Last decades we hear the term "Hubble tension", which implies the inconsistency between local measurements of the current expansion rate of the universe, for example, based on supernovae as standard candles, giving around 73 (km s^–1 Mpc^–1). Using The ΛCDM model measuring the cosmic microwave background (CMB) value of the Hubble constant appears around 67( km s^–1 Mpc^–1), and the discrepancy with local measurements is around 10%! Do we need further experiments if the Hubble tension already makes the ΛCDM model inconsistent? What is your guess for correct H_0?