corundum Al2O3 NaOH; less reactive than boehmite
Cu Chalcopyrite CuFeS2 Main Cu mineral HCl/oxidant, H2SO4/oxidant. Mainly treated by pyrometallurgy.
Cu2S H2SO4/oxidant
Chalcocite CuS H2SO4/oxidant
Covellite Cu5FeS4 H2SO4/oxidant
Bornite Cu2O H2SO4/oxidant
Cuprite Cu metal (rare) H2SO4/oxidant; NH3/O2
Native Cu CuCO3·Cu(OH)2 Dilute H2SO4
Malachite 2CuCO3·Cu(OH)2 Dilute H2SO4
Azurite CuO Dilute H2SO4
Tenorite CuSiO3·2H2O Dilute H2SO4
Chrysocolla 3CuO·CuCl2·3H2O Dilute H2SO4
Atacamite Cu3AsS4 Difficult to leach or smelt
Enargite Cu3SbS3 Difficult to leach or smelt
Tetrahedrite
Zn Sphalerite ZnS Main H2SO4/oxidant
Marmatite (Zn,Fe)S minerals H2SO4/oxidant
Zincite ZnO (uncommon mineral; roasting ZnSZnO; common) Dilute H2SO4
Fe Magnetite Fe3O4 Dilute acid
Hematite Fe2O3 Unreactive
Limonite FeO(OH)·nH2O Acid (limonite may bear Ni)
Goethite FeO(OH) Acid (goethite may bear Ni)
Siderite FeCO3 Dilute acid
Pyrite FeS2 (may bear Au) H2SO4/oxidant
Marcasite FeS2 H2SO4/oxidant
Pyrrhotite Fe1-xS, 1-x ~ 1 Acid or acid/oxidant
Arsenopyrite FeAsS (may bear Au)
Pb Galena PbS Main mineral; usually smelted HCl/aq. Cl- salt/oxidant
PbO
Litharge PbSO4 HCl/aq. Cl- salt; HNO3
Anglesite PbCO3 HCl/aq. Cl- salt
Cerussite HCl/aq. Cl- salt
Ni Pentlandite (Ni,Fe)9S8 H2SO4 or HCl/oxidant
Garnierite (Ni,Mg)6Si4O10(OH)8 Strong H2SO4
Millerite NiS H2SO4 or HCl/oxidant; NH3/O2
Laterites, with Complex oxides/silicates, including (Fe,Ni)O(OH)·nH2O H2SO4; reductive roasting then leach with NH3/(NH4)2CO3
nickeliferrous
limonite
Co Smaltite CoAs2
Cobaltite CoAsS
Linnaeite Co3S4 H2SO4 or HCl/oxidant
Laterites As per Ni
CoS "Concentrate" formed from laterite leach; leach with NH3/O2
Sn Cassiterite SnO2 Mainly by pyrometallurgy
Ti Ilmenite FeTiO3 Very strong acids
Rutile TiO2 Very strong acids
Mo Molybdenite MoS2 Mainly by pyrometallurgy
Molybdite MoO3
Wulfenite PbMoO4
Powellite Ca(Mo,W)O4
W Scheelite CaWO4 HCl, H2SO4
Wolframite (Fe,Mn)WO4 NaOH
Sb Stibnite Sb2S3 Generally undesirable impurities. May leach in acid/oxidant
Jamesonite FePb4Sb6S14
As Realgar As4S4 Generally undesirable impurities. May leach in H2SO4/oxidant, cyanide/O2 systems
Orpiment As2S3
Bi Bismite Bi2O3 Acid/chloride
Bismuthinite Bi2S3 Acid/oxidant
Native Bi Elemental Bi Acid/oxidant
Lanthanides (“Ln”) Monazite (La,Th,Ln)PO4 Hot strong acid; NaOH
U Pitchblende UO2.x; H2SO4/oxidant; Na2CO3/oxidant
x < 0.67
Ag Argentite Ag2S CN-/oxidant; S2O32-/oxidant
Cerargyrite AgCl NH3; CN-
Native Ag Ag metal CN-/oxidant
Au Native Au Au metal CN-/oxidant; S2O32-/oxidant
Calaverite AuTe2 Hard to leach
Sylvanite (Au,Ag)Te2 Hard to leach
Hg Cinnabar HgS Usually by pyrometallurgy
PGM’s Various and complex

Table 3.4 - Common Gangue Minerals. Superscripted Roman numerals, e.g. MII, Refer to a Formally +2 Metal Cation.
Mineral Composition Reactivity (Partial or Total Dissolution)
Quartz SiO2 (may host gold) Fluorides or strong NaOH
Feldspars M1-M2-Al-silicates
M1, M2 = Na, K, Ca
Relatively unreactive
Mica, Chlorite K2Al4(Si6Al2)O20(OH)4
Mg10Al2(Si6Al2)O20(OH)16
Dilute acids
Amphiboles MIIy-(Si4O11)(OH)x: many
forms; MII = e.g. Ca, Mg, or
both; includes asbestos
Strong acids
Clays Layered aluminosilicates Acids
Pyroxene,

Olivine

MIISiO3, (M1II,M2II)SiO3
MII, M1II, M2II = e.g. Ca, Mg
(Mg,Fe)2SiO4
Acids
Garnets,

Staurolite,
Kyanite

M3IIM2III(SiO4)3 MII = e.g. Ca, Mg, Fe; MIII = e.g. Al, Cr, Fe
(FeII,Mg,Zn)2Al9(Si,Al)4O22(OH)2
Al2SiO5
Relatively unreactive
Andalusite,
Sillimanite
Al2SiO5
Al2SiO5
Acids
Calcite CaCO3 Readily with dilute acids
Magnesite,
Dolomite
MgCO3
CaMg(CO3)2
Acids
Pyrrhotite Fe1-xS, 1-x ~ 1 Dilute acids; CN-/O2
Marcasite,
Pyrite
FeS2
FeS2
Acids/oxidants; CN-/O2
Magnetite
Limonite
Goethite

Hematite

Fe3O4
FeO(OH)·nH2O
FeO(OH)

Fe2O3

Acids (rates depend
Acids on particle
Acids size and
crystallinity.)
Practically unreactive

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Aqueous Pathways (DRAFT) Copyright © by Bé Wassink and Amir M. Dehkoda is licensed under a Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International License, except where otherwise noted.

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