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Motivated from the observations of yet-unexplained explosive phenomena associated with massive blue-supergiant stars with zero-age main sequence (ZAMS) masses around 50 M, new light has been shed on the old idea that the appearance of QCD degrees of freedom may explain such cosmic events. Obeying chiral physics and taking yet-another important observation of the very existence of massive neutron stars of 2 M seriously into account, puts sever constraints on the behavior of the equation of state at supersaturation density (sat). In particular, sufficient stiffness with increasing density is required. Both aspects indicate rather high densities for the hadron-quark phase transition in excess of 2sat (at zero temperature). As a consequence, this excludes low- and intermediate mass stars ( 10 -15 M) - they are canonically considered in supernova studies - from the presence of 'exotic' high-density phases. On the other hand, during the evolution of very massive core collapse supernova progenitors with ZAMS masses of about 50 M, significantly higher core temperatures and densities are reached, where the appearance of the hadron-quark phase transition triggers not only the supernova explosion onset but also a millisecond neutrino burst is released. The latter observable signal provides evidence not only for the presence of a 1st-order phase transition at supersaturation density but contains also details about its properties. The future observation of such a feature from the next galactic event will allow us to either confirm such scenario or, if not observed, rule out a (strong) 1st-order phase transition at high densities encountered in astrophysics. In this talk I will review this scenario in the light of presently known constraints from nuclear physics as well as observations. The latter includes the first binary neutron star merger event associated with GW170817. Furthermore, I will discuss implications for astrophysics, e.g., the remnants from such supernova explosions are massive neutron stars with quark-matter core of 2 M at birth.