79. We use F= Gmsmm/r2, where msis the mass of the satellite, mmis the mass of the meteor, and ris the distance between their centers. The distance between centers is r= R+d= 15 m + 3 m = 18 m. Here Ris 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.