Apparent molar volumes and apparent molar heat capacities of Pr(NO 3) 3(aq), Gd(NO 3) 3(aq), Ho(NO 3) 3(aq), and Y(NO 3) 3(aq) at T = (288.15, 298.15, 313.15, and 328.15) K and p = 0.1 MPa

Abstract

Relative densities and relative massic heat capacities have been measured for acidified solutions of Y(NO 3) 3(aq), Pr(NO 3) 3(aq), and Gd(NO 3) 3(aq) at T = (288.15, 298.15, 313.15, and 328.15) K and p = 0.1 MPa. In addition, relative densities and massic heat capacities have been measured at the same temperatures and pressure for Y(NO 3) 3(aq) and Ho(NO 3) 3(aq) solutions without excess acid (n.b. measurements at T = 328.15 K for Ho(NO 3) 3(aq) were not performed due to the limited volume of solution available). Apparent molar volumes and apparent molar heat capacities for the aqueous salt solutions have been calculated from the experimental apparent molar properties of the acidified solutions using Young’s rule, whereas the apparent molar properties of the solutions without excess acid were calculated directly from the measured densities and massic heat capacities. The two sets of data for the Y(NO 3) 3(aq) systems provide a check of the internal consistency of the Young’s rule approach we have utilised. The concentration dependences of the apparent molar volumes and heat capacities of the aqueous salt solutions have been modelled at each investigated temperature using the Pitzer ion interaction equations to yield apparent molar properties at infinite dilution. Complex formation within the aqueous rare earth nitrate systems is discussed qualitatively by probing the concentration dependence of apparent molar volumes and heat capacities. In spite of the complex formation in the aqueous rare earth nitrate systems, there is a high degree of self-consistency between the apparent molar volumes and heat capacities at infinite dilution reported in this manuscript and those previously reported for aqueous rare earth perchlorates.