[I asked this at History of Science and Mathematics but there was no answers. I'm asking here too, after all the Newton's gravitational constant is fundamental in physics.]
I'm trying to compute the value of Newton's gravitational constant $G$ from Cavendish's own observations. I get $G_{\mathrm{Cav}}=5.27501×10^{−10}$ which is 8 times bigger than the accepted value of $G_{\mathrm{True}}=6.67430×10^{−11}$. Do you see anything wrong with my computations below?
I'm using this formula (from Wikipedia)
$$ G = \frac{2\pi^2 L r^2 \theta}{M T^2} $$
where
- $G =$ Gravitational constant
- $L =$ Length of torsion balance (the distance between the centers of balls)
- $r =$ The distance of attraction (between weights and balls)
- $\theta =$ Deflection of the arm from its rest position due to gravitational attraction
- $M =$ Mass of attracting lead weight
- $T =$ Natural period of oscillation of the balance
I take $\theta$ and T (Cavendish's N) from the 4th experiment, (Page 520 in Cavendish's paper), the rest are constants,
L = 1.862 m
r = 0.2248 m
$r^2$ = 0.05053 $m^2$
$\theta$ = 0.00806788 radians
M = 158.04 kg
T = 421 s
$T^2$ = 177241 $s^2$
Substituting in the numbers,
$$ G_{Cav} = \frac{2 \times \pi^2 \times 1.836 \times 0.05053504 \times 0.00806788}{158.04 \times 177241} = 5.27501\times 10^{-10} $$
This is eight times bigger than the accepted value,
$$ \frac{G_{Cav}}{G_{True}} = 7.90 $$
What's wrong with these calculations?
Cavendish uses the formula $D= \frac{N^2}{10683\times B}$ to compute density $D$ of the earth. When the weights are moved from + to - and from - to +, the arm of the pendulum moves twice as much then when the weights are moved from middle position to + or - positions. He does not say it explicitly but for experiments with double values ($2B$) Cavendish uses the formula, $D= \frac{N^2}{10683\times (B/2)}$.
I computed $G$ by halving $B$ but I still did not get the correct value. But when I halved $2B$ values and double the period I got the correct value.
And, this is how I computed the radian value of B:
On page 509, Cavendish gives the distance of the ivory scale from the center of motion: "But the ivory scale at the end of the arm is 38.3 inches from the center of motion." On the same page he says that each division of the ivory scale is 1/20 of an inch, that is, 0.050 inch. By the radian rule, $\theta = \frac{l}{r} = \frac{0.050}{38.3}= 0.0013054$.
For this experiment $B=6.18$ So, I multiply 6.18 by 0.00130 to get 0.008067 radians as the angle of deflection.
There are more details here