This is a speculative theoretical synthesis developed independently by the author, originating from reflections on Henri Bergson’s concept of durée. It combines elements of Density-Indexed Time (a personal proposal) with David Wiltshire’s Timescape cosmology and Buchert averaging. It is not a refereed publication and is shared in its current form specifically to invite constructive criticism and/or discussion. The more philosophical and extrapolative sections (e.g., galaxies as miniuniverses, temporal interpretations of the Fermi paradox) are explicitly exploratory. The standard ΛCDM cosmological model assumes a single universal cosmic time inherited from the Friedmann–Lemaître–Robertson–Walker (FLRW) metric. This assumption is mathematically convenient but physically unrealistic: general relativity teaches that proper time is path-dependent and environment-dependent. Clocks in deep gravitational potentials tick more slowly than clocks in underdense regions, and the universe is inhomogeneous on all scales below ~100 Mpc. Density-Indexed Time (DIT) proposes replacing the universal cosmic time with a density-dependent lapse function 𝐹(𝜌)such that 𝑑𝜏 = 𝐹(𝜌) 𝑑𝑡. However, standalone DIT suffers a fatal gauge problem: in a homogeneous universe, 𝐹(𝜌)becomes a function of time alone and can be absorbed into a coordinate redefinition, rendering the theory physically empty. Timescape cosmology provides the missing physical machinery. By partitioning the universe into wall and void regions with different densities, expansion rates, and gravitational potentials, Timescape introduces a genuine, dynamically evolving clock-rate contrast. The Timescape lapse y𝑤 is not a gauge artifact but a physical observable derived from the Buchert averaging of Einstein’s equations. The unified DIT–Timescape framework identifies 𝐹(𝜌) with the Timescape lapse, generalizing the discrete wall–void contrast into a continuous, differentiable function suitable for perturbation theory.