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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 ⟨1.9e8,0,−1.9e8⟩ 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 ⟨1.9e8,0,−1.9e8⟩ m
- Earth is origin of coordinate system ⟨0,0,0⟩ m
- G, the gravitational constant = 6.7e−11Nm2/kg2
Lacking
- The mass of the Earth is not given but can be found online (5.9e24kg)
- The mass of the Moon is not given but can be found online (7.3e22kg)
Approximations & Assumptions
- Assume no other forces acting on the moon.
Representations
Solution
First calculate the distance between moon and earth
|→rM−E|=√(rM−Ex)2+(rM−Ey)2+(rM−Ez)2
=√(1.9x108m)2+(0m)2+(−1.9x108m)2
=2.7x108m
Find the unit vector of →rM−E
ˆrM−E=→rM−E|→rM−E|
=⟨1.9x108,0,−1.9x108⟩m2.7x108m
=⟨0.7,0,−0.7⟩
You now have everything needed to calculate the gravitational force exerted by the Earth on the Moon:
→FM−E=→FgravonMbyE
=−GmMmE|→rM−E|2ˆrM−E
=(6.7x10−11Nm2/kg2)(7.3x1022kg)(5.9x1024kg)(2.7x108m)⟨0.7,0,−0.7⟩
=1.0x1029N⟨0.7,0,−0.7⟩
=⟨7.0x1028,0,−7.0x1028⟩