li* 123 637 THS AUSTENI‘NC GRAIN SIZE IN MARTENSITIC STEBLS UNDER POLARlZED LIGHT Thesis for the Degree of M. S. MICHIGAN STATE COLLEGE Ralph Wenzel Rogers, 11'. I942 THESE. AUSTENITIC GRAIN SIZE IN MARTENSITIC STEELS UNDER PJLARIZED LIGHT by RALPH WENZEL ROGERS, JR. M A THESIS Submitted to the Graduate School of Michigan State College of Agriculture and Applied Science in partial fulfilment of the requirements for the degree of MASTER OF SCIENCE Department of Chemical and Metallurgical Engineering 1942 (145.9425 Ac knowledgme nts The author wishes to express his gratitude for the encouragement and advice given by Professor R. L. Sweet, under whose guidance this work was accomplished, and Mr. D. D. MCGrady. 1.12680 Table 9: Contents ForewordCOOOOOOOO.C...00......O00.....‘OOOOOOOOCOOOOOOOi Austenitic Grain Size in Martensitic Steels Under POlarized LigkétOOOOOOOOOOOOOOO'.00.01.000.000.0.0.0.0000]. Methods for Revealing Martensite Grains...........5 Austenite Grains and Martensite Grains...........16 Summary..........................................28 Appendix: Electrolytic Polishing of Steel.............30 Apparatus........................................33 Experiments on Electrolytic Polishing............36 Summary and Conclusions..........................58 Suggestions for Further Investigation............62 Bibliogx‘apllyCCOO0.000000000000000000.00.00.0000000000064 E0: gwgd The original purpose of this investigation was to explore the possibilities of using polarized light to reveal the previous austenite grains in fully hardened steels. ' After performing a number of experiments toward this end by mechanically polishing steel specimens, it was decided to use some electrolytically polished specimens to secure an.undistorted scratch-free surface. Because of the incompleteness of the literature descriptive of electrolytic polishing of steels and other metals, it was necessary to investigate and‘ experiment rather thoroughly before satisfactory polishing resulting. In the end, much of the time devoted to this thesis was spent in the latter phase or the invest- igation; hence the appendix, which contains the theory, data, and results of the experiments of electrolytic polishing, constitutes a not incons siderable part of the thesis. Apstenitic grain §ize In martensitic Steels Under Eolarized Light Throughout the many years of investigation of the metallography of steel, a problem about which there still remains considerable doubt is that of the nature of martensite and the reason for its hardness. Be- cause of the acicular or needle-like structure of martensite and its apparent lack of grain structure, many theories have been evolved on the basis of hypo- thetical structure in contradiction to the prevalent one that hardening is caused primarily by lattice distortion in the super saturated solid solution of carbon incxbiron, caused by rapid cooling when austenite is severely quenched. For example, Jefferies and Archerl formulated their "slip interference" theory on the basis of the formation of extremely small crystals (in martensite) oftxhirons-the hardness being caused entirely by the sub-microscopic size of the grains and their resulting resistance to slip. Heindlhofer and Being, however, by the application and careful interpretation of x-ray analysis, showed that the crystallograms of martensite are indicative of comparatively large,grains. In.addition.to the xpray, these investigators used polarized light to show that grains or "blocks" of martensite do exist and are of a size corresponding to that of the parent austenite grains. 1‘ (2) It is the purpose of this paper, then, to estab- lish methods for best revealing the martensite grains clearly, to investigate further the relationship of austenite grains and martensite_grains over a range of sizes, and to establish the practicability of using polarized light to determine the grains size of the parent austenite, since the latter is of prime import- ance in establishing the prOperties of a steel. Polarized light is made up of waveswhose vibrations are in one plane only as opposed to ordinary light in which the waves vibrate in all directions. Its use in the examination of metals depends on the ability to distinguish between isotropic and anisotropic crystals under polarized light. 0516C} Diane. ' Opiecfve. r A 1 F ‘ ---—-——— V Prism has? ' A CW/ e e fete diner ”P at ....... Figure 1. Light Train.For Metallograph Equipped With Polarized Light ' In the Bausch and Lamb research metallograph used (Figure l), the light from a tungsten are is polarized by passing through a Nicol prism in.the (3) vertical illuminator. After reflection.from a surface* which does not change the polarization of the beam, it passes back into the same prism in such a way that the beam is totally reflected and the effect of "crossed" Nicole is complete darkness. If the polarization of the beam.is changed.hy reflection, the components of the reflected light perpendicular to the original bean are transmitted by the prism and viewed in the eyepiece or camera. An isotropic crystal is one whose properties are the same in all directions. Polarized light is unp changed on reflection from such a surface so that under "crossed Nicola" total extinction of light occurs in all positions of the crystal. An anisotropic crystal has different properties in different directions and changes the plane of polarization on reflecting a polarized beam. Hence when viewed under "crossed Nicole", anisotropic crystals 'will very in intensity from.total extinction to maximum intensity, depending upon the angle formed between each crystal's reflecting plane and the plane of polar- ization of the beam. ( 'Austenite, which.has a face-centered cubic structure, transforms to martensite upon quenching, the latter belonging to the body-centered cubic type. An inter- mediate product of tetragonal type lattice, which trans- forms to the body-centered cubic at low temperatures, is believed to form first. If the transformation takes (4) place along the crystal planes of the austenite, the ' resulting martensite should show a grain structure similar to the parent austenite. As the martensite lattice varies distinctly from an exact body-centered crystal because of the carbon held in super-saturated solution causing the axes to have a ratio as high as 1.0S, the martensite grains show anisotropy. If it is composed of crystals of relatively parallel planes, martensite will appear under polarized light to be made up of grains which vary in intensity according to their orientation. Moreover, on revolving the martensite specimen, the intensities will change, each grain.going through two maxima and two minima in a 360° revolution. Some of the practical difficulties associated ‘with polarized light make its use limited.to a greater extent than is at first apparent. For example, the low intensity and low contrast of the reflected light make photography difficult. Also much that can be seen visually by rotating the specimen and.changing the intensities of the grains cannot be retained on a photomicrograph. The amorphous or "Beilby" layer of flowed metal formed on polishing is isotropic and must be removed to form.a reflecting surface of the aniso- trOpio martensite only. This is usually accomplished by etching, but the resulting roughening of the sur- face makes the intensity of the reflected beam con- siderably less. (5) W ESE. hassling ism ens__i_te grains The technique used to secure a surface for invest- igation under polarized light is important because of the rather exacting limits set by its use. various factors were investigated in order to determine the optimum conditions for revealing the grain structure of marten- site under polarized light. Particular attention.was devoted to the smallsgrained specimens since the large- grained martensite can be revealed with comparative ease by any methods satisfactory for the former. The factors investigated were the methods of re- moving the amorphous layer of disturbed metal and the effect of tempering. The methods used to remove the surface metal were etching and electrolytic polishing. As mentioned.before, it is necessary to remove the disturbed layer of metal, which is amorphous and iso- tropic in nature, in order to obtain reflection from the anisotropic metal beneath. If this is done by etching, it is necessary to avoid over-etching since the already low intensity of reflected polarizedlight is rendered considerably lower by roughness caused by too deep an attack. The ordinary etching solutions used did not seem to improve the revelation of a small grain size except for a special reagent for austenite grain boundaries (6) in martensite. This reagent, proposed by J.R. Vilellaa, consists of one gram of picric acid in five parts of hydrochloric acid and 95 parts of ethyl alcohol. In”. large-grained martensite, the previous austenite grains show up under ordinary light with this reagent (figure 2), but small grained specimens show little or nothing. With small grains under polarized light, fair results ' can'be obtained with this reagent. much.of its advan- tage lies in its slow rate of attack so that the degree of etch can be closely controlled and over-etching avoided. The use of electrolytic polishing to remove the surface layer offers the advantages of a strainpfree, undisturbed surface secured by electropolishing instead of mechanical_polishing to remove scratches left by the fine emery paper. Here the danger of roughening the surface and diffusing the light is again present and conditions for obtaining a good polish were invest- igated to considerable length as the literature on this process is quite incomplete and misleading. The theory, results and data of this part of the invest- , igation are contained in an appendix to this thesis. . In general, as might be expected, it was found that with electrOpolishing no further etching is needed. Sometimes, however, a light attack by Vilella's reagent, 2% picral, or 2% nital was found to increase (7) the clarity of the picture. It was found best to ex- amine the specimen unetched and then to etch if nec- essary as no definite procedure could be specified. Figure 3 is a specimen of S.A.E. 1090 steel quenched from 15500 F., electropolished and not etched, while Figure 4 is the same steel etched with Vilella's reagent. Figure 5 is S.A.E. 1090 steel, quenched from 17000 F., electropolished and not etched. Figure 6 is S.A.E. 1090 steel quenched from 1900° F. and etched with nital. Figures 7,8,9 and 10 are S.A.E. 1040 steel in.the annealed, normalized, water-quenched, and oil-quenched conditions under polarized light after electropolishing and etching with nital. The purpose of tempering martensite steels for observation under polarized light is to complete the transformation fromttetragonal to more nearly cubic body centered crystals. Probably because the latter is in a more strainpfree state, the crystal planes are more perfect and so the light is reflected in a more orderly manner with resulting clarity in the pictures. Figures 11,12,13 are specimens of S.A.E. 1090 steel quenched from 14500 F. Figure 11 shows the resulting structure while figures 13 and 12 were tem- pered at 450° F. for 15 minutes and 30 minutes respect- -ively. (8) Figures 14 and 15 are photomicrographs of a specimen of S.AtE. 1090 steel quenched from 1900° F., before and after tempering at 475° F. for 15 minutes. From these photomicrographs it is seen that tempering is only a slight aid in improving the clarity of small grained martensite under polarized light, but it improves the observation of large grained steel to a greater degree. Figure 2 SAE 1090 . quenched from 1900° F. etched with Vilella'a reagent 100x Figure 3 SAE 1090 quenched from 1550° F. tempered at 450° F. electrolytically pol- ished, no etch 100x polarized light (10) Figure 4 SAE 1090 quenched from 15500 F. tempered at 450° F. electnolytically polisl- ed and etched with Vilella's reagent 100x polarized light Figure 5 quenched from 17000 F. tempered at 450° F. electrolytically y01-. ished, no etch lth polarized light (11) Figure 6 SAE 1090 quenched from 19000 F. electrolytically pol- ished and etched with nital 375x polarized light Figure 7 SAE 1040 annealed electrolytically pol- ished and etched.with ‘ nital 375x polarized light (12) Figure 8 SAE 1040 normalized - l 0 D. V. l l a C m l 0 r t C e l e ished and etched with nital 750x polarized light Figure 9 SAE 1040 water quenched - l 0 P V. l l a c .1 n. l 0 r t C e l e ished and etcned with Vilella's reagent 100x polarized light (13) Figure 10 SAE 1040 oil quenched electrolytically pol- ished and etched with picral 100x polarized light Figure 11 SAE 1090 quenched from 14500 F. etched with Vilella's reagent 100x polarized light (l4) 2 l m. .1 F F O O 5 4 l mu 1 SH 00 lr f ma 9 a n e U 0. tempered for 30 minutes at 475° F. etched with Vilella's reagent 100x polarized light Figure 13 SAE 1090 quenched from 14500 F. S e m n .1 m 5 l .r O f d e P e M; H e t at 475° F. etched With Vilella's reagent 100x polarized light (15) Figure 14 SAE 1090 quenched from 19000 F. etched with picral and nital 100x polarized light Figure 15 SAE 1090 quenched from 19000 F. tempered 15 minutes at 475° F. etched with Vilella's reagent 100x polarized light (16) austenitg gagins 5nd gartegsite grgins There are a number of methods used by the metal- lurgist to determine the previous austenitic grain size in.martensitic steels. Among these are the arrested quench, gradient quench, slow cooling, preferential oxidation, heat tinting and case carburization methods and the use of special reagents. All of these are limited to steels of certain carbon ranges or by the necessity of using unusual equipment, or because of . the inordinate length of time required for the test. martensitic steels of approximately eutectoid compos- ition are those in.which it is most difficult to es- tablish the austenitic grain size so that for these experiments S.A.E. 1090 steel was used. Eutectoid steel also has the advantage of consisting of onxy one constituent-martensite- in a quenched structure,aso that there is no other structure present to complicate the observations. ' To establish the relationship between austenite grains and martensite grains, samples of steel were quenched from 18500 F. and 1450° F. into cold water. Samples from the same bars were submitted to a gradient quench from the same temperatures. This consists of quenching one end of the specimen only--so that at a certain point along the axis of the specimen, the cooling rate is such to cause the formation of troostite (I ~ V v , . _ ‘ ‘ y . .4 no ' . ' . , . . a . . u 'e a . - - .7 ' A I A a - x . . . o . . a . , .- . a ‘ . | O is v . ' ,.’ ' ~ . (17) in the grain boundaries of the austenite as rapid cooling occurs. At room temperature this zone con- sists of martensite outlined by thin lines of dark- etching troostite, thus showing the location of the previous austenite grain boundaries. Figures 16 and 17 were quenched from 1450° F., the former a gradient quench under ordinary light and the latter an identical steel after regular quenching and photographed under polarized light. Figures 18 and 19 represent a similar treatment from.1850° F., the former being the gradient quench. From these comparisons, it is readily seen that the grains in martensite under polarized light are of the same order of magnitude as the parent austenite grains. Also, the difference in clarity of the photo- micrographs by both methods between the large and small grains is illustrated. The temperaturesof 1450° F. and 1850° F. were chosen to secure austenite grains before and after the coarsening temperature of this steel was reached, and so a considerable diff- erence in the austenitic grain size obtains upon quenching. Figures 20-27 together with Figures 17 and 19 show the structure of martensite under polarized light secured by quenching steel from temperatures which varied by increments of 50° F. between 1450° F. and 1900° F. From a comparison of these pictures, it is illlllllll||l|l|lll1llll|lllvll (18) soon that the specimens quenched from 1700° F. and below are small grained and lacking in distinctness, while those quenched from above this temperature are both large grained and well defined. The border case, Figure 24, shows evidence of duplex structure but lacks the distinctness of Figures 25 and 26. The coarsening temperature of this steel may be established at about 1750° F. by these photomicrographs. That more than merely increased.grain.growth occurs at this temper- ature seems likely since such a considerable difference in appearance and distinctness results from quenching from above and below this temperature. The general appearance of the grain revealed by polarized light is typical of a face-centered crystal such as austenite-~the grain being equi~axed and roughly hexagonal, especially in the large—grained specimens. In examining martensite under polarized light, care must be taken in determining the size of grains. For ex, ample in Figure 28, several orientations within one grain.are visible as shown by the same picture under ordinary light, Figure 29. By rotating the specimens, the areas of a grain showing different orientations will display a maxima or minima at approximately or exactly the same angle. Figure 30 illustrates this, as it was taken at an angle of 33 degrees from.Figure 5. This is the same way that "twinned" austenite grains show different orientations under polarized light and for the same reason; stresses are relieved F. (19) in a grain by a "twisting" of a part of the structure so that the orientation varies in different parts of the original grain. As the light reflected varies in intensity according to the angle made with the plane of polarization, the differently oriented parts vary in intensity. Twinning is especially evident in Figures 27 and 6. magnifications beyond 100 diameters showed no add- itional detail under polarized light and are at a dis- advantage as the number ef grains under observation is correspondingly smaller. Since the percentage of well- outlined grains is low, to determine the size of the grains, as large a field as is possible should be used. Figures 6, 7, and 8 and Figure 31, which is of the same area shown in Figure 24, were taken at magnifications other than 100 diameters. II‘AI (20) Figure 16 SAE 1080 m 0 n h c n m 0.. m e .1 d a m. 1450° F. 100x Figure 17 SAE 1090 r.. 0 no % l m m pl .a e a n e u o. tempered at 4000 F. 100x polarized light (21) Figure 18 SAE 1090 m 0 r f .L C n m q t n e .1 d m n“ O o % 1 x me C 1 Op 1 M» .1. F O .(C C l .n o m l m o r f d e a. n e u C. tempered at 4000 F. 100x polarized light (22) Figure 20 SAE 1090 F O 0 w l m 0 P f d 6. qr. C n e u 0.. tempered at 4500 F. 100x polarized light 1.. 2 m .1 F n“ O 0 a l 0. am if Md e a n e u 0. tempered at 450° F. ’100x polarized light (23) Figure 22 SAE 1090 quenched froml600o F. tempered at 4500 F. 100x polarized light Figure 23 SAE 1090 quenched from 16-500 F. tempered at 450° F. 100x polarized light (24) Figure 24 SAE 1090 quenched from 1700° F. tempered at 450° F. 100x polarized light Figure 25 SAE 1090 quenched from 1750° F. tempered at 450° F. 100x polarized light (25) Figure 26 SAE 1090 quenched from 1800°F. tempered at 450° F. 100x polarized light Figure 27 SAE~1090 quenched from 1900° F. tempered at 450° F. 100x polarized light (26) Figure 28 SAE 1090 Quenched from 1900° F. etched with Vilella's reagent 100x polarized light Figure 29 SAE 1090 quenched from 1900° F etched'with Vilella‘s reagent 100x (27) Figure 30 SAE 1090 quenched from 1900° F. etched with Vilella's reagent 100x polarized light Figure 31 SAE 1090 quenched from 1700° F. electrolytically polished 500x polarized light (28) §EEE§£I From the series of pictures taken under polarized light, it may be seen that the size of grains revealed is of the same order of magnitude as the parent aus- tenite. According to Heindlhofer and Bainz, these are actual grains of martensite, and not merely traces of the austenite. For the purposes of making an estimate of the grain size of the parent austenite and for a determination of the coarsening temperature of a steel, polarized light can be used successfully. For steels near the eutec- toid composition, this method is especially valuable and is the only simple method available. In other steels, it offers advantages in time saving as no slow annealing is required; quenching and a fifteen minute tempering is the only heat treatment required. In steels which are already hardened, this is the only method for ascertaining the grain size and structure, except for special martensitic etches, the successful use of which is frequently impossible. For further investigation, it is suggested that the alloy and plain carbon steels over a range of compositions be studied to determine the limits of polarized light for as the composition of martensite approaches alpha-ferrite, the anisotropy disappears .oe.‘ (29) at some point. This was borne out by attempts to observe 1010 steel under polarized light which were unsuccessful. Apps ndix (30) APPENDIX Electrolytic Eolishigg 9; Steel The electrolytic polishing of metals was first attempted by Jacquet who successfully polished coppers’5 and tin7L by this method. Briefly, it consists of the reverse of e1ectro~p1ating; the specimen is placed at the anode of an electro-plating bath and conditions are so controlled as to secure the removal of a layer of metal at the anode rather than an even deposit at the cathode. Conditions for successful electrolytic polishing must be controlled very carefully to avoid a rough surface caused by pitting, etching, or uneven attack. The variables which have an influence on the quality of polish are the electrolyte, current density, voltage, time, agitation, temperature, and the shape, area and location of the cathode. These variables have been the subject of consid- erable investigation and while results have been ob- tained for many metals, there is still lacking enough information to be able to duplicate results in most instances. It was the object of this investigation to deter- mine the conditions necessary and to construct the apparatus with which to electrolytically polish commer- cial steels quickly and so secure a strainpfree, scratch- less surface. (31) A procedure for systematic investigation was also devised as a guide for future investigations of this type of work. i The most important factor in either polishing or plating is the proper choice of electrolyte. In- vestigators agree that a viscous, nonsconducting film is necessary to establish a concentration.gradient between.the elevations and depressions of the surface to be polished. Uhlig4 points out that according to the- oretical electricity, high gradients of potential exist- in the vicinity of points of great curvature-- even though the total gradient be small--hence at the elevations a better anode efficiency exists and the removal of Ametal proceeds at‘a greater rate than in the depressions. This film.man.be an oxide film, a layer of gas, insoluble products of electrolyte and metal, a static liquid film. or any combination of these, and it is especially necessary to secure a good film for the pol- ishing of nonphomogeneous alloys to avoid uneven attack on different phasesa. The choice of electrolyte then should be one in which.such a film is formed. The formation of metal salts which are but slightly soluble in the electrolyte satisfies the requirements. The addition of organic liquids to reduce the diffusion of the film and to lower the conductivity of the electrolyte is recommended by Uhlig4. (32) To determine the proper current density and voltage, and whether the electrolyte will result in satisfactory polishing, a curve of current versus voltage should be made, using the metal and electrolyte in question. The curve for a successful combination will have a shape similar to one of the following, which were secured by 1 various investigators. (6 co. A (a) co. A s 2 f (x1 " B as V Figure 32. Voltage-Current Density Curves For curves b and c of Figure 32,_the range for successful polishing occurs in the flat part between A and B9’l°’°. In the portion of the curve above B, gas is evolved and an uneven surface results while below A, etching occurss. For curve a, the critical point A-is the lower limit at which polishing proceeds successfully. Below this, the rate of diffusion of the film exceeds its rate of formation and hence the film is net maintained4. Experimental polishes at the voltage values so determined will ascertain their correctness, and by varying conditions such as temperature, cathode distance, (33) and the like, the optimum conditions for polishing the metal can be determined. W The apparatus used for electrolytic polishing was based upon the use of 220 volt direct current which was available in the laboratory. Since the voltages to be applied were not that high, the fol- lowing setup was used to secure the desired voltage and current. R2. Figure 330.. Electrical Circuit for Electrolytic Polishing The switch 81 permits the use of high or low voltage while 32 throws in either the ammeter or : uw‘ (34) milliammeter. The rheostats R1 and.R2 control the current, the latter being used for close control. The cell consisted of a battery jar, usually set in cooling bathe“ of ice water, with a motor driven stirrer. The cathode was placed parallel to the bot- tom while the specimen was clamped to the holder. This holder was built from an old microscope frame and makes possible close regulation of the depth of the specimen in the electrolyte, and easy removal of the specimen from both, because of a hinged frame. Figure 33bis a photograph of the cell, including the ; holder and stirrer, but without the external cooling bath. Figure 33cshows the control panel as diagrammed in Figure 33a. Airflfln—‘u ‘ . h— , 1:th _ Figure 33c. Control Board (36) Experiments 9. Electrolytic Polishing The experiments on electrolytic polishing of steel were primarily concerned with S.A.E. 1090 steel since that is what is used throughout the polarized light exPeriments. Other steels were also polished electro- lytically to verify the conclusions reached with 1090. These included S.A.E. 1040, 1010, and 10120. For the first attempts to polish electrolytically, a storage battery was used for the current source. After a number of trials, the voltage secured proved to be too low to polish steel so that the 220 volt D.C. setup previously described was devised and proved successful. The electrolyte used in all of the experiments was one recommended for steel by a number of writers and consisted of 765 parts of acetic anhydride, 185 parts of perchloric acid, and 50 parts of water. The film formed in this electrolyte with steel is said to be [FeaAc6 (OH);ICIO4°4H20 by Jacquet and Rocquetll. The solution is made up by chilling the chemicals before and during mixing, as considerable heat is evolved and the danger of a violent reaction is present. The solution is allowed to stand for 24 hours before using. Most reports on electrolytic polishing emphasize 'the current density as the prime factor in securing a (37) successful polish, so that in the first of these ex- periments the current density was the primary subject of investigation. Hewever, this did not prove to be very successful in controlling the quality of polish because of the difficulty encountered in keeping a constant area in contact with the electrolyte. As. the apparatus was designed to be a simple and rapid means of polishing metals, the sample to be polished was simply suspended in the electrolyte, the total area immersed being subject to polishing action. Hence, when the solution was agitated, the wave motion caused a variation in area. Also, the depth of immersion was difficult to ascertain because of the low surface tension of the solution showing in the high degree of adhesion to the metal. Coating the sides of the spec- imen with paraffin.was tried in order to maintain a constant area but the paraffin was attacked by the electrolyte and failed to protect the specimen. For these reasons, control by current density was not con- sistent and results were not always successful. 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