[en] The goal of the molybdenum solar neutrino experiment is to deduce the ⁸B solar neutrino flux, averaged over the past several million years, from the concentration of ⁹⁸Tc in a deeply buried molybdenum deposit. The experiment is important to an understanding of stellar processes because it will shed light on the reason for the discrepancy between theory and observation of the chlorine solar neutrino experiment. Possible reasons for the discrepancy may lie in the properties of neutrinos (neutrino oscillations or massive neutrinos) or in deficiencies of the standard solar model. The chlorine experiment only measures the ⁸B neutrino flux in current times and does not address possible temporal variations in the interior of the sun, which are also not considered in the standard model. In the molybdenum experiment, we plan to measure ⁹⁸Tc (4.2 Myr), also produced by ⁸B neutrinos, and possibly ⁹⁷Tc (2.6 Myr), produced by lower energy neutrinos