We explore the prospect of constraining light mediators at the next generation direct detection dark matter detectors through coherent elastic neutrino-nucleus scattering (CEνNS) and elastic neutrino-electron scattering (EνES) measurements.Taking into account various details like the quenching factor corrections and atomic binding effects, we obtain the model independent projected sensitivities for all possible Lorentz invariant interactions, namely scalar (S), pseudoscalar (P ), vector (V ), axial vector (A) and tensor (T ). For the case of vector interactions, we also focus on two concrete examples: the well-known U (1) B−L and U (1) Lµ−Lτ gauge symmetries.For all interaction channels X = {S, P, V, A, T }, our results imply that the upcoming dark matter detectors have the potential to place competitive constraints, improved by about one order of magnitude compared to existing ones from dedicated CEνNS experiments, XENON1T, beam dump experiments and collider probes.