Background: Uncertainty in the operating temperatures of Oklo reactor zones impacts the precision of bounds derived for time variation of the fine structure constant α. have been undertaken by many groups investigating whether the fine structure constant α has changed over the 2 GY period since the reactors operated. As first pointed out by Shlyachter [2], the samarium isotopic ratios are sensitive to the value of α through the overlap of the 149 Sm E 0 =97.3-meV neutron resonance with the thermal and epithermal portions of the neutron flux in the reactor. While the majority of Oklo analyses [3][4][5][6][7], have been consistent with no shift in the resonance energy, and therefore no change in α, a change has been argued for from astronomical observations [8].All Oklo analyses make assumptions about the operating temperatures of the reactors. But there is as yet no agreement on what these temperatures actually were. Utilizing the 176 Lu/ 175 Lu isotope ratio method to determine temperatures was recently revisited by Gould and Sharapov [9] . The method is based on the temperature dependence of the large thermal neutron capture cross section of 176 Lu (natural abundance 2.599 % [10]), and on knowing with certainty the (small) ground state branching ratio for thermal neutron neutron capture on the more abundant lutetium isotope, 175 Lu (natural abundance 97.401 %). The dominant capture branch σ