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Example: Calculating the gravitational force exerted by the Earth on the Moon.
At a particular moment in time the Moon is located $\langle 1.9e8, 0, -1.9e8 \rangle$ m in a coordinate system in which the origin is located at the center of the Earth.
Determine the gravitational force exerted by the Earth on the Moon.
Facts
- The relative position vector from the Earth to the Moon is $\langle 1.9e8, 0, -1.9e8 \rangle$ m
- Earth is origin of coordinate system $\langle 0,0,0 \rangle$ m
- G, the gravitational constant = $ 6.7e-11 Nm^2/kg^2 $
Lacking
- The mass of the Earth is not given but can be found online ($5.9e24 kg$)
- The mass of the Moon is not given but can be found online ($7.3e22 kg$)
Approximations & Assumptions
- Assume no other forces acting on the moon.
Representations
Solution
First calculate the distance between moon and earth
$$|\vec{r}_{M-E}| = \sqrt{(r_{M-E_x})^2+(r_{M-E_y})^2+(r_{M-E_z})^2}$$
$$ = \sqrt{(1.9 x 10^8 m)^2 + (0m)^2 + (-1.9 x 10^8 m)^2}$$
$$ = 2.7 x 10^8 m$$
Find the unit vector of $\vec{r}_{M-E}$
$$ \hat{r}_{M-E} = \dfrac{\vec{r}_{M-E}}{|\vec{r}_{M-E}|} $$
$$ = \dfrac{\langle 1.9 x 10^8, 0, -1.9 x 10^8 \rangle m}{2.7 x 10^8 m}$$
$$ = \langle 0.7,0,-0.7 \rangle$$
You now have everything needed to calculate the gravitational force exerted by the Earth on the Moon:
$$ \vec{F}_{M-E} = \vec{F}_{grav\,on\,M\,by\,E}$$
$$ = -G\dfrac{{m}_M{m}_E}{|\vec{r}_{M-E}|^2}\hat{r}_{M-E}$$
$$ = (6.7 x 10^{-11} Nm^2/kg^2)\dfrac{(7.3 x 10^{22} kg)(5.9 x 10^{24} kg)}{(2.7 x 10^8 m)}\langle 0.7,0,-0.7 \rangle$$
$$ = 1.0 x 10^{29}N \langle 0.7,0,-0.7 \rangle$$
$$ = \langle 7.0 x 10^{28}, 0, -7.0 x 10^{28} \rangle N $$