Beschreibung:
<jats:title>Abstract</jats:title><jats:p>Radionuclide activities were measured in the low‐background gamma‐ray spectrometry facility Ge<jats:styled-content style="fixed-case">MSE</jats:styled-content> in eight meteorite falls (Lost City, Tamdakht, Huaxi, Boumdeid, Xining, Kamargaon, Degtevo, and Ouidiyat Sbaa) and two finds (SaU 606 and Mürtschenstock) to evaluate the use of radionuclides for terrestrial age estimates. Results indicate that these meteorites were all derived from small‐ (<jats:italic>r</jats:italic> < 25 cm) to medium‐sized (<jats:italic>r</jats:italic> < 65 cm) meteoroids. Short‐lived <jats:sup>48</jats:sup>V (t<jats:sub>1/2</jats:sub> = 16.0 d) and <jats:sup>51</jats:sup>Cr (t<jats:sub>1/2</jats:sub> = 27.7 d) were only detected in Oudiyat Sbaa (<jats:styled-content style="fixed-case">EH</jats:styled-content>), while <jats:sup>7</jats:sup>Be (t<jats:sub>1/2</jats:sub> = 53.1 d) was also detected in Degtevo (H) and Kamargaon (L), in agreement with reported fall dates. The <jats:sup>22</jats:sup>Na/<jats:sup>26</jats:sup>Al activity ratio in Huaxi agrees with the previously reported short cosmic‐ray exposure age of this meteorite while <jats:sup>22</jats:sup>Na/<jats:sup>26</jats:sup>Al in Kamargaon likely records a complex exposure history. Bayesian statistical analysis verifies the detection of very low activities of <jats:sup>44</jats:sup>Ti (t<jats:sub>1/2</jats:sub> = 60 a) in the relatively large H chondrites (>100 g) Degtevo, Huaxi, Tamdakht, Lost City, and SaU 606. Additionally, large samples from Oudiyat Sbaa (<jats:styled-content style="fixed-case">EH</jats:styled-content>) and Kamargaon (L) gave positive detections. For H chondrite target compositions, detected <jats:sup>44</jats:sup>Ti(Fe+Ni)/<jats:sup>26</jats:sup>Al averaged 0.055 ± 0.013. Activities of <jats:sup>22</jats:sup>Na and <jats:sup>54</jats:sup>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 <jats:sup>22</jats:sup>Na in the Mürtschenstock meteorite shows that it fell prior to 1999 and is not related to a bolide observation in 2015. Mürtschenstock shows <jats:sup>137</jats:sup>Cs ~10× higher than previously determined in Oman meteorites, likely due to Chernobyl fallout.</jats:p>