THE RARE EARTH ELEMENTS AND THEIR COMPOUNDS: THE PURIFICATION AND PROPERTIES OF PRASEODYMIUM OXIDE By MURRELL LEON SALUTSKY A THESIS Submitted to the School of Graduate Studies of Michigan State College of Agriculture and Applied Science in partial fulfillment of the requirements for the degree of DOCTOR OF PHILOSOPHY Department of Chemistry 1950 ACKNOWLEDGMENT Sincere appreciation is expressed to Dr. L. L. Quill for his direction and guidance through­ out the research program and during the preparation of this thesis. Thanks are also extended to Dr. G.L. Goemer for his assistance in the organic phase of this work and to Dr. E. Leininger for his analytical suggestions. Receipt of the Graduate Council Fellow­ ship presented by the Graduate Council for the academic year 1948-49 is hereby gratefully acknowledged0 TABLE OF CONTENTS Page No. Introduction I Qualitative Solubility and Distribution Studies............... II 4 Preparation and Properties of the Rare Earth Trichloroacetates......... 7 III Preparation of Rare Earth Carbonates ........ 15 IV Separation of Praseodymium and Lanthanum . . . 20 A. The Trichloroacetate Separation......... 22 B. The Dimethyloxalate Separation .......... 32 V The Trichloroacetate Separation of Cerium. . . 37 VI Analytical Methods for the Rare Earth Elements.................................. 42 A. Principal Analytical Methods ............ 43 B. The Determination of Praseodymium* . . . . 51 C. Average Atomic Weight Determinations: An Iodometric Correction for "Excess" VII O x y g e n ......................... * . . . . 59 The Praseodymium Oxides............. * . . . . 65 A. Properties of the Praseodymium Oxides. B. Effect of Other Rare Earth Oxides on Praseodymium Oxides . . 66 .... 77 C. Effects of Praseodymium Oxides on Magnetic Susceptibility Measurements of Rare Earth Oxides....................... 91 D. VIII Conclusion............................. 95 Discussion and Suggestions for Future Researches................................. 97 Summary.......................................... 103 Literature Cited ................................ 105 INTRODUCTION The development of new techniques for the separation of the rare earth metals is the ultimate goal of practically all rare earth research. Because of the chemical similarities of the rare earth elements, 29,85,38 the utilization of fractional procedures has been necessary. Any method which lends itself to both continuous operation and automatic control would be highly desirable. Two such methods, fractional distil­ lation and liquid-liquid counter-current extraction, have been suggested, but as yet not developed. Apple2 ton and Selwood proposed the utilization of rare thiocyanates for extraction procedures; later, Templeton 86 and Peterson had considerable success in extracting saturated rare earth nitrate solutions with n-hexyl alcohol. For this dissertation the original research problem consisted of a study of the distribution of rare earth compounds between water and various organic solvents to find qualitatively a suitable combination of solvents which might be used in the development of a liquid-liquid counter-current extraction separation. 2 Rare earth acetylacetonates, nitrates, acetates, nvalerates, benzoates, p-hydroxybenzoates, 8 -hydroxyquinolates, mono-, di-, and trichloroacetates were prepared and their solubilities in a number of common organic solvents investigated. In this study the rare earth trichloroace­ tates were observed to decompose in hot solutions to form insoluble compounds, identified as rare earth carbonates. When a water solution of both lanthanum and praseodymium trichloroacetates was heated, the carbonate precipitate was found to be enriched in praseodymium. Because of this discovery, attention was focused upon the development of separations by homogeneous phase reactions, such as the precipitation of carbonates due to the decomposition of the tri­ chloroacetates and the precipitation of oxalates upon the hydrolysis of dimethyloxalate. It was also observed that trichloroacetic acid precipitated eerie ions from aqueous solutions and formed extremely soluble salts with the trivalent rare earths. These observations suggested a procedure for the separation of cerium. In order to follow the separation of rare earth mixtures, new analytical procedures were developed: 3 a) an iodometric procedure for the determination of praseodymium in binary mixtures, and b) an iodometric correction for "excess" oxygen in the oxalate-oxide average atomic weight determination. During the development of the analytical procedures, the nature of praseodymium oxide was observed to vary considerably in the presence of different rare earth oxides. Although the charac­ ter of praseodymium oxide has been the subject of extensive work by many investigators, a complete answer has not been obtained. Accordingly, this problem was studied to clarify the behavior of these praseodymium compounds in binary rare earth mixtures. A number of research ideas were formulated during this study and one section is devoted to them. 4 SECTION I Qualitative Solubility and Distribution Studies The solubilities of several neodymium salts in water and various organic solvents were studied quali­ tatively. Neodymium was chosen for this study because of its strong and characteristic absorption spectrum and because an adequate amount of pure neodymium material was available. If the saturated solution were pink, the salt was considered soluble; if the neodymium spectrum were visible through 10 cm. of solution with a hand spectroscope, the salt was considered as moderately soluble; if visible through 2 0 cm. of solution, slightly soluble; if not visible through 20 cm., insoluble. results are listed in Table I. The The trichloroacetates show a greater range of solubilities in a larger variety of solvents than do the normal acetates, suggesting the possibility of using the rare earth trichloroacetates in liquid-liquid counter-current extraction techniques. The extraction of 0.1 N neodymium nitrate solu­ tions with various organic solvents was also studied. The organic solvent layer in each case was examined for dissolved neodymium compounds with a hand spectroscope. Neodymium nitrate could be extracted from a 0.1 N aqueous TABLE I Qualitative Solubilities ( Neodymium Salts Insoluble Soluble Moderately Soluble Slightly Soluble Acetate Water Methyl Carbon Benzyl Benzyl Benzyl Chloroform Nitrobenzene Chlorobenzene n-Amyl Alcohol Monochloroacetate Water Ethyl Alcohol Acetone Dichloroacetate Water Ethyl Ether Trichloroacetate Water Acetone Alcohol Ethyl Alcohol Acetone Hexone* Ethyl Acetate n-Amyl Alcohol Water Ethyl Acetate Benzene Hexane Carbon Tetrachloride Butyl Bromide Xylene Hexone* Toluene Methyl Iodide Ethyl Ether Benzene Benzene Ethyl Ether Chloroform Benzene Hexane Salt n-Valerate Acetylacetonate Salicylate Disulfide Chloride Alcohol Carbinol Water Benzoate p-Hydroxybenzoate Hexone* Acids Acids Acids 8 -Eydroxyquincflate Acids Chloroform Carbon Disulfide Carbon Tetra­ chloride * - Methyl Isobutyl Ketone V/ater Organic Solvents Water Organic Solvents Benzene Hexone* Ethyl Acetate Water VJl 6 solution with n-butyl alcohol and n-valeric acid, but probably not with hexane, carbon tetrachloride, n-arayl alcohol, t-amyl alcohol, or hexone (methyl isobutyl ketone). Mayper 55 indicated a distribution of rare earth nitrates between water and methyl butanol. 86 Templeton and Peterson succeeded in extracting satu­ rated nitrate solutions with n-hexyl alcohol. i 7 SECTION II Preparation and Properties of the Rare Earth Trichloroacetates Since trichloroacetic acid and its salts are not widely used in inorganic chemistry a brief resume of their properties will be outlined. 21 Dumas first prepared trichloroacetic acid by adding dry chlorine gas to crystalline acetic acid in a glass-stoppered flask and placing the flask in sunlight for a day. The chlorine disappeared and large rhombohedral crystals of trichloroacetic acid formed. Dumas analyzed this acid and characterized many of its properties. He prepared the silver, ammonium, and potassium salts by evaporating their water solutions at room temperature. He observed that when solutions of the trichloroacetates were heated, chloroform was liberated and a carbonate was formed. Barium carbonate was prepared by boiling a solution of barium hydroxide and trichloroacetic acid. This decomposition reaction is of particular importance since it offers a method for the preparation of many carbonates which cannot be easily prepared as pure and crystalline compounds. i 8 Although trichloroacetic acid has been known for over a hundred years, only a few of its inorganic salts have been studied. It is a strong acid, compa­ rable to hydrochloric acid, and forms ionic salts with the more basic elements, e.g. the alkali and alkaline earth elements. Trichloroacetic and acetic acids have many of the same properties, such as the tendency to form complex ions with certain transition elements and insoluble basic acetates with the amphoteric elements. The normal and basic trichloroacetates which have been reported are listed in Table II. The normal trichloroacetates are ionic salts which are highly soluble in water, alcohol, and acetone, but practically insoluble in carbon tetrachloride and benzene. They will decompose in aqueous solutions to 93 produce carbonates. Verhoek studied the kinetics of the decomposition of trichloroacetic acid and its sodium 21 and barium salts; Hall and Verhoek studied its sodium, barium, calcium, and lithium salts (Section IV). The basic trichloroacetates are sparingly solu­ ble in water, but may be recrystallized from 9 5 per cent 45 ethyl alcohol. This solubility phenomenon usually indi­ cates the formation of an internal complex between the metal and organic acid. A 9 TABLE II Inorganic Salts of Trichloroacetic Acid Normal Compounds Metal Formula of Salt Reference Ammonium NH4.C2C13C^ Barium Ba(0201302 )2 *592 ° 93 Ba(C2 Cl302 )2 *2 H20 83 Beryllium Be(C2 Cl302 )2 *2 H20 83 Cadmium Cd(C2 Cl302 )2 *l-l/2 H20 28 Cerium Ce(C2 Cl302 )3 *3H20 Cobalt Co(C2 C1302 )2 ,5 -1/2 H20 Copper 5 100 28 Co(C2Clz02)z 'kE2° 1 Cu(C2C1302)2*5^2 0 4 C u (C2C1302 )2*6H20 43 Lead Pb( O ^ l ^ V ^ O 43 Manganese MnCCaCLjQ^^KaO 28 Potassium 21 Silver AgC2Cl302 21 Sodium NaC2Cl302 93 Basic Compounds Beryllium Be0(C2Cl302)2 33 Cobalt Co(0H)2 *2Co (C2C1302 )2 •L-H20 1 Copper Cu(C2Cl302 )2*3Cu (0H)2 ‘x I^O 12 Indium ln(0H)(c2cl302)2 22 Thorium Th(0H)2(C2Cl302)2*H20 Uranium U0 (C2C1302)2*3 H20 44,45 57 10 50 Mandl precipitated zirconium from a nitrate solution by the addition of trichloroacetic acid and suggested the formation of a basic salt, but failed to report an analysis of the compound. In the present research basic eerie trichloro­ acetate was prepared and studied (Section V). Solutions of ferric trichloroacetate may be rendered colorless by the addition of excess trichloro47 acetic acid. Absorption studies give evidence for the formation of a soluble complex ion /Fe(C2C1^02)^_7 There is some indication that chromium may form a simi­ lar complex ion with trichloroacetic acid. Beilstein lists mercuric trichloroacetate as having been prepared by Clermont. However, other 4,13,46 workers have not been successful in preparing this salt since apparently it immediately decomposes to form insoluble mercurous chloride when mercuric oxide is added to trichloroacetic acid in water. 100 Wolff prepared cerous trichloroacetate, Ce(C2 C1 ^ 0 2 )^*3 H2 0 , as long needles by concentrating its water solution in a vacuum desiccator. A thorough search of the available literature did not reveal the preparation of any of the other rare earth trichloro90 acetates, although Urbain did attempt to fractionally precipitate the rare earths as acetates and chloroacetates. 4 The preparation of the rare earth trichloro­ acetates consists of dissolving the oxide in a concen­ trated solution of trichloroacetic acid, heating the solution until rare earth carbonate begins to precipi­ tate, cooling the solution in an ice bath, filtering the carbonate, and crystallizing the salt at room temperature by evaporating the water in a vacuum desiccator. The salt may be dried over phosphorous pentoxide or concentrated sulfuric acid. If recrystal­ lized from alcohol, there is evidence that some of the solvent is retained as alcohol of crystallization. The procedure for the preparation of neo­ dymium trichloroacetate follows. Neodymium oxide, 25 g., is dissolved in 300 ml. of 25 per cent trichloroacetic acid solution. The excess acid is decomposed by heating the solution to about 90° C. When neodymium carbonate begins to precipitate, the solution is quickly cooled to room temperature and the carbonate filtered. The filtrate is a solution of neodymium trichloroacetate free of excess trichloroacetic acid. The salt is crystallized at room temperature by evaporating the water in a vacuum desiccator. Yields of 90 per cent or better are obtained. The composition of neodymium trichloroacetate prepared by the above method and air dried was determined. Analysis for neodymium oxide was made by dissolving a weighed sample of the salt in water, precipitating neo­ dymium oxalate with oxalic acid, igniting the oxalate in a muffle furnace, and weighing the resulting oxide. For the chlorine analysis a weighed sample was decom89 posed by the method of Umhoefer. This consisted of refluxing the salt with sodium in isopropyl alcohol for two hours. After the solution was neutralized with 6 N nitric acid, chloride was determined by the 96 Volhard method. Comparison of the theoretical and experi­ mental values for the neodymium oxide and chlorine (Table III) indicates that the formula for the neo­ dymium trichloroacetate is ^ ( 0 2 0 1 3 0 2 )3 *3 H2 0 . TABLE III The Analysis of Neodymium Trichloroacetate For Nd (C2 CI3 O2 )3*3 H2 0 Per Cent NdgC^ Cl Experimental 24.4 46.3 Theoretical 24.6 46.5 Neodymium trichloroacetate forms heavy pink needles when crystallized from water. The crystals are very soluble in water, acetone, and alcohol; less solu­ ble in ether, hexone, ethyl acetate, n-amyl alcohol, and chloroform; and insoluble in benzene and n-hexane. 13 The anhydrous salt was not obtained by moderate heating since the salt and its water of hydration react. The neodymium trichloroacetate is contaminated with carbonate. Upon ignition the salt does not melt but decomposes to yield neodymium oxide and a gas which has an odor simi­ lar to phosgene. In warm water the course of the decom­ position reaction appears to be represented by the equation 2 Nd(C2 Cl3 0 2 )3 + 3H0H --- ^ 3C02 + 6 CHCI3 + ^ ( 0 0 3 )3 . Decomposition of neodymium trichloroacetate is not observed in anhydrous acetone, but proceeds at room temperature upon the addition of water. The solubility of neodymium trichloroacetate o was determined at 25 C. A known volume of the satu­ rated solution was weighed, diluted with water, and the neodymium oxalate precipitated with oxalic acid, and ignited in a muffle furnace. The solubility of neo­ dymium trichloroacetate was calculated from the weight of oxide obtained and found to be 2 2 5 . 8 g. of Nd(C2 Cl3 0 2 )3 *3 H2 0 per 100 g. of water. The density of the saturated solution at 25° C. was 1.636 g. per ml. It is of interest to compare the solubilities of the neodymium acetate and trichloroacetate. Meyer 66 and Muller reported the solubility of a monohydrated neodymium acetate as 2 0 . 7 6 g. per 100 g. of water, 14 whereas Thomas 87 gave the solubility in terms of anhydrous salt as 20.19 g. of acetate per 100 g. of saturated solution. It is observed that the solubility of the acetate is very appreciably lower than that of the trichloroacetate. From these data, and from obser­ vations made during the separation studies involving the trichloroacetates, it may be stated that the latter salts of the rare earth ions are definitely more soluble than the acetates, the increase in the case of the neodymium compounds being approximately tenfold. 1 15 SECTION III Preparation of Rare Earth Carbonates Two methods have been used to prepare rare earth carbonates, neither of which is entirely satis­ factory for producing a pure crystalline compound. The 91,92 older method was first used by Vauquelin, who pre­ cipitated cerous carbonate by the addition of an alkali carbonate to a cerous salt solution. This method usually produces amorphous flakes which become crystalline only after standing in the liquid several days. Priess and 77 Dussik obtained a more crystalline product by using alkali bicarbonates for the precipitation. Neverthe­ less, the carbonate is usually contaminated with alkali carbonates because the rare earths also form insoluble 64alkali double carbonates. A second method for pre19,20 paring rare earth carbonates was proposed by Cleve. He obtained them by passing a current of carbon dioxide through a suspension of the rare earth hydroxides in water. Such a conversion of one solid to another is seldom complete. Rare earth carbonates free from hydroxide impurities are not obtained. For this study pure crystalline rare earth carbonates were prepared by the decomposition of rare Barth trichloroacetates according to the following procedure. 16 Approximately 10 g. of a rare earth oxide is dissolved with warming in slight excess of 25 per cent trichloro­ acetic acid. This solution is diluted to 500 ml. with distilled water and heated on a steam bath for about 6 hours after the first precipitate of carbonate is formed. The carbonate is filtered by suction, washed with distilled water, and air dried. The precipitated carbonate may be washed with alcohol and then ether in order to hasten drying. Since all of the rare earth is not precipitated by this method, the filtrate should be treated with oxalic acid to recover the rare earth as the oxalate. An excess of trichloroacetic acid is required to dissolve the rare earth oxide, but the carbonate will not precipitate until the excess acid has bean removed. The time required for this operation is dependent upon the amount of the excess acid and the temperature of the bath. The carbonates as described in the above pro­ cedure appear to be normal carbonates of the formula **2 ^ 0 3 ) 3 ,xH2°* This conclusion is based upon the experi­ mental determination of the percentages of rare earth oxide and carbon dioxide and the calculation of the mole ratio C0 2 /R2 0 3 * This ratio is 3 only for normal carbonates. A value less than 3 is obtained for basic 17 carbonates and greater than 3 for acid carbonates. For example, the mole ratios C0 p/R2 0 ^ would be 2 and 6 respectively for R(0H)C0^ and R(HCO^)^. Weighed samples of a particular carbonate were ignited in a muffle furnace at a temperature of 925° C. The resulting oxides were weighed and the per cent rare earth oxide in the carbonate calculated. Other weighed 96 samples were treated in a C02 gas analysis apparatus with dilute hydrochloric acid. The liberated carbon dioxide was collected in an absorption bottle and weighed. The per cent carbon dioxide in the carbonate and the mole ratio CO2 /R2 O3 were calculated. Lanthanum, neodymium, and samarium carbonates were prepared and analyzed. The results are listed in Table IV. TABLE IV The Analysis of Rare Earth Carbonates $ co2 h 2o r 2°3 R2°3 r 2°3_ co2 h2 o* Lanthanum 58.55 2 3 .6 0 17.85 2.98 5.51 La2(C03)3 •5.5H20 Neodymium 65.80 25.35 8.85 2.95 2.51 Nd2(C03)^ *2,5H20 Samarium 65.88 2 3 .4 3 10.69 2.82 3.14 Sm2 (CO3 ) 3 *3H20 Carbonate * - (100 - ^r2o 3 - ^C02 ) Formula Since the mole ratios C0 2 /R2 ° 3 indicate normal carbonates, the difference between 100 and the sum of the percentages of rare earth oxide and carbon dioxide must be the per cent of water in the carbonates. The mole ratio H2 O/R2 O3 in each case may then be calculated. These results were not verified experimentally. The mole ratio CO2 /R2 O3 is smaller for samarium carbonate than for the other two. This indicates a slight tendency toward basic salt formation; a condition which might be expected for the less basic rare earth elements (yttrium group). The preparation of anhydrous neodymium carbon­ ate was attempted. Samples of neodymium carbonate were dried under different conditions and analyzed for neo­ dymium oxide as before and for carbon dioxide by a volu­ metric procedure which consisted of dissolving weighed samples in an excess of standard 1 N nitric acid, diluting with water, boiling to remove the carbon dioxide, and determining the excess acid by titration with a standard 0.1 N sodium hydroxide solution using methyl red as the indicator. The mole ratios and J ^ O A ^ O ^ were calculated and are listed in Table V. The mole ratio 0 0 2 / ^ 2 0 ^ remained approxi­ mately 3 for the above drying conditions; the mole ratio 19 TABLE V Effect of Heat on Hydrated Neodymium Carbonate y ft y JO COo d HpO d Drying Conditions NdgO^ CO2 H2 O Nd2 0 ^ A Air dried* 65.8 25.4 8 .8 2.96 2.50 B 1 hr. at 110°C. 68.2 26.7 5.1 3.00 1.40 C 12 hrs. at 110°C. 70.8 2 7 09 1.3 3.02 0.34 D 3 days at 120°C. 71.4 2 7 .8 0;8 2.98 0.21 7 1 .8 28.2 0.0 0.00 Sample Nd2(C03 )3 (theoretical) Nd2 Q3 3.00 * - Washed with alcohol and ether. H20 /Nd20 3 decreased continually, indicating dehydration. For an extended drying period, as in the case of Sample D, a carbonate was obtained which was essentially anhydrous. The preparation of rare earth carbonates by the decomposition of the trichloroacetates from hot water solutions is more satisfactory than older preparations. Pure normal carbonates are produced since no interfering ions are introduced. 20 SECTION IV Separation of Praseodymium and Lanthanum Among the reactions used for fractional pre­ cipitation methods of separating the rare earths, homo­ geneous phase reactions have been very satisfactory even though some of them have certain disadvantages. The hydrolysis reactions that have been used are listed by 68 Moeller and Kremers in an excellent review article on the basicity characteristics of the rare earths. Some of the more important ones involve the separation of cerium by oxidation to the eerie form followed by hydroly­ sis of rare earth nitrites, phthalates, lactates, sulfites, citrates, tartrates, ra-nitrobenzoates, phenoxyacetates to form basic salts. In most of these methods the desired anion was added in the form of an alkali salt. The resulting high concentration of alkali ions in the reaction mixtures is disadvantageous. 97 Willard and Gordon separated thorium and the rare earths from monazite by a homogeneous phase reaction involving the hydrolysis of dimethyloxalate to precipitate insoluble thorium and rare earth oxalates. Thorium was separated from the rare earths by the hydrolysis of urea in the presence of formic acid; an insoluble basic thorium formate precipitated. A more recent method 35 involves the 21 hydrolysis of tetrachlorophthalic acid to produce an insoluble thorium compound. No data about these homo­ geneous phase separations being applied to the rare earth group have been published. Since praseodymium and lanthanum salts have very similar chemical and physical properties, their separation is difficult. Slight differences in solu­ bilities and basicities are the important criteria in such separations. Methods which depend upon the immedi­ ate formation of a precipitate after addition of a reagent resulting in local action do not give maximum efficiency. This difficulty is minimized by the use of homogeneous phase reactions in which the reagents are formed in solution. Two homogeneous phase reactions which have been investigated for the separation of praseodymium and lanthanum are the decomposition of the trichloro­ acetate ion in the presence of rare earth ions to form the insoluble rare earth carbonates, and the hydrolysis of dimethyloxalate in rare earth solutions to yield insoluble rare earth oxalates. 22 Part A. The Trichloroacetate Separation The rate of decomposition of the trichloro­ acetate ion to form chloroform and carbon dioxide has 37,93,94,95 been studied rather extensively by Verhoek. In water the rate of decomposition of the trichloro­ acetate ion is dependent upon the temperature and concen­ tration but almost independent of the nature or size of the accompanying cation. Verhoek 37 claims that for a fixed temperature and salt concentration there is very little difference in the rate of decomposition of sodium, ammonium, barium, and even tetraethylamine trichloroacetat.es in water. Because of the dissimilarities in proper­ ties of the above mentioned cations, it may be assumed that lanthanum and praseodymium trichlcroacetates decom­ pose st essentially the same rate and that the separation of these two rare earths does not depend upon a difference in the rate of decomposition of their respective trichloroacetates. 93,94 Verhoek has shown that it is the trichloro­ acetate ion which decomposes and not the free acid or its salts. The trichloroacetate ion under the influence of heat yields carbon dioxide and the strongly basic trichlaromethyl ion, which immediately reacts with water to form chloroform. 23 CCl^COO CCI3 + co2 CCl3~+ H20 — CHCI3 + OH Since chloroform is insoluble in water it is evolved; the carbon dioxide reacts with the y?ater and any cation present to form a carbonate. If the carbonate is an insoluble one, such as an alkaline earth or rare earth carbonate, a precipitate forms. When several different cations are present, the carbonate of the one which is the least soluble has the greatest tendency to precipi­ tate. For a lanthanum-praseodymium mixture, the praseo­ dymium has the greater tendency to precipitate as the carbonate leaving the mother liquor enriched in lanthanum. If the reaction continues until all the trichloroacetate ion has decomposed, the filtrate contains only a small quantity of rare earth chloride. The chloride ion is formed during the reaction- by the secondary oxidation of chloroform in the hot solution. Praseodymium may be concentrated by the following method. The lanthanum and praseodymium oxide mixture is dissolved in the theoretical quantity of hot 25 per cent trichloroacetic acid solution by sifting the oxide gradu­ ally into a flask containing the acid. A slight excess of acid may be necessary to effect complete solution. Oxides containing a high praseodymium content are more difficult to dissolve. The rare earth trichloroacetate i 24 solution is diluted with water until the rare earth concen­ tration is approximately 10 grains of oxide per liter. The o solution is heated to 90 C. on an electric mantle. This temperature is maintained for 20 minutes after the first appearance of a precipitate. During the heating the solution is stirred continuously. The reaction is stopped by cooling the flask to room temperature in an ice water bath. The carbonate precipitate, containing about 30 per cent of the rare earth, is filtered in a Buchner funnel and washed with a small quantity of water. The filtrate o is reheated to 90 C. and the decomposition reaction carried on for 35 minutes. The mixture is cooled and the precipitate (another approximately 30 per cent of the rare earth) filtered as before. Its praseodymium content exceeds that of the original sample by about 10 per cent. The filtrate from the second precipitation is treated with oxalic acid to recover the remaining rare earth. A typical example illustrating the concentration of praseodymium consisted of treating 72 grams of an oxide sample containing 36 per cent Pr^O^ (Separation I, Table VI). the method outlined Upon ignition the first carbonate precipitate yielded 22 grams of an oxide containing 53 per cent Pr^On, indicating an enrichment of 18 per cent. A second precipitate gave 21 grams of oxide containing 46 per cent Pr^O-j^, or a praseodymium oxide enrichment exceeding 25 the original by 10 per cent. The final filtrate yielded 29 grams of rare earth oxide which had been reduced to 21 per cent Pr^O^i* The rare earth obtained in the first precipi­ tate was treated in similar fashion to further concen­ trate the praseodymium (Separation II, Table VI). The 53 per cent material yielded in the first precipitate 6.5 grams of an oxide which contained 72 per cent Pr^O-Qj in the second precipitate 6.5 grams of an oxide which contained 62 per cent Pf ^O-q ; and from the filtrate 9 grams of an oxide, which by coincidence had the same composition as the original sample, namely 36 per cent Pr6°ll° The results of these two separations are listed in Table VI from which it can be seen that the praseodymium TABLE VI The Enrichment of Praseodymium by the Trichloroacetate Separation Weight Per Cent Pr^Opi* Sample Separation I Original 36 First Carbonate 53 Second Carbonate 46 Filtrate 21 * Separation II - The oxides were analyzed for praseodymium by the absorption spectra method (Section VI). ** - This sample is the same as the first carbonate precipitate Separation I. 26 content was doubled in two steps from 3 6 to 72 per cent Pr6 °ll* The effects of two variables, temperature and concentration, upon this separation were investigated. The results obtained show that the degree of separation of lanthanum and praseodymium is dependent upon the concentration of rare earth trichloroacetates in solution, and essentially independent of the temperature at which the reaction is carried out. The temperature effect was investigated by heating trichloroacetate solutions containing 10 grams of lanthanum-praseodymium oxide mixture per liter at o o o o 60 , 70 , 80 , and 90 C. Two fractions of carbonates, each containing about 3 0 per cent of the original oxide sample, were removed and analyzed-for praseodymium. The reaction times and analyses are listed in Table VII. TABLE VII The Effect of Temperature on the Trichloroacetate Separation Reaction Time (Hrs.) Weight Per Cent Pr£,0n* Temp. Carbonate Carbonate Carbonate Carbonate C°C.) I_____ II__ O r i g i n a l ____I___ _____ II 90 0.33 0 .6 53 72 60 80 1.5 2 .5 53 70 61 70 6.5 11.5 53 73 63 60 32.5 62 .5 53 71 62 * - Analyzed by the absorption spectra method (Section VI). i 27 The reaction time in each case was calculated using the 94 rate constants reported by Verhoek for the decomposition of sodium trichloroacetate in water. From these results it is evident that the separation of praseodymium is not improved by carrying out the decomposition at a lower temperature and a slower rate. The effect of rare earth concentration was investigated in a similar manner. The decomposition reaction was carried out at 90° C. with trichloroacetate solutions containing 10 and 20 grams of rare earth oxide per liter. The first carbonate fraction was removed 20 minutes after the appearance of a precipitate, the second after an additional 35-minute period. Each fraction contained approximately 3 0 per cent of the original rare earth. The carbonates and the final filtrate were ana­ lyzed for praseodymium and the average results of several reactions are listed in Table VIII. TABLE VIII The Effect of Rare Earth Concentration on the Trichloroacetate Separation Weight % Pr^O^* Rare Earth Oxide Concentration (g./l.)______ Original Carbonate I ___ Carbonate II Filtrate 10 53 72 62 36 20 53 65 61 41 * - Analyzed by the absorption spectra method (Section VI). 28 The results clearly indicate that a better separation of praseodymium is obtained in the more dilute solutions. In other experiments it was observed that if the concentration is less than 1 0 grams per liter, the carbonates tend to be gelatinous and diffi­ cult to filter. A. comparison of the enrichment of praseodymium at 90° C. in carbonate fractions removed after permitting the trichloroacetate decomposition to run for long periods of time with those removed after short time intervals was made. The mixed oxides of lanthanum and praseodymium were dissolved in 25 per cent trichloroacetic acid. The solution, diluted with water so that the rare earth concen­ tration was 2 5 ’ grams of oxide per liter, was heated to and maintained at 90° C. for two hours. During the heating the solution was stirred continuously. The carbonate was filtered off and dissolved in the minimum quantity of 5 per cent trichloroacetic acid. This solution was then heated for two hours in the same manner as the original solution to decompose the acid and precipitate another carbonate fraction. The carbonate was filtered, dissolved in the 5 per cent acid, and the decomposition again effected. This process of precipitating a carbonate fraction, dis­ solving it and reprecipitating was repeated several times. 29 The analyses of the different fractions obtained in one typical separation are given in Table IX. The original oxide sample weighed 26.2 grams and contained 6 7 per cent Pr^011; Fraction 8 , consisting of high purity praseodymium, weighed 4.5 grams and represented a yield of approximately 2 5 per cent with respect to the original praseodymium content. For this type of separation it is also observed that the carbonate precipitate is enriched in praseodymium. TABLE IX The Purification of Praseodymium by the Trichloroacetate Separation Fraction Weight % Original 67 1 74 2 3 4 5 79 86 91 94 97 99 99+ 6 7 8 * - Analyzed by the absorption spectra method (Section VI), Of the two procedures the former is the better for quickly concentrating small amounts of praseodymium from samples which contain less than 80 per cent praseodymium oxide. For samples containing more than 80 per cent praseo­ dymium, the latter procedure is better. Although the 30 enrichment per step is less, the major part of the sample remains intact and much less praseodymium is sacrificed. The latter procedure was utilized for the puri­ fication of some praseodymium oxide (about 16 grams) which contained about 5 per cent lanthanum oxide. The decom­ position time was increased to 3 hours in order to pre­ cipitate a larger portion of the rare earth. After 10 fractionations the carbonate obtained was ignited. About 8 grams of oxide was secured. Arc spectrum analysis* showed the following elements to be present as impurities: lanthanum, less than 0 . 0 2 per cent; iron, less than 0.02 per cent; silicon, 0.04 per cent. Elements not detected were aluminum, calcium, cerium, cobalt, chromium, dysprosium, erbium, europium, gadolinium, holmium, lutetium, magnesium, manganese, molybdenum, neodymium, nickel, lead, scandium, samarium, strontium, terbium, thulium, titanium, vanadium, yttrium, ytterbium, and zirconium. It is evi­ dent that the method may be applied to the separation of small amounts of lanthanum from oxides rich in praseodymium. Cerium interferes and should be removed before attempting to separate lanthanum and praseodymium. In a hot solution cerium is oxidized and precipitated as hydrated eerie oxide. Its presence imparts a gelatinous character * - Analysis by Dr. F. S. Tomkins, Argonne National Labora­ tory, Chicago, Illinois, tc the carbonate precipitate and filtration becomes diffi­ cult. However, if a small quantity of cerium is present when the oxide is dissolved in trichloroacetic acid, it precipitates as an insoluble yellow basic eerie trichloro­ acetate which can be filtered. The filtrate is then treated for the separation of lanthanum and praseodymium. The trichloroacetate separation of praseodymium and lanthanum is rapid, requires a minimum of labor and space, uses ordinary laboratory equipment, requires no expensive chemicals, and can be applied to large scale production. 32 Part B The Dimethyloxalate Separation 85 Several procedures, which may be classified into two groups, have been developed for the fractional precipitation of rare earth oxalates. In one type, oxalic acid solution is added drop by drop to a hot acidic rare earth solution until a slight permanent precipitate is formed. The solution is then allowed to cool after which some rare earth oxalate precipitates. The mixture is filtered and the filtrate subjected to the same treatment as the original solution. The order of decreasing solubiDity from the most to the least solu­ ble oxalate is lanthanum, cerium, praseodymium, neodymium, 80 and samarium. In the second type of separation a partial solution of rare earth oxalates in alkali oxalate solutions is effected. Due to the formation of soluble complex oxalates, the order of solubility is reversed; lanthanum oxalate is the least soluble and samarium oxalate the most soluble in alkali oxalate solutions. Recently 10 Beck developed a varjation of the latter procedure by dissolving rare earth oxalates in a solution of sodium nitrilotriacetate, NCCHgCOONa)^, ana fractionally reprecipitating them as the solution is acidified. Lanthanum oxalate precipitated first, followed by the oxalates of 35,97 the less basic rare earth elements. Willard and i 33 co-workers suggested the hydrolysis of dimethyloxalate in perchloric acid solutions for the separation of the rare earths and thorium from monazite. Complete pre­ cipitation was not obtained due to incomplete hydrolysis of the dimethyloxalate. A. small quantity of oxalic acid was finally added to complete the precipitation. No report was given about the use of this reaction to sepa­ rate the members of the rare earth group itself. The fractional precipitation of rare earth oxalates based upon the internal hydrolysis reaction of dimethyloxalate to produce oxalate ions in solution minimizes the interference due to local action when oxalate solutions are added directly. The reaction may be represented as 2 RCI3 + 3 (CH3 )2 C2 04 + 6H0H -> R2 (C2 04 ) 3 + 6 CH3 OH + 6HC1. It was found that praseodymium may be concentrated by the following method. About 5 g. of a mixture of lantha num and praseodymium oxides is moistened with water and dissolved in the minimum quantity of concentrated hydro­ chloric acid. The solution is diluted with 600 ml. of 1 N hydrochloric acid. About 2.8 g. of dimethyloxalate is dissolved in 400 ml. of 1 N hydrochloric acid. (This is sufficient dimethyloxalate to precipitate half the rare earths in solution as oxalates if all the ester hydrolyzes.) The dimethyloxalate solution is added from 34 a dropping funnel to the rare earth solution at a rate of about one drop per 2-3 seconds. The reaction mixture is stirred continuously during the addition of the ester solution. After all the dimethyloxalate has been added, the solution is stirred for an hour. Approximately one- third of the original quantity of rare earth is precipi­ tated as a very dense crystalline rare earth oxalate, which is filtered in a Buchner funnel and ignited to the oxide. The rare earth in the filtrate is precipi­ tated with oxalic acid; the oxalate is filtered and ignited to the oxide. The precipitation of rare earth oxalates by the hydrolysis of dimethyloxalate is rapid in neutral solution, but considerably slower in acid medium. If the concentration of rare earth and ester is low, the precipitation is still slower. Since rapid precipitations generally result in poorer products than slow ones, the conditions which favor a slow oxalate precipitation are utilized. The original oxide and the oxides obtained from the precipitate and the filtrate were analysed for praseodymium by the iodometric method. The results of two different dimethyloxalate separations are listed in Table X as Experiments 1 and 2, In one variation of the above procedure, Experi­ ment 3 , all of the dimethyloxalate solution was added at 4 35 one time and the solution stirred for two hours before being filtered. In Experiment 4 the dimethyloxalate solution was added dropwise as in Experiments 1 and 2 except that 1 N sulfuric acid was used instead of 1 N hydrochloric acid as the solvent for the sample. TABLE X The Enrichment of Praseodymium by the Dimethyloxalate Method Weight Per Cent Pr^O^* Experiment Original Precipitate Filtrate 1 64 85 59 2 64 85 60 3 64 80 58 4 64 70 - * - Oxides analyzed by the iodometric procedure (Section VI). Since the idea for the dimethyloxalate sepa­ ration was conceived late in the research program, con­ ditions which govern the degree of separation, such as concentration of rare earth and dimethyloxalate, tempera­ ture, pH, and effect of various acids and complexing agents, have not been studied as completely as in the trichloro­ acetate separation. However, the following facts may be observed from the values listed in Table X: a) the per­ centage of praseodymium in a rare earth sample may be incieased by 2 q per cent in one step, b) a poorer separation 36 is obtained if all the dimethyloxalate is added at one time, c) the separation is considerably better in chloride solutions than in sulfate solutions. The dimethyloxalate procedure appears to have advantages over the trichloroacetate procedure in that cerium does not interfere and does not have to be previ­ ously separated and heating is unnecessary since the reaction proceeds at room temperature. Its principle disadvantage is that the oxalates must be ignited and the resulting oxide dissolved before carrying out a second fractionation, while the trichloroacetate decom­ position produces a carbonate which is easily dissolved in a dilute trichloroacetic acid solution. i 37 SECTION V The Trichloroacetate Separation of Cerium The usual separation of cerium from the other rare earths is based upon the facts that cerium may be oxidized to the tetravalent state and that eerie compounds are easily hydrolyzed to insoluble basic salts. The two methods most commonly used in the laboratory are the 24,41,42 potassium bromate method and the permanganate79 eerie oxide method. In the former, cerium is oxidized by potassium bromate in a solution buffered by lumps of marble. A basic eerie nitrate is precipitated slowly as the solution is boiled. The method is slow; the physical nature of the marble is important. If powdered marble is used, the pH will be too high and some rare earth hydroxide will contaminate the basic eerie salt. In the permanganate method cerium is oxidized by potassium permanganate and is precipitated as a hydrated eerie oxide pH to about 3.5 by adjusting the with dilute hydroxide solution. Although this method is faster than the bromate method, it has the disadvantage of adding manganese to the solution. Several precipitations of the rare earths as oxalates are often necessary to separate all the manganese. of pH is critical. The adjustment If it is too low not all the cerium is precipitated, if too high the trivalent earths precipitate. 38 When the hydroxide is added some of the trivalent earths have a tendency to precipitate due to a high local hydroxide concentration where the drops come in contact with the solution. The rare earth hydroxides are not always com­ pletely redissolved; hence the cerium is frequently con­ taminated with other rare earths. While studying the properties of the rare earth trichloroacetates it was observed that tetravalent cerium and thorium form insoluble basic trichloroacetates. The compounds were similar to the basic acetates produced with acetic acid. soluble. The rare earth trichloroacetates are extremely This difference in solubility between the basic and normal salts immediately suggested a possible sepa­ ration of cerium. Trichloroacetic acid is used to separate cerium from lanthanum, praseodymium, and neodymium by the following procedure. One hundred grams of the freshly ignited rare earth oxide is dissolved in the minimum quantity of concen­ trated nitric acid. one liter with water. The solution is cooled and diluted to Seventy-five grams of trichloro­ acetic acid dissolved in a few milliliters of water is added to the rare earth solution. £Chis is approximately the quantity of trichloroacetic acid equivalent to the formation of the rare earth salt RCC2 GI2 O2 Although i the solution is strongly acid from the addition of the trichloroacetic acid, a large portion of the cerium sepa­ rates immediately as a light yellow precipitate. The basic eerie trichloroacetate is filtered with gentle suction in a Buchner funnel supplied with a filter mat. (A. suitable mat may be prepared from filter paper pulp.) The precipitate is washed with a 5-10 per cent trichloro­ acetic acid solution, which dissolves any trivalent earth hydroxides that may have coprecipitated with the cerium compound, but will not dissolve the basic salt. Water must not be used as a wash solution because the basic tri­ chloroacetate becomes colloidal ana is washed through the filter. The major portion of the cerium is removed in this first precipitation. Any remaining cerium may be removed from the filtrate by adding 6 N ammonium hydroxide slowly with stirring until the solution becomes neutral to litmus. At this higher pH the remaining cerium is precipitated along with some rare earth hydroxide. A few milliliters of 2 0 per cent trichloroacetic acid solution is added until the solution is again acid to litmus. The rare earth hydroxide redissolves, but the basic eerie trichloro­ acetate remains insoluble and may be fjltered as before. The process of adding b N ammonium hydroxide followed by 2 0 per cent trichloroacetic acid is continued until the precipitate formed by the ammonia is soluble in the acid. 40 A. clear solution upon the addition of a small quantity of the trichloroacetic acid is an indication that the solution is free of eerie cerium. The basic eerie tri­ chloroacetate is dissolved in concentrated nitric acid and the cerium recovered as the oxalate. A concentrated nitrate solution of the cerium obtained by this method yields a colorless solution when the cerium is reduced with hydrogen peroxide, and the absorption spectra of neodymium and praseodymium are not detectable. Cerium of rather high purity may be obtained by this trichloroacetate method. The procedure given above is dependent upon all the cerium being in the tetravalent form. It has 7 been shown by Barthauer and Pearce that all of the cerium in freshly ignited rare earth oxide mixtures exists in the tetravalent form only. Unlike praseo­ dymium, the oxidation state of cerium is not affected by the presence of other rare earth oxides. The exact chemical composition of basic eerie trichloroacetate is not known, although basic thorium trichloroacetate, (CljC*C0 0 )2 Th(0 H)2 , was prepared by 44 Karl who recrystallized it from hot 95 per cent alcohol. He found the thorium compound to be only slightly soluble o in water; 100 ml. of water at 25 q. dissolved 0.0091 g. (Cl-^C •C0 0 )2 Th(0 H)2 . In this study qualitative solubility < 41 determinations indicate that the cerium compound is even less soluble; the basic trichloroacetate separation of cerium depends upon a low solubility of the eerie compound in water and dilute trichloroacetic acid solutions. Basic eerie trichloroacetate is an insoluble yellow compound of a slightly gelatinous nature. In physical appearance it resembles other basic salts of tetravalent cerium. It is not a normal trichloroace­ tate since these compounds are crystalline and extremely soluble in water, yet it is not gelatinous enough to be confused with hydrated eerie oxide. It is soluble in concentrated nitric acid, less soluble in alcohol, and almost insoluble in excess trichloroacetic acid solution. It becomes colloidal in very dilute solutions probably due to further hydrolysis. The compound is difficult to ana­ lyze, since any of the common drying techniques cause some decomposition of the trichloroacetate ion. 42 SECTION VI Analytical Methods for the Rare Earth Elements In any rare earth separation research the choice of a suitable analytical method is important. Methods which are both rapid and accurate are highly desirable. It is often necessary to develop new methods to suit the particular mixture being investigated. The first part of this section is a discussion of the principal analytical methods for the determination of the rare earth elements. Since a large part of the present research deals with the separation of praseodymium and lanthanum, the methods used for the determination of praseodymium, including a new iodometric method, are dealt with in the second part of this section. The last part describes a correction for average atomic weight determi­ nations of rare earth mixtures by the oxalate-oxide method. Part A Principal Analytical Methods The five fundamental methods for the quanti­ tative determination of mixtures of rare earth elements are average atomic weight determinations, special methods involving a change in valence state of a particular rare earth element, spectroscopic methods, magnetochemical analyses, and the use of radioactive tracers. The first two are based upon chemical reactions in common usage. However, the second method is applicable only to those rare earth elements which are capable of existing in more than one valence state. The last three methods are based upon physical properties, the measurement of which requires special equipment that is not always available in the ordi­ nary chemical laboratory. The relationships most frequently used to evalu­ ate the average atomic weight of a rare earth mixture are the determinations of the acid equivalence of a weighed 23 quantity of rare earth oxide, rare earth chloride to 9 81 silver ratio, oxide to sulfate ratio, and oxalate to 8,24,32 oxide ratio. The determination of the chloride to silver ratio is the most accurate, but also the most time consuming. It requires the preparation of a pure anhydrous chloride; weighed quantities of which are treated with silver nitrate solution. The resulting silver chloride is collected and weighed. routine application. This method is impracticable for Similarly, the determination of oxide to sulfate ratio requires the preparation of an anhydrous sulfate from a weighed quantity of the oxide. Common sources of error in this method are the difficulty of removing the last traces of free sulfuric acid from the sulfate without causing decomposition, and the difficulty of weighing the anhydrous sulfates which are exceedingly hygroscopic. Since the oxalate to oxide method is rapid and fairly accurate, it is widely used. It involves the preparation of an oxalate, a weighed sample of which is ignited to the sesquioxide. A second sample is dissolved in sulfuric acid and titrated with a standard permanganate solution in order to determine the oxalate content. The average atomic weight is calculated from the oxide to oxalate ratio. In this ratio the two sample weights are directly proportional and no error is intro­ duced due to the hydrated nature of the oxalate. This method becomes inaccurate due to the formation of an oxide higher than the sesquioxide if rather large quantities of cerium, praseodymium, or terbium are present. The positive error in the case of high purity praseodymium may amount to several atomic weight units and is frequently misinterpreted as indicating a high percentage of samarium and yttrium earths in the sample. Nevertheless, this method is one of the most frequently used. 45 A volumetric method which has had limited use depends upon dissolving a weighed sample of oxide in a known excess of 0.5 N sulfuric acid and titrating the excess acid with 0.1 N alkali using methyl orange as indicator. The average atomic weight is calculated from the number of acid equivalents required to neutralize the oxide. The rare earths differ in basicity, hence the hydrolysis effect may introduce an error. It is also important that the original oxide be ignited strongly enough to free it of carbonate. The above atomic weight determinations yield the average composition of the mixture and cannot be used if the percentage of any particular element is desired. Certain of the rare earth elements, namely cerium, praseodymium, samarium, europium, terbium, and ytterbium, exist in more than one oxidation state. A few special ana­ lytical methods involving these changes in oxidation state have been developed for cerium, praseodymium, and europium. 16,30 The most common analytical procedures for the determination of cerium are the iodometric method, the ferricyanide and permanganate method, the hydrogen peroxide and permanganate method, the alkaline permanganate method, the bisrauthate and permanganate method, the persulfate „U J 5 8 >99 and the perchloric acid method* 84 In Bunsen's method, 7,88 iodometric method eerie oxide is dissolved in hydrochloric 1 acid in the presence of potassium iodide, and the liberated iodine determined with a standard sodium thiosulfate solution. This method gives inaccurate results if praseodymium or terbium are present since they also form higher oxides that are capable of liberating iodine. Potassium ferri- cyanide oxidizes trivalent cerium to the tetravalent form in alkaline solution. The eerie hydroxide is filtered off and the ferrocyanide formed titrated with permanganate in acid solution. The hydrogen peroxide and permanganate method is based on the fact that eerie sulfate is reduced in a dilute sulfuric acid solution by hydrogen peroxide. The excess hydrogen peroxide is then determined by titration with permanganate. The alkaline permanganate method depends upon the oxidation of cerous salts in alkaline solution by permanganate. Special care must be taken because of the oxidation of cerous hydroxide by air. One of the better methods involves the oxidation of cerium in dilute sulfuric acid by sodium bismuthate. off. The excess bismuthate is filtered A measured excess of standard ferrous ammonium sulfate is added to the filtered solution and the excess ferrous iron is then back titrated with standard permanganate. The cerium may be oxidized by adding solid ammonium persulfate and boiling the sulfate solution. A small amount of silver nitrate solution is added as catalyst. The tetravalent cerium is determined as in the bismuthate method, or it may 47 be titrated electrometrically with a ferrous sulfate solution which has been standardized against a eerie sulfate solution of known strength. A. later variation of this method utilizes the oxidation of cerium in a hot mixture of sulfuric and per­ chloric acids. The solution is then cooled, the cerium reduced by a standard ferrous ammonium sulfate solution, and the excess determined by a suitable standard oxi­ dizing agent. Europium may be reduced in a Jones reductor to 58,59,60 the divalent state and determined directly by 61 titration with permanganate or iodine solutions. In order to decrease the effect of air oxidation, the europous salt may be determined indirectly by collecting it in a standard ferric sulfate solution and titrating the equiva­ lent amount of ferrous sulfate formed with permanganate. Ytterbium and samarium may interfere since they may be reduced to the divalent ions. The black oxides of praseodymium are capable of liberating iodine from acidified potassium iodide solutions. It seems probable that the Bunsen iodometric method for cerium could be applied to praseodymium. has been proposed 6 This procedure but not completely investigated. The method would require a working curve of percentage compo­ sition of praseodymium oxide versus liberated iodine or 48 active oxygen. Since the function is not linear, the preparation of such a curve would require the mixing of pure rare earths in order to determine a series of points. Three kinds of spectral methods, X-ray, absoiption, and emission, are used in the determination of the rare earth elements; all require the use of special equipment. Absorption spectra analysis is almost indispensable in following the purification of these elements. The quantity of rare earth ions in a solution may be determined in two ways. A definite volume of the unknown solution is diluted until certain absorption bands begin to disappear. A standard solution of the pure element is diluted in a similar manner. The concentration of the element in the unknown solution is calculated by comparing the two 76 dilutions. A second way requires the application of 15,73 Lambert's and Beer's laws. A working curve con­ sisting of a plot of extinction versus concentration may be prepared for the pure element. ^ The extinction of the unknown solution is measured and the concentration of the colored ions determined from the graph. However, many of the absorption bands overlap, and the choice of the proper wave length is of extreme importance. Moeller and Brantley 67 made an extensive study of the application of the absorption spectra to the determination of the rare earths. The proper wave lengths for the determination of praseodymium, neodymium, 49 samarium, europium, gadolinium, erbium, thulium, and ytterbium are listed along with correction factors for interfering ions. Nevertheless, the accuracy of absorption methods is usually no better than one per cent. The analysis of the rare earths by emission spectra is extremely sensitive. This type of analysis is usually applied to the determination of trace impurities in high grade samples. Unfortunately the emission spectra of the rare earths are enormously line rich. fication of these lines is a complex problem. The classi­ Oatterer and Junkes with the assistance of V. Frodl have prepared enlarged plates of the arc and spark spectra of the various elements along with a complete list of their 31 emission lines. The most accurate of all the spectroscopic methods for the rare earths utilizes the well defined X-ray spectra. If a rare earth compound is bombarded with cathode rays, X rays are emitted. The spectra of these X rays differ for each element and are extremely 29 simple. Thus it has an immediate advantage over the analysis by emission spectra if proper equipment is available. Most of the rare earth elements are paramag­ netic. In some cases, such as with europium and gado­ linium, they differ widely in magnetic susceptibilities i 50 82 and magnetochemical analysis may be applied« It is especially useful in the purification of the first and last members of the rare earth series, namely lanthanum and lutetium, which are diamagnetic. The measurement of magnetic susceptibilities requires the use of a magnetic balance, which is not always available to the rare earth chemist. For quantitative determinations a disadvantage is that magnetic methods are usually limited to binary mixtures. A more recent analytical method for the rare earths uses radioactive tracers. This type of analysis has been used extensively in following separations by ion exchange methods. A known quantity of a radio­ active isotope of one of the elements to be separated is added to the mixture. Chemically there is no differ­ ence between the radioactive and ordinary atoms of the element. Since the ratio of these two types of atoms should remain constant throughout any chemical process, the degree of separation may be determined by measuring the radioactivity with a Geiger-Muller counter or other suitable means. However, radioactive tracers and the special equipment needed for their measurement are not always available. i 51 Part B The Determination of Praseodymium Two quantitative methods were used to follow the progress of separation of lanthanum and praseodymium: a) the absorption spectrum method, and b) the iodometric method. The latter was developed while attempting to improve the oxalate-oxide method for the determination of the average atomic weight of rare earth mixtures. After its development the iodometric method was used exclusively. A mixture of lanthanum and praseodymium is especially easy to analyze by means of absorption spectrum since lanthanum ions are colorless and offer no inter­ ference to absorption measurements of the green praseo­ dymium ions. Solutions approximately 0.01 M in were prepared by dissolving weighed samples of the unknown oxides in nitric acid and diluting to a known volume. The solutions were analyzed for praseodymium using 5 cm. cells in a Cenco-Sheard Spectrophotolometer, and measuring the extinction values in the 589 myu region and by applying Beer's E and Lambert's laws, C * with C representing molar concen­ tration of praseodymium oxide, E the observed extinction, k the extinction coefficient of a standard solution, and d the thickness of the solution. The percentage Pr.O.. in o 11 52 the original oxide was calculated as follows: *Pr6 Ou with = C x Pr6 Ou x representing the molecular weight of praseo­ dymium oxide and S.W. the sample weight. The iodometric method was developed for this study by utilising the fact that praseodymium exists in a higher oxidation state in oxides than it does in solution. 7,70 The formula of the pure oxide has been found to be Pr 6 °1 X which corresponds to an oxygen content 3 . 1 2 per cent in excess over that needed for sesquioxide formation. Under the proper conditions the "excess" oxygen in a weighed oxide sample liberates an equivalent amount of iodine from potassium iodide solutions. The iodine is titrated with standard thiosulfate, and the per cent "excess" oxygen calculated. However, in binary mixtures of praseodymium and lanthanum oxides the per cent "excess" oxygen varies 6,74 with the ratio of the two oxides. Accordingly, it was also necessary to determine the variation experi­ mentally and construct a graph from which the per cent praseodymium oxide can be read. The determination of praseodymium by the iodonetric method consists of dissolving about 0 . 5 gram of the oxide in a slight excess of nitric acid. The nitrate solution is diluted to about 150 m3., heated to 90° C., and the rare earth precipitated with the minimum quantity i of hot dilute oxalic acid. After the solution has cooled the precipitate is filtered in a Buchner funnel, washed with 95 per cent ethyl alcohol, and air dried with suction. The oxalate is transferred to a crucible and ignited for 2-3 hours at 925° C. in a muffle furnace. The crucible is removed from the hot furnace and allowed to cool for about one minute; the oxide is transferred immediately to a weighing bottle and covered tightly. It is then allowed to cool to room temperature and is ready for weighing. Three samples of 0.10-0.12 g. of the above oxide are weighed into 250 ml. iodine flasks. To the sample in each flask are added first 10 ml. of 0.1 M potassium iodide solution and then 25 ml. of 6 N sulfuric acid. The flask is immediately stoppered and gently swirled to dissolve the oxide. The solution time varies from 5 to 30 minutes depending upon the nature of the oxide. The liberated iodine is titrated with 0.01 N sodium thiosulfate using 3-4- ml. of 1 per cent starch solution as the indicator, A blank correction on water is made and the volume of thiosulfate required for the blank is subtracted from that of the sample. Blank corrections amount to approxi­ mately 0 . 0 2 ml. of thiosulfate for each 5 minutes of solution time. 54 The calculation for the per cent "excess” oxygen is % "Excess" Oxygen = NV x £o6'd x l?wV* N repre­ sents the normality of the sodium thiosulfate solution, 0 V the volume of the sodium thiosulfate solution, 2000 the milliequivalent weight of oxygen, and S.W. the sample weight. The graph used to determine the per cent praseo­ dymium oxide in binary mixtures with lanthanum oxide with relation to "excess" oxygen was obtained by preparing synthetic mixtures covering the entire percentage range. Weighed samples of the two pure oxides were dissolved in dilute nitric acid, the rare earth ions coprecipitated as oxalates, and the mixed oxalates ignited at 925° C. for 2-3 hours in a muffle furnace. The "excess" oxygen was determined in these oxide mixtures by the iodometric method. The variation of per cent: "excess" oxygen against per cent praseodymium oxide is graphed in Figure 1 and the data for it are listed in Table XI. Since the curve for the praseodymium-lanthanum mixtures indicated such a variable behavior for the "excess" oxygen-oxide relationship, data were also obtained in the same manner for neodymium-praseodymium and samariumpraseodytnium mixtures. These relationships are discussed in the section on the properties of praseodymium oxides. \ EXCESS" OXYGE % PRASEODYMIUM" "OXTD E VJI 56 TABLE XI Comparison of "Excess" Oxygen and Praseodymium Oxide Percentages in Lanthanum-Praseodymium Oxides Per Cent Praseodymium Oxide Per Cent "Excess" Oxygen 100.0 90.0 79.9 64.0 60.0 50.0 40.0 29.8 20.0 0.0 3.08 2.98 2.83 2.39 2.17 1.28 0.50 0.06 0.02 0.00 Factors which may affect the accuracy of the iodometric method are the conditions of ignition of the oxalate, the effect of air oxidation on the potassium iodide solutions, and the effect of other rare earths on the formation of praseodymium oxide. However, check values of two parts per thousand with an accuracy of - 1 per cent may be obtained if the conditions given in the procedure are closely followed. Since any carbonate character in the oxide would lead to low results, all oxalates must be Ignited at a temperature exceeding 910° C., the temperature requiredi 78 for the complete decomposition of lanthanum carbonates. (In this study a temperature of 925° C. was used.) The oxides must be cooled quickly because they have a tendency to absorb oxygen if cooled slowly. true at the surface of the oxide. This effect is especially Slowly cooled samples 57 yield high results. The effect of temperature conditions on praseodymium oxide and binary mixtures of it and other rare earths is discussed later. The effect of air oxidation on acidified potassium iodide solutions must be considered in any iodometric method. Air oxidation is usually increased by heat, light, high acidity, and high concentration of iodide ion. In order to decrease the action of air to a minimum, the oxides are dissolved in a cold moderately dilute sulfuric acid solution protected from direct sunlight as is usual in other iodometric procedures. In most iodometric methods a large excess of potassium iodide is used in order to take advantage of the law of mass action and to produce a solvent for the iodine, which is more soluble in potassium iodide solutions than in water. However, the higher concentration of iodide ions favors more oxidation by the air. For samples which may require a rather long solution time the concentration of potassium iodide should be reduced to a minimum, and the titration carried out in an iodine flask to prevent the escape of iodine. In the procedure for the iodometric determi­ nation of praseodymium it was suggested that the oxides be dissolved in the acidified potassium iodide solution by gently swirling the iodine flask. The flask should 1 58 not be shaken since this increases the surface exposed to air. Samples that were shaken were found to have a larger and more inconsistent blank correction. By applying the suggestions given above the blank correction is seldom larger than 0 .1-0.2 ml. of 0.01 N sodium thio­ sulfate solution. To check the validity of the procedure, two samples were analysed for praseodymium by the absorption spectrum method and the iodometric procedure. These results are given in Table XII. TABLE XII The Comparison of Absorption Spectrum and Iodometric Methods % Praseodymium Oxide__ Sample Absorption Iodometric 1 65 65 2 84 87 Since neither method may be considered more accurate than - 1 per cent, the above determinations are reasonably good checks. Therefore, the iodometric method for the determi­ nation of praseodymium in binary oxide mixtures with lantha­ num is both rapid and accurate. 1 59 Fart C Average Atomic Weight Determinations: An Iodometric Correction for "Excess" Oxygen The oxalate-oxide average atomic weight determi8,24,32 nation can be improved by applying an iodometric correction for "excess" oxygen to the weight of the oxide sample; the interference of praseodymium and other rare earth elements which form oxides higher than sesquloxides is eliminated. The suggested improved procedure follows. The starting materia] for the analysis is freshly ignited rare earth oxide. The ignition tempera­ ture must exceed 910° C., the temperature of complete 78 decomposition of lanthanum carbonate. A sample of the oxide is analyzed for "excess" oxygen by the iodometric procedure. A second sample, about 0.2 g., is dissolved in 10 ml. of water containing 1 - 2 ml. of concentrated nitric acid. The solution is evaporated almost to dryness on a steam bath to remove the excess acid. The resulting rare earth nitrate is dissolved in 100 ml. of water. This solution is heated to boiling and the rare earth precipi­ tated as an oxalate by the slow addition of a hot solution of one gram of oxalic acid dissolved in 50 ml. of water. The rare earth oxalate is digested on a steam bath for 1 5 - 2 0 minutes, allowed to cool to room temperature, and 60 filtered on an asbestos mat in a Gooch crucible or in a sintered porcelain crucible. The oxalate is washed several times with 50 ml. portions of cold water to remove any oxalic acid. The filtering and washing process is carried out by decanting the supernatant liquid into the crucible, thereby leaving most of the oxalate in the beaker. The crucible is placed in the beaker and the combined oxalates are dissolved in 40 ml. of 10 N sulfuric acid. This solution is diluted with 100 ml. of water and titrated with a 0.1 N potassium permanganate solution. About 75 per cent of the permanganate is added to the cold oxalate solution, but the titration is completed at 50-60° C. The molecular weight of the rare earth sesquioxide is calculated as follows: 6000 ) N = normality of the potassium permanganate solution, V = volume of the potassium permanganate solution, R2 O3 = molecular weight of rare earth sesquioxide, ^2 ^ = milliequivalent weight of the rare earth sesquioxide, ' "0 " = per cent "excess" oxygen determined iodometrically, 61 S.W. = sample weight cf original rare earth oxide, <■>11 n i l S.Y/. x ^ 100 = total weight of "excess" oxygen. The average atomic weight of the rare earths may then be calculated from the molecular weight of the sesqui­ oxide . „ R2 O3 - 48 R g--The atomic weights of lanthanum, praseodymium, and neodymium determined using the above procedure are 8.18,32 listed in Table XIII with the results of other workers^ who also used an oxalate-oxide method for their determi­ nations . A. comparison of the determined atomic weights with the international atomic weights indicates the accuracy of the method. This is especially true in the case of praseodymium, since the older method gives results that are often high by as much as 5 - 6 atomic weight units. In a statistical treatment of average atomic weight data obtained by the oxalate-oxide method described in Inorganic Syntheses, Audrieth and co-workers 18 found the mean of three atomic weight determinations will not deviate from the true mean by more than 1 1.28 atomic wejght units in 95 per cent of the cases. All the results reported in Table XIII are well within this limit. 62 TABLE XIII of Several Rare Earths Atomic Wei by Oxalate-Oxide Methods Lanthanum Determined Atomic Weight Audrieth (La-29) 18 32 g Pearce Gibbs 138.5 139.1 138.4 139*0 139.1 139.4 140.0 139.7 Av. 138.8 1 3 8 .8 139.7 139.7 International Atomic Weight 138.92 Praseodymium 18 Audrieth + International Determined Atomic Weight (Pr-1) (Pr-8 ) Inorganic Syntheses Atomic Weight 140.7 140.7 146.1 146.1 145.7 146.6 144.7 144.9 145.3 Av. 140.7 146,0 145.4 145.3 140.92 Neodymium Determined Atomic Weight Pearce 343.5 144.7 144.5 145.8 Av. 144.1 145.7 8 International Atomic Weight 144.27 * - One sample was analyzed by the method described in Inorganic Syntheses. i 63 18 In agreement with Audrieth and co-workers it was found that no error was introduced by standardizing the potassium permanganate against pure sodium oxalate instead of pure rare earth oxalates. Barthauer and g Pearce, however, claim a higher normality is obtained with the rare earth oxalates probably due to contami­ nation of the oxalates with nitrato-oxalates. This possible source of error was not neglected, but reduced to a minimum by evaporating the excess nitric acid on a steam bath and then precipitating the oxalates from very dilute hot solutions; the mixture is cooled to room temperature before filtering. Since the starting material is a rare earth oxide, it is extremely important that the sample be freshly ignited. The presence of carbon dioxide leads to inconsistent high results. The average atomic weights of a few mixtures were determined by the procedure described above and results are listed in Table XIV. The values obtained, if no iodometric correction for "excess" oxygen is calculated, are given for comparison with the theo­ retical average atomic weight of the mixture. The iodometric correction for "excess" oxygen is negligible for binary or ternary mixtures of praseo­ dymium with lanthanum and neodymium oxides if the 64 TABLE XIV Average Atomic Weights of Rare Earth Mixtures $0% La2 C>3 -50 ^ pr2°3 Mixture Uncorrected for "Excess'* Oxygen Corrected for "Exces^1 Oxygen Theoretical Average Atomic Weight 141.6 139.9 142.1 140.5 142.2____________ 140.6__________________________ Av. 142.0 140.3 139.9 41.4# La2 O3 -2 5 .Q# Pr2 0 3 -3 3 .6 /o M 2 O3 Mixture Uncorrected for "Excess" Oxygen Corrected for "Excess" Oxygen Theoretical Average Atomic Weight 140.8 140.8 140.7 140.7 140.9___________ 140.9____________________________ Av. 140.8 140.8 141.2 praseodymium content does not exceed 30 per cent as illustrated by the data for the second mixture in Table XIV. However, the presence of small quantities of cerium or samarium increases the "excess" oxygen content so that the iodometric correction is significant. (See Section VII.) The advantages of this procedure over the one 24 outlined in Inorganic Syntheses are greater accuracy when elements which form higher oxides than sesquioxides are present and greater rapidity since no gravimetric determinations are necessary. 65 SECTION VII The Praseodymium Oxides The behavior of praseodymium in rare earth oxide mixtures has been a difficulty in average atomic weight determinations, magnetic susceptibility investi­ gations, separations based upon the dry oxidation of 25 54 69 praseodymium, ’ ’ crystallographic studies, etc. The anomalous behavior of praseodymium is due to the existence of the element in more than one oxidation state in the rare earth oxide mixtures; this behavior cannot be completely explained without additional structural studies and perhaps magnetic susceptibility investigations. A. clarification of the chemistry of praseodymium has been attempted by a) reviewing the properties of the praseodymium oxides, b) determining the oxidation state of praseodymium in binary oxide systems with lanthanum, neo­ dymium, and samarium oxides, c) suggesting an explanation for the behavior of praseodymium in oxide mixtures with the other rare earth elements. Several formulas are pre­ sented for which there is very meager evidence, e.g. the formation of pyropraseodymates. They are given to stimulate future research in this field of study. 66 Part A Properties of the Praseodymium Oxides Three oxides of praseodymium are known: a sesquioxide, P^O^; a dioxide, Pr0 2 > and an intermedi­ ate oxide, common. The intermediate oxide is the most Special techniques are required for the prepa­ ration of the other two. Physical properties of the three oxides are listed for comparison in Table XV. In addition, two other oxides, a pentoxide, P^O*,74- and 54 a monoxide, PrO, have been reported; but their existence has not been confirmed. Praseodymium sesquioxide, P^O^, is prepared by 70 the reduction of Pr^O]^ °r P i ^ in hydrogen. Gold^4 schmidt and co-workers found that the sesquioxide had crystal structures belong to three types, A, B, and C. A is the high temperature form and C the low temperature form. Greenish-yellow flakes of Type A may be prepared by fusing the black oxide* in the flame of an acetylene blowpipe. The crystals belong to the trigonal trapezo- hedral class of the hexagonal system. The reduction of praseodymium sulfate by hydrogen at 900° C. gives, in addition to the A-modification, clear yellow crystals of a pseudotrigonal variety, Type B. If the reduction * - This designation, black oxide, refers to Pr/0-,throughthis thesis. 6 11 TABLE XV Physical Properties of the Praseodymium Oxides Pr +3 +4 — 0 =Pr + e; E - 49 1.6 Pr2°3 PrO, Pr6 ° H Color Greenishyellow Yellowishwhite Black Black Symmetry Hexagonal Cubic Cubic Cubic Structure Type La20^ CaF2 CaF2 CaF„ Lattice Constants a=3.85lA 102 74 17 Solubility in Water at 20 C.(Moles/L.)* 71 74 Heat of Solution in * 8 N HNO3 (Calories) 62 a=5«468A 6.61 7.07 0 . 6 1 x 10 62 34 5.488A c =5.996a Density (20° C.) a=5.570A -6 a=5.394A 62 5.41A34 6.82 3.9 x 10-6 54,750(V2Pr2 03 ) 45,100(l/6Pr601]L) 42,800(Pr02 ) Magnetic Susceptibility ( X ’106 ) C29) 82 -56 15.6 y (9)** $ Available Oxygen 0 3.13 4.63 Ratio "0 ,I:Pr2 03 0 0.667 1.000 - Although the solubilities of Pr2 03 and Pr^O^ reported by Bush ^ are correct in the order of magnitude, the actual values are questionable since the higher oxides of the rare earth elements are more insoluble than the sesquioxides. ** - Estimated value. * 68 temperature is 500°-600° C., Type C, a yellowish-white 26 cubic variety, is obtained. Foex studied the allotropy of praseodymium sesquioxide and found that the B- and Cmodifications are transformed irreversibly to the A-type at temperatures exceeding 600° C. The C-type cannot be prepared from the A-type, but only by the low temperature reduction of the black oxide. Praseodymium sesquioxide is converted quantitatively to Pf ^O-q when heated to a dull red color in a current of oxygen or air. 3Pr2 03 * 02 Acids hei>- '> - Pr6 011 dissolve the oxide forming green praseodymium salts. Praseodymium dioxide, Pr02 , is prepared by low temperature ignition of the sesquioxide. Prandtl and 74 Huttner prepared it by heating the sesquioxide at 300° C. for several days. This procedure was very slow and the dioxide was always contaminated with lower oxides. They also prepared the dioxide by fusing P^O^i with several times its weight of.potassium chlorate at a temperature of 270°-280° C. After cooling, the product was leached 70 with water and dried at 120° C. Pagel and Brinton prepared praseodymium dioxide of 9 9 . 2 per cent purity by heating the lower oxides in pure oxygen at high pressures and studied the stability of the oxide at different tempera­ tures and pressures. When heated above 400° C. the dioxide 69 decomposes into Pr^O-^ and oxygen. The dioxide crystal­ lizes in the fluorite structure analogous to cerium dioxide Praseodymium dioxide is a strong oxidizing agent liberating iodine from hydriodic acid, chlorine from hydro chloric acid, and converting manganous salts to permanga11 nates and cerous salts to eerie salts. It oxidizes ferrous, stannous, and arsenious salts5 but part of the available oxygen is always lost, probably due to the oxi­ dation of water. Praseodymium dioxide is soluble in oxyacids, forming trivalent salts and liberating oxygen and, in some cases, traces of ozone. Since hydrogen peroxide is not formed when the dioxide is treated with cold sulfuric acid, it does not appear to be a peroxide but rather an oxide actually containing tetravalent praseo dymium. It does not show acidic or basic properties; thus, the dioxide does not form tetravalent praseodymium or praseodymate ions in solution. Attempts to oxidize a suspension of praseodymium hydroxide in strongly alkaline solutions with chlorine, bromine, and ozone have been 74 unsuccessful. The black oxide, P^O-q j some" times designated as praseodymium praseodymate, is prepared by the ignition of praseodymium sesquioxide, dioxide, hydroxide, or salts of volatile acids in air. This oxide is stable between 500°c o 900 3., but when heated at 1100 C. in a current of 70 nitrogen it undergoes appreciable decomposition with the loss of active oxygen. When ignited to red heat in a covered crucible, it is reduced to the greenish-yellow sesquioxide. However, as the crucible cools, the oxide reabsorbs oxygen; if the cooling is very rapid, only a surface layer of Pr^On is formed. The sesquioxide is not oxidized by air at room temperature, but may be recon­ verted to the black oxide if heated in an open crucible. The chemical properties of the intermediate oxide are similar to those of praseodymium dioxide, for the inter­ mediate oxide liberates chlorine from hydrochloric acid, iodine from hydriodic acid, and oxidizes manganous, cerous, stannous, ferrous, and arsenious ions. Like praseodymium dioxide, Pr^O-^ has no per­ oxide characteristics but may be considered an oxide salt. Cold hydrofluoric acid, concentrated or dilute, attacks the oxide; the hot acid slowly gives the diffi­ cultly soluble salt, A. complex potassium praseo­ dymium fluoride, easily soluble in dilute acids, may be prepared by adding Pr^O-j^ to fused potassium hydrogen fluoride. 72 Sulfuric and nitric acids react with the oxide more or less violently, depending upon the tempera­ ture and concentration, liberating oxygen containing traces of ozone and forming trivalent praseodymium salts. 71 When placed on the anticathode of an X-ray tube and bombarded with electrons, praseodymium praseo71 dyrnate is rapidly converted into the sesquioxide. X-ray studies of the oxide show that the microcrystalline 36 black powder has the "fluorite" structure. The formula of this oxide has been definitely 7,70,74 85 established, although earlier workers found other praseodymium oxygen ratios. bly due to impure praseodymium. Their error was proba­ If the oxide is treated with a slight excess of acetic acid and the dissolving action continued until only a fifth of the oxide remains, the product, after washing and drying at 120°-130° C., is a deep reddish-brown powder which has a formula of 74 Pr4 °8 *H2 °* ^be a^ove experiment indicates that the intermediate oxide, Pr^O.^, is actuaH y a compound of praseodymium sesquioxide and dioxide, PrgO^^PrOg. Praseodymateshave never been prepared in solution because tetravalent praseodymium oxidizes water. 8 H+ + 2Pr02 + 2 e ---------- 2pr+++ + 4H2 0; HOH + 6H - 2 e ------- ^ + 2H+ 5 t02 E° - (?) E° = -2.42 +++ + 2pr02 >• 2pr + £0 2 + 3H20 However, they have been prepared in the dry state. Zintl 103 and Morawietz prepared sodium praseodymate, Na^rO^, by heating praseodymium sesquioxide and sodium oxide at 72 470° C. in oxygen. It has a density of 4.60 and a rock- salt (face-centered) cubic structure with a 4.84A, analo­ gous to sodium cerate, ^2060^, with a 4.82A. The sodium and tetravalent praseodymium ions are distributed over equivalent positions, each unit cell containing 1-1/3 sodium atoms and 2-2/3 praseodymium atoms0 The 4 chlorine atoms in the unit cell of rock salt have been replaced by 4 oxygen atoms. Barium cerate, BaCeO^, 39 27 a=4.377A, a=4.386A, has been prepared, but the corres­ ponding praseodymate has not. Barium praseodymate, if it can be made, should have an analogous structure to BaCeO^. 34 Goldschmidt was the first to show a relation­ ship between the crystalline form of the rare earth sesqui40 oxides and ignition temperatures. landelli verified this previous work; his results are tabulated in Table XVI. Type A is a hexagonal form; Type B is a pseudotrigonal form, and Type C is cubic. It is noted that with the increasing atomic number of the rare earths, the Ctype is more stable over an extended temperature range; ancl that for the first members of the group the C-form is the lovi temperature type which changes to the A-form at moderately high temperatures. 54 Marsh states that the sesquioxides and dioxides form solid solutions, if the sesquioxides have the C-type structure. The dioxides possess a fluorite structure; i 73 TABLE XVI Dependence of the Type Sesquioxide Upon the Ignition Temperature Pr2°3 Nd203 Sm20^ Eu20^ Gd20^ C c C c c C c c + 0 C + A > A J _______ 350 450 500 600 700 ^a2®3 11 0 1 + 11 9 Temperature (° C.) C C A 775 0 ir\ 00 A | C C C A 900 1000 1100 A A A A C C 1 1200 B ; 1300 b ! 1400 B 1500 B : 1 1 1 1 1 1 2000 A 1 1 c 74 the C-type or cubic sesquioxide has a subtraction lattice of the fluorite type with slight modifications. (The trivalent metals replace the calcium ions, but only threefourths of the fluorine positions are filled with oxygen ions.) Because of this similarity in structure, the two types of cubic oxides are able to form solid solutions with each other. The A-type sesquioxides have hexagonal structures and do not tend to form solid solutions with praseodymium dioxide. formation. Their presence inhibits dioxide Therefore, any conditions which promote C- type sesquioxide formation should also promote praseo­ dymium dioxide formation. The effect of temperature upon the oxidation state of praseodymium may be explained by Table XVI. Starting with praseodymium sesquioxide low temperature ignition favors the formation of the C-modification. Since this cubic type can form solid solutions with cubic Pr02 , the tendency to take up oxygen is increased and the formation of praseodymium dioxide from the sesqui­ oxide is favored. However, the oxidation is seldom com70 plete. If the ignition temperature is raised, the small amount of sesquioxide remaining tends to change into the A-modification which inhibits oxygenation, and oxygen is liberated until Pr^Ojj results. In the absence of oxygen and at very high temperatures the A-type praseodymium 75 sesquioxide is formed. However, if this oxide is cooled slowly in the presence of oxygen, Pr^O-j^ again results. Reactions involved can be represented as: p^o^Cc) + £o2 < 400 > 400 6Pr02 -- ^ -- > >noo° Pr6°ll Pr^011(Pr20^*4Pr02 ) + £02 3Pr203(A) ♦ o2 . It can be assumed from the limited data reported that the first reaction is very slow, the second is rapid to the right, and the third is rapid to the left. Since praseo­ dymium sesquioxide (C-type) cannot be prepared by the low 26 temperature ignition of the dioxide, the first reaction apparently is not an equilibrium reaction. If the C-type sesquioxide is ignited above 400° C., it forms Pr^O-^ immediately. 36 Recently Gruen, Koehler, and Katz have obtained evidence for a continuous transition from Pr2 ° 3 Pr02 * Several intermediates were prepared and their lattice TABLE XVII Oxygen Content and Lattice Parameters of Praseodymium Oxide Formula Oxygen/Metal Ratio___ Pr203 1.50 Pr01.65 Pr6 °ll Pr01<99 Pr02 ’ 1,65 ^ 1 .99 2.00 Pr02 .02 2 *02 Constant Reference 62 5.570 5.530 5.468 36 62 5.399 5.394 5.380 36 62 36 % 76 constants measured. A contraction in the lattice was observed as the oxidation state increased. Thus, the extent of oxidation was indicated by changes in the lattice parameters. i 77 Part B Effect of Other Rare Earth Oxides on Praseodymium Oxides The tendency of praseodymium to form three oxides has been very troublesome in studies of rare earth oxide mixtures. This effect of the composition of rare earth 51 mixtures is reviewed in the next few paragraphs. Marc claimed that the presence of a little cerium was necessary for the higher oxidation of praseodymium and that lantha­ num and neodymium hindered its oxidation. These effects 65 14 were confirmed by Meyer and Koss. In addition, Brauner stated incorrectly that a small quantity of praseodymium in neodymium sesquioxide caused the production of a higher oxide of neodymium, probably a dioxide. 6 However, more recent studies by Barthauer, 54 74 75 Marsh, Prandtl and Huttner, and Prandtl and Rieder indicate that in praseodymium-cerium oxide mixtures of very low cerium content, the cerium dioxide seems to inhibit oxidation of the praseodymium. In binary oxide mixtures of lanthanum-, neodymium-, or samarium-praseodymium, con­ taining praseodymium in excess of the ratio the oxidation state of this latter element is increased. Likewise, if larger amounts of lanthanuq neodymium, or samarium oxides are present, the degree of oxygenation of the praseodymium is decreased. The reduction in the 78 amount of oxygenation is greatest with the addition of lanthanum oxide, intermediate with neodymium oxide, and least with samarium oxide. 54 Marsh has correlated the types of sesqui­ oxides with the ionic radius ratios of the rare earths, Table XVIII. He states that the C-type sesquioxide is stable for the ionic radius ratios of 0 . 5 3 to 0 . 8 6 (R =ionic radius of rare earth, R =ionic radius of oxygen), m ° and that larger values than 0.86 favor the A-modification. TABLE XVIII Dependence of the Type Sesquioxide Upon the Ionic Radius Ratio R+++ Ionic Radii (A)* Ionic Ratios Radius (Rn/Rp) Type Sesquioxide** La 1.22 0.92 A Ce 1.18 0.89 A Pr 1.16 0.88 A Nd 1.15 0.87 A. Sm 1.13 0.86 C Eu 1.13 0.86 C Gd 1.11 0.84 C * -Goldschmidt ** - Marsh Observations by Prandtl and Rieder 75 and by 54 Marsh indicate complete oxygenation of praseodymium oxide 79 to form praseodymium dioxide in binary mixtures with samarium oxide (Rm/R0 -0.8 6 ), gadolinium oxide (Rm/Ro=0.84), and yttrium oxide (Rm/Ro =0.80), but not with the earlier (lower atomic number) rare earth oxides such as lanthanum oxide (Rm/Ro=0.S2). However, complete oxygenation is also obtained with neodymium oxide (Rm/Ro=0.87), if the mixture is heated moderately in an atmosphere of oxygen. The above examples illustrate the dependence of the oxidation state of praseodymium upon ionic radius ratios. It will be recalled that an iodometric analysis for praseodymium in binary oxide mixtures (Section VI) con­ taining the element was developed. Since most analyses for praseodymium are on mixtures, it was necessary to learn how the degree of oxygenation varied with the composition of the mixture. In Tables XIX, XX, and XXI the results of these analyses for 0 - 1 0 0 per cent ranges for binary mixtures of praseodymium oxide with the oxides of samarium, neo­ dymium, and lanthanum are tabulated. In Figure 2, weight per cent of R2 0^ (R=Sm, Nd, or La) is plotted against weight per cent "excess" oxygen. The straight line is the theo­ retical curve expected if praseodymium oxide remains as Pr6 °ll without change for the various ratios. In Figure 3, mole per cent R2 O3 is plotted against mole ratio of "excess" oxygen. The straight line corresponds to the composition of pure Pr^O-j^. Figure 2 is more valuable 80 in analytical work; Figure 3 in theoretical discussions since it shows the apparent oxidation state of praseo­ dymium. TABLE XIX Samarium-Praseodymium Oxide System wt. % Sn^ 0^ Wt. % "Excess" Oxygen Mole % Sn^O^ “Excess*1 Oxygen Moles Pr20^__ 0.658 0.0 3.08 2.92 20.3 0.787 0.825 29.8 2.69 0.844 2.34 39.7 49.8 0.839 1.95 6 0 .2 59.8 0.835 1.55 69.6 0.779 70.1 1.09 0.714 80.0 79.5 0.67 89.6 0.23 90.0* 0.485 93.8 0.16 94.0* 0.565 o.ooo 100.0 0.00 100.0 * - Errors in the determinations rather large due to the small quantity of standard thiosulfate solution required. 0.0 20.6 30.2 40.1 50.2 TABLE XX Neodymium-Praseodymlum Oxide System Wt. % Nd203 Wt. $ "Excess" Oxygen Mole % Nd203 "Excess" 0: Moles Pr. 0.0 0.658 0.0 3.08 20.2 2.94 19.9 0.785 2.71 30.4 30.0 0.831 2 .3 2 40.1 0.830 40.5 50.4 50.0 0.810 1.89 60.0 0.719 60.3 1.35 60.4 0.694 1.29 60.7 62.1 0.304 62.0 0.55 63.8* 0.18 0.103 63.5 7 0 .1 * 0.04 0.028 69.7 79.6 80.0* 0.031 0.03 100.0 100.0 0.000 0.00 * - Errors in the determinations rather large due to the small quantity of standard thiosulfate solution required. TABLE XXI Lanthanum-Praseodymium Oxide System Wt. % La2°3 Mole % La20^ Wt. fo "Excess" Oxygen "Excess" Oxygen Moles P^O^ 0.658 0.0 3.08 0.0 10.4 2.98 10.0 0.707 0.758 20.9 20.1 2.83 2.61** 0.799 30.0** 31.5 0.800 37.2 2.39 36.0 41.2 2.17 0.774 40.0 0.542 5i.o 1.28 5o.o 60.6 0.261 0.50 60.0 65.6 0.13 0.077 65.1* 0.042 70.6 70.2* 0.06 80.2 0.021 0.02 80.0* 0.000 100.0 0.00 100.0 * - Errors in the determination rather large due to the small quantity of standard thiosulfate solution required. ** - Values taken from a plot of weight per cent La2 0_, and weight per cent "excess" oxygen. ^ The curves indicate considerable differences in the behavior of praseodymium oxide in the presence of the oxides of samarium, neodymium, or lanthanum. The changing oxidation state of praseodymium with mole per cent samarium will be considered first. It is observed that the amounts of "excess" oxygen are greatest for the lowest percentages of Sn^O^ and exceed the theoretical amount for about 85 per cent of the composition range. The maximum "excess" oxygen (0.84 atom per mole P^O^) is noted in the region 40-50 per cent S1112O3 ; the composition of this oxide may be represented by the formula 4Sm20^»Pr203«10Pr02. For the upper 15 per cent the amounts of "excess" oxygen are slightly less than that expected. tp ; so : 4.0 ; so .«!o .: t!o a so 82 "e x c e s s " o x y g e n /M O L E S Pr20 3 r 2 CO CO CO -<■<-< C/> CO c/> H m rn rn Z 3C CO *0*d > O ro i* iv> O wO wO oT Z cx> u> 84 From the work of Goldschmidt 34 and Iandelli, 40 it is learned that Sn^O^ tends to form the C- or cubicsesquioxide structure in the temperature range used for this study. The ionic radius ratio of samarium oxide also favors the formation of the C-type sesquioxide. It has been stated that both Pr02 and Pr^O^ exist in cubic forms. It appears reasonable, therefore, that the cubic Sm2 0 ^ and one of the cubic praseodymium oxides might form solid solutions. If such were the case, it could also be expected that oxygenation of praseodymium towards the highest oxide, Pr02 , might occur. Such a behavior is indicated by the curves for the saraarium-praseodymium system. Complete oxygenation to Pr02 was not observed. However, the results in this study are in agreement with those of Prandtl and Rieder 75 who reported 0.80 to 0.85 atom of "excess" oxygen per mole of P^O^ for a mixture of 3 Pr2 0 ^/2 Sm2 C^ (approximately 40 mole per cent SnigO^). In considering the oxide system for lanthanumpraseodymium, the ionic radius ratio of lanthanum oxide (0.92) and the ignition temperature (925° C.) favor the formation of the A- or hexagonal-type sesquioxide. As 54 Marsh points out, the hexagonal La2 0^ and the cubic Pr6 °ll would n°t tend to form solid solutions. This would suggest that the oxygenation of praseodymium is inhibited. In this study it was found that samples con­ taining more than 70 mole per cent lanthanum oxide gave 85 very small ratios of "excess" oxygen to moles of Pr2 0 ^. This observation would indicate that the degree of oxy­ genation is inhibited so that practically all the praseo­ dymium is present as the sesquioxide. Samples containing 0 - 3 5 mole per cent lanthanum oxide show a steady increase in the amount of "excess" oxygen. Marsh made a similar observation and suggested that the increase was due to the formation of a lanthanum praseodymate, 4Pr02 *La2 0^; praseodymium sesquioxide is substituted by lanthanum sesquioxide in the fluorite-type structure of 4Pr02 #Fr2 0^ (i.e., P r ^ * Complete oxygenation is not obtained. peak value of the "excess" oxygen/moles The is 0 .8 0 ; the composition of the oxide mixture which produces this peak oxygenation value may be represented by the formula 74,75 3 La2 0 ^*Pr2 0 2 •8Pr0p. Prandtl and co-workers reported a ratio of 0 . 8 6 for a sample containing • The tendency of the lanthanum oxide to form an A-type sesquioxide and suppress oxygenation may be observed even in the 0 - 3 5 mole per cent lanthanum oxide region; the rise in oxygenation is more gradual than with samarium oxide, which forms only a C-type sesquioxide under the conditions given. The region from 35-70 mole per cent lanthanum oxide represents a transition from the C-type to the A-type sesquioxide with a corresponding gradual 86 decrease in oxygenation. The I^Ch-Pr^O-Q curve is in 54 agreement with a statement by Marsh, "In the presence of lanthanum oxide (up to S P ^ O y ^ l ^ O ^ ) there is an increase in the degree of oxygenation of the praseodymium, but larger amounts cause a rapid fall." The curve obtained for the neodymium-praseodymium oxide system differs from those of the samarium- and lanthanum-praseodymium systems. It follows rather closely the Sn^O^-Pr^O^ curve for samples containing low per­ centages of neodymium oxide, but breaks away and follows the LagO^-Pr^O-Q curve for high percentage samples. The two factors, the ionic radius ratio of neodymium sesqui­ oxide (0.87) and the ignition temperature (925° C.) only slightly favor the formation of the A-type sesquioxide; actually both of these conditions correspond to the tran­ sition region between C- and A-modifications. If the conditions favor formation of the hexagonal ^ 2 0 ^, there should be little tendency for solid solution with the cubic Pr02 , but increased solid solution with Pr-^O^; a combi­ nation of hexagonal P^O^ and M 2 O3 would not favor oxy­ genation. Also, cubic Nd2 0 ^ and cubic P^O^ could form solid solutions with an increased tendency for oxygenation. For samples containing 0-40 mole per cent neodymium oxide, the degree of oxygenation of praseodymium sesquioxide is about the same as with samarium oxide (a typical C-type sesquioxide). From 40-60 mole per cent it appears that 87 the A-type neodymium sesquioxide is beginning to affect the degree of oxygenation, from 6 0 - 6 5 mole per cent a very large decrease occurs. It may be that this system does not tolerate over 60 mole per cent neodymium oxide with the maintenance of the cubic-type lattice. Solid solutions of Pr02 and Nd2 0 ^ probably are formed up to but not beyond this percentage composition. This concept is in agreement with the X-ray data recently obtained by 62,63 McCullough for rare earth sesquioxide-dioxide systems. He found that for samples containing over 65 mole per cent neodymium oxide the A-type sesquioxide is formed and the fluorite-type structure is not tolerated. This behavior corresponds with the data in this study on the oxygenation of praseodymium sesquioxide. For these conditions the amount of oxygenation is inhibited, producing results that follow closely the curve of lanthanum oxide (a typical Atype sesquioxide). The peak oxygenation value found is 0.83 atom of "excess" oxygen per mole P^Oo which agrees 75 with the value obtained by Prandtl and Rieder. For this study and that of Prandtl and Rieder the peak occurs at about 40 mole per cent neodymium oxide (3Pr2 0 ^/2 ^ 2 0 3 ). The composition of the oxide which produces the peak oxy­ genation value may be represented by the formula 4Nd2 O3 •Pr2 O3 •lOPr02 . 88 It is obvious that the composition of praseo­ dymium oxide in binary mixtures with other rare earth oxides varies continuously over the entire percentage range. The ratios of the oxides at peak oxygenation in each system are: 3La202 •Pr202*8Pr02 or 3(La2C>3*2Pr02 ) + Pr20y2pr02 4Nd20^ •Pr20^ •10Pr02 or 4(Nd20y2Pr02 ) + Pr20y2Pr02 4Sm202*Pr20^*10Pr02 or 4(Sm20^*2Pr02 ) + Pr20^»2pr02 It will be of interest to conjecture about these ratios or formulas. For example, it might be asked if there is any significance to the repetition of the R2C>3 »2 Pr0 2 ratio. It might be stated that except in the case of praseodymium oxide, Pr^O-j^, this ratio of one mole of sesquioxide to two of praseodymium dioxide is common to each formula. Whether R20^»2Pr02 represents compound formation or simply a particularly stable solid solution ratio can only be answered by more detailed crystallographic or other structural studies. One suggestion is to assume that if compounds are formed, the above compositions could be represented gener­ ally as R2Pr2 0r;, derived from a parent pyropraseodymic acid (H^Pr20y) which corresponds to the loss of one mole­ cule of water from two molecules of orthopraseodymic acid. Neither this acid nor any of its salts have been reported in the literature. Continuing the assumption, it is 89 possible to explain the complex oxide ratios at peak oxy­ genation as salts of pyropraseodymic acid. formula will fit these oxide ratios. No other simple At peak oxygenation these ratios would be: 3 La2 0 ^ *Pr2 03 *8 Pr02 or 3 La2 Pr2 0 r7 + Pr2 Pr2 0 r7 4 Nd2 C>3 'P^O^ .10Pr02 or 4 Nd2 Pr2 C>7 + P^P^Or? 4 S1112O3 »Pr2 02 *10Pr02 or 4 Sm2 Pr2 0 y + Pr2 Pr2 0y High ignition temperatures as used in preparing these oxides (925° C.) usually favor the formation of pyrorather than ortho- compounds. only for provoking thought. This concept is suggested One can probably devise structures based on close packed ionic structures to explain the behavior although the meager X-ray data will not permit elaboration along this line at present* 103 Zintl and Morawietz prepared a complex oxide composed of sodium, lanthanum, and praseodymium oxides, Nai 8Pl*0 8La0 ? ° 2 8 * They reported that the complex oxide exhibited a rock-salt-type lattice similar in lattice constants to sodium praseodymate, Na2 Pr0 2 * No interference from NaLaC^j which they found did not form a cubic-type lattice, was observed. They did not offer an explanation as to the nature of the complex oxide except to point out that the oxide is an example of the rock-salt-type lattice containing three kinds of cations. < 90 The formula of the complex oxide of Zintl and 103 Morawietz, Na^Prgl^O^g, obtained by increasing the ratio Na. QPr^ QLart o0 o Q tenfold, can be represented as 1*0 0*o •o a mixture of sodium oxide, lanthanum sesquoxide, and praseodymium dioxide or, as a mixture of sodium and lantha­ num pyropraseodymates. Na1 gPrgLa2 0 2g or 9 Na2 0 *La2 0 g« 8 Pr02 or 3 NagPr2 0 ,r, + La2 Pr2 0 r, Since all oxides concerned can exhibit a cubic-type lattice, it might be assumed that their solid solutions exhibit a cubic-type lattice. When a binary mixture of La2 0g and Na20 is fused, NaLa02 is formed which does not have a cubic-type lattice; when a binary mixture of Pp^0 ^^ and Na20 is fused, a cubic-type compound, Na2 Pr0g, is formed. However, X-ray analysis did not reveal any NaLaO^ or NaPr02 in the ternary oxide mixture, but as stated before, a cubic-type compound of approximately the same lattice constants as Na2 Pr0 g. 4 91 Part C Effects of Praseodymium Oxides on Magnetic Susceptibility Measurements of Rare Earth Oxides The effect of the changing ratio P^O^/PrC^ in oxide mixtures is of interest in connection with other properties, such as its relationship with respect to the magnetic susceptibilities of mixtures. The susceptibility of trivalent praseodymium should be considerably larger than tetravalent praseodymium (Table XV). Thus, the con­ ditions which promote A-type sesquioxide formation and low oxygenation of praseodymium should correlate with higher magnetic susceptibilities, and those which promote C-type sesquioxide formation and high oxygenation should be accompanied by lower magnetic susceptibilities. This 56 idea agrees with the data of Mazza, who measured the specific magnetic susceptibilities of the following binary systems: Nd2 0 2 ~Sm2 0 ^ and Pr^0^^-Nd2 0^, (Table XXII, Figure 4). The rule of additive magnetic susceptibilities for mixtures is represented by a straight line. for the Nd2 0 ^-Sm203 data agrees with the rule. The graph For the Pr6 °ll“^d2 °3 system the experimental and theoretical values 56 do not agree and Mazza considered this system anomalous. In view of the "excess" oxygen studies listed above, the behavior of the Pr£)0 2 ^-Nd2 0 ^ system can be explained. 91 Part C Effects of Praseodymium Oxides on Magnetic Susceptibility Measurements of Rare Earth Oxides The effect of the changing ratio P^O^/PrC^ in oxide mixtures is of interest in connection with other properties, such as its relationship with respect to the magnetic susceptibilities of mixtures. The susceptibility of trivalent praseodymium should be considerably larger than tetravalent praseodymium (Table XV). Thus, the con­ ditions which promote A-type sesquioxide formation and low oxygenation of praseodymium should correlate with higher magnetic susceptibilities, and those which promote C-type sesquioxide formation and high oxygenation should be accompanied by lower magnetic susceptibilities. This 56 idea agrees with the data of Mazza, who measured the specific magnetic susceptibilities of the following binary systems: NdjjO^-Sn^O^ and Pr6 0 n - N d 2 C>2 , (Table XXII, Figure 4). The rule of additive magnetic susceptibilities for mixtures is represented by a straight line. for the Nd^^-Sn^O^ data agrees with the rule. The graph For the Pr60ll“Nd2°3 system the experimental and theoretical values 56 do not agree and Mazza considered this system anomalous. In view of the "excess" oxygen studies listed above, the behavior of the Pr^O^-N^O^ system can be explained. 92 TABLE XXII Magnetic Susceptibilities of Binary Mixtures of Rare Earth Oxides Nd20^ Pr6°ll-Nd2°3 ( X*io6) 0 10 20 30 40 50 60 70 80 90 100 Nd20^-Sm20^ ( X-io6) 6.1 8.5 11.0 13.4 16.0 18.4 21.0 23.4 25.9 28.4 31.0 15.6 15.8 16.4 17.5 18.9 20.8 23.1 25.6 28.7 30.3 31.1 It can be assumed that Mazza actually had a ternary mixture of Pr2 0 ^-Pr0 2 “Nd2 0 ^ and that since the ratio Pr2 0 ^/Pr02 varies with each addition of neodymium oxide, a straight line relationship between magnetic susceptibility and per cent neodymium sesquioxide should not be expected. The curve (Figure 4) for 0-75 per cent neodymium oxide falls below the dotted straight line which represents a linear relationship. The oxides containing small quantities of neodymium favor the oxygenation of praseodymium. Since the specific magnetic susceptibility of praseodymium dioxide i is much lower than that of the sesquioxides (Table XV), these samples have values lower than the susceptibility values obtained by the additive rule. Oxides containing i S P E C IF IC MAGNETIC S U S C E P T IB IL IT Y ro o 04 o O Oi ro o 0 01 at o C/> (/> C/) P 1 •4 O 00 O to o o o £6 c/> u> -< CO -< O) V* m X*IO€ 94 more than 75 per cent neodymium oxide have a specific magnetic susceptibility greater than that obtained by the additive rule (fall above the dotted line) because the oxygenation of praseodymium sesquioxide, which has a specific magnetic susceptibility almost as large as that of neodymium sesquioxide (Table XV) is inhibited in these samples. Hence,the curve obtained by Mazza does not seem to be anamolous. It is believed that the ^r6°ll”^2°3 system might conform to the additive rule of specific magnetic susceptibilities if it is considered as a ternary system of Pr20^-Pr02-Nd202• This hypothesis can be confirmed only by a detailed study of the magnetic susceptibilities of the Pr£t0 2 1-Nd20 ^ system in reducing and oxidizing atmospheres. That is, the binary systems, PrgO^-NdgO^ and Pr0 2 “Nd2 0 ^ should conform to the additive rule to give a linear relationship of specific magnetic susceptibilities versus per cent neodymium sesquioxide. 95 Part D Conclusion The properties of the praseodymium oxides, Pr20^, Pr^O-^, and Pr02 , as well as their nature in binary mixtures with other rare earth oxides have been described. In general, praseodymium oxide exists as a combination of P?2 °3 and Pr02 in rare earth oxide mixtures. For praseodymium rich samples it tends to form Pr02 and for praseodymium poor samples, P^O^. The changing Pr20 ^/Pr02 ratio affects the physical properties of rare earth oxides. The failure of a Pr^O^-NdrjO^ system to conform to the additive rule of specific magnetic sus­ ceptibilities may be due to this effect. The conditions which enhance oxygenation of praseodymium oxide in mixtures with other rare earth oxides have been listed. An ignition temperature of 925° C. was chosen to insure complete decomposition of 78 rare earth carbonates which are always formed as inter­ mediate ignition products of the rare earth oxalates. It must be stated that the characteristics of binary rare earth oxides containing praseodymium may be differ­ ent from those reported in this thesis if the conditions of ignition are changed. Lower ignition temperatures, shorter ignition periods, and greater oxygen pressure would enhance the oxygenation of the praseodymium. 96 The nature of praseodymium oxide is very com­ plex, and its complete description will require the corre­ lation of magnetic susceptibility, available oxygen, phase rule, X-ray and other structural studies. 97 SECTION VIII Discussion and Suggestions for Future Researches Rare earth separations which depend upon the fractional precipitation of a very slightly soluble compound may be improved by the slow even addition of the precipitating reagent and by reducing the rare earth ion concentration in solution to a minimum. One very good method of obtaining a slow even addition of the precipitating reagent with the minimum of local effects is by the use of internal decomposition or hydrolysis reactions, such as the decomposition of the trlchloroacetate ion in hot solutions to precipitate insoluble carbonates or the hydrolysis of dimethyloxalate in cold acid solutions to precipitate insoluble oxalates. There are several ways to reduce the rare earth ion concentration in solution, the most common being by dilution. However, when working with extremely dilute solutions, the use of large quantities of solvent, the production of gelatinous precipitates, the difficulty of recovering the rare earth remaining in the filtrate, and other similar disadvantages present problems. Another method of reducing rare earth ion concentration is to employ a complexing reagent so that most of the rare earth ions are present as complex ions. 98 Nitrilotriacetic acid, NCC^COOH)^, has been found to be a good reagent for the formation of soluble 10 complex ions with the rare earths. Beck found that this reagent would dissolve rare earth oxalates and fluorides in neutral or slightly basic solutions and that the oxalates could be fractionally precipitated upon the addition of dilute acetic acid. Under these conditions lanthanum oxalate precipitated first, followed by the oxalates of the less basic cerium earths as the pH 11 was lowered. Beck and Gasser applied a modification of this procedure to the yttrium earths. Although this method is fractional and presents the disadvantage that the change in pH is brought about by dropwise addition of acetic acid, it appears to be faster than most rare earth separations. It is possible that the decrease in pH necessary to bring about precipitation in the method proposed by Beck may be produced by the application of homogeneous phase reactions. For example, dimethyloxalate may be added to the rare earth solution containing the nitrilotriacetate complexes and subsequently hydrolyzed to produce a gradual increase of oxalate ions and a decrease in pH. Both conditions would favor the slow formation of rare earth oxalates from a solution containing the nitrilotriacetate complexes. 99 Similarly, perhaps, rare earth carbonates could be fractionally precipitated from solutions of the nitrilotriacetate complexes by the decomposition of the rare earth trichloroacetates. The formation of carbon dioxide would result in a lowering of the pH of the rare earth solution. The probable order of precipitation of the carbonates for this type of reaction would be lanthanum carbonate followed by the carbonates of the less basic rare earths. If the nitrilotriacetate complex contained oxalate ions, the oxalates would probably precipitate in preference to the carbonates. Other reagents which might have good complexing properties are amines, amides, imides, ureas, hydrazines, and hydroxylamines in which the hydrogen atoms attached to the nitrogen atoms have been replaced by alkanoic acids. Ethylenediamine tetra acetic acid (H00CCH2)2n CH2CH2N(CH2C00H^ , and hydrazoformic acid, HOOCNHNHCOOH, are typical examples. 64 Meyer found that concentrated potassium carbon­ ate solutions readily dissolve rare earth carbonates and that the rare earths could be fractionally precipitated as double potassium carbonates upon the dropwise addition of water, the lanthanum double salt precipitating first. This procedure was used to obtain pure lanthanum compounds 3,52,69 rather quickly. Although other workers have since improved the method, it is still fractional. The separation 100 must be carried out in concentrated potassium carbonate solutions; the necessity of using these highly alkaline solutions is a distinct disadvantage. In this study an attempt was made to purify some lanthanum oxide which contained 1-2 per cent praseo­ dymium and neodymium oxides by decomposing trichloroacetate ions in a concentrated potassium carbonate solution containing the rare earths. The rare earth oxide mixture was dissolved in trichloroacetic acid, and the potassium double carbonates were precipitated and then redissolved with concentrated potassium carbon­ ate solution. The rare earth solution was heated at o 40 C., and the double carbonates reprecipitated by carbon dioxide, which is an acidic substance in strongly alkaline solutions, liberated in the decomposition of the trichloroacetate ions. The reaction was continued until most of the rare earth had been reprecipitated. The rare earths in the precipitate and in the filtrate were recovered as oxalates and ignited to oxides. The rare earth oxide obtained from the precipitated carbon­ ate was white, whereas that from the filtrate was tan. The absorption bands of praseodymium and neodymium were observed for a nitrate solution prepared from the latter oxide, but not in the former. It is evident that small quantities of the other rare earths may be removed from lanthanum by this method, which appears to be rapid; the chief disadvantage is the necessity of working with strongly alkaline solutions almost saturated with potassium carbon­ ate. However, lack of time prevented a thorough investi­ gation of the problem and continued research may prove profitable. Samarium like europium may be reduced to a 101 divalent state and precipitated as an insoluble sulfate. Europium, but not samarium, may be reduced in a Jones 53 reductor. Marsh carried out the reduction of samarium with sodium amalgam. It seems possible that samarium might be reduced in a column containing a more electro­ positive metal than zinc, as for example, titanium. The titanous solution formed when titanium metal dissolves is probably an excellent reagent for collecting the samarous salt. The use of titanium hydride for the reduction of samarium should also be investigated. In addition to the above suggestions many other research ideas were conceived during the problem and are listed briefly: a) the fractional precipitation of rare earth sulfates resulting from the decomposition of sulfamic 4-8 acid, b) the use of the rare earth trichloroacetates in liquid-liquid counter-current extraction separations, c) tho determination of the solubilities and other proper­ ties of the rare earth trichloroacetates and carbonates, 102 d) phase rule studies based upon the decomposition of the rare earth carbonates, e) the application of the trichloroacetate and dimethyloxalate separations to other rare earth mixtures, f) the separation of cerium and thorium from monazite based upon the formation of insoluble basic trichloroacetates, g) further investi­ gations of the effects of cerium, the other rare earths and related elements on the crystal structures, magnetic susceptibilities, oxidation states, densities, etc. of binary and higher oxide mixtures containing praseodymium or terbium oxides, h) the effects of ignition conditions on an oxide mixture containing praseodymium, and i) the preparation of insoluble praseodymates for the separation of praseodymium. i 103 SUMMARY 1. The solubilities of neodymium salts in water and organic solvents and the distribution of neo­ dymium nitrate between water and organic solvents were studied. 2. A brief resume of the properties of the inorganic salts of trichloroacetic acid and the pro­ cedure for the preparation of the rare earth trichloro­ acetates were given. Neodymium trichloroacetate was prepared and analyzed. 3. Lanthanum, neodymium, and samarium carbon­ ates were prepared by the decomposition of their tri­ chloroacetates from hot water solutions. The advantages of this decomposition method over older methods for preparing rare earth carbonates were discussed. 4. Two homogeneous phase reactions, the decom­ position of the trichloroacetate ion in the presence of rare earth ions to form the insoluble rare earth carbon­ ates and the hydrolysis of dimethyloxalate in rare earth solutions to yield insoluble rare earth oxalates, were investigated for the separation of praseodymium and lanthanum. The effects of conditions, such as temperature, pH, and rare earth concentration, are discussed. Praseo­ dymium of high purity was obtained using these methods. 104 5. The advantages and disadvantages of various cerium separations, including a description of a new method based upon the insolubility of a basic eerie tri­ chloroacetate, were discussed. 6. Five fundamental methods for the quanti­ tative determination of the rare earth elements were reviewed. A. new iodometric procedure for the determi­ nation of praseodymium and an improved procedure for the oxalate-oxide average atomic weight determination of rare earth mixtures were described, both of which depend upon the iodometric determination of "excess" oxygen in the oxide, 7. The properties of the praseodymium oxides, including a study of the oxidation state of praseodymium in binary oxide mixtures with lanthanum, neodymium, and samarium, were discussed. 8. were given. 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