Estimating Number of Stars in Milky Way Galaxy: Kepler Problem Solution

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SUMMARY

The discussion centers on estimating the number of stars in the Milky Way galaxy using the Kepler problem solution. Given the Sun's mass of 2.0 x 1030 kg and its distance of 2.2 x 1020 m from the galactic center, the estimation process involves calculating the galaxy's total mass and dividing it by the Sun's mass. The assumption is made that stars are uniformly distributed in a spherical shape around the galactic center, allowing for a simplified calculation despite the actual spatial distribution of stars.

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CinderBlockFist
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Our Sun, with mass 2.0 1030 kg, revolves about the center of the Milky Way galaxy, which is 2.2 1020 m away, once every 2.5 108 years. Assuming that each of the stars in the galaxy has a mass equal to that of our Sun, that the stars are distributed uniformly in a sphere about the galactic center, and that our Sun is essentially at the edge of that sphere, estimate roughly the number of stars in the galaxy.

How can i find this answer if the stars don't fill up the space because they are spheres?
 
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Compute the galaxy's mass and divide it to the mass of the sun (i assumed that the average mass of a star is roughly equal to the one of the sun).

Daniel.
 
It doesn't matter that the stars don't fill space. Treat it as if all mass were concentrated at the center of the galaxy.
 

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