177Lu-microspheres were prepared through a precipitation method by using silica microspheres as matrix. K
3PO
4 and KOH were used to adjust the pH of the reaction medium as the precipitation reactions of
177Lu
3+ are generally pH-dependent. As shown in
Fig. 1A, the radiolabeling efficiency increases dramatically against pH and reaches a plateau around 96.8% ± 0.5% at pH 12. In addition, the effect of reaction time on the radiolabeling efficiency was also studied. According to the results given in
Fig. 1B, the radiolabeling efficiency higher than 96% can be achieved within 1 min, nearly independent of the reaction time. The following studies suggested that the specific activity, calculated by dividing the radioactivity of
177Lu by the number of microspheres, could be varied from 1 Bq/microsphere to 1 × 10
5 Bq/microsphere through the approach mentioned above. High specific activity is favorable for avoiding arterial stasis caused by excessive microspheres, as less number of microspheres is required for achieving the same radiation dose [
37,
38]. To characterize the morphology, size and size distribution of the microspheres after
177Lu labeling,
175LuCl
3 was used instead of
177LuCl
3 to prepare non-radioactive microspheres (denoted as Lu-microspheres) following the same preparative procedures for
177Lu-microspheres. The average size of the Lu-microspheres determined by optical microscopy is of 20.7 ± 0.7 µm and the polydisperse index is of 0.034, as shown in
Fig. 1C and Fig. S1A (Supporting information). The scanning electron microscopy (SEM) image given in
Fig. 1D reveals that the Lu-microspheres are perfectly spherical in shape. In comparison with the mother silica microspheres, the Lu-microspheres present nearly unchanged shape, size and size distribution, suggesting that the coprecipitation approach did not alter the morphology of the mother silica microspheres at all (Figs. S1B-D in Supporting information). The radiostability of
177Lu-microspheres in saline and 10% FBS was tested and the free
177Lu in saline and 10% FBS was measured to be less than 2% and 20% (
Fig. 1E), respectively, indicating that
177Lu-microspheres are very stable for further
in vitro and
in vivo experiments. The transformation of
177Lu to
177Hf is accompanied by emission of gamma rays of 113 keV (3%) and 210 keV (11%) which are suitable for SPECT imaging. To verify the SPECT imaging capacity of the
177Lu-microspheres, tube phantom imaging was carried out. The results given in
Fig. 1F and Fig. S2 (Supporting information) reveal that the signal intensity extracted from SPECT images increases linearly against the radioactivity of
177Lu-microspheres, suggesting that the
177Lu-microspheres are potentially suitable for SPECT imaging of tumors
in vivo. Most importantly, the SPECT signal offers a non-invasive way to track the
177Lu-microspheres
in vivo.