The Sun, which is 2.2 1020 m from the center
of the Milky Way galaxy, revolves around that center once every2.5 108 years. Assuming each star in the Galaxy has a mass equalto the Sun’s mass of 2.0 1030 kg, the stars are distributed uniformlyin a sphere about the galactic center, and the Sun is at theedge of that sphere, estimate the number of stars in the Galaxy.
The Sun, which is 2.2 1020 m from the center
of the Milky Way galaxy, revolves around that center once every
2.5 108 years. Assuming each star in the Galaxy has a mass equal
to the Sun’s mass of 2.0 1030 kg, the stars are distributed uniformly
in a sphere about the galactic center, and the Sun is at the
edge of that sphere, estimate the number of stars in the Galaxy.