First, let's find the diagonal distance:
diagonal distance = s * sqrt(2) = 0.60m * sqrt(2) ≈ 0.85m
Now, let's calculate the gravitational force exerted by the spheres on each other:
Fg = Gmm (1/diagonal distance^2 + 2*.707/s^2)
Fg = (6.674 x 10^-11 N(m/kg)^2)(9.5kg)^2 (1/(0.85m)^2 + 2*.707/(0.60m)^2)
Fg = (6.674 x 10^-11 N(m/kg)^2)(90.25kg^2) (1/(0.7225m^2) + 2*.707/(0.36m^2))
Fg ≈ (6.674 x 10^-11 N(m/kg)^2)(90.25kg^2)(2.679)
Fg ≈ 1.61 x 10^-9 N
Now, let's find the direction. Since the forces from the adjacent masses cancel each other out horizontally, we only need to consider the vertical components:
Vertical component = Fg * sin(45)
Vertical component = (1.61 x 10^-9 N) * sin(45)
Vertical component ≈ 1.14 x 10^-9 N
So, the total gravitational force exerted on one sphere by the other three is 1.14 x 10^-9 N in the vertical direction (upwards or downwards, depending on the specific sphere being considered).
four 9.5kg spheres are located at the corners of a square of side 0.60m. calculate the magnitude and direction of the total gravitational force exerted on one sphere by the other three
Let s be the side length, so the diagnoal length is s * sqrt2.
This is a vector problem. Note the adjacent masses operate at 45 degrees, so the force component is Fg*.707 in the direction of the diagnol. The other component is canceled by the other adjacent mass (opposite direction). Add the three forces.
Fg= Gmm/1 (1/diagonaldistance^2 + 2*.707/s^2 )
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