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CHAPTER 2
STEEL
Robert J. King
U.S. Steel Group, USX Corporation
Pittsburgh, Pennsylvania
2.1 METALLOGRAPHY AND HEAT
TREATMENT
2.4.5
Austempering
28
18
2.4.6
Normalizing
28
2.4.7
Annealing
29
2.2 IRON-IRON CARBIDE PHASE
DIAGRAM
2.4.8
Isothermal Annealing
29
19
2.4.9
Spheroidization Annealing
31
2.2.1
Changes on Heating and
Cooling Pure Iron
2.2.10 Process Annealing
31
19
2.4.11 Carburizing
31
2.2.2
Changes on Heating and
Cooling Eutectoid Steel
2.4.12 Nitriding
31
19
2.2.3
Changes on Heating and
Cooling Hypoeutectoid Steels 20
2.5 CARBON STEELS
31
2.5.1
Properties
32
2.2.4
Changes on Heating and
Cooling Hypereutectoid Steels 20
2.5.2
Microstructure and Grain
Size
32
2.2.5
Effect on Alloys on the
Equilibrium Diagram
2.5.3
Microstructure of Cast Steels 33
20
2.5.4
Hot Working
33
2.2.6
Grain Size— Austenite
20
2.5.5
Cold Working
34
2.2.7
Microscopic-Grain-Size
Determination
2.5.6
Heat Treatment
34
21
2.5.7
Residual Elements
35
2.2.8
Fine- and Coarse-Grain
Steels
21
2.6 DUAL-PHASESHEETSTEELS
35
2.2.9
Phase Transformations —
Austenite
21
2.7 ALLOYSTEELS
36
2.2.10 Isothermal Transformation
Diagram 21
2.2.11 Pearlite 23
2.2.12 Bainite 23
2.2.13 Martensite 23
2.2.14 Phase Properties— Pearlite 23
2.2.15 Phase Properties — Bainite 23
2.2.16 Phase Properties — Martensite 23
2.2.17 Tempered Martensite
2.7.1
Functions of Alloying
Elements
36
2.7.2
Thermomechanical
Treatment
36
2.7.3
High-Strength Low-Alloy
(HSLA) Steels
36
2.7.4
AISI Alloy Steels
36
2.7.5
Alloy Tool Steels
37
23
2.7.6
Stainless Steels
37
2.2.18 Transformation Rates
23
2.7.7
Martensitic Stainless Steels
37
2.2.19 Continuous Cooling
24
2.7.8
Ferrite Stainless Steels
39
2.7.9
Austenitic Stainless Steels
39
2.3 HARDENABILITY
25
2.7.10 High-Temperature Service,
Heat-Resisting Steels
40
2.4 HEAT-TREATINGPROCESSES
26
2.7. 1 1 Quenched and Tempered
Low-Carbon Constructional
Alloy Steels
2.4. 1
Austenitization
26
2.4.2
Quenching
27
41
2.4.3
Tempering
27
2.7.12 Maraging Steels
41
2.4.4
Martempering
28
2.7.13 Silicon-Steel Electrical
Sheets
41
Reprinted from Kirk-Othmer Encyclopedia of Chemical Technology, 3rd ed., Wiley, New York, 1983,
Vol. 21, by permission of the publisher.
Mechanical Engineers' Handbook, 2nd ed., Edited by Myer Kutz.
ISBN 0-471-13007-9 © 1998 John Wiley & Sons, Inc.
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2.1 METALLOGRAPHY AND HEAT TREATMENT
The great advantage of steel as an engineering material is its versatility, which arises from the fact
that its properties can be controlled and changed by heat treatment. 1 ' 3 Thus, if steel is to be formed
into some intricate shape, it can be made very soft and ductile by heat treatment; on the other hand,
heat treatment can also impart high strength.
The physical and mechanical properties of steel depend on its constitution, that is, the nature,
distribution, and amounts of its metallographic constituents as distinct from its chemical composition.
The amount and distribution of iron and iron carbide determine the properties, although most plain
carbon steels also contain manganese, silicon, phosphorus, sulfur, oxygen, and traces of nitrogen,
hydrogen, and other chemical elements such as aluminum and copper. These elements may modify,
to a certain extent, the main effects of iron and iron carbide, but the influence of iron carbide always
predominates. This is true even of medium-alloy steels, which may contain considerable amounts of
nickel, chromium, and molybdenum.
The iron in steel is called ferrite. In pure iron-carbon alloys, the ferrite consists of iron with a
trace of carbon in solution, but in steels it may also contain alloying elements such as manganese,
silicon, or nickel. The atomic arrangement in crystals of the allotrophic forms of iron is shown in
Fig. 2.1.
Cementite, the term for iron carbide in steel, is the form in which carbon appears in steels. It has
the formula Fe 3 C, and consists of 6.67% carbon and 93.33% iron. Little is known about its properties,
except that it is very hard and brittle. As the hardest constituent of plain carbon steel, it scratches
glass and feldspar but not quartz. It exhibits about two-thirds the induction of pure iron in a strong
magnetic field.
Austenite is the high-temperature phase of steel. Upon cooling, it gives ferrite and cementite.
Austenite is a homogeneous phase, consisting of a solid solution of carbon in the y form of iron. It
forms when steel is heated above 79O 0 C. The limiting temperatures for its formation vary with
composition and are discussed below. The atomic structure of austenite is that of y iron, fee; the
atomic spacing varies with the carbon content.
When a plain carbon steel of ~ 0.80% carbon content is cooled slowly from the temperature
range at which austenite is stable, ferrite and cementite precipitate together in a characteristically
lamellar structure known as pearlite. It is similar in its characteristics to a eutectic structure but, since
it is formed from a solid solution rather than from a liquid phase, it is known as a eutectoid structure.
At carbon contents above and below 0.80%, pearlite of ~ 0.80% carbon is likewise formed on slow
cooling, but excess ferrite or cementite precipitates first, usually as a grain-boundary network, but
occasionally also along the cleavage planes of austenite. The excess ferrite or cementite rejected by
the cooling austenite is known as a proeutectoid constituent. The carbon content of a slowly cooled
steel can be estimated from the relative amounts of pearlite and proeutectoid constituents in the
microstructure.
Bainite is a decomposition product of austenite consisting of an aggregate of ferrite and cementite.
It forms at temperatures lower than those where very fine pearlite forms and higher than those at
which martensite begins to form on cooling. Metallographically, its appearance is feathery if formed
Fig. 2.1 Crystalline structure of allotropic forms of iron. Each white sphere represents an atom
of (a) a and 8 iron in bcc form, and (b) y iron, in fee (from Ref. 1).
815049314.005.png
in the upper part of the temperature range, or acicular (needlelike) and resembling tempered marten-
site if formed in the lower part.
Martensite in steel is a metastable phase formed by the transformation of austenite below the
temperature called the M s temperature, where martensite begins to form as austenite is cooled con-
tinuously. Martensite is an interstitial supersaturated solid solution of carbon in iron with a body-
centred tetragonal lattice. Its microstructure is acicular.
2.2 IRON-IRON CARBIDE PHASE DIAGRAM
The iron-iron carbide phase diagram (Fig. 2.2) furnishes a map showing the ranges of compositions
and temperatures in which the various phases such as austenite, ferrite, and cementite are present in
slowly cooled steels. The diagram covers the temperature range from 60O 0 C to the melting point of
iron, and carbon contents from O to 5%. In steels and cast irons, carbon can be present either as iron
carbide (cementite) or as graphite. Under equilibrium conditions, only graphite is present because
iron carbide is unstable with respect to iron and graphite. However, in commercial steels, iron carbide
is present instead of graphite. When a steel containing carbon solidifies, the carbon in the steel usually
solidifies as iron carbide. Although the iron carbide in a steel can change to graphite and iron when
the steel is held at ~ 90O 0 C for several days or weeks, iron carbide in steel under normal conditions
is quite stable.
The portion of the iron-iron carbide diagram of interest here is that part extending from O to
2.01% carbon. Its application to heat treatment can be illustrated by considering the changes occurring
on heating and cooling steels of selected carbon contents.
Iron occurs in two allotropic forms, a or 8 (the latter at a very high temperature) and y (see Fig.
2.1.) The temperatures at which these phase changes occur are known as the critical temperatures,
and the boundaries in Fig. 2.2 show how these temperatures are affected by composition. For pure
iron, these temperatures are 91O 0 C for the a-y phase change and 1390° for the y-8 phase change.
2.2.1 Changes on Heating and Cooling Pure Iron
The only changes occurring on heating or cooling pure iron are the reversible changes at —910 0 C
from bcc a iron to fee y iron and from the fee 8 iron to bcc y iron at ~1390°C.
2.2.2 Changes on Heating and Cooling Eutectoid Steel
Eutectoid steels are those that contain 0.8% carbon. The diagram shows that at and below 727 0 C the
constituents are a-ferrite and cementite. At 60O 0 C, the a-ferrite may dissolve as much as 0.007%
carbon. Up to 727 0 C, the solubility of carbon in the ferrite increases until, at this temperature, the
Fig. 2.2 Iron-iron carbide phase diagram (from Ref. 1).
815049314.006.png
ferrite contains about 0.02% carbon. The phase change on heating an 0.8% carbon steel occurs at
727 0 C which is designated as A 1 , as the eutectoid or lower critical temperature. On heating just above
this temperature, all ferrite and cementite transform to austenite, and on slow cooling the reverse
change occurs.
When a eutectoid steel is slowly cooled from —738 0 C, the ferrite and cementite form in alternate
layers of microscopic thickness. Under the microscope at low magnification, this mixture of ferrite
and cementite has an appearance similar to that of a pearl and is therefore called pearlite.
2.2.3 Changes on Heating and Cooling Hypoeutectoid Steels
Hypoeutectoid steels are those that contain less carbon than the eutectoid steels. If the steel contains
more than 0.02% carbon, the constituents present at and below 727 0 C are usually ferrite and pearlite;
the relative amounts depend on the carbon content. As the carbon content increases, the amount of
ferrite decreases and the amount of pearlite increases.
The first phase change on heating, if the steel contains more than 0.02% carbon, occurs at 727 0 C.
On heating just above this temperature, the pearlite changes to austenite. The excess ferrite, called
proeutectoid ferrite, remains unchanged. As the temperature rises further above A 1 , the austenite
dissolves more and more of the surrounding proeutectoid ferrite, becoming lower and lower in carbon
content until all the proeutectoid ferrite is dissolved in the austenite, which now has the same average
carbon content as the steel.
On slow cooling the reverse changes occur. Ferrite precipitates, generally at the grain boundaries
of the austenite, which becomes progressively richer in carbon. Just above A 1 , the austenite is sub-
stantially of eutectoid composition, 0.8% carbon.
2.2.4 Changes on Heating and Cooling Hypereutectoid Steels
The behavior on heating and cooling hypereutectoid steels (steels containing >0.80% carbon) is
similar to that of hypoeutectoid steels, except that the excess constituent is cementite rather than
ferrite. Thus, on heating above A 1 , the austentie gradually dissolves the excess cementite until at the
A cm temperature the proeutectoid cementite has been completely dissolved and austenite of the same
carbon content as the steel is formed. Similarly, on cooling below A cm , cementite precipitates and
the carbon content of the austenite approaches the eutectoid composition. On cooling below A 1 , this
eutectoid austenite changes to pearlite and the room-temperature composition is, therefore, pearlite
and proeutectoid cementite.
Early iron-carbon equilibrium diagrams indicated a critical temperature at ~768°C. It has since
been found that there is no true phase change at this point. However, between —768 and 79O 0 C there
is a gradual magnetic change, since ferrite is magnetic below this range and paramagnetic above it.
This change, occurring at what formerly was called the A 2 change, is of little or no significance with
regard to the heat treatment of steel.
2.2.5 Effect of Alloys on the Equilibrium Diagram
The iron-carbon diagram may, of course, be profoundly altered by alloying elements, and its appli-
cation should be limited to plain carbon and low-alloy steels. The most important effects of the
alloying elements are that the number of phases that may be in equilibrium is no longer limited to
two as in the iron-carbon diagram; the temperature and composition range, with respect to carbon,
over which austenite is stable may be increased or reduced; and the eutectoid temperature and com-
position may change.
Alloying elements either enlarge the austenite field or reduce it. The former include manganese,
nickel, cobalt, copper, carbon, and nitrogen and are referred to as austenite formers.
The elements that decrease the extent of the austenite field include chromium, silicon, molyb-
denum, tungsten, vanadium, tin, niobium, phosphorus, aluminum, and titanium; they are known as
ferrite formers.
Manganese and nickel lower the eutectoid temperature, whereas chromium, tungsten, silicon,
molybdenum, and titanium generally raise it. All these elements seem to lower the eutectoid carbon
content.
2.2.6 Grain Size—Austenite
A significant aspect of the behavior of steels on heating is the grain growth that occurs when the
austenite, formed on heating above A 3 or A cm , is heated even higher; A 3 is the upper critical tem-
perature and A c m is the temperature at which cementite begins to form. The austenite, like any metal
composed of a solid solution, consists of polygonal grains. As formed at a temperature just above
A 3 or A cm , the size of the individual grains is very small but, as the temperature is increased above
the critical temperature, the grain sizes increase. The final austenite grain size depends, therefore, on
the temperature above the critical temperature to which the steel is heated. The grain size of the
austenite has a marked influence on transformation behavior during cooling and on the grain size of
the constituents of the final microstructure. Grain growth may be inhibited by carbides that dissolve
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slowly or by dispersion of nonmetallic inclusions. Hot working refines the coarse grain formed by
reheating steel to the relatively high temperatures used in forging or rolling, and the grain size of
hot-worked steel is determined largely by the temperature at which the final stage of the hot-working
process is carried out. The general effects of austenite grain size on the properties of heat-treated
steel are summarized in Table 2.1.
2.2.7 Microscopic-Grain-Size Determination
The microscopic grain size of steel is customarily determined from a polished plane section prepared
in such a way as to delineate the grain boundaries. The grain size can be estimated by several methods.
The results can be expressed as diameter of average grain in millimeters (reciprocal of the square
root of the number of grains per mm 2 ), number of grains per unit area, number of grains per unit
volume, or a micrograin-size number obtained by comparing the microstructure of the sample with
a series of standard charts.
2.2.8 Fine- and Coarse-Grain Steels
As mentioned previously, austenite-grain growth may be inhibited by undissolved carbides or non-
metallic inclusions. Steels of this type are commonly referred to as fine-grained steels, whereas steels
that are free from grain-growth inhibitors are known as coarse-grained steels.
The general pattern of grain coarsening when steel is heated above the critical temperature is as
follows: Coarse-grained steel coarsens gradually and consistently as the temperature is increased,
whereas fine-grained steel coarsens only slightly, if at all, until a certain temperature known as the
coarsening temperature is reached, after which abrupt coarsening occurs. Heat treatment can make
any type of steel either fine or coarse grained; as a matter of fact, at temperatures above its coarsening
temperature, the fine-grained steel usually exhibits a coarser grain size than the coarse-grained steel
at the same temperature.
Making steels that remain fine grained above 925 0 C involves the judicious use of deoxidation
with aluminum. The inhibiting agent in such steels is generally conjectured to be a submicroscopic
dispersion of aluminum nitride or, perhaps at times, aluminum oxide.
2.2.9 Phase Transformations—Austenite
At equilibrium, that is, with very slow cooling, austenite transforms to pearlite when cooled below
the A 1 temperature. When austenite is cooled more rapidly, this transformation is depressed and
occurs at a lower temperature. The faster the cooling rate, the lower the temperature at which trans-
formation occurs. Furthermore, the nature of the ferrite-carbide aggregate formed when the austenite
transforms varies markedly with the transformation temperature, and the properites are found to vary
correspondingly. Thus, heat treatment involves a controlled supercooling of austenite, and in order
to take full advantage of the wide range of structures and properties that this treatment permits, a
knowledge of the transformation behavior of austenite and the properties of the resulting aggregates
is essential.
2.2.10 Isothermal Transformation Diagram
The transformation behavior of austenite is best studied by observing the isothermal transformation
at a series of temperatures below A 1 . The transformation progress is ordinarily followed metallo-
graphically in such a way that both the time-temperature relationships and the manner in which the
microstructure changes are established. The times at which transformation begins and ends at a given
temperature are plotted, and curves depicting the transformation behavior as a function of temperature
are obtained by joining these points (Fig. 2.3) Such a diagram is referred to as an isothermal trans-
formation (IT) diagram, a time-temperature-transformation (TTT) diagram, or, an S curve. 4
Table 2.1 Trends in Heat-Treated Products
Property
Coarse-grain Austenite
Fine-grain Austenite
Quenched and Tempered Products
Hardenability
Increasing
Decreasing
Toughness
Decreasing
Increasing
Distortion
More
Less
Quench cracking
More
Less
Internal stress
Higher
Lower
Annealed or Normalized Products
Machinability
Rough
finish
Better
Inferior
Fine
finish
Inferior
Better
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