Faculty of Mechanical EngineeringEngineering Computing Panel
MKMM 1213 Advanced Engineering Mathematics
Vector-Valued Functions and Motion in Space
Abu Hasan Abdullah
April 2015
noone�dev.null MKMM 1213 Advanced Engineering Mathematics Vector-Valued Functions & Motion 1 / 32
Outline I
1 Curves in Space and Their Tangents
Overview
Limits and Continuity
Derivatives and Motion
Differentiation Rules
Vector Functions of Constant Length
2 Integrals of Vector Functions; Projectile Motion
Integrals of Vector Functions
3 Arc Length in Space
Arc Length Along a Space Curve
Speed on a Smooth Curve & Unit Tangent Vector
4 Curvature and Normal Vectors of a Curve
Curvature of a Plane Curve
5 Curvature and Normal Vectors of a Curve
6 Tangential and Normal Components of Acceleration
7 Velocity and Acceleration in Polar Coordinates
Motion in Polar and Cylindrical Coordinates
Planets Move in Planes
8 Bibliographynoone�dev.null MKMM 1213 Advanced Engineering Mathematics Vector-Valued Functions & Motion 2 / 32
Curves in Space and Their TangentsOverview
When a particle moves through space
during a time interval I, we think of the
particle’s coordinates as functions defined
on I:
x = f(t), y = g(t), z = h(t), t ∈ I. (1)
The points (x, y, z) = (f(t), g(t), h(t)), t ∈ I,
make up the curve in space that we call the
particle’s path. The equations and interval
in Eq. (1) parametrize the curve.
A curve in space can also be represented in
vector form:
r(t) =⇀
OP = f(t)i + g(t)j + h(t)k (2)
from the origin to the particle’s position
P(f(t), g(t), h(t)) at time t is the particle’s
position vector—see Figure 1).
Figure 1: The position vector r =
⇀OP of a
particle moving through space is afunction of time.
noone�dev.null MKMM 1213 Advanced Engineering Mathematics Vector-Valued Functions & Motion 3 / 32
Curves in Space and Their TangentsOverview
The functions f , g, and h are the
component functions (components)
of the position vector. We think of
the particle’s path as the curve
traced by r during the time interval
I.
Eq. (2) defines r as a vector function
of the real variable t on the interval
I. More generally, a vector-valued
function or vector function on a
domain set D is a rule that assigns a
vector in space to each element in D.
For now, the domains will be
intervals of real numbers resulting
in a space curve.
When the domains are regions in
the plane, vector functions will then
represent surfaces in space.
Vector functions on a domain in the
plane or space also give rise to
vector fields, which are important to
the study of the flow of a fluid,
gravitational fields, and
electromagnetic phenomena.
Real-valued functions are called scalar functions to distinguish them from vector
functions. The components of r in Eq. (2) are scalar functions of t. The domain of a
vector-valued function is the common domain of its components.noone�dev.null MKMM 1213 Advanced Engineering Mathematics Vector-Valued Functions & Motion 4 / 32
Curves in Space and Their TangentsLimits and Continuity
DEFINITION: Limits of vector-valued functions
Let r = f(t)i + g(t)j + h(t)k be a vector function with domain D, and L a vector.
We say that r has limit L as t approaches t0 and write
limt→t0
r(t) = L
if, for every number ǫ > 0, there exists a corresponding number δ > 0 such that
for all t ∈ D
|r(t) − L| < ǫ whenever 0 < |t − t0| < δ.
If L = L1i + L2j + L3k, then it can be shown that limt→t0 r(t) = L precisely when
limt→t0
f(t) = L1, limt→t0
g(t) = L2, and limt→t0
h(t) = L3
Omitting the the proof (for now), the equation
limt→t0
r(t) =
„
limt→t0
f(t)
«
i +
„
limt→t0
g(t)
«
j +
„
limt→t0
h(t)
«
k (3)
provides a practical way to calculate limits of vector functions.noone�dev.null MKMM 1213 Advanced Engineering Mathematics Vector-Valued Functions & Motion 5 / 32
Curves in Space and Their TangentsLimits and Continuity
DEFINITION: Continuity for vector functions
A vector function r(t) is continuous at a point t = t0 in its domain if limt→t0 r(t) =r(t0). The function is continuous if it is continuous at every point in its domain.
From Eq. (3), we see that r(t) is continuous at t = t0 if and only if each component
function is continuous there.
Example 1:
Graph the vector function
r(t) = (cos t)i + (sin t)j + tk
Example 2:
If r = (cos t)i + (sin t)j + tk, find
limt→π/4 r(t).
Example 3:
The function
g(t) = (cos t)i + (sin t)j + tk
is discontinuous at every integer,
where the greatest integer function t
is discontinuous.noone�dev.null MKMM 1213 Advanced Engineering Mathematics Vector-Valued Functions & Motion 6 / 32
Curves in Space and Their TangentsDerivatives and Motion
Suppose that r(t) = f(t)i + g(t)j + h(t)k is the position vector of a particle moving
along a curve in space and that f , g, and h are differentiable functions of t. Then
the difference between the particle’s positions at time t and time t + ∆t is
∆r = r(t + ∆t) − r(t)
Figure 2: Derivative of a vector function.
In terms of components,
∆r = r(t + ∆t) − r(t)
= [ f(t + ∆t)i + g(t + ∆t)j + h(t + ∆t)k] − [ f(t)i + g(t)j + h(t)k]noone�dev.null MKMM 1213 Advanced Engineering Mathematics Vector-Valued Functions & Motion 7 / 32
Curves in Space and Their TangentsDerivatives and Motion
The quotient ∆r/∆t approaches the limit
lim∆t→0
∆r
∆t=
»
f(t + ∆t)f(t)
∆t
–
i +
»
g(t + ∆t)g(t)
∆t
–
j +
»
h(t + ∆t)h(t)
∆t
–
k
=
»
df
dt
–
i +
»
dg
dt
–
j +
»
dh
dt
–
k
Figure 3: Derivative of a vector function.noone�dev.null MKMM 1213 Advanced Engineering Mathematics Vector-Valued Functions & Motion 8 / 32
Curves in Space and Their TangentsDerivatives and Motion
DEFINITION: Derivative of a vector function
The vector function r(t) = f(t)i + g(t)j + h(t)k has a derivative (is differentiable)
at t if f , g, and h have derivatives at t. The derivative is the vector function
r′(t) =dr
dt= lim
∆t→0
r(t + ∆t) − r(t)
∆t=
df
dti +
dg
dtj +
dh
dtk
A vector function r is differentiable if it is differentiable at every point of its
domain. The curve traced by r is smooth if dr/dt is continuous and never 0, that is,
if f , g, and h have continuous first derivatives that are not simultaneously 0.
The vector r′(t), when different from 0, is defined to be the vector tangent to the
curve at P. The tangent line to the curve at a point f(t0), g(t0), h(t0) is defined to
be the line through the point parallel to r′(t0).
noone�dev.null MKMM 1213 Advanced Engineering Mathematics Vector-Valued Functions & Motion 9 / 32
Curves in Space and Their TangentsDerivatives and Motion
We require dr/dt 6= 0 for a smooth
curve to make sure the curve has a
continuously turning tangent at
each point.
On a smooth curve, there are no
sharp corners or cusps!
A curve that is made up of a finite
number of smooth curves pieced
together in a continuous fashion is
called piecewise smooth (Figure 4).Figure 4: A piecewise smooth curve made upof five smooth curves connected end to end ina continuous fashion. The curve here is notsmooth at the points joining the five smoothcurves.
noone�dev.null MKMM 1213 Advanced Engineering Mathematics Vector-Valued Functions & Motion 10 / 32
Curves in Space and Their TangentsDerivatives and Motion
DEFINITION: Velocity & Acceleration
If r is the position vector of a particle moving along a smooth curve in space, then
v(t) =dr
dt
is the particle’s velocity vector, tangent to the curve. At any time t, the direction
of v is the direction of motion, the magnitude of v is the particle’s speed, and
the derivative a = dv/dt, when it exists, is the particle’s acceleration vector. In
summary,
1 Velocity is the derivative of position: v =dr
dt.
2 Speed is the magnitude of velocity: Speed = |v|.
3 Acceleration is the derivative of velocity: a =dv
dt=
d2r
dt2.
4 The unit vector v/|v| is the direction of motion at time t.noone�dev.null MKMM 1213 Advanced Engineering Mathematics Vector-Valued Functions & Motion 11 / 32
Curves in Space and Their TangentsDerivatives and Motion
Example 4:
Find the velocity, speed, and acceleration of
a particle whose motion in space is given
by the position vector
r(t) = 2 cos ti + 2 sin tj + 5 cos 2tk.
Sketch the velocity vector v(7π/4).
Figure 5: The curve and the velocityvector when t = 7π/4 for the motion givenin Example 4.
noone�dev.null MKMM 1213 Advanced Engineering Mathematics Vector-Valued Functions & Motion 12 / 32
Curves in Space and Their TangentsDifferentiation Rules
Let u and v be differentiable vector functions of t, C a constant vector, c any scalar, and f
any differentiable scalar function.
Constant Function Rule:
d
dtC = 0
Scalar Multiple Rule:
d
dt[cu(t)] = cu′(t)
d
dt[ f(t)u(t)] = f
′(t)u(t) + f(t)u′(t)
Sum Rule:
d
dt[u(t) + v(t)] = u′(t) + v′(t)noone�dev.null MKMM 1213 Advanced Engineering Mathematics Vector-Valued Functions & Motion 13 / 32
Curves in Space and Their TangentsDifferentiation Rules
Continued . . .
Difference Rule:
d
dt[u(t) − v(t)] = u′(t) − v′(t)
Dot Product Rule:
d
dt[u(t) · v(t)] = u′(t) · v(t) − u(t) · v′(t)
Cross Product Rule:
d
dt[u(t) × v(t)] = u′(t) × v(t) − u(t) × v′(t)
Chain Rule:
d
dt[u(f(t))] = f
′(t)u′(f(t)t)noone�dev.null MKMM 1213 Advanced Engineering Mathematics Vector-Valued Functions & Motion 14 / 32
Curves in Space and Their TangentsVector Functions of Constant Length
Continued . . .
For a particle moving on a sphere,
Figure 6, the position vector has a
constant length equal to the radius of
the sphere. The velocity vector dr/dt,
tangent to the path of the motion, is
tangent to the sphere and hence
perpendicular to r.
The vector and its first derivative are
orthogonal. By direct calculation
r(t) · r(t) = c2
d
dt[r(t) · r(t)] = 0
r′(t) · r(t) + r(t) · r′(t) = 0
2r′(t) · r(t) = 0
Figure 6: Particle moving on a sphere.
The vectors r′(t) and r(t) are
orthogonal because their dot product
is 0. In summary,
r · dr
dt= 0 (4)noone�dev.null MKMM 1213 Advanced Engineering Mathematics Vector-Valued Functions & Motion 15 / 32
Integrals of Vector Functions; Projectile MotionIntegrals of Vector Functions
A differentiable vector function R(t) is an antiderivative of a vector function r(t) on
an interval I if dR/dt = r at each point of I.
DEFINITION: Indefinite Integral
The indefinite integral of r with respect to t is the set of all antiderivatives of r,
denoted byR
r(t)dt. If R is any antiderivative of r, then
Z
r(t)dt = R(t) + C
Example 1:
To integrate a vector function, we integrate each of its components.
Z
((cos t)i + j − 2tk)dt =
„
Z
cos tdt
«
i +
„
Z
dt
«
j −„
Z
2tdt
«
k
= (sin t + C1)i + (t + C2)j − (t2 + C3)k
= (sin t)i + tj − t2k + Cnoone�dev.null MKMM 1213 Advanced Engineering Mathematics Vector-Valued Functions & Motion 16 / 32
Integrals of Vector Functions; Projectile MotionIntegrals of Vector Functions
DEFINITION: Definite Integral
If the components of r(t) = f(t)i + g(t)j + h(t)k are integrable over [a, b], then so
is r, and the definite integral of r from a to b is
Z b
a
r(t)dt =
„
Z b
a
f(t)dt
«
i +
„
Z b
a
g(t)dt
«
j +
„
Z b
a
h(t)dt
«
k
Example 2:As in Example 1, we integrate each component.
Z π
0
((cos t)i + j − 2tk)dt =
„
Z π
0
cos t dt
«
i +
„
Z π
0
dt
«
j −„
Z π
0
2t dt
«
k
= [sin t]π0 i + [t]π0 j −h
t2iπ
0k
= [0 − 0] i + [π − 0] j −h
π2 − 02i
k
= πj − π2knoone�dev.null MKMM 1213 Advanced Engineering Mathematics Vector-Valued Functions & Motion 17 / 32
Integrals of Vector Functions; Projectile MotionIntegrals of Vector Functions
Example 3:
Suppose we do not know the path of a
hang glider, but only its acceleration
vector:
a(t) = −(3 cos t)i − (3 sin t)j + 2k.
We also know that initially (at time
t = 0) the glider departed from the
point (4, 0, 0) with velocity v(0) = 3j.Find the glider’s position as a function
of t.
Figure 7: Flight path of a hang glider.
noone�dev.null MKMM 1213 Advanced Engineering Mathematics Vector-Valued Functions & Motion 18 / 32
Arc Length in SpaceArc Length Along a Space Curve
Smooth space and plane curves have a
measurable length, thus allowing us
to locate points along these curves by
giving their directed distance s along
the curve from some base point, see
Figure 8. Figure 8: Arc length of a curve.
DEFINITION: Arc Length of a Curve
The length of a smooth curve r(t) = x(t)i + y(t)j + z(t)k, a ≤ t ≤ b, that is traced
exactly once as t increases from t = a to t = b, is
L =
Z b
a
s
„
dx
dt
«2
+
„
dy
dt
«2
+
„
dz
dt
«2
dt (5)
The square root in Eq. 5 is |v|, i.e. the length of a velocity vector dr/dt, thus
L =
Z b
a
|v|dt (6)noone�dev.null MKMM 1213 Advanced Engineering Mathematics Vector-Valued Functions & Motion 19 / 32
Arc Length in SpaceArc Length Along a Space Curve
Example 1:
A glider is soaring upward along the
helix
r(t) = (cos t)i + (sin t)j + tk
Figure 9. How long is the glider’s path
from t = 0 to t = 2π?
Figure 9: A helix.
noone�dev.null MKMM 1213 Advanced Engineering Mathematics Vector-Valued Functions & Motion 20 / 32
Arc Length in SpaceArc Length Along a Space Curve
If we choose a base point P(t0) on a
smooth curve C parametrized by t,
each value of t determines a point
P(t) = (x(t), y(t), z(t)) on C and a
directed distance
s(t) =
Z t
to
|v(τ )| dτ (7)
measured along C from point P(t0). Figure 10: The directed distance.
If t > t0, s(t) is the distance along the curve from P(t0) to P(t). If t < t0, s(t) is the
negative of the distance.
Each value of s determines a point on C, and this parametrizes C with respect to s.
We call s an arc length parameter for the curve.
s(t) =
Z t
to
p
[ x′(τ )]2 + [ y′(τ )]2 + [ z′(τ )]2 =
Z t
to
|v(τ )| dτ (8)noone�dev.null MKMM 1213 Advanced Engineering Mathematics Vector-Valued Functions & Motion 21 / 32
Arc Length in SpaceArc Length Along a Space Curve
Example 2:
This is a continuation of Example 1 for which we can actually find the arc length
parametrization of a curve. If t0 = 0, the arc length parameter along the helix
r(t) = (cos t)i + (sin t)j + tk
from t0 to t is
s(t) =
Z t
to
|v(τ )|dτ =
Z t
0
√2 dτ =
√2 t
Solving this equation for t gives t = s/√
2. Substituting into the position vector r
gives the following arc length parametrization for the helix:
r(t(s)) =
„
coss√2
«
i +
„
sins√2
«
j +
„
s√2
«
k
P.S.: Unlike this example, the arc length parametrization is generally difficult to find analytically for a
curve already given in terms of some other parameter t.noone�dev.null MKMM 1213 Advanced Engineering Mathematics Vector-Valued Functions & Motion 22 / 32
Arc Length in SpaceSpeed on a Smooth Curve & Unit Tangent Vector
The arc length s is a differentiable function of t with derivative
ds
dt= |v(t)| (9)
Eq. 9 is the speed with which a particle moves along its path is the magnitude of v.
The velocity vector v = dr/dt is
tangent to the curve r(t) and that the
vector
T =v
|v|ds
dt= |v(t)| (10)
is the unit tangent vector, Figure 11.
Figure 11: Unit tangent vector.noone�dev.null MKMM 1213 Advanced Engineering Mathematics Vector-Valued Functions & Motion 23 / 32
Arc Length in SpaceSpeed on a Smooth Curve & Unit Tangent Vector
Example 3:
Find the unit tangent vector of the
curve
r(t) = (1 + 3 cos t)i + (3 sin t)j + t2k
representing the path of a glider.
Figure 12: Counterclockwise motion aroundthe unit circle.
noone�dev.null MKMM 1213 Advanced Engineering Mathematics Vector-Valued Functions & Motion 24 / 32
Arc Length in SpaceSpeed on a Smooth Curve & Unit Tangent Vector
The velocity vector is the change in the position vector r with respect to time t, but
how does the position vector change with respect to arc length, s? More precisely,
what is the derivative dr/ds?
Since ds/dt > 0 for the curves we are considering, s is one-to-one and The
derivative of the inverse is
dt
ds=
1
ds/dt=
1
|v|
This makes r a differentiable function of s whose derivative can be calculated with
the Chain Rule to be
dr
ds=
dr
dt
dt
ds= v
1
|v| =v
|v| = T (11)
noone�dev.null MKMM 1213 Advanced Engineering Mathematics Vector-Valued Functions & Motion 25 / 32
Curvature and Normal Vectors of a CurveCurvature of a Plane Curve
As a particle moves along a smooth
curve in the plane, T = dr/ds turns as
the curve bends. Since T is a unit
vector, its length remains constant
and only its direction changes as the
particle moves along the curve. See
Figure 13.Figure 13: Curvature of a curve.
DEFINITION: Curvature
Curvature, κ, is the rate at which T turns per unit of length along the curve,
κ =
˛
˛
˛
˛
dT
ds
˛
˛
˛
˛
If dT/ds is large, T turns sharply and the curvature at P is large. If dT/ds is close to
zero, T turns more slowly and the curvature at P is smaller.noone�dev.null MKMM 1213 Advanced Engineering Mathematics Vector-Valued Functions & Motion 26 / 32
Velocity and Acceleration in Polar CoordinatesMotion in Polar and Cylindrical Coordinates
When a particle at P(r, θ) moves along
a curve in the polar coordinate plane,
we express its position, velocity, and
acceleration in terms of the moving
unit vectors
ur = (cos θ)i + (sin θ)j (12a)
uθ = −(sin θ)i + (sin θ)j (12b)
See Figure 14.
We differentiate ur and uθ with
respect to θ to get
dur
dθ= −(sin θ)i + (cos θ)j
duθ
dθ= −(cos θ)i − (cos θ)j
Figure 14: Position vector in polar coordinates.
We differentiate ur and uθ with
respect to t to see how they change
with time
ur =dur
dθθ = θuθ (13a)
uθ =duθ
dθθ = −θur (13b)noone�dev.null MKMM 1213 Advanced Engineering Mathematics Vector-Valued Functions & Motion 27 / 32
Velocity and Acceleration in Polar CoordinatesMotion in Polar and Cylindrical Coordinates
The velocity vector is expressed in
terms of ur and uθ as
v = r =d
dt(rur)
= rur + rur
= rur + rθuθ
See Figure 15.
The acceleration is
a = v
= (rur + rur) + (rθuθ + rθuθ + rθuθ)
Figure 15: Velocity vector in polar coordinates.
Acceleration in terms of ur and uθ is
a = (r − rθ2)ur + (rθ + 2rθ)uθ.
noone�dev.null MKMM 1213 Advanced Engineering Mathematics Vector-Valued Functions & Motion 28 / 32
Velocity and Acceleration in Polar CoordinatesMotion in Polar and Cylindrical Coordinates
To extend these equations of motion to space, we add zk to the right-hand side of
the equation r = rur. Then, in cylindrical coordinates, we have
r = rur + zk (14a)
v = rur + rθuθ + zk (14b)
a = (r − rθ2)ur + (rθ + 2rθ)uθ + zk (14c)
The vectors ur, uθ, and k make a
right-handed frame in which
ur × uθ = k, uθ × k = ur, k × ur = uθ.
See Figure 16.
Figure 16: Position vector and basic unitvectors in cylindrical coordinates.noone�dev.null MKMM 1213 Advanced Engineering Mathematics Vector-Valued Functions & Motion 29 / 32
Velocity and Acceleration in Polar CoordinatesPlanets Move in Planes
Newton’s law of gravitation says that if r is
the radius vector from the centre of a sun
of mass M to the center of a planet of mass
m, then the force F of the gravitational
attraction between the planet and sun is
F = −GmM
|r2|r
|r|
where G ≈ 6.6726× 10−11 Nm2 kg−2 is the
universal gravitational constant. See
Figure 17.
Combining the gravitation law with
Newton’s second law, F = mr, for the force
acting on the planet gives
mr = −GmM
|r2|r
|r| =⇒ r = −GM
|r2|r
|r|
Figure 17: The force of gravity is directedalong the line joining the centers of mass.
The planet is accelerated toward
the sun’s center of mass at all
times.
noone�dev.null MKMM 1213 Advanced Engineering Mathematics Vector-Valued Functions & Motion 30 / 32
Velocity and Acceleration in Polar CoordinatesPlanets Move in Planes
Since r is a scalar multiple of r, we have
r × r = 0.
and from this
d
dt(r × r) = r × r + r × r = r × r = 0.
It follows that
r × r = C (15)
for some constant vector C.
Eq. (15) tells us that r and r always lie in a
plane perpendicular to C. Hence, the planet
moves in a fixed plane through the center
of its sun. See Figure 18.
Figure 18: A planet that obeys Newton’slaws of gravitation and motion travels inthe plane through the sun’s center of mass.
The planet is accelerated toward
the sun’s center of mass at all
times.
noone�dev.null MKMM 1213 Advanced Engineering Mathematics Vector-Valued Functions & Motion 31 / 32
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noone�dev.null MKMM 1213 Advanced Engineering Mathematics Vector-Valued Functions & Motion 32 / 32