ANSWER TO CHAPTER 8 HOMEWORK
1. (a) Because the force F = (-kx + ax3 + bx4) is a function only of position, it is conservative.
(b) We find the form of the potential energy function from
U = - ò F × dr = - ò (-kx + ax3 + bx4)i × (dxi + dyj + dzk)
= - ò (-kx + ax3 + bx4)dx = 1/2kx2 - 1/4ax4 - 1/5bx5 + constant.<
2. We choose the potential energy to be zero at the level of the center of mass before the jump (y = )). We find the minimum speed by ignoring any frictional forces. Energy is conserved, so we have
E = K1 + U1 = K2 + U2;
1/2mv12 + mgy1 = 1/2mv2 + mgy2;
1/2mv12 + m(9.80m/s2)(0) = 1/2m(0.70m/s)2 + m(9.80m/s2)(2.10m), which gives v1 = 6.5m/s.
Note that the initial velocity will not be horizontal, but will have a horizontal component of 0.70m/s.
4. On the level the normal force is FN = mg, so the friction force is Ffr = mkmg.
For the work-energy principle, we have
WNC = DK + DU = (1/2mvf2 - 1/2mvi2) + mg(hf - hi);
F(L1 + L2) - mkmgL2 = (1/2mvf2 - 0) + mg(0 - 0);
(350N)(15m + 15m) - (0.25)(90kg)(9.80m/s2)(15m) = 1/2(90kg)vf2,
which gives vf = 13m/s.
5. The escape velocity from a mass M, as determined by energy conservation, is from
vesc2 = 2GM/r.
(a) To escape from the the Sun's surface, we have
vesc2 = 2GMS/rS
= 2(6.67 x 10-11N.m2/kg2)(2.0 x 1030kg)/(7.0 x 108m),
which gives vesc = 6.2 x 105m/s.
(b) To escape from the Sun when at the Earth's location, we have
vesc2 = 2GMS/r
= 2(6.67 x 10-11N.m2/kg2)(2.0 x 1030kg)/(1.50 x 1011m),
which gives vesc = 4.2 x 104m/s.
Because the gravitational attraction provides the radial acceleration of the Earth, we have
GMSME/r2 = MEvorbit2/r, or v orbit2 = GMS/r.
for the ratio we get =
vesc2/vorbit2 = (2GMS/r)/(GMS/r), or vesc/vorbit = Ö2.
6. We find the average resistance force from the acceleration:
FR = ma = mDv/Dt = (1000kg)(70km/h - 90km/h)/(3.6ks/h)(60s) = -926N.
If we assume that this is the resistance force at 80km/h, the engine must provide an equal and opposite force to
maintain a constant speed. We find the power required from
P = Fv = (926N)(80km/h)/(3.6ks/h) = 2.1 x 104W = (2.1) x 104W)/(746W/hp) = 28hp.
x = (5.0m/s3)t3 - (8.0m/s2)t2 - (30m/s)t;
v = dx/dt = (15.0m/s3)t2 - (16.0m/s2)t - (30m/s);
a = dv/dt = (30.0m/s3)t - (16.0m/s3).
Thus the rate of work is
P = Fv = mav = m[(30.0m/s3)t - (16.0m/s2)][(15.0m/s3)t2 - (16.0m/s2)t - ((30m/s)].
(a) At t = 2.0s, we have
P = (0.280kg)[(30.0m/s3)(2.0s) - (16.0m/s2)][(15.0m/s3)(2.0s)2 - (16.0m/s2)(2.0s) - (30m/s))]
= - 25W.
(b) At t = 4.0s, we have
P = (0.280kg)[(30.0m/s3)(4.0s) - (16.0m/s2)][(15.0m/s3)(4.0s)2 - (16.0m/s2)(4.0s) - (30m/s))]
= + 4.3 x 103W.
(c) Over a time interval, the average net power produces the change in kinetic energy:
P = W/t = DK/Dt = (1/2mvf2 - 1/2mvi2)/Dt = 1/2m(vf2 - vi2)/Dt.
We find the velocities at the three times:
v0 = (15.0m/s3)(0)2 - (16.0m/s2)(0) - (30m/s) = - 30m/s;
v2 = (15.0m/s3)(2.0s)2 - (16.0m/s2)(2.0s) - (30m/s) = - 2.0m/s;
v4 = (15.0m/s3)(4.0s)2 - (16.0m/s2)(4.0s) - (30m/s) = 146m/s.
From t = 0 to t = 2.0s, we have
P = 1/2(0.280kg)[(-2.0m/s)2 - (-30m/s)2]/(2.0s - 0) = -63W.
From t = 2.0s to t = 4.0s, we have
P = 1/2(0.280kg)[(146m/s)2 - (-2.0m/s)2]/(4.0s - 2.0s) = + 1.5 x 103W.