Textbook ExpertVerified Tutor
4 Dec 2021
Given information
Given that Cepheid variable stars change in luminosity with a typical period of several days and the period has been found to have a definite relationship with the average intrinsic luminosity of the star we are asked how these stars could be used to measure the distance to galaxies.
Step-by-step explanation
Step 1.
Calculate the period of a Cepheid variable star's changing luminosity. To determine its absolute luminosity, use the well-known relationship between period and luminosity. To determine the distance to the galaxy in which it is located, compare its absolute luminosity to its apparent brightness (the observed brightness).
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