Radionuclide activities were measured in the low-background gamma-ray spectrometry facility GeMSE in eight meteorite falls (Lost City, Tamdakht, Huaxi, Boumdeid, Xining, Kamargaon, Degtevo, and Ouidiyat Sbaa) and two finds (SaU 606 and M€ urtschenstock) to evaluate the use of radionuclides for terrestrial age estimates. Results indicate that these meteorites were all derived from small-(r < 25 cm) to medium-sized (r < 65 cm) meteoroids. Short-lived 48 V (t 1/2 = 16.0 d) and 51 Cr (t 1/2 = 27.7 d) were only detected in Oudiyat Sbaa (EH), while 7 Be (t 1/2 = 53.1 d) was also detected in Degtevo (H) and Kamargaon (L), in agreement with reported fall dates. The 22 Na/ 26 Al activity ratio in Huaxi agrees with the previously reported short cosmic-ray exposure age of this meteorite while 22 Na/ 26 Al in Kamargaon likely records a complex exposure history. Bayesian statistical analysis verifies the detection of very low activities of 44 Ti (t 1/2 = 60 a) in the relatively large H chondrites (>100 g) Degtevo, Huaxi, Tamdakht, Lost City, and SaU 606. Additionally, large samples from Oudiyat Sbaa (EH) and Kamargaon (L) gave positive detections. For H chondrite target compositions, detected 44 Ti(Fe+Ni)/ 26 Al averaged 0.055 AE 0.013. Activities of 22 Na and 54 Mn in SaU 606 show that this meteorite fell between July and September 2012, making SaU 606 the second recent fall from Oman identified using gamma-ray spectrometry. The upper activity limit of 22 Na in the M€ urtschenstock meteorite shows that it fell prior to 1999 and is not related to a bolide observation in 2015. M€ urtschenstock shows 137 Cs~109 higher than previously determined in Oman meteorites, likely due to Chernobyl fallout.