Abstract
An energy threshold alone does not establish a civilization’s ability to persist. Building on two Galaxies studies of Type I and Type II development, we propose additional qualifications based on stewardship, autonomous habitation, and resilience to loss of the original home world or star. Type I couples planetary energy capability with maintenance of a habitable Earth; Type II adds a self-sustaining Solar System network; Type III combines Galactic energy capability and transport with communities able to continue beyond the Sun. These qualifications complement the conventional power scale. A finite-speed expansion model couples access to stellar luminosity with gradual local construction and conditional continuity. In a stipulated exponential disk, the conventional 10³⁶ W threshold is crossed approximately 0.68, 6.7, or 67 million years after expansion begins; reaching the entire modeled disk takes 2.28, 22.8, or 228 million years. Neither result establishes autonomous habitation or stewardship, and neither is a forecast. Sufficient usable luminosity is a necessary condition for power attainment, while cumulative hazard constrains continuity. Independence from the Sun can occur before the energy threshold. The framework separates physical access, usable power, and durable civilizational viability, identifies their distinct timescales, and provides reproducible scenario calculations.