Originally posted by deda
If you combine Archimedes' laws of lever with Newton's gravity and Coulomb's law you'll see that the last are not quite accurate.
\frac{F_1}{F_2}=\frac{M_1}{M_2}=\frac{D_2}{D_1}
is the Archimedes' law of lever.
-------------------------------
F=force
M=mass
D=equi.distance
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The "wrong laws" will say that each mass or charge is subjected to absolutely same force but it's not always how it is:
\frac{F_1}{M_1}=\frac{GM_2}{D^3}D_1=
and
\frac{F_2}{M_2}=\frac{GM_1}{D^3}D_2=
=>
M_1=-M_2
period.
Let me give you an example of how this works.
Example: Consider two weights on a bar which is supported by a pivot in a
uniform gravitational field which has a gravitational acceleration of g. Let the weights be at opposite ends of the bar. Let the weight on the left end be #1 and have mass M
1 and the one on the right end be #2 and have mass M
2. Assume the masses are, in general, different and the distance each is from the pivot are, in general, different. Assume the system is in static equalibrium. Then the total torque on the system will equal zero.
Let the force on end #1 be F
1 and the force on end #2 be F
2. Let the magnitude of the distance between pivot and end #1 be D
1 and the magnitude of the distance between pivot and end #2 be D
1. Use the x,y,z coordinate system using the unit vectors i,j,k in those directions. The g-field is parallel to the z-axis and points in the -z direction.
Calculate the torque using the pivot point as the origin of the cordinate system
\overrightarrow {T} = \overrightarrow {T}_{1} + \overrightarrow {T}_{2} = \overrightarrow {F}_{1}\times \overrightarrow {r}_{1} + \overrightarrow {F}_{2}\times \overrightarrow {r}_{2}
This reduces to
\overrightarrow {T} = [F_{1}D_{1} - F_{2}D_{2}]\hat{k} = 0
F_{1}D_{1} = F_{2}D_{2}
Since F
1 = M
1g and = F
2 = M
2g then
(M_{1}g)D_{1} = (M_{2}g)D_{2}
or
M_{1}D_{1} = M_{2}D_{2}
So that is how and why and when that relationship holds true.
In your equations above you incorrectly applied the gravitational force law since you seem to think that one of the either M
1 or M
2 is the mass of the Earth where in fact neither is. We can go back before I put the masses in and let
g = \frac{GM}{R^{2}}
where R = radius of Earth and M = mass of Earth and use this as an approximation to the uniform g-field if you'd like. But the answer will be the same.
One needs to be very careful when claiming that something is wrong. One should first ask oneself
Am I missing something that I can't see?. I do that when I come to a conclusion in a derivation. I e-mail a friend when I have high confidence in my result and I get feedback.