Answer to Question 1
Certain types of variable stars, such as Cepheids and RR Lyrae stars, pulsate with a precise period that is easily determined by observing variations in the star's apparent magnitude. The period of a Cepheid is directly related to the absolute magnitude of the Cepheid and RR Lyrae stars have generally all the same absolute magnitude. When the apparent and absolute magnitudes of a star are known, its distance can be immediately calculated. Because Cepheids, in particular, are among the brightest stars known, they can be seen over large distances. Thus Cepheids are excellent for determining distances to remote objects.
Answer to Question 2
A