Problem 13.151* From astronomical data, Kepler
deduced that the line from the sun to a planet traces out
equal areas in equal times (Fig. a). Show that this result
follows from the fact that the transverse component aθof
the planet’s acceleration is zero. [When rchanges by an
amount dr and θchanges by an amount dθ (Fig. b), the
resulting differential element of area is dA =1
2r(rdθ)].
(a)
t2 +
∆
tt1 +
∆
t
t1
t2
A
A
Solution: From the solution to Problem 13.150, aθ=0 implies
Problem 13.152 The bar rotates in the x–yplane with
constant angular velocity ω0=12 rad/s. The radial com-
ponent of acceleration of the collar C(in m/s2) is given
as a function of the radial position in meters by ar=
−8r. When r=1 m, the radial component of velocity
of Cis vr=2 m/s. Determine the velocity of Cin terms
of polar coordinates when r=1.5 m.
Strategy: Use the chain rule to write the first term in
the radial component of the acceleration as
d2r
dt2=dvr
dt =dvr
dr
dr
dt =dvr
dr vr
y
r
C
v0
Solution: We have