A star, which is 1.9 x 1020 m from the center of a galaxy, revolves around that center once every 2.6 x 108 years. Assuming each star in the galaxy has a mass equal to the Sun's mass of 2.0 x 1030 kg, the stars are distributed uniformly in a sphere about the galactic center, and the star of interest is at the edge of that sphere, estimate the number of stars in the galaxy.

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Chapter1: Units, Trigonometry. And Vectors
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A star, which is 1.9 x 1020 m from the center of a galaxy, revolves
around that center once every 2.6 x 108 years. Assuming each star
in the galaxy has a mass equal to the Sun's mass of 2.0 x 1030 kg,
the stars are distributed uniformly in a sphere about the galactic
center, and the star of interest is at the edge of that sphere,
estimate the number of stars in the galaxy.
Transcribed Image Text:A star, which is 1.9 x 1020 m from the center of a galaxy, revolves around that center once every 2.6 x 108 years. Assuming each star in the galaxy has a mass equal to the Sun's mass of 2.0 x 1030 kg, the stars are distributed uniformly in a sphere about the galactic center, and the star of interest is at the edge of that sphere, estimate the number of stars in the galaxy.
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