ch13-p079 - 79 We use F = Gmsmm/r2 where ms is the mass of...

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79. We use F = Gm s m m /r 2 , where m s is the mass of the satellite, m m is the mass of the meteor, and r is the distance between their centers. The distance between centers is r = R + d = 15 m + 3 m = 18 m. Here R is the radius of the satellite and
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This note was uploaded on 05/17/2011 for the course PHY 2049 taught by Professor Any during the Spring '08 term at University of Florida.

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