The Gamow-Teller strength distribution from 88 Sr was extracted from a (t, 3 He + γ) experiment at 115 MeV/u to constrain estimates for the electron-capture rates on nuclei around N = 50, between and including 78 Ni and 88 Sr, which are important for the late evolution of core-collapse supernovae. The observed strength below an excitation energy of 8 MeV was consistent with zero and below 10 MeV amounted to 0.1 ± 0.05. Except for a very-weak transition that could come from the 2.231-MeV 1 + state, no γ lines that could be associated with the decay of known 1 + states were identified. The derived electron-capture rate from the measured strength distribution is more than an order of magnitude smaller than rates based on the single-state approximation presently used in astrophysical simulations for most nuclei near N = 50. Rates based on shell-model and quasiparticle random-phase approximation calculations that account for Pauli blocking and core-polarization effects provide better estimates than the single-state approximation, although a relatively strong transition to the first 1 + state in 88 Rb is not observed in the data. Pauli unblocking effects due to high stellar temperatures could partially counter the low electron-capture rates. The new data serves as a zero-temperature benchmark for constraining models used to estimate such effects.