Answered: To model a moon in the solar system,… | bartleby

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To model a moon in the solar system, consider a sphere with radius R
and uniform mass density p. Let gm = the acceleration due to gravity
on the surface of the sphere. Calculate gm for these values of R and p:
R = 2.0×106 m; p= 2.7x103 kg/m^3;
(in m/s^2)
OA:
OB:
1.509 2.007
OC:
2.669
OD:
3.549
OE:
OF:
4.721 6.279
OG:
8.351
OH:
1.111x101

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