Daniel B. answered 04/25/21
A retired computer professional to teach math, physics
This is an application of Koenig's theorem
L = L0 + L', where
L is the angular momentum of a body rotating around a point O,
L0 is the angular momentum of the center of gravity, with all mass concentrated there,
L' is the angular momentum of the body relative to the center of gravity.
Before solving your problem with two specific spheres, lets solve
the problem for a general sphere where the matter is uniformly distributed.
Let
r be the radius of the sphere,
R be the distance of the center of gravity of the sphere from the center of rotation,
V = 4πr³/3 be the volume of the sphere,
s be the specific density of the sphere,
M = sV be the mass of the sphere,
ω be the angular velocity.
Notice that in your situation,
ω is the angular velocity of the center of gravity around the point O,
as well as the angular velocity of the sphere around its center of gravity.
As you have demonstrated
L0 = MωR²
To calculate L' think of the whole solid sphere as composed of concentric hollow sub-spheres,
each with radius x and thickness dx,
where x ranges from 0 to r.
The area of each sub-sphere is 4πx², its volume is 4πx²dx, its mass is s4πx²dx,
and its angular momentum is ωs4πx4dx.
The angular momentum of the whole sphere is the integral over all the sub-spheres.
The indefinite
∫ωs4πx4dx = ωs4πx5/5
Therefore for the definite integral from 0 to r we get
L' = ωs4πr5/5
In order to express it in terms of the mass M instead of density s we rewrite it as
L' = 3ωr²/5 × s4πr³/3 = 3Mωr²/5
Thus
L = MωR² + 3Mωr²/5 = Mω(R² + 3r²/5)
Now applying it to your two spheres, and expressing ω in terms of your given velocity v:
L1 + L2 =
m1ω(R² + 3r²/5) + m2ω(R² + 3r²/5) =
(m1+m2)ω(R² + 3r²/5) =
(m1+m2)(v/R)(R² + 3r²/5)
Substituting actual numbers
L1 + L2 = 7 × (5.8/0.5) × (0.5² + 3×0.145²/5) = 21.32
As a side note. You said that the direction of the angular momentum is in +z. From the statement of the problem I cannot tell whether it is +z or -z, because it does not mention the direction of rotation. But I assume that your picture had that.
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This is an application of Koenig's theorem
L = L0 + L', where
L is the angular momentum of a body rotating around a point O,
L0 is the angular momentum of the center of gravity, with all mass concentrated there,
L' is the angular momentum of the body relative to the center of gravity.
Before solving your problem with two specific spheres, lets solve
the problem for a general sphere where the matter is uniformly distributed.
Let
r be the radius of the sphere,
R be the distance of the center of gravity of the sphere from the center of rotation,
V = 4πr³/3 be the volume of the sphere,
s be the specific density of the sphere,
M = sV be the mass of the sphere,
ω be the angular velocity.
Notice that in your situation,
ω is the angular velocity of the center of gravity around the point O,
as well as the angular velocity of the sphere around its center of gravity.
As you have demonstrated
L0 = MωR²
To calculate L' think of the whole solid sphere as composed of concentric hollow cylinders,
each with radius x and thickness dx,
where x ranges from 0 to r.
The cylinders are centered around the axis of rotation parallel to the z-axis
and going though the center of the sphere.
The perimeter is of each cylinder is 2πx, and by Pythagorean theorem,
the height of each cylinder is 2√(r²-x²).
The area of each cylinder is then 4πx√(r²-x²),
its volume is 4πx√(r²-x²)dx,
its mass is s4πx√(r²-x²)dx,
and its angular momentum is ωs4πx³√(r²-x²)dx.
The angular momentum of the whole sphere is then the integral over all the cylinders.
Call the indefinite integral F(x), where
F(x) = ∫ωs4πx³√(r²-x²)dx = ωs4π∫x³√(r²-x²)dx
We solve the integral by parts using the formula
∫uv' = uv - ∫u'v
where
u = x², u' = 2x
v' = x√(r²-x²), v = (-1/3)(r²-x²)3/2
Thus
F(x)
= ωs4π ( (-1/3)x²(r²-x²)3/2 - ∫2x(-1/3)(r²-x²)3/2 dx )
= ωs4π ( (-1/3)x²(r²-x²)3/2 + (2/3) ∫x(r²-x²)3/2 dx )
= ωs4π ( (-1/3)x²(r²-x²)3/2 + (2/3)(-1/5)(r²-x²)5/2 )
= ωs4π ( (-1/3)x²(r²-x²)3/2 - (2/15)(r²-x²)5/2 )
The value of L' is the definite integral from 0 to r, i.e.,
L' = F(r) - F(0)
F(r) = ωs4π ( (-1/3)r²(r²-r²)3/2 - (2/15)(r²-r²)5/2 ) = 0
F(0) = ωs4π ( (-1/3)0²(r²)3/2 - (2/15)(r²)5/2 ) = -(8/15)ωsπr5
L' = (8/15)ωsπr5
In order to express it in terms of the mass M instead of density s we rewrite it as
L' = (2/5)ωr² × (4/3)sπr³ = (2/5)Mωr²
Thus
L = MωR² + (2/5)Mωr² = Mω(R² + 2r²/5)
Now applying it to your two spheres, and expressing ω in terms of your given velocity v:
L1 + L2 =
m1ω(R² + 2r²/5) + m2 ω(R² + 2r²/5) =
(m1+m2)ω(R² + 2r²/5) =
(m1+m2)(v/R)(R² + 2r²/5)
Substituting actual numbers
L1 + L2 = 7 × (5.8/0.5) × (0.5² + 2×0.145²/5) = 20.98

Daniel B.
04/25/21