Problem#1
An 8.00-kg point mass and a 15.0-kg point mass are held in place 50.0 cm apart. A particle of mass m is released from a point between the two masses 20.0 cm from the 8.00-kg mass along the line connecting the two fixed masses. Find the magnitude and direction of the acceleration of the particle.Answer:
Let +x be toward the 15.0 kg mass.
The magnitude of the interaction force between mass 3 and mass 1 and mass 2 is respectively
Fig.9 |
F31 = Gm1m3/r31² = (6.67 x 10⁻¹¹ Nm²/kg²)(8 kg)m3/(0.200 m)2 = 1.334 x 10⁻8 m3N/kg in the (─x) direction
F32 = Gm2m3/r32² = (6.67 x 10⁻¹¹ Nm²/kg²)(15 kg)m3/(0.400 m)2 = 1.112 x 10⁻8 m3N/kg in the (+x) direction
The net force is
Fnet,x = F31 + F32
Fnet,x = ─1.334 x 10⁻8 m3N/kg + 1.112 x 10⁻8 m3N/kg = ─2.2 x 10⁻8 m3N/kg
Using Newton’s second law,
ax = ∑Fnet,x/m3
ax = (─2.2 x 10⁻8 m3N/kg)/m3 = ─2.2 x 10⁻8 N/kg
Problem#2
In Fig. 10a, a square of edge length 20.0 cm is formed by four spheres of masses m1 = 5.00 g, m2 = 3.00 g, m3 = 1.00 g, and m4 = 5.00 g. In unit-vector notation, what is the net gravitational force from them on a central sphere with mass m5 = 2.50 g?
Fig.10 |
Answer:
From the superposition principle, we have:
Fnet = F51 + F52 + F53 + F54
The gravitational forces │F51│ = │F54│ on m5 from the two 5.00 g masses m1 and m4 cancel each other. Contributions to the net force on m5 come from the remaining two masses:
Fnet = F52 + F53
Fnet = Gm5m2/r522 + [─Gm5m3/r532]
Fnet = [Gm5/r522][m2 ─ m3]
Fnet = [(6.67 x 10⁻¹¹ Nm²/kg²)(2.50 x 10⁻3 kg)/(√2 x 10⁻1 m)2][3.00 x 10⁻3 kg ─ 1.00 x 10⁻3 kg]
Fnet = 1.67 x 10⁻¹4 N
The force is directed along the diagonal between m2 and m3, towards m2. In unit-vector notation, we have
Fnet = Fnet(cos 450i + cos 450j) = 1.18 x 10⁻¹4 N(i + j)
Problem#3
As seen in Fig. 11a, two spheres of mass m and a third sphere of mass M form an equilateral triangle, and a fourth sphere of mass m4 is at the center of the triangle. The net gravitational force on that entral sphere from the three other spheres is zero. (a) What is M in terms of m? (b) If we double the value of m4, what then is the magnitude of the net gravitational force on the central sphere?
Fnet = F51 + F52 + F53 + F54
The gravitational forces │F51│ = │F54│ on m5 from the two 5.00 g masses m1 and m4 cancel each other. Contributions to the net force on m5 come from the remaining two masses:
Fnet = F52 + F53
Fnet = Gm5m2/r522 + [─Gm5m3/r532]
Fnet = [Gm5/r522][m2 ─ m3]
Fnet = [(6.67 x 10⁻¹¹ Nm²/kg²)(2.50 x 10⁻3 kg)/(√2 x 10⁻1 m)2][3.00 x 10⁻3 kg ─ 1.00 x 10⁻3 kg]
Fnet = 1.67 x 10⁻¹4 N
The force is directed along the diagonal between m2 and m3, towards m2. In unit-vector notation, we have
Fnet = Fnet(cos 450i + cos 450j) = 1.18 x 10⁻¹4 N(i + j)
Problem#3
As seen in Fig. 11a, two spheres of mass m and a third sphere of mass M form an equilateral triangle, and a fourth sphere of mass m4 is at the center of the triangle. The net gravitational force on that entral sphere from the three other spheres is zero. (a) What is M in terms of m? (b) If we double the value of m4, what then is the magnitude of the net gravitational force on the central sphere?
Fig.11 |
Answer:
(a) The picture above shows all four masses and three gravitational forces acting from each of the masses to mass m4 . The choice of the coordinate axes is also shown in this picture. The net force acting on m4 is zero, which means that
∑Fx = 0 and ∑Fy = 0
Since both masses m are in symmetric positions with respect to mass m4 , they both provide the same components of forces in y-direction, and the same in magnitude but opposite in sign components in x-direction. Moreover, the force acting between m4 and M has only y-component, so the equation for the x-direction does not involve any unknowns and we do not need it to solve the problem. The only equation necessary is the equation for y-direction. Let r be the distance between the central sphere and any of the other three spheres. It is the same for all of them, since this is the equilateral triangle. This means that the gravitational force between the mass m4 and any of the masses m is
Fm = Gm4m/r2
and between mass m4 and mass M is
FM = Gm4M/r2
The equation for the forces' components in y-direction becomes
FM ─ 2Fmy = 0
(Gm4M/r2) ─ (2Gm4m/r2) cos 600 = 0
M ─ 2m x ½ = 0
So, M = m
(b) if one doubles mass m4 it will double all three gravitational forces acting on it. Since they all will change in proportional manner this will neither change their directions, nor the fact that they all are of the same magnitude. This means that the net gravitational force will stay zero in this case
Problem#4
Figure 12 shows a spherical hollow inside a lead sphere of radius R = 4.00 cm; the surface of the hollow passes through the center of the sphere and “touches” the right side of the sphere. The mass of the sphere before hollowing was M = 2.95 kg.With what gravitational force does the hollowed-out lead sphere attract a small sphere of mass m = 0.431 kg that lies at a distance d = 9.00 cm from the center of the lead sphere, on the straight line connecting the centers of the spheres and of the hollow?
∑Fx = 0 and ∑Fy = 0
Since both masses m are in symmetric positions with respect to mass m4 , they both provide the same components of forces in y-direction, and the same in magnitude but opposite in sign components in x-direction. Moreover, the force acting between m4 and M has only y-component, so the equation for the x-direction does not involve any unknowns and we do not need it to solve the problem. The only equation necessary is the equation for y-direction. Let r be the distance between the central sphere and any of the other three spheres. It is the same for all of them, since this is the equilateral triangle. This means that the gravitational force between the mass m4 and any of the masses m is
Fm = Gm4m/r2
and between mass m4 and mass M is
FM = Gm4M/r2
The equation for the forces' components in y-direction becomes
FM ─ 2Fmy = 0
(Gm4M/r2) ─ (2Gm4m/r2) cos 600 = 0
M ─ 2m x ½ = 0
So, M = m
(b) if one doubles mass m4 it will double all three gravitational forces acting on it. Since they all will change in proportional manner this will neither change their directions, nor the fact that they all are of the same magnitude. This means that the net gravitational force will stay zero in this case
Problem#4
Figure 12 shows a spherical hollow inside a lead sphere of radius R = 4.00 cm; the surface of the hollow passes through the center of the sphere and “touches” the right side of the sphere. The mass of the sphere before hollowing was M = 2.95 kg.With what gravitational force does the hollowed-out lead sphere attract a small sphere of mass m = 0.431 kg that lies at a distance d = 9.00 cm from the center of the lead sphere, on the straight line connecting the centers of the spheres and of the hollow?
Fig.12 |
Answer:
This is a job for negative mass. We take the force the solid sphere would exert, then subtract the force of the material which makes up the hollow. In effect, we treat the hollow as negative mass.
F = GMm/d2 – GMhm/(d − R/2)2
Since the radius of the hollow region is half of that of the sphere, we obtain for Mh:
Mh =ρ⋅4π/3⋅(R/2)3= M/8
Finally, we obtain:
F = GMm/d2 – G(M/8)m/(d − R/2)2
F = GMm[1/d2− ½(2d − R)2]
F = (6.67 x 10⁻¹¹ Nm²/kg²)(2.95 kg)(0.431 kg)[1/(0.09 m)2− ½(2 x 0.09 m – 0.04 m)2]
F = 8.31 × 10−9 N
Problem#5
A solid sphere of mass m and radius r is placed inside a hollow thin spherical shell of mass M and radius R as shown in figure (13). A particle of mass m' is placed on the line joining the two centers at a distance x from the point of contact of the sphere and the shell. Find the magnitude of the resultant gravitational force on this particle due to the sphere and the shell if (a) r < x < 2r, (b) 2r < x < 2R and
(c) x > 2R.
F = GMm/d2 – GMhm/(d − R/2)2
Since the radius of the hollow region is half of that of the sphere, we obtain for Mh:
Mh =ρ⋅4π/3⋅(R/2)3= M/8
Finally, we obtain:
F = GMm/d2 – G(M/8)m/(d − R/2)2
F = GMm[1/d2− ½(2d − R)2]
F = (6.67 x 10⁻¹¹ Nm²/kg²)(2.95 kg)(0.431 kg)[1/(0.09 m)2− ½(2 x 0.09 m – 0.04 m)2]
F = 8.31 × 10−9 N
Problem#5
A solid sphere of mass m and radius r is placed inside a hollow thin spherical shell of mass M and radius R as shown in figure (13). A particle of mass m' is placed on the line joining the two centers at a distance x from the point of contact of the sphere and the shell. Find the magnitude of the resultant gravitational force on this particle due to the sphere and the shell if (a) r < x < 2r, (b) 2r < x < 2R and
(c) x > 2R.
Fig.13 |
Answer:
For situations in (a) and (b) x < 2R, the shell does not force the particle m'
(a) if r < x < 2r (Fig.14a)
The distance of the particle m' from the center of the solid sphere d = x - r
The resultant gravitational force on m' will be the force due to the solid sphere of radius s = x – r
F = Gmm'd/r³
F = Gmm'(x – r)/r³
(b) If 2r < x < 2R (Fig.14b)
In this case, the particle m' is between the space of the solid sphere and the shell. The resultant gravitational force on the particle will be due to the solid sphere only and its magnitude will be
F = Gmm'/d², here d = x - r, the distance of the particle from the center of the solid sphere
F = Gmm'/(x – r)²
(c) If x > 2R, (Fig.14c)
Now both the shell and the solid sphere will exert the gravitational force on the particle m'. The masses of the sphere and the shell will be assumed to be concentrated at their respective centers.
Force by the solid sphere:
The distance of the particle from the center of the solid sphere is d = x - r
Hence force
F = Gmm'/s² = Gmm'/(x – r)²
Force by the shell:
The distance of the particle from the center of the shell
s = x – R
Hence force
F = GMm'/s²
F = GMm'/(x – R)²
Since both of these forces are in the same direction (towards the line joining two centers) hence the magnitude of the resultant force will be added, i.e.
The resultant gravitational force on m'
F = Gmm'/(x – r)² + GMm'/(x – R)²
F = Gm’[m/(x – r)² + GM/(x – R)²]
(a) if r < x < 2r (Fig.14a)
The distance of the particle m' from the center of the solid sphere d = x - r
The resultant gravitational force on m' will be the force due to the solid sphere of radius s = x – r
F = Gmm'd/r³
F = Gmm'(x – r)/r³
(b) If 2r < x < 2R (Fig.14b)
In this case, the particle m' is between the space of the solid sphere and the shell. The resultant gravitational force on the particle will be due to the solid sphere only and its magnitude will be
F = Gmm'/d², here d = x - r, the distance of the particle from the center of the solid sphere
F = Gmm'/(x – r)²
(c) If x > 2R, (Fig.14c)
Fig.14 |
Force by the solid sphere:
The distance of the particle from the center of the solid sphere is d = x - r
Hence force
F = Gmm'/s² = Gmm'/(x – r)²
Force by the shell:
The distance of the particle from the center of the shell
s = x – R
Hence force
F = GMm'/s²
F = GMm'/(x – R)²
Since both of these forces are in the same direction (towards the line joining two centers) hence the magnitude of the resultant force will be added, i.e.
The resultant gravitational force on m'
F = Gmm'/(x – r)² + GMm'/(x – R)²
F = Gm’[m/(x – r)² + GM/(x – R)²]
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