The implications of the mixing for the mixing angle is investigated. Based on the mixing angle suggested from the analysis for a substantial body of data concerning the and , the masses of the and are determined to be $\sim 1307.35\pm 0.631370.03\pm 9.69$ MeV, respectively, which therefore suggests that the mixing angle is about $\pm (59.55\pm 2.81)^\circh^\prime_1(^1P_1)s\bar{s}1495.18\pm 8.82$ MeV. Comparison of the predicted results and the available experimental information of the shows that without further confirmation on the , the assignment of the as the member of the meson nonet may be premature.

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