What specific stellar characteristic, measured by Henrietta Swan Leavitt, allowed Hubble to determine the intrinsic brightness of Cepheids?

Answer

The Period-Luminosity Relationship

The foundational insight that made extragalactic distance measurement possible was the Period-Luminosity Relationship, established by Henrietta Swan Leavitt. This cosmic law dictates a direct correlation between how long it takes a Cepheid variable star to cycle through its brightening and dimming phases (its period) and how luminous the star intrinsically is (its absolute magnitude). By accurately measuring the pulsation period of a Cepheid like V1 in Andromeda, Hubble could use Leavitt's established relationship to find out how bright the star truly was, regardless of its distance.

What specific stellar characteristic, measured by Henrietta Swan Leavitt, allowed Hubble to determine the intrinsic brightness of Cepheids?
measurementHubblegalaxyDistanceAndromeda Galaxy