Natural radiative lifetimes have been measured for three odd‐parity levels of neutral lead using time‐resolved UV laser‐induced fluorescence from a laser‐produced plasma. These new lifetimes, as well as additional recent values obtained by laser spectroscopy, combined with theoretical branching ratios deduced from a relativistic Hartree–Fock calculation taking core polarization effects into account, have allowed the deduction of a new set of accurate f‐values of astrophysical interest. Using the new lifetime value for 6p7s (1/2, 1/2)°0, a refined value of the lead abundance in the solar photosphere is deduced: APb= 2.00±0.06 on the usual logarithmic scale, allowing the resolution of the long‐standing discrepancy previously observed between the solar photosphere and meteorites.