In order to find the gravitational force we must first calculate the distance between the moon and the earth
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In order to find the gravitational force we must first calculate the center to center distance between the moon and the earth
|→rM−E|=√(rM−Ex)2+(rM−Ey)2+(rM−Ez)2
|→rM−E|=√(rM−Ex)2+(rM−Ey)2+(rM−Ez)2
Line 47:
Line 47:
=⟨0.7,0,−0.7⟩
=⟨0.7,0,−0.7⟩
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You now have everything needed to calculate the gravitational force exerted by the Earth on the Moon:
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Adding both the direction of the radius and the length of the radius to the mass of the Earth and the mass of the Moon and the gravitational constant we now have all of the variables needed to compute the gravitational force exerted by the Earth on the Moon. The force between the Earth and the moon is the same as the gravitational force exerted by the Earth on the Moon.
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→FM−E=→FgravonMbyE
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→FM−E=→FgravonMbyEThis is the representation we identified for gravitational force. There is a minus in front of the G as the direction of the gravitational force is opposite to the direction of the unit vector ˆr, which points from object 1 (Moon) to object 2(Earth).
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=−GmMmE|→rM−E|2ˆrM−E
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=−GmMmE|→rM−E|2ˆrM−EInput all the values identified for the various variables.