RI 5783 Radiochemical Precipitation Studies Of Rare-Earth Oxalates ? Summary And Introduction

The objective of this rare-earth oxalate study by the Bureau of Mines was to determine systematically by radiochemical techniques what effects, if any, could be attributed to the several variables--temperature, digestion time, acid concentration, rare-earth concentration, oxalic acid concentration, stirring, and the presence of other rare-earth ions. A Latin Square experimental design was used to evaluate statistically some of the variables. Precipitation losses ranged from near zero to about 7 percent, and mineral acid and rare-earth concentration were the predominant factors affecting completeness of precipitation. Quantitative oxalate precipitation of the rare-earth elements was achieved by controlling the experimental conditions as follows: (1) Maintaining rare-earth concentrations above 0.01M; (2) stirring the mixture several minutes after precipitation; (3) using an adequate (two to five-fold) excess of oxalic acid; (4) precipitating at room or iced temperature and digesting for at least 1 hour; (5) avoiding an excess of mineral acid and, if possible, maintaining the pH above 2.0; and (6) avoiding excess complexing agents such as EDTA (ethylenediaminetetraacetic acid). In the past 20 years research aimed at developing more efficient separation and purification techniques applicable to the rare-earth elements and yttrium has been extensive. Common to most of these procedures has been the use of oxalic acid to precipitate this group of elements selectively. However, this particular use of oxalic acid has a much earlier origin; its application in precipitating yttrium was first reported by Mosander (8)4 in 1843. Despite long and popular employment of this technique, only limited and somewhat conflicting data are available regarding the many factors affecting the degree of rare-earth oxalate precipitations.