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The death of massive stars is shrouded in many mysteries. One of them is themechanism that overturns the collapse of the degenerate iron core into anexplosion, a process that determines the supernova explosion energy, propertiesof the surviving compact remnant, and the nucleosynthetic yields. The number ofcore-collapse supernova observations has been growing with an accelerating pacethanks to modern time-domain astronomical surveys and new tests of theexplosion mechanism are becoming possible. We review predictions ofparameterized supernova explosion models and compare them with explosionproperties inferred from observed light curves, spectra, and neutron starmasses.

The Explosion Mechanism of Core-Collapse Supernovae and Its Observational Signatures