The gravitational attraction between the Earth and the Hubble telescope is given by:
![F=G(M m)/(r^2)](https://img.qammunity.org/2019/formulas/physics/middle-school/y5rd9nbukb3p80prepdcp2ja9hojw8bsuo.png)
where
G is the gravitational constant
M is the Earth's mass
m is the Hubble mass
r is the distance of the Hubble telescope from the earth's center
By rearranging the equation and substituting the numbers given by the problem, we find the mass of the telescope:
![m=(F r^2)/(GM)=((9.21 \cdot 10^4 N)(6.94 \cdot 10^6 m)^2)/((6.67 \cdot 10^(-11) m^3 kg^(-1) s^(-2) )(5.98 \cdot 10^(24)kg) ) = 11121 kg](https://img.qammunity.org/2019/formulas/physics/middle-school/n2nxci2hgccez8q3ytz2xii952lnwke764.png)