11 PARAMETRICEQUATIONS AND ET 10 POLAR...
Transcript of 11 PARAMETRICEQUATIONS AND ET 10 POLAR...
11 PARAMETRIC EQUATIONS AND ET 10POLAR COORDINATES
11.1 Curves Defined by Parametric Equations ET 10.1
1. x = 1 +√t, y = t2 − 4t, 0 ≤ t ≤ 5
t 0 1 2 3 4 5
x 1 2 1 +√2
2.41
1 +√3
2.73
3 1 +√5
3.24
y 0 −3 −4 −3 0 5
3. x = 5 sin t, y = t2, −π ≤ t ≤ π
t −π −π/2 0 π/2 π
x 0 −5 0 5 0
y π2
9.87
π2/4
2.47
0 π2/4
2.47
π2
9.87
5. x = 3t− 5, y = 2t+ 1
(a)t −2 −1 0 1 2 3 4
x −11 −8 −5 −2 1 4 7
y −3 −1 1 3 5 7 9
(b) x = 3t− 5 ⇒ 3t = x+ 5 ⇒ t = 13(x+ 5) ⇒
y = 2 · 13(x+ 5) + 1, so y = 2
3x+ 13
3.
7. x = t2 − 2, y = 5− 2t, −3 ≤ t ≤ 4(a)
t −3 −2 −1 0 1 2 3 4
x 7 2 −1 −2 −1 2 7 14
y 11 9 7 5 3 1 −1 −3
(b) y = 5− 2t ⇒ 2t = 5− y ⇒ t = 12(5− y) ⇒
x = 12 (5− y)
2 − 2, so x = 14 (5− y)2 − 2, −3 ≤ y ≤ 11.
1
2 ¤ CHAPTER 11 PARAMETRIC EQUATIONS AND POLAR COORDINATES ET CHAPTER 10
9. x =√t, y = 1− t
(a)t 0 1 2 3 4
x 0 1 1.414 1.732 2
y 1 0 −1 −2 −3
(b) x =√t ⇒ t = x2 ⇒ y = 1− t = 1− x2. Since t ≥ 0, x ≥ 0.
So the curve is the right half of the parabola y = 1− x2.
11. (a) x = sin θ, y = cos θ, 0 ≤ θ ≤ π. x2 + y2 = sin2 θ + cos2 θ = 1. Since
0 ≤ θ ≤ π, we have sin θ ≥ 0, so x ≥ 0. Thus, the curve is the right half ofthe circle x2 + y2 = 1.
(b)
13. (a) x = sin t, y = csc t, 0 < t < π2. y = csc t = 1
sin t=1
x. For 0 < t < π
2,
we have 0 < x < 1 and y > 1. Thus, the curve is the portion
of the hyperbola y = 1/x with y > 1.
(b)
15. (a) x = e2t ⇒ 2t = lnx ⇒ t = 12lnx.
y = t+ 1 = 12 lnx+ 1.
(b)
17. (a) x = sinh t, y = cosh t ⇒ y2 − x2 = cosh2 t− sinh2 t = 1. Sincey = cosh t ≥ 1, we have the upper branch of the hyperbola y2 − x2 = 1.
(b)
19. x = 3 + 2 cos t, y = 1 + 2 sin t, π/2 ≤ t ≤ 3π/2. By Example 4 with r = 2, h = 3, and k = 1, the motion of the particle
takes place on a circle centered at (3, 1) with a radius of 2. As t goes from π2 to
3π2 , the particle starts at the point (3, 3) and
moves counterclockwise to (3,−1) [one-half of a circle].
21. x = 5 sin t, y = 2cos t ⇒ sin t =x
5, cos t = y
2. sin2 t+ cos2 t = 1 ⇒ x
5
2
+y
2
2
= 1. The motion of the
particle takes place on an ellipse centered at (0, 0). As t goes from−π to 5π, the particle starts at the point (0,−2) and movesclockwise around the ellipse 3 times.
SECTION 11.1 CURVES DEFINED BY PARAMETRIC EQUATIONS ET SECTION 10.1 ¤ 3
23. We must have 1 ≤ x ≤ 4 and 2 ≤ y ≤ 3. So the graph of the curve must be contained in the rectangle [1, 4] by [2, 3].
25. When t = −1, (x, y) = (0,−1). As t increases to 0, x decreases to −1 and yincreases to 0. As t increases from 0 to 1, x increases to 0 and y increases to 1.
As t increases beyond 1, both x and y increase. For t < −1, x is positive anddecreasing and y is negative and increasing. We could achieve greater accuracy
by estimating x- and y-values for selected values of t from the given graphs and
plotting the corresponding points.
27. When t = 0 we see that x = 0 and y = 0, so the curve starts at the origin. As t
increases from 0 to 12, the graphs show that y increases from 0 to 1 while x
increases from 0 to 1, decreases to 0 and to −1, then increases back to 0, so wearrive at the point (0, 1). Similarly, as t increases from 1
2to 1, y decreases from 1
to 0 while x repeats its pattern, and we arrive back at the origin. We could achieve greater accuracy by estimating x- and
y-values for selected values of t from the given graphs and plotting the corresponding points.
29. As in Example 6, we let y = t and x = t− 3t3 + t5 and use a t-interval of [−3, 3].
31. (a) x = x1 + (x2 − x1)t, y = y1 + (y2 − y1)t, 0 ≤ t ≤ 1. Clearly the curve passes through P1(x1, y1) when t = 0 andthrough P2(x2, y2) when t = 1. For 0 < t < 1, x is strictly between x1 and x2 and y is strictly between y1 and y2. For
every value of t, x and y satisfy the relation y − y1 =y2 − y1x2 − x1
(x− x1), which is the equation of the line through
P1(x1, y1) and P2(x2, y2).
Finally, any point (x, y) on that line satisfies y − y1y2 − y1
=x− x1x2 − x1
; if we call that common value t, then the given
parametric equations yield the point (x, y); and any (x, y) on the line between P1(x1, y1) and P2(x2, y2) yields a value of
t in [0, 1]. So the given parametric equations exactly specify the line segment from P1(x1, y1) to P2(x2, y2).
(b) x = −2 + [3− (−2)]t = −2 + 5t and y = 7 + (−1− 7)t = 7− 8t for 0 ≤ t ≤ 1.
33. The circle x2 + (y − 1)2 = 4 has center (0, 1) and radius 2, so by Example 4 it can be represented by x = 2cos t,y = 1 + 2 sin t, 0 ≤ t ≤ 2π. This representation gives us the circle with a counterclockwise orientation starting at (2, 1).
(a) To get a clockwise orientation, we could change the equations to x = 2cos t, y = 1− 2 sin t, 0 ≤ t ≤ 2π.(b) To get three times around in the counterclockwise direction, we use the original equations x = 2 cos t, y = 1+ 2 sin t with
the domain expanded to 0 ≤ t ≤ 6π.
4 ¤ CHAPTER 11 PARAMETRIC EQUATIONS AND POLAR COORDINATES ET CHAPTER 10
(c) To start at (0, 3) using the original equations, we must have x1 = 0; that is, 2 cos t = 0. Hence, t = π2 . So we use
x = 2cos t, y = 1 + 2 sin t, π2≤ t ≤ 3π
2.
Alternatively, if we want t to start at 0, we could change the equations of the curve. For example, we could use
x = −2 sin t, y = 1 + 2 cos t, 0 ≤ t ≤ π.
35. Big circle: It’s centered at (2, 2) with a radius of 2, so by Example 4, parametric equations are
x = 2 + 2 cos t, y = 2 + 2 sin t, 0 ≤ t ≤ 2π
Small circles: They are centered at (1, 3) and (3, 3) with a radius of 0.1. By Example 4, parametric equations are
(left) x = 1+ 0.1 cos t, y = 3+ 0.1 sin t, 0 ≤ t ≤ 2πand (right) x = 3+ 0.1 cos t, y = 3+ 0.1 sin t, 0 ≤ t ≤ 2π
Semicircle: It’s the lower half of a circle centered at (2, 2) with radius 1. By Example 4, parametric equations are
x = 2 + 1 cos t, y = 2 + 1 sin t, π ≤ t ≤ 2π
To get all four graphs on the same screen with a typical graphing calculator, we need to change the last t-interval to [0, 2π] in
order to match the others. We can do this by changing t to 0.5t. This change gives us the upper half. There are several ways to
get the lower half—one is to change the “+” to a “−” in the y-assignment, giving us
x = 2 + 1 cos(0.5t), y = 2− 1 sin(0.5t), 0 ≤ t ≤ 2π37. (a) x = t3 ⇒ t = x1/3, so y = t2 = x2/3.
We get the entire curve y = x2/3 traversed in a left to
right direction.
(b) x = t6 ⇒ t = x1/6, so y = t4 = x4/6 = x2/3.
Since x = t6 ≥ 0, we only get the right half of thecurve y = x2/3.
(c) x = e−3t = (e−t)3 [so e−t = x1/3],
y = e−2t = (e−t)2 = (x1/3)2 = x2/3.
If t < 0, then x and y are both larger than 1. If t > 0, then x and y are between 0
and 1. Since x > 0 and y > 0, the curve never quite reaches the origin.
39. The case π2 < θ < π is illustrated. C has coordinates (rθ, r) as in Example 7,
andQ has coordinates (rθ, r + r cos(π − θ)) = (rθ, r(1− cos θ))[since cos(π − α) = cosπ cosα+ sinπ sinα = − cosα], so P has coordinates(rθ − r sin(π − θ), r(1− cos θ)) = (r(θ − sin θ), r(1− cos θ))[since sin(π − α) = sinπ cosα− cosπ sinα = sinα]. Again we have theparametric equations x = r(θ − sin θ), y = r(1− cos θ).
SECTION 11.1 CURVES DEFINED BY PARAMETRIC EQUATIONS ET SECTION 10.1 ¤ 5
41. It is apparent that x = |OQ| and y = |QP | = |ST |. From the diagram,x = |OQ| = a cos θ and y = |ST | = b sin θ. Thus, the parametric equations are
x = a cos θ and y = b sin θ. To eliminate θ we rearrange: sin θ = y/b ⇒
sin2 θ = (y/b)2 and cos θ = x/a ⇒ cos2 θ = (x/a)2. Adding the two
equations: sin2 θ + cos2 θ = 1 = x2/a2 + y2/b2. Thus, we have an ellipse.
43. C = (2a cot θ, 2a), so the x-coordinate of P is x = 2a cot θ. Let B = (0, 2a).
Then ∠OAB is a right angle and ∠OBA = θ, so |OA| = 2a sin θ andA = ((2a sin θ) cos θ, (2a sin θ) sin θ). Thus, the y-coordinate of P
is y = 2a sin2 θ.
45. (a) There are 2 points of intersection:
(−3, 0) and approximately (−2.1, 1.4).
(b) A collision point occurs when x1 = x2 and y1 = y2 for the same t. So solve the equations:
3 sin t = −3 + cos t (1)
2 cos t = 1 + sin t (2)
From (2), sin t = 2cos t− 1. Substituting into (1), we get 3(2 cos t− 1) = −3 + cos t ⇒ 5 cos t = 0 ( ) ⇒cos t = 0 ⇒ t = π
2 or3π2 . We check that t =
3π2 satisfies (1) and (2) but t =
π2 does not. So the only collision point
occurs when t = 3π2 , and this gives the point (−3, 0). [We could check our work by graphing x1 and x2 together as
functions of t and, on another plot, y1 and y2 as functions of t. If we do so, we see that the only value of t for which both
pairs of graphs intersect is t = 3π2.]
(c) The circle is centered at (3, 1) instead of (−3, 1). There are still 2 intersection points: (3, 0) and (2.1, 1.4), but there areno collision points, since ( ) in part (b) becomes 5 cos t = 6 ⇒ cos t = 6
5> 1.
47. x = t2, y = t3 − ct. We use a graphing device to produce the graphs for various values of c with −π ≤ t ≤ π. Note that all
the members of the family are symmetric about the x-axis. For c < 0, the graph does not cross itself, but for c = 0 it has a
cusp at (0, 0) and for c > 0 the graph crosses itself at x = c, so the loop grows larger as c increases.
6 ¤ CHAPTER 11 PARAMETRIC EQUATIONS AND POLAR COORDINATES ET CHAPTER 10
49. Note that all the Lissajous figures are symmetric about the x-axis. The parameters a and b simply stretch the graph in the
x- and y-directions respectively. For a = b = n = 1 the graph is simply a circle with radius 1. For n = 2 the graph crosses
itself at the origin and there are loops above and below the x-axis. In general, the figures have n− 1 points of intersection,all of which are on the y-axis, and a total of n closed loops.
a = b = 1 n = 2 n = 3
11.2 Calculus with Parametric Curves ET 10.2
1. x = t sin t, y = t2 + t ⇒ dy
dt= 2t+ 1, dx
dt= t cos t+ sin t, and dy
dx=
dy/dt
dx/dt=
2t+ 1
t cos t+ sin t.
3. x = t4 + 1, y = t3 + t; t = −1. dy
dt= 3t2 + 1, dx
dt= 4t3, and dy
dx=
dy/dt
dx/dt=3t2 + 1
4t3. When t = −1,
(x, y) = (2,−2) and dy/dx = 4−4 = −1, so an equation of the tangent to the curve at the point corresponding to t = −1
is y − (−2) = (−1)(x− 2), or y = −x.
5. x = e√t, y = t− ln t2; t = 1. dy
dt= 1− 2t
t2= 1− 2
t, dxdt=
e√t
2√t, and dy
dx=
dy/dt
dx/dt=
1− 2/te√t/ 2
√t· 2t2t=2t− 4√te√t.
When t = 1, (x, y) = (e, 1) and dy
dx= −2
e, so an equation of the tangent line is y − 1 = −2
e(x− e), or y = −2
ex+ 3.
7. (a) x = 1 + ln t, y = t2 + 2; (1, 3). dy
dt= 2t,
dx
dt=1
t, and dy
dx=
dy/dt
dx/dt=2t
1/t= 2t2.
At (1, 3), x = 1 + ln t = 1 ⇒ ln t = 0 ⇒ t = 1 and dy
dx= 2, so an equation of the tangent is y − 3 = 2(x− 1),
or y = 2x+ 1.
(b) x = 1 + ln t ⇒ x− 1 = ln t ⇒ t = ex−1, so y = (ex−1)2 + 2 = e2x−2 + 2 and dy
dx= 2e2x−2.
When x = 1, dydx
= 2e0 = 2, so an equation of the tangent is y = 2x+ 1, as in part (a).
9. x = 6 sin t, y = t2 + t; (0, 0).
dy
dx=
dy/dt
dx/dt=2t+ 1
6 cos t. The point (0, 0) corresponds to t = 0, so the
slope of the tangent at that point is 16 . An equation of the tangent is therefore
y − 0 = 16(x− 0), or y = 1
6x.
SECTION 11.2 CALCULUS WITH PARAMETRIC CURVES ET SECTION 10.2 ¤ 7
11. x = 4 + t2, y = t2 + t3 ⇒ dy
dx=
dy/dt
dx/dt=2t+ 3t2
2t= 1 +
3
2t ⇒
d2y
dx2=
d
dx
dy
dx=
d(dy/dx)/dt
dx/dt=(d/dt) 1 + 3
2t
2t=3/2
2t=3
4t.
The curve is CU when d2y
dx2> 0, that is, when t > 0.
13. x = t − et, y = t + e−t ⇒
dy
dx=
dy/dt
dx/dt=1− e−t
1− et=1− 1
et
1− et=
et − 1et
1− et= −e−t ⇒ d2y
dx2=
d
dt
dy
dx
dx/dt=
d
dt(−e−t)dx/dt
=e−t
1− et.
The curve is CU when et < 1 [since e−t > 0] ⇒ t < 0.
15. x = 2 sin t, y = 3cos t, 0 < t < 2π.
dy
dx=
dy/dt
dx/dt=−3 sin t2 cos t
= −32tan t, so d2y
dx2=
d
dt
dy
dx
dx/dt=− 32sec2 t
2 cos t= −3
4sec3 t.
The curve is CU when sec3 t < 0 ⇒ sec t < 0 ⇒ cos t < 0 ⇒ π2< t < 3π
2.
17. x = 10− t2, y = t3 − 12t.dy
dt= 3t2 − 12 = 3(t+ 2)(t− 2), so dy
dt= 0 ⇔
t = ±2 ⇔ (x, y) = (6,∓16).dx
dt= −2t, so dx
dt= 0 ⇔ t = 0 ⇔ (x, y) = (10, 0).
The curve has horizontal tangents at (6,±16) and a verticaltangent at (10, 0).
19. x = 2cos θ, y = sin 2θ.
dy
dθ= 2 cos 2θ, so dy
dθ= 0 ⇔ 2θ = π
2 + nπ
[n an integer] ⇔ θ = π4 +
π2n ⇔
(x, y) = ±√2,±1 . Also, dxdθ= −2 sin θ, so
dx
dθ= 0 ⇔ θ = nπ ⇔ (x, y) = (±2, 0).
The curve has horizontal tangents at ±√2,±1 (four points), and vertical tangents at (±2, 0).
21. From the graph, it appears that the rightmost point on the curve x = t− t6, y = et
is about (0.6, 2). To find the exact coordinates, we find the value of t for which the
graph has a vertical tangent, that is, 0 = dx/dt = 1− 6t5 ⇔ t = 1/ 5√6.
Hence, the rightmost point is
1/ 5√6− 1/ 6 5
√6 , e1/
5√6 = 5 · 6−6/5, e6−1/5 ≈ (0.58, 2.01).
8 ¤ CHAPTER 11 PARAMETRIC EQUATIONS AND POLAR COORDINATES ET CHAPTER 10
23. We graph the curve x = t4 − 2t3 − 2t2, y = t3 − t in the viewing rectangle [−2, 1.1] by [−0.5, 0.5]. This rectanglecorresponds approximately to t ∈ [−1, 0.8].
We estimate that the curve has horizontal tangents at about (−1,−0.4) and (−0.17, 0.39) and vertical tangents at
about (0, 0) and (−0.19, 0.37). We calculate dydx
=dy/dt
dx/dt=
3t2 − 14t3 − 6t2 − 4t . The horizontal tangents occur when
dy/dt = 3t2 − 1 = 0 ⇔ t = ± 1√3, so both horizontal tangents are shown in our graph. The vertical tangents occur when
dx/dt = 2t(2t2− 3t− 2) = 0 ⇔ 2t(2t+1)(t− 2) = 0 ⇔ t = 0,− 12or 2. It seems that we have missed one vertical
tangent, and indeed if we plot the curve on the t-interval [−1.2, 2.2] we see that there is another vertical tangent at (−8, 6).
25. x = cos t, y = sin t cos t. dx/dt = − sin t, dy/dt = − sin2 t+ cos2 t = cos 2t.(x, y) = (0, 0) ⇔ cos t = 0 ⇔ t is an odd multiple of π
2 . When t =π2 ,
dx/dt = −1 and dy/dt = −1, so dy/dx = 1. When t = 3π2, dx/dt = 1 and
dy/dt = −1. So dy/dx = −1. Thus, y = x and y = −x are both tangent to thecurve at (0, 0).
27. x = rθ − d sin θ, y = r − d cos θ.
(a) dxdθ= r − d cos θ, dy
dθ= d sin θ, so dy
dx=
d sin θ
r − d cos θ.
(b) If 0 < d < r, then |d cos θ| ≤ d < r, so r − d cos θ ≥ r − d > 0. This shows that dx/dθ never vanishes,
so the trochoid can have no vertical tangent if d < r.
29. x = 2t3, y = 1 + 4t− t2 ⇒ dy
dx=
dy/dt
dx/dt=4− 2t6t2
. Now solve dydx
= 1 ⇔ 4− 2t6t2
= 1 ⇔
6t2 + 2t− 4 = 0 ⇔ 2(3t− 2)(t+ 1) = 0 ⇔ t = 23or t = −1. If t = 2
3, the point is 16
27, 299, and if t = −1,
the point is (−2,−4).
31. By symmetry of the ellipse about the x- and y-axes,
A= 4a
0y dx = 4
0
π/2b sin θ (−a sin θ) dθ = 4ab π/2
0sin2 θ dθ = 4ab
π/2
012 (1− cos 2θ) dθ
= 2ab θ − 12sin 2θ
π/2
0= 2ab π
2= πab
SECTION 11.2 CALCULUS WITH PARAMETRIC CURVES ET SECTION 10.2 ¤ 9
33. The curve x = 1 + et, y = t− t2 = t(1− t) intersects the x-axis when y = 0,
that is, when t = 0 and t = 1. The corresponding values of x are 2 and 1 + e.
The shaded area is given byx=1+e
x=2
(yT − yB) dx=t=1
t=0
[y(t)− 0]x0(t) dt = 1
0(t− t2)et dt
=1
0tet dt− 1
0t2et dt =
1
0tet dt− t2et
1
0+ 2
1
0tet dt [Formula 97 or parts]
= 31
0tet dt− (e− 0) = 3 (t− 1)et 1
0− e [Formula 96 or parts]
= 3[0− (−1)]− e = 3− e
35. x = rθ − d sin θ, y = r − d cos θ.
A =2πr
0y dx =
2π
0(r − d cos θ)(r − d cos θ) dθ =
2π
0(r2 − 2dr cos θ + d2 cos2 θ) dθ
= r2θ − 2dr sin θ + 12d2 θ + 1
2sin 2θ
2π
0= 2πr2 + πd2
37. x = t − t2, y = 43t3/2, 1 ≤ t ≤ 2. dx/dt = 1 − 2t and dy/dt = 2t1/2, so
(dx/dt)2 + (dy/dt)2 = (1− 2t)2 + (2t1/2)2 = 1− 4t+ 4t2 + 4t = 1 + 4t2.
Thus, L = b
a(dx/dt)2 + (dy/dt)2 dt =
2
1
√1 + 4t2 dt ≈ 3.1678.
39. x = t+ cos t, y = t− sin t, 0 ≤ t ≤ 2π. dx/dt = 1− sin t and dy/dt = 1− cos t, sodxdt
2+ dy
dt
2= (1− sin t)2 + (1− cos t)2 = (1− 2 sin t+ sin2 t) + (1− 2 cos t+ cos2 t) = 3− 2 sin t− 2 cos t.
Thus, L = b
a(dx/dt)2 + (dy/dt)2 dt =
2π
0
√3− 2 sin t− 2 cos t dt ≈ 10.0367.
41. x = 1 + 3t2, y = 4 + 2t3, 0 ≤ t ≤ 1.dx/dt = 6t and dy/dt = 6t2, so (dx/dt)2 + (dy/dt)2 = 36t2 + 36t4.
Thus, L =1
0
√36t2 + 36t4 dt =
1
06t√1 + t2 dt
= 62
1
√u 1
2du [u = 1 + t2, du = 2t dt]
= 3 23u
3/22
1= 2(23/2 − 1) = 2 2√2− 1
43. x = t
1 + t, y = ln (1 + t), 0 ≤ t ≤ 2. dx
dt=(1 + t) · 1− t · 1
(1 + t)2=
1
(1 + t)2and dy
dt=
1
1 + t,
so dx
dt
2
+dy
dt
2
=1
(1 + t)4+
1
(1 + t)2=
1
(1 + t)41 + (1 + t)2 =
t2 + 2t+ 2
(1 + t)4. Thus,
L=2
0
√t2 + 2t+ 2
(1 + t)2dt =
3
1
√u2 + 1
u2du
u = t+ 1,
du = dt
24= −
√u2 + 1
u+ ln u+ u2 + 1
3
1
= −√103+ ln 3 +
√10 +
√2− ln 1 +√2
10 ¤ CHAPTER 11 PARAMETRIC EQUATIONS AND POLAR COORDINATES ET CHAPTER 10
45. x = et cos t, y = et sin t, 0 ≤ t ≤ π.
dxdt
2+ dy
dt
2= [et(cos t− sin t)]2 + [et(sin t+ cos t)]2= (et)2(cos2 t− 2 cos t sin t+ sin2 t)
+ (et)2(sin2 t+ 2 sin t cos t+ cos2 t
= e2t(2 cos2 t+ 2 sin2 t) = 2e2t
Thus, L = π
0
√2e2t dt =
π
0
√2 et dt =
√2 et
π
0=√2 (eπ − 1).
47. x = et − t, y = 4et/2, −8 ≤ t ≤ 3dxdt
2+ dy
dt
2= (et − 1)2 + (2et/2)2 = e2t − 2et + 1 + 4et
= e2t + 2et + 1 = (et + 1)2
L =3
−8 (et + 1)2 dt =3
−8(et + 1) dt = et + t
3t
−8
= (e3 + 3)− (e−8 − 8) = e3 − e−8 + 11
49. x = t − et, y = t + et, −6 ≤ t ≤ 6.
dxdt
2+ dy
dt
2= (1− et)2 + (1 + et)2 = (1− 2et + e2t) + (1 + 2et + e2t) = 2 + 2e2t, so L = 6
−6√2 + 2e2t dt.
Set f(t) =√2 + 2e2t. Then by Simpson’s Rule with n = 6 and ∆t = 6−(−6)
6= 2, we get
L ≈ 23[f(−6) + 4f(−4) + 2f(−2) + 4f(0) + 2f(2) + 4f(4) + f(6)] ≈ 612.3053.
51. x = sin2 t, y = cos2 t, 0 ≤ t ≤ 3π.
(dx/dt)2 + (dy/dt)2 = (2 sin t cos t)2 + (−2 cos t sin t)2 = 8 sin2 t cos2 t = 2 sin2 2t ⇒
Distance = 3π
0
√2 |sin 2t| dt = 6√2 π/2
0sin 2t dt [by symmetry] = −3√2 cos 2t
π/2
0= −3√2 (−1− 1) = 6√2.
The full curve is traversed as t goes from 0 to π2 , because the curve is the segment of x+ y = 1 that lies in the first quadrant
(since x, y ≥ 0), and this segment is completely traversed as t goes from 0 to π2. Thus, L = π/2
0sin 2t dt =
√2, as above.
53. x = a sin θ, y = b cos θ, 0 ≤ θ ≤ 2π.dxdt
2+ dy
dt
2= (a cos θ)2 + (−b sin θ)2 = a2 cos2 θ + b2 sin2 θ = a2(1− sin2 θ) + b2 sin2 θ
= a2 − (a2 − b2) sin2 θ = a2 − c2 sin2 θ = a2 1− c2
a2sin2 θ = a2(1− e2 sin2 θ)
So L = 4 π/2
0a2 1− e2 sin2 θ dθ [by symmetry] = 4a π/2
01− e2 sin2 θ dθ.
55. (a) x = 11 cos t− 4 cos(11t/2), y = 11 sin t− 4 sin(11t/2).Notice that 0 ≤ t ≤ 2π does not give the complete curve becausex(0) 6= x(2π). In fact, we must take t ∈ [0, 4π] in order to obtain thecomplete curve, since the first term in each of the parametric equations has
period 2π and the second has period 2π11/2
= 4π11, and the least common
integer multiple of these two numbers is 4π.
SECTION 11.2 CALCULUS WITH PARAMETRIC CURVES ET SECTION 10.2 ¤ 11
(b) We use the CAS to find the derivatives dx/dt and dy/dt, and then use Theorem 6 to find the arc length. Recent versions
of Maple express the integral 4π
0(dx/dt)2 + (dy/dt)2 dt as 88E 2
√2 i , where E(x) is the elliptic integral
1
0
√1− x2t2√1− t2
dt and i is the imaginary number√−1.
Some earlier versions of Maple (as well as Mathematica) cannot do the integral exactly, so we use the command
evalf(Int(sqrt(diff(x,t) 2+diff(y,t) 2),t=0..4*Pi)); to estimate the length, and find that the arc
length is approximately 294.03. Derive’s Para_arc_length function in the utility file Int_apps simplifies the
integral to 11 4π
0−4 cos t cos 11t
2− 4 sin t sin 11t
2+ 5 dt.
57. x = 1 + tet, y = (t2 + 1)et, 0 ≤ t ≤ 1.dxdt
2+ dy
dt
2= (tet + et)2 + [(t2 + 1)et + et(2t)]2 = [et(t+ 1)]2 + [et(t2 + 2t+ 1)]2
= e2t(t+ 1)2 + e2t(t+ 1)4 = e2t(t+ 1)2[1 + (t+ 1)2], so
S = 2πy ds =1
02π(t2 + 1)et e2t(t+ 1)2(t2 + 2t+ 2) dt =
1
02π(t2 + 1)e2t(t+ 1)
√t2 + 2t+ 2 dt ≈ 103.5999
59. x = t3, y = t2, 0 ≤ t ≤ 1. dxdt
2+ dy
dt
2= 3t2
2+ (2t)2 = 9t4 + 4t2.
S =1
0
2πy dxdt
2+ dy
dt
2dt =
1
0
2πt2 9t4 + 4t2 dt = 2π1
0
t2 t2(9t2 + 4) dt
= 2π13
4
u− 49
√u 1
18 duu = 9t2 + 4, t2 = (u− 4)/9,du = 18t dt, so t dt = 1
18 du=
2π
9 · 1813
4
(u3/2 − 4u1/2) du
= π81
25u5/2 − 8
3u3/2
13
4= π
81· 215
3u5/2 − 20u3/2 13
4
= 2π1215
3 · 132√13− 20 · 13√13 − (3 · 32− 20 · 8) = 2π1215
247√13 + 64
61. x = a cos3 θ, y = a sin3 θ, 0 ≤ θ ≤ π2. dx
dθ
2+ dy
dθ
2= (−3a cos2 θ sin θ)2 + (3a sin2 θ cos θ)2 = 9a2 sin2 θ cos2 θ.
S =π/2
02π · a sin3 θ · 3a sin θ cos θ dθ = 6πa2 π/2
0sin4 θ cos θ dθ = 6
5πa2 sin5 θ
π/2
0= 6
5πa2
63. x = t+ t3, y = t− 1
t2, 1 ≤ t ≤ 2. dx
dt= 1 + 3t2 and dy
dt= 1 +
2
t3, so dx
dt
2+ dy
dt
2= (1 + 3t2)2 + 1 +
2
t3
2
and S = 2πy ds =2
1
2π t− 1
t2(1 + 3t2)2 + 1 +
2
t3
2
dt ≈ 59.101.
65. x = 3t2, y = 2t3, 0 ≤ t ≤ 5 ⇒ dxdt
2+ dy
dt
2= (6t)2 + (6t2)2 = 36t2(1 + t2) ⇒
S =5
02πx (dx/dt)2 + (dy/dt)2 dt =
5
02π(3t2)6t
√1 + t2 dt = 18π
5
0t2√1 + t2 2t dt
= 18π26
1(u− 1)√udu u = 1 + t2,
du = 2t dt= 18π
26
1(u3/2 − u1/2) du = 18π 2
5u5/2 − 2
3u3/2
26
1
= 18π 25 · 676
√26− 2
3 · 26√26 − 2
5 − 23
= 245 π 949
√26 + 1
12 ¤ CHAPTER 11 PARAMETRIC EQUATIONS AND POLAR COORDINATES ET CHAPTER 10
67. If f 0 is continuous and f 0(t) 6= 0 for a ≤ t ≤ b, then either f 0(t) > 0 for all t in [a, b] or f 0(t) < 0 for all t in [a, b]. Thus, f
is monotonic (in fact, strictly increasing or strictly decreasing) on [a, b]. It follows that f has an inverse. Set F = g ◦ f−1,
that is, define F by F (x) = g(f−1(x)). Then x = f(t) ⇒ f−1(x) = t, so y = g(t) = g(f−1(x)) = F (x).
69. (a) φ = tan−1 dy
dx⇒ dφ
dt=
d
dttan−1
dy
dx=
1
1 + (dy/dx)2d
dt
dy
dx. But dy
dx=
dy/dt
dx/dt=
y
x⇒
d
dt
dy
dx=
d
dt
y
x=
yx− xy
x2⇒ dφ
dt=
1
1 + (y/x)2yx− xy
x2=
xy − xy
x2 + y2. Using the Chain Rule, and the
fact that s =t
0
dxdt
2+ dy
dt
2dt ⇒ ds
dt =dxdt
2+ dy
dt
2= x2 + y2
1/2, we have that
dφ
ds=
dφ/dt
ds/dt=
xy − xy
x2 + y21
(x2 + y2)1/2=
xy − xy
(x2 + y2)3/2. So κ = dφ
ds=
xy − xy
(x2 + y2)3/2=
|xy − xy|(x2 + y2)3/2
.
(b) x = x and y = f(x) ⇒ x = 1, x = 0 and y = dy
dx, y = d2y
dx2.
So κ =1 · (d2y/dx2)− 0 · (dy/dx)
[1 + (dy/dx)2]3/2=
d2y/dx2
[1 + (dy/dx)2]3/2.
71. x = θ − sin θ ⇒ x = 1− cos θ ⇒ x = sin θ, and y = 1− cos θ ⇒ y = sin θ ⇒ y = cos θ. Therefore,
κ =cos θ − cos2 θ − sin2 θ[(1− cos θ)2 + sin2 θ]3/2 =
cos θ − (cos2 θ + sin2 θ)(1− 2 cos θ + cos2 θ + sin2 θ)3/2 =
|cos θ − 1|(2− 2 cos θ)3/2 . The top of the arch is
characterized by a horizontal tangent, and from Example 2(b) in Section 11.2 [ ET 10.2], the tangent is horizontal when
θ = (2n− 1)π, so take n = 1 and substitute θ = π into the expression for κ: κ = |cosπ − 1|(2− 2 cosπ)3/2 =
|−1− 1|[2− 2(−1)]3/2 =
1
4.
73. The coordinates of T are (r cos θ, r sin θ). Since TP was unwound from
arc TA, TP has length rθ. Also ∠PTQ = ∠PTR− ∠QTR = 12π − θ,
so P has coordinates x = r cos θ + rθ cos 12π − θ = r(cos θ + θ sin θ),
y = r sin θ − rθ sin 12π − θ = r(sin θ − θ cos θ).
11.3 Polar Coordinates ET 10.3
1. (a) 2, π3
By adding 2π to π3, we obtain the point 2, 7π
3. The direction
opposite π3is 4π
3, so −2, 4π
3is a point that satisfies the r < 0
requirement.
SECTION 11.3 POLAR COORDINATES ET SECTION 10.3 ¤ 13
(b) 1,− 3π4 r > 0: 1,− 3π
4 + 2π = 1, 5π4
r < 0: −1,− 3π4+ π = −1, π
4
(c) −1, π2 r > 0: −(−1), π2 + π = 1, 3π2
r < 0: −1, π2+ 2π = −1, 5π
2
3. (a) x = 1cosπ = 1(−1) = −1 andy = 1 sinπ = 1(0) = 0 give us
the Cartesian coordinates (−1, 0).
(b) x = 2cos − 2π3
= 2 − 12= −1 and
y = 2 sin −2π3
= 2 −√32
= −√3
give us −1,−√3 .
(c) x = −2 cos 3π4 = −2 −√22
=√2 and
y = −2 sin 3π4= −2
√22
= −√2
gives us√2,−√2 .
5. (a) x = 2 and y = −2 ⇒ r = 22 + (−2)2 = 2√2 and θ = tan−1 −22
= −π4. Since (2,−2) is in the fourth
quadrant, the polar coordinates are (i) 2√2, 7π
4and (ii) −2√2, 3π
4.
(b) x = −1 and y = √3 ⇒ r = (−1)2 + √3
2= 2 and θ = tan−1
√3
−1 = 2π3. Since −1,√3 is in the second
quadrant, the polar coordinates are (i) 2, 2π3and (ii) −2, 5π
3.
14 ¤ CHAPTER 11 PARAMETRIC EQUATIONS AND POLAR COORDINATES ET CHAPTER 10
7. The curves r = 1 and r = 2 represent circles with center
O and radii 1 and 2. The region in the plane satisfying
1 ≤ r ≤ 2 consists of both circles and the shaded regionbetween them in the figure.
9. The region satisfying 0 ≤ r < 4 and −π/2 ≤ θ < π/6
does not include the circle r = 4 nor the line θ = π6.
11. 2 < r < 3, 5π3≤ θ ≤ 7π
3
13. Converting the polar coordinates (2, π/3) and (4, 2π/3) to Cartesian coordinates gives us 2 cos π3, 2 sin π
3= 1,
√3 and
4 cos 2π3, 4 sin 2π
3= −2, 2√3 . Now use the distance formula.
d = (x2 − x1)2 + (y2 − y1)
2 = (−2− 1)2 + 2√3−√3 2
=√9 + 3 =
√12 = 2
√3
15. r = 2 ⇔ x2 + y2 = 2 ⇔ x2 + y2 = 4, a circle of radius 2 centered at the origin.
17. r = 3 sin θ ⇒ r2 = 3r sin θ ⇔ x2 + y2 = 3y ⇔ x2 + y − 32
2= 3
2
2, a circle of radius 32centered at 0, 3
2.
The first two equations are actually equivalent since r2 = 3r sin θ ⇒ r(r − 3 sin θ) = 0 ⇒ r = 0 or r = 3 sin θ. But
r = 3 sin θ gives the point r = 0 (the pole) when θ = 0. Thus, the single equation r = 3 sin θ is equivalent to the compound
condition (r = 0 or r = 3 sin θ).
19. r = csc θ ⇔ r =1
sin θ⇔ r sin θ = 1 ⇔ y = 1, a horizontal line 1 unit above the x-axis.
21. x = 3 ⇔ r cos θ = 3 ⇔ r = 3/ cos θ ⇔ r = 3 sec θ.
23. x = −y2 ⇔ r cos θ = −r2 sin2 θ ⇔ cos θ = −r sin2 θ ⇔ r = − cos θsin2 θ
= − cot θ csc θ.
25. x2 + y2 = 2cx ⇔ r2 = 2cr cos θ ⇔ r2 − 2cr cos θ = 0 ⇔ r(r − 2c cos θ) = 0 ⇔ r = 0 or r = 2c cos θ.r = 0 is included in r = 2c cos θ when θ = π
2+ nπ, so the curve is represented by the single equation r = 2c cos θ.
27. (a) The description leads immediately to the polar equation θ = π6 , and the Cartesian equation y = tan
π6
x = 1√3x is
slightly more difficult to derive.
(b) The easier description here is the Cartesian equation x = 3.
SECTION 11.3 POLAR COORDINATES ET SECTION 10.3 ¤ 15
29. θ = −π/6 31. r = sin θ ⇔ r2 = r sin θ ⇔ x2 + y2 = y ⇔x2 + y − 1
2
2= 1
2
2. The reasoning here is the same
as in Exercise 17. This is a circle of radius 12centered at 0, 1
2.
33. r = 2(1− sin θ). This curve is a cardioid. 35. r = θ, θ ≥ 0
37. r = 4 sin 3θ
39. r = 2 cos 4θ
41. r = 1− 2 sin θ
16 ¤ CHAPTER 11 PARAMETRIC EQUATIONS AND POLAR COORDINATES ET CHAPTER 10
43. r2 = 9 sin 2θ
45. r = 2 cos 32θ
47. r = 1 + 2 cos 2θ
49. For θ = 0, π, and 2π, r has its minimum value of about 0.5. For θ = π2and 3π
2, r attains its maximum value of 2.
We see that the graph has a similar shape for 0 ≤ θ ≤ π and π ≤ θ ≤ 2π.
51. x = (r) cos θ = (4 + 2 sec θ) cos θ = 4cos θ + 2. Now, r→∞ ⇒
(4 + 2 sec θ)→∞ ⇒ θ → π2
− or θ → 3π2
+ [since we need only
consider 0 ≤ θ < 2π], so limr→∞
x = limθ→π/2−
(4 cos θ + 2) = 2. Also,
r→ −∞ ⇒ (4 + 2 sec θ)→−∞ ⇒ θ → π2
+ or θ → 3π2
−, so
limr→−∞
x = limθ→π/2+
(4 cos θ + 2) = 2. Therefore, limr→±∞
x = 2 ⇒ x = 2 is a vertical asymptote.
SECTION 11.3 POLAR COORDINATES ET SECTION 10.3 ¤ 17
53. To show that x = 1 is an asymptote we must prove limr→±∞
x = 1.
x = (r) cos θ = (sin θ tan θ) cos θ = sin2 θ. Now, r→∞ ⇒ sin θ tan θ→∞ ⇒θ → π
2
−, so limr→∞
x = limθ→π/2−
sin2 θ = 1. Also, r→−∞ ⇒ sin θ tan θ →−∞ ⇒
θ → π2
+, so limr→−∞
x = limθ→π/2+
sin2 θ = 1. Therefore, limr→±∞
x = 1 ⇒ x = 1 is
a vertical asymptote. Also notice that x = sin2 θ ≥ 0 for all θ, and x = sin2 θ ≤ 1 for all θ. And x 6= 1, since the curve is notdefined at odd multiples of π
2. Therefore, the curve lies entirely within the vertical strip 0 ≤ x < 1.
55. (a) We see that the curve r = 1 + c sin θ crosses itself at the origin, where r = 0 (in fact the inner loop corresponds to
negative r-values,) so we solve the equation of the limaçon for r = 0 ⇔ c sin θ = −1 ⇔ sin θ = −1/c. Now if|c| < 1, then this equation has no solution and hence there is no inner loop. But if c < −1, then on the interval (0, 2π)
the equation has the two solutions θ = sin−1(−1/c) and θ = π − sin−1(−1/c), and if c > 1, the solutions are
θ = π + sin−1(1/c) and θ = 2π − sin−1(1/c). In each case, r < 0 for θ between the two solutions, indicating a loop.
(b) For 0 < c < 1, the dimple (if it exists) is characterized by the fact that y has a local maximum at θ = 3π2. So we determine
for what c-values d2y
dθ2is negative at θ = 3π
2, since by the Second Derivative Test this indicates a maximum:
y = r sin θ = sin θ + c sin2 θ ⇒ dy
dθ= cos θ + 2c sin θ cos θ = cos θ + c sin 2θ ⇒ d2y
dθ2= − sin θ + 2c cos 2θ.
At θ = 3π2, this is equal to −(−1) + 2c(−1) = 1− 2c, which is negative only for c > 1
2. A similar argument shows that
for −1 < c < 0, y only has a local minimum at θ = π2(indicating a dimple) for c < − 1
2.
57. r = 2 sin θ ⇒ x = r cos θ = 2 sin θ cos θ = sin 2θ, y = r sin θ = 2 sin2 θ ⇒dy
dx=
dy/dθ
dx/dθ=2 · 2 sin θ cos θcos 2θ · 2 =
sin 2θ
cos 2θ= tan 2θ
When θ = π
6, dydx
= tan 2 · π6
= tanπ
3=√3. [Another method: Use Equation 3.]
59. r = 1/θ ⇒ x = r cos θ = (cos θ)/θ, y = r sin θ = (sin θ)/θ ⇒
dy
dx=
dy/dθ
dx/dθ=sin θ(−1/θ2) + (1/θ) cos θcos θ(−1/θ2)− (1/θ) sin θ ·
θ2
θ2=− sin θ + θ cos θ
− cos θ − θ sin θ
When θ = π, dydx
=−0 + π(−1)−(−1)− π(0)
=−π1= −π.
61. r = cos 2θ ⇒ x = r cos θ = cos 2θ cos θ, y = r sin θ = cos 2θ sin θ ⇒dy
dx=
dy/dθ
dx/dθ=
cos 2θ cos θ + sin θ (−2 sin 2θ)cos 2θ (− sin θ) + cos θ (−2 sin 2θ)
When θ = π
4, dydx
=0√2/2 +
√2/2 (−2)
0 −√2/2 +√2/2 (−2) =
−√2−√2 = 1.
18 ¤ CHAPTER 11 PARAMETRIC EQUATIONS AND POLAR COORDINATES ET CHAPTER 10
63. r = 3 cos θ ⇒ x = r cos θ = 3cos θ cos θ, y = r sin θ = 3 cos θ sin θ ⇒dydθ= −3 sin2 θ + 3 cos2 θ = 3 cos 2θ = 0 ⇒ 2θ = π
2or 3π
2⇔ θ = π
4or 3π
4.
So the tangent is horizontal at 3√2, π4and − 3√
2, 3π4
same as 3√2,−π
4.
dxdθ= −6 sin θ cos θ = −3 sin 2θ = 0 ⇒ 2θ = 0 or π ⇔ θ = 0 or π
2. So the tangent is vertical at (3, 0) and 0, π
2.
65. r = 1 + cos θ ⇒ x = r cos θ = cos θ (1 + cos θ), y = r sin θ = sin θ (1 + cos θ) ⇒dydθ = (1 + cos θ) cos θ − sin2 θ = 2cos2 θ + cos θ − 1 = (2 cos θ − 1)(cos θ + 1) = 0 ⇒ cos θ = 1
2 or −1 ⇒θ = π
3, π, or 5π
3⇒ horizontal tangent at 3
2, π3, (0, π), and 3
2, 5π3.
dxdθ = −(1 + cos θ) sin θ − cos θ sin θ = − sin θ (1 + 2 cos θ) = 0 ⇒ sin θ = 0 or cos θ = −1
2 ⇒θ = 0, π, 2π
3, or 4π
3⇒ vertical tangent at (2, 0), 1
2, 2π3, and 1
2, 4π3.
Note that the tangent is horizontal, not vertical when θ = π, since limθ→π
dy/dθ
dx/dθ= 0.
67. r = 2 + sin θ ⇒ x = r cos θ = (2 + sin θ) cos θ, y = r sin θ = (2 + sin θ) sin θ ⇒dydθ = (2 + sin θ) cos θ + sin θ cos θ = cos θ · 2(1 + sin θ) = 0 ⇒ cos θ = 0 or sin θ = −1 ⇒θ = π
2or 3π
2⇒ horizontal tangent at 3, π
2and 1, 3π
2.
dxdθ = (2 + sin θ)(− sin θ) + cos θ cos θ = −2 sin θ − sin2 θ + 1− sin2 θ = −2 sin2 θ − 2 sin θ + 1 ⇒
sin θ =2±√4 + 8
−4 =2± 2√3−4 =
1−√3−2
1 +√3
−2 < −1 ⇒
θ1 = sin−1 − 1
2+ 1
2
√3 and θ2 = π − θ1 ⇒ vertical tangent at 3
2+ 1
2
√3, θ1 and 3
2+ 1
2
√3, θ2 .
Note that r(θ1) = 2 + sin sin−1 − 12 +
12
√3 = 2− 1
2 +12
√3 = 3
2 +12
√3.
69. r = a sin θ + b cos θ ⇒ r2 = ar sin θ + br cos θ ⇒ x2 + y2 = ay + bx ⇒x2 − bx+ 1
2b2+ y2 − ay + 1
2a2= 1
2 b2+ 1
2a2 ⇒ x− 1
2b2+ y − 1
2a2= 1
4 (a2 + b2), and this is a circle
with center 12b, 1
2a and radius 1
2
√a2 + b2.
Note for Exercises 71–76: Maple is able to plot polar curves using the polarplot command, or using the coords=polar option in a regularplot command. In Mathematica, use PolarPlot. In Derive, change to Polar under Options State. If your graphing device cannotplot polar equations, you must convert to parametric equations. For example, in Exercise 71, x = r cos θ = [1 + 2 sin(θ/2)] cos θ,y = r sin θ = [1 + 2 sin(θ/2)] sin θ.
71. r = 1 + 2 sin(θ/2). The parameter interval is [0, 4π]. 73. r = esin θ − 2 cos(4θ). The parameter interval is [0, 2π].
SECTION 11.3 POLAR COORDINATES ET SECTION 10.3 ¤ 19
75. r = 2− 5 sin(θ/6). The parameter interval is [−6π, 6π].
77. It appears that the graph of r = 1 + sin θ − π6is the same shape as
the graph of r = 1 + sin θ, but rotated counterclockwise about the
origin by π6. Similarly, the graph of r = 1 + sin θ − π
3is rotated by
π3 . In general, the graph of r = f(θ − α) is the same shape as that of
r = f(θ), but rotated counterclockwise through α about the origin.
That is, for any point (r0, θ0) on the curve r = f(θ), the point
(r0, θ0 + α) is on the curve r = f(θ − α), since r0 = f(θ0) = f((θ0 + α)− α).
79. (a) r = sinnθ.
n = 2 n = 3 n = 4 n = 5
From the graphs, it seems that when n is even, the number of loops in the curve (called a rose) is 2n, and when n is odd,
the number of loops is simply n. This is because in the case of n odd, every point on the graph is traversed twice, due to
the fact that
r(θ + π) = sin[n(θ + π)] = sinnθ cosnπ + cosnθ sinnπ =sinnθ if n is even
− sinnθ if n is odd
(b) The graph of r = |sinnθ| has 2n loops whether n is odd or even, since r(θ + π) = r(θ).
n = 2 n = 3 n = 4 n = 5
20 ¤ CHAPTER 11 PARAMETRIC EQUATIONS AND POLAR COORDINATES ET CHAPTER 10
81. r = 1− a cos θ
1 + a cos θ. We start with a = 0, since in this case the curve is simply the circle r = 1.
As a increases, the graph moves to the left, and its right side becomes flattened. As a increases through about 0.4, the right
side seems to grow a dimple, which upon closer investigation (with narrower θ-ranges) seems to appear at a ≈ 0.42 [theactual value is
√2− 1]. As a→ 1, this dimple becomes more pronounced, and the curve begins to stretch out horizontally,
until at a = 1 the denominator vanishes at θ = π, and the dimple becomes an actual cusp. For a > 1 we must choose our
parameter interval carefully, since r →∞ as 1 + a cos θ → 0 ⇔ θ → ± cos−1(−1/a). As a increases from 1, the curvesplits into two parts. The left part has a loop, which grows larger as a increases, and the right part grows broader vertically,
and its left tip develops a dimple when a ≈ 2.42 [actually,√2 + 1]. As a increases, the dimple grows more and morepronounced. If a < 0, we get the same graph as we do for the corresponding positive a-value, but with a rotation through π
about the pole, as happened when c was replaced with −c in Exercise 80.
a = 0 a = 0.3 a = 0.41, |θ| ≤ 0.5
a = 0.42,|θ| ≤ 0.5 a = 0.9, |θ| ≤ 0.5 a = 1, |θ| ≤ 0.1
a = 2
a = 2.41, |θ − π| ≤ 0.2
a = 2.42, |θ − π| ≤ 0.2
a = 4
SECTION 11.4 AREAS AND LENGTHS IN POLAR COORDINATES ET SECTION 10.4 ¤ 21
83. tanψ = tan(φ− θ) =tanφ− tan θ1 + tanφ tan θ
=
dy
dx− tan θ
1 +dy
dxtan θ
=
dy/dθ
dx/dθ− tan θ
1 +dy/dθ
dx/dθtan θ
=
dy
dθ− dx
dθtan θ
dx
dθ+
dy
dθtan θ
=
dr
dθsin θ + r cos θ − tan θ dr
dθcos θ − r sin θ
dr
dθcos θ − r sin θ + tan θ
dr
dθsin θ + r cos θ
=r cos θ + r · sin
2 θ
cos θdr
dθcos θ +
dr
dθ· sin
2 θ
cos θ
=r cos2 θ + r sin2 θ
dr
dθcos2 θ +
dr
dθsin2 θ
=r
dr/dθ
11.4 Areas and Lengths in Polar Coordinates ET 10.4
1. r = θ2, 0 ≤ θ ≤ π4. A =
π/4
0
12r2 dθ =
π/4
0
12(θ2)2 dθ =
π/4
0
12θ4 dθ = 1
10θ5
π/4
0= 1
10π4
5= 1
10,240π5
3. r = sin θ, π3 ≤ θ ≤ 2π3 .
A=2π/3
π/3
12sin2 θ dθ = 1
4
2π/3
π/3
(1− cos 2θ) dθ = 14θ − 1
2sin 2θ
2π/3
π/3= 1
42π3− 1
2sin 4π
3− π
3+ 1
2sin 2π
3
= 14
2π3 − 1
2−√32
− π3 +
12
√32
= 14
π3 +
√32
= π12 +
√38
5. r =√θ, 0 ≤ θ ≤ 2π. A =
2π
0
12r
2 dθ =2π
0
12
√θ
2
dθ =2π
0
12θ dθ =
14θ
2 2π
0= π2
7. r = 4 + 3 sin θ, −π2≤ θ ≤ π
2.
A=π/2
−π/212 ((4 + 3 sin θ)
2 dθ = 12
π/2
−π/2(16 + 24 sin θ + 9 sin2 θ) dθ
= 12
π/2
−π/2(16 + 9 sin2 θ) dθ [by Theorem 5.5.6(a) [ ET 5.5.7(a)] ]
= 12 · 2
π/2
0
16 + 9 · 12 (1− cos 2θ) dθ [by Theorem 5.5.6(a) [ ET 5.5.7(a)] ]
=π/2
0
412 − 9
2 cos 2θ dθ = 412 θ − 9
4 sin 2θπ/2
0= 41π
4 − 0 − (0− 0) = 41π4
9. The area above the polar axis is bounded by r = 3 cos θ for θ = 0
to θ = π/2 [not π]. By symmetry,
A = 2π/2
012r2 dθ =
π/2
0(3 cos θ)2 dθ = 32
π/2
0cos2 θ dθ
= 9π/2
012 (1 + cos 2θ) dθ =
92θ + 1
2 sin 2θπ/2
0= 9
2π2 + 0 − (0 + 0) = 9π
4
Also, note that this is a circle with radius 32, so its area is π 3
2
2= 9π
4.
11. The curve goes through the pole when θ = π/4, so we’ll find the area for
0 ≤ θ ≤ π/4 and multiply it by 4.
A = 4π/4
012r2 dθ = 2
π/4
0(4 cos 2θ) dθ
= 8π/4
0cos 2θ dθ = 4 sin 2θ
π/4
0= 4
22 ¤ CHAPTER 11 PARAMETRIC EQUATIONS AND POLAR COORDINATES ET CHAPTER 10
13. One-sixth of the area lies above the polar axis and is bounded by the curve
r = 2 cos 3θ for θ = 0 to θ = π/6.
A = 6π/6
012(2 cos 3θ)2 dθ = 12
π/6
0cos2 3θ dθ
= 122
π/6
0(1 + cos 6θ) dθ
= 6 θ + 16sin 6θ
π/6
0= 6 π
6= π
15. A= 2π
012 (1 + 2 sin 6θ)
2 dθ = 12
2π
0(1 + 4 sin 6θ + 4 sin2 6θ) dθ
= 12
2π
01 + 4 sin 6θ + 4 · 1
2 (1− cos 12θ) dθ
= 12
2π
0(3 + 4 sin 6θ − 2 cos 12θ) dθ
= 123θ − 2
3cos 6θ − 1
6sin 12θ
2π
0
= 12(6π − 2
3− 0)− 0− 2
3− 0 = 3π
17. The shaded loop is traced out from θ = 0 to θ = π/2.
A=π/2
012r
2 dθ = 12
π/2
0sin2 2θ dθ
= 12
π/2
012 (1− cos 4θ) dθ = 1
4θ − 1
4 sin 4θπ/2
0
= 14
π2= π
8
19. r = 0 ⇒ 3 cos 5θ = 0 ⇒ 5θ = π2⇒ θ = π
10.
A =π/10
−π/1012(3 cos 5θ)2 dθ =
π/10
09 cos2 5θ dθ = 9
2
π/10
0(1 + cos 10θ) dθ = 9
2θ + 1
10sin 10θ
π/10
0= 9π
20
21. This is a limaçon, with inner loop traced
out between θ = 7π6and 11π
6[found by
solving r = 0].
A= 23π/2
7π/6
12 (1 + 2 sin θ)
2 dθ =3π/2
7π/6
1 + 4 sin θ + 4 sin2 θ dθ =3π/2
7π/6
1 + 4 sin θ + 4 · 12 (1− cos 2θ) dθ
= θ − 4 cos θ + 2θ − sin 2θ 3π/2
7π/6= 9π
2− 7π
2+ 2
√3−
√32
= π − 3√3
2
23. 2 cos θ = 1 ⇒ cos θ = 12 ⇒ θ = π
3 or5π3 .
A= 2π/3
012[(2 cos θ)2 − 12] dθ = π/3
0(4 cos2 θ − 1) dθ
=π/3
04 1
2(1 + cos 2θ) − 1 dθ =
π/3
0(1 + 2 cos 2θ) dθ
= θ + sin 2θπ/3
0= π
3+√32
SECTION 11.4 AREAS AND LENGTHS IN POLAR COORDINATES ET SECTION 10.4 ¤ 23
25. To find the area inside the leminiscate r2 = 8 cos 2θ and outside the circle r = 2,
we first note that the two curves intersect when r2 = 8 cos 2θ and r = 2,
that is, when cos 2θ = 12. For −π < θ ≤ π, cos 2θ = 1
2⇔ 2θ = ±π/3
or ±5π/3 ⇔ θ = ±π/6 or ±5π/6. The figure shows that the desired area is4 times the area between the curves from 0 to π/6. Thus,
A= 4π/6
012(8 cos 2θ)− 1
2(2)2 dθ = 8
π/6
0(2 cos 2θ − 1) dθ
= 8 sin 2θ − θπ/6
0= 8
√3/2− π/6 = 4
√3− 4π/3
27. 3 cos θ = 1 + cos θ ⇔ cos θ = 12 ⇒ θ = π
3 or −π3 .
A= 2π/3
012[(3 cos θ)2 − (1 + cos θ)2] dθ
=π/3
0(8 cos2 θ − 2 cos θ − 1) dθ = π/3
0[4(1 + cos 2θ)− 2 cos θ − 1] dθ
=π/3
0(3 + 4 cos 2θ − 2 cos θ) dθ = 3θ + 2 sin 2θ − 2 sin θ π/3
0
= π +√3−√3 = π
29.√3 cos θ = sin θ ⇒ √
3 =sin θ
cos θ⇒ tan θ =
√3 ⇒ θ = π
3.
A=π/3
012(sin θ)2 dθ +
π/2
π/312
√3 cos θ
2dθ
=π/3
012· 12(1− cos 2θ) dθ + π/2
π/312· 3 · 1
2(1 + cos 2θ) dθ
= 14θ − 1
2sin 2θ
π/3
0+ 3
4θ + 1
2sin 2θ
π/2
π/3
= 14
π3−√34
− 0 + 34
π2+ 0 − π
3+√34
= π12−√3
16+ π
8− 3
√3
16= 5π
24−√34
31. sin 2θ = cos 2θ ⇒ sin 2θ
cos 2θ= 1 ⇒ tan 2θ = 1 ⇒ 2θ = π
4 ⇒θ = π
8⇒
A= 8 · 2 π/8
012sin 22θ dθ = 8
π/8
012(1− cos 4θ) dθ
= 4 θ − 14 sin 4θ
π/8
0= 4 π
8 − 14 · 1 = π
2 − 1
33. sin 2θ = cos 2θ ⇒ tan 2θ = 1 ⇒ 2θ = π4⇒ θ = π
8
A= 4π/8
012sin 2θ dθ [since r2 = sin 2θ]
=π/8
02 sin 2θ dθ = − cos 2θ π/8
0
= − 12
√2− (−1) = 1− 1
2
√2
24 ¤ CHAPTER 11 PARAMETRIC EQUATIONS AND POLAR COORDINATES ET CHAPTER 10
35. The darker shaded region (from θ = 0 to θ = 2π/3) represents 12 of the desired area plus12 of the area of the inner loop.
From this area, we’ll subtract 12 of the area of the inner loop (the lighter shaded region from θ = 2π/3 to θ = π), and then
double that difference to obtain the desired area.
A = 22π/3
012
12 + cos θ
2dθ − π
2π/312
12 + cos θ
2dθ
=2π/3
014+ cos θ + cos2 θ dθ − π
2π/314+ cos θ + cos2 θ dθ
=2π/3
014 + cos θ +
12 (1 + cos 2θ) dθ
− π
2π/314 + cos θ +
12 (1 + cos 2θ) dθ
=θ
4+ sin θ +
θ
2+sin 2θ
4
2π/3
0
− θ
4+ sin θ +
θ
2+sin 2θ
4
π
2π/3
= π6+√32+ π
3−√38
− π4+ π
2+ π
6+√32+ π
3−√38
= π4 +
34
√3 = 1
4π + 3
√3
37. The pole is a point of intersection.
1 + sin θ = 3 sin θ ⇒ 1 = 2 sin θ ⇒ sin θ = 12⇒
θ = π6or 5π
6.
The other two points of intersection are 32, π6and 3
2, 5π6.
39. 2 sin 2θ = 1 ⇒ sin 2θ = 12⇒ 2θ = π
6, 5π6, 13π
6, or 17π
6.
By symmetry, the eight points of intersection are given by
(1, θ), where θ = π12 ,
5π12 ,
13π12 , and
17π12 , and
(−1, θ), where θ = 7π12, 11π12, 19π12, and 23π
12.
[There are many ways to describe these points.]
41. The pole is a point of intersection. sin θ = sin 2θ = 2 sin θ cos θ ⇔sin θ (1− 2 cos θ) = 0 ⇔ sin θ = 0 or cos θ = 1
2⇒
θ = 0, π, π3 , or −π3 ⇒ the other intersection points are
√32 , π3
and√32, 2π3
[by symmetry].
SECTION 11.4 AREAS AND LENGTHS IN POLAR COORDINATES ET SECTION 10.4 ¤ 25
43.
From the first graph, we see that the pole is one point of intersection. By zooming in or using the cursor, we find the θ-values
of the intersection points to be α ≈ 0.88786 ≈ 0.89 and π − α ≈ 2.25. (The first of these values may be more easilyestimated by plotting y = 1 + sinx and y = 2x in rectangular coordinates; see the second graph.) By symmetry, the total
area contained is twice the area contained in the first quadrant, that is,
A= 2α
0
12(2θ)2 dθ + 2
π/2
α
12(1 + sin θ)2 dθ =
α
0
4θ2 dθ +π/2
α
1 + 2 sin θ + 12(1− cos 2θ) dθ
= 43θ
3 α
0+ θ − 2 cos θ + 1
2θ − 14 sin 2θ
π/2
α= 4
3α3 + π
2 +π4− α− 2 cosα+ 1
2α− 14 sin 2α ≈ 3.4645
45. L =b
a
r2 + (dr/dθ)2 dθ =π/3
0
(3 sin θ)2 + (3 cos θ)2 dθ =π/3
0
9(sin2θ + cos2θ) dθ
= 3π/3
0
dθ = 3 θπ/3
0= 3 π
3= π.
As a check, note that the circumference of a circle with radius 32is 2π 3
2= 3π, and since θ = 0 to π = π
3traces out 1
3of the
circle (from θ = 0 to θ = π), 13(3π) = π.
47. L =b
a
r2 + (dr/dθ)2 dθ =2π
0
(θ2)2 + (2θ)2 dθ =2π
0
θ4 + 4θ2 dθ
=2π
0
θ2(θ2 + 4) dθ =2π
0
θ θ2 + 4 dθ
Now let u = θ2 + 4, so that du = 2θ dθ θ dθ = 12 du and
2π
0
θ θ2 + 4 dθ =4π2+4
4
12
√udu = 1
2· 23u3/2
4(π2+1)
4= 1
3[43/2(π2 + 1)3/2 − 43/2] = 8
3[(π2 + 1)3/2 − 1]
49. The curve r = 3 sin 2θ is completely traced with 0 ≤ θ ≤ 2π. r2 + drdθ
2= (3 sin 2θ)2 + (6 cos 2θ)2 ⇒
L =2π
09 sin2 2θ + 36 cos2 2θ dθ ≈ 29.0653
26 ¤ CHAPTER 11 PARAMETRIC EQUATIONS AND POLAR COORDINATES ET CHAPTER 10
51. The curve r = sin θ2is completely traced with 0 ≤ θ ≤ 4π. r2 + dr
dθ
2= sin2 θ
2+ 1
2 cosθ2
2 ⇒
L =4π
0
sin2 θ2+ 1
4cos2 θ
2dθ ≈ 9.6884
53. The curve r = cos4(θ/4) is completely traced with 0 ≤ θ ≤ 4π.r2 + (dr/dθ)2 = [cos4(θ/4)]2 + 4cos3(θ/4) · (− sin(θ/4)) · 14
2
= cos8(θ/4) + cos6(θ/4) sin2(θ/4)
= cos6(θ/4)[cos2(θ/4) + sin2(θ/4)] = cos6(θ/4)
L =4π
0cos6(θ/4) dθ =
4π
0cos3(θ/4) dθ
= 22π
0cos3(θ/4) dθ [since cos3(θ/4) ≥ 0 for 0 ≤ θ ≤ 2π] = 8
π/2
0cos3 udu u = 1
4θ
68= 8 1
3(2 + cos2 u) sinu
π/2
0= 8
3[(2 · 1)− (3 · 0)] = 16
3
55. (a) From (11.2.7) [ET (10.2.7)],
S =b
a2πy (dx/dθ)2 + (dy/dθ)2 dθ
=b
a2πy r2 + (dr/dθ)2 dθ [from the derivation of Equation 11.4.5 [ ET 10.4.5] ]
=b
a2πr sin θ r2 + (dr/dθ)2 dθ
(b) The curve r2 = cos 2θ goes through the pole when cos 2θ = 0 ⇒2θ = π
2⇒ θ = π
4. We’ll rotate the curve from θ = 0 to θ = π
4and double
this value to obtain the total surface area generated.
r2 = cos 2θ ⇒ 2rdr
dθ= −2 sin 2θ ⇒ dr
dθ
2
=sin2 2θ
r2=sin2 2θ
cos 2θ.
S = 2π/4
0
2π√cos 2θ sin θ cos 2θ + sin2 2θ /cos 2θ dθ = 4π
π/4
0
√cos 2θ sin θ
cos2 2θ + sin2 2θ
cos 2θdθ
= 4ππ/4
0
√cos 2θ sin θ
1√cos 2θ
dθ = 4ππ/4
0
sin θ dθ = 4π − cos θ π/4
0= −4π
√22− 1 = 2π 2−√2
SECTION 11.5 CONIC SECTIONS ET SECTION 10.5 ¤ 27
11.5 Conic Sections ET 10.5
1. x = 2y2 ⇒ y2 = 12x. 4p =
12 , so p =
18 . The vertex
is (0, 0), the focus is 18, 0 , and the directrix is x = − 1
8.
3. 4x2 = −y ⇒ x2 = − 14y. 4p = − 1
4 , so p = − 116 .
The vertex is (0, 0), the focus is 0,− 116, and the
directrix is y = 116.
5. (x+ 2)2 = 8 (y − 3). 4p = 8, so p = 2. The vertex is(−2, 3), the focus is (−2, 5), and the directrix is y = 1.
7. y2 + 2y + 12x+ 25 = 0 ⇒y2 + 2y + 1 = −12x− 24 ⇒(y + 1)2 = −12(x+ 2). 4p = −12, so p = −3.The vertex is (−2,−1), the focus is (−5,−1), and thedirectrix is x = 1.
9. The equation has the form y2 = 4px, where p < 0.
Since the parabola passes through (−1, 1), we have12 = 4p(−1), so 4p = −1 and an equation is y2 = −xor x = −y2. 4p = −1, so p = − 1
4and the focus is
− 14 , 0 while the directrix is x = 1
4 .
11. x2
9+
y2
5= 1 ⇒ a =
√9 = 3, b =
√5,
c =√a2 − b2 =
√9− 5 = 2. The ellipse is centered at
(0, 0), with vertices at (±3, 0). The foci are (±2, 0).
28 ¤ CHAPTER 11 PARAMETRIC EQUATIONS AND POLAR COORDINATES ET CHAPTER 10
13. 4x2 + y2 = 16 ⇒ x2
4+
y2
16= 1 ⇒
a =√16 = 4, b =
√4 = 2,
c =√a2 − b2 =
√16− 4 = 2√3. The ellipse is
centered at (0, 0), with vertices at (0,±4). The fociare 0,±2√3 .
15. 9x2 − 18x+ 4y2 = 27 ⇔9(x2 − 2x+ 1) + 4y2 = 27 + 9 ⇔
9(x− 1)2 + 4y2 = 36 ⇔ (x− 1)24
+y2
9= 1 ⇒
a = 3, b = 2, c =√5 ⇒ center (1, 0),
vertices (1,±3), foci 1,±√5
17. The center is (0, 0), a = 3, and b = 2, so an equation is x2
4+
y2
9= 1. c =
√a2 − b2 =
√5, so the foci are 0,±√5 .
19. x2
144− y2
25= 1 ⇒ a = 12, b = 5, c =
√144 + 25 = 13 ⇒
center (0, 0), vertices (±12, 0), foci (±13, 0), asymptotes y = ± 512x.
Note: It is helpful to draw a 2a-by-2b rectangle whose center is the center
of the hyperbola. The asymptotes are the extended diagonals of the
rectangle.
21. y2 − x2 = 4 ⇔ y2
4− x2
4= 1 ⇒ a =
√4 = 2 = b,
c =√4 + 4 = 2
√2 ⇒ center (0, 0), vertices (0,±2),
foci 0,±2√2 , asymptotes y = ±x
23. 4x2 − y2 − 24x− 4y + 28 = 0 ⇔4(x2 − 6x+ 9)− (y2 + 4y + 4) = −28 + 36− 4 ⇔
4(x− 3)2 − (y + 2)2 = 4 ⇔ (x− 3)21
− (y + 2)2
4= 1 ⇒
a =√1 = 1, b =
√4 = 2, c =
√1 + 4 =
√5 ⇒
center (3,−2), vertices (4,−2) and (2,−2), foci 3±√5,−2 ,asymptotes y + 2 = ±2(x− 3).
SECTION 11.5 CONIC SECTIONS ET SECTION 10.5 ¤ 29
25. x2 = y + 1 ⇔ x2 = 1(y + 1). This is an equation of a parabola with 4p = 1, so p = 14 . The vertex is (0,−1) and the
focus is 0,− 34.
27. x2 = 4y − 2y2 ⇔ x2 + 2y2 − 4y = 0 ⇔ x2 + 2(y2 − 2y + 1) = 2 ⇔ x2 + 2(y − 1)2 = 2 ⇔x2
2+(y − 1)2
1= 1. This is an equation of an ellipse with vertices at ±√2, 1 . The foci are at ±√2− 1, 1 = (±1, 1).
29. y2 +2y = 4x2 +3 ⇔ y2 +2y+1 = 4x2 +4 ⇔ (y+1)2 − 4x2 = 4 ⇔ (y + 1)2
4− x2 = 1. This is an equation
of a hyperbola with vertices (0,−1± 2) = (0, 1) and (0,−3). The foci are at 0,−1±√4 + 1 = 0,−1±√5 .
31. The parabola with vertex (0, 0) and focus (0,−2) opens downward and has p = −2, so its equation is x2 = 4py = −8y.
33. The distance from the focus (−4, 0) to the directrix x = 2 is 2− (−4) = 6, so the distance from the focus to the vertex is12(6) = 3 and the vertex is (−1, 0). Since the focus is to the left of the vertex, p = −3. An equation is y2 = 4p(x+ 1) ⇒
y2 = −12(x+ 1).
35. A parabola with vertical axis and vertex (2, 3) has equation y − 3 = a(x− 2)2. Since it passes through (1, 5), we have5− 3 = a(1− 2)2 ⇒ a = 2, so an equation is y − 3 = 2(x− 2)2.
37. The ellipse with foci (±2, 0) and vertices (±5, 0) has center (0, 0) and a horizontal major axis, with a = 5 and c = 2,
so b2 = a2 − c2 = 25− 4 = 21. An equation is x2
25+
y2
21= 1.
39. Since the vertices are (0, 0) and (0, 8), the ellipse has center (0, 4) with a vertical axis and a = 4. The foci at (0, 2) and (0, 6)
are 2 units from the center, so c = 2 and b =√a2 − c2 =
√42 − 22 = √12. An equation is (x− 0)
2
b2+(y − 4)2
a2= 1 ⇒
x2
12+(y − 4)216
= 1.
41. An equation of an ellipse with center (−1, 4) and vertex (−1, 0) is (x+ 1)2
b2+(y − 4)242
= 1. The focus (−1, 6) is 2 units
from the center, so c = 2. Thus, b2 + 22 = 42 ⇒ b2 = 12, and the equation is (x+ 1)2
12+(y − 4)216
= 1.
43. An equation of a hyperbola with vertices (±3, 0) is x2
32− y2
b2= 1. Foci (±5, 0) ⇒ c = 5 and 32 + b2 = 52 ⇒
b2 = 25− 9 = 16, so the equation is x2
9− y2
16= 1.
45. The center of a hyperbola with vertices (−3,−4) and (−3, 6) is (−3, 1), so a = 5 and an equation is(y − 1)252
− (x+ 3)2
b2= 1. Foci (−3,−7) and (−3, 9) ⇒ c = 8, so 52 + b2 = 82 ⇒ b2 = 64− 25 = 39 and the
equation is (y − 1)2
25− (x+ 3)2
39= 1.
30 ¤ CHAPTER 11 PARAMETRIC EQUATIONS AND POLAR COORDINATES ET CHAPTER 10
47. The center of a hyperbola with vertices (±3, 0) is (0, 0), so a = 3 and an equation is x2
32− y2
b2= 1.
Asymptotes y = ±2x ⇒ b
a= 2 ⇒ b = 2(3) = 6 and the equation is x
2
9− y2
36= 1.
49. In Figure 8, we see that the point on the ellipse closest to a focus is the closer vertex (which is a distance
a− c from it) while the farthest point is the other vertex (at a distance of a+ c). So for this lunar orbit,
(a− c) + (a+ c) = 2a = (1728 + 110) + (1728 + 314), or a = 1940; and (a+ c)− (a− c) = 2c = 314− 110,
or c = 102. Thus, b2 = a2 − c2 = 3,753,196, and the equation is x2
3,763,600+
y2
3,753,196= 1.
51. (a) Set up the coordinate system so that A is (−200, 0) and B is (200, 0).
|PA|− |PB| = (1200)(980) = 1,176,000 ft = 245011
mi = 2a ⇒ a = 122511, and c = 200 so
b2 = c2 − a2 =3,339,375121
⇒ 121x2
1,500,625− 121y2
3,339,375= 1.
(b) Due north of B ⇒ x = 200 ⇒ (121)(200)2
1,500,625− 121y2
3,339,375= 1 ⇒ y =
133,575539
≈ 248 mi
53. The function whose graph is the upper branch of this hyperbola is concave upward. The function is
y = f(x) = a 1 +x2
b2=
a
b
√b2 + x2, so y0 = a
bx(b2 + x2)−1/2 and
y00 =a
b(b2 + x2)−1/2 − x2(b2 + x2)−3/2 = ab(b2 + x2)−3/2 > 0 for all x, and so f is concave upward.
55. (a) If k > 16, then k − 16 > 0, and x2
k+
y2
k − 16 = 1 is an ellipse since it is the sum of two squares on the left side.
(b) If 0 < k < 16, then k − 16 < 0, and x2
k+
y2
k − 16 = 1 is a hyperbola since it is the difference of two squares on the
left side.
(c) If k < 0, then k − 16 < 0, and there is no curve since the left side is the sum of two negative terms, which cannot equal 1.
(d) In case (a), a2 = k, b2 = k − 16, and c2 = a2 − b2 = 16, so the foci are at (±4, 0). In case (b), k − 16 < 0, so a2 = k,
b2 = 16− k, and c2 = a2 + b2 = 16, and so again the foci are at (±4, 0).
57. x2 = 4py ⇒ 2x = 4py0 ⇒ y0 =x
2p, so the tangent line at (x0, y0) is
y − x204p=
x02p(x− x0). This line passes through the point (a,−p) on the
directrix, so −p− x204p=
x02p(a− x0) ⇒ −4p2 − x20 = 2ax0 − 2x20 ⇔
x20 − 2ax0 − 4p2 = 0 ⇔ x20 − 2ax0 + a2 = a2 + 4p2 ⇔
SECTION 11.5 CONIC SECTIONS ET SECTION 10.5 ¤ 31
(x0 − a)2 = a2 + 4p2 ⇔ x0 = a± a2 + 4p2. The slopes of the tangent lines at x = a± a2 + 4p2
area± a2 + 4p2
2p, so the product of the two slopes is
a+ a2 + 4p2
2p· a− a2 + 4p2
2p=
a2 − (a2 + 4p2)4p2
=−4p24p2
= −1,
showing that the tangent lines are perpendicular.
59. For x2 + 4y2 = 4, or x2/4 + y2 = 1, use the parametrization x = 2 cos t, y = sin t, 0 ≤ t ≤ 2π to get
L = 4π/2
0(dx/dt)2 + (dy/dt)2 dt = 4
π/2
04 sin2 t+ cos2 t dt = 4
π/2
03 sin2 t+ 1 dt
Using Simpson’s Rule with n = 10,∆t = π/2− 010
= π20, and f(t) = 3 sin2 t+ 1, we get
L ≈ 43
π20
f(0) + 4f π20
+ 2f 2π20
+ · · ·+ 2f 8π20
+ 4f 9π20
+ f π2
≈ 9.69
61. x2
a2− y2
b2= 1 ⇒ y2
b2=
x2 − a2
a2⇒ y = ± b
a
√x2 − a2.
A= 2c
a
b
ax2 − a2 dx
39=2b
a
x
2x2 − a2 − a2
2ln x+ x2 − a2
c
a
=b
ac√c2 − a2 − a2 ln c+
√c2 − a2 + a2 ln |a|
Since a2 + b2 = c2, c2 − a2 = b2, and√c2 − a2 = b.
=b
acb− a2 ln(c+ b) + a2 ln a =
b
acb+ a2(ln a− ln(b+ c))
= b2c/a+ ab ln[a/(b+ c)], where c2 = a2 + b2.
63. Differentiating implicitly, x2
a2+
y2
b2= 1 ⇒ 2x
a2+2yy0
b2= 0 ⇒ y0 = − b2x
a2y[y 6= 0]. Thus, the slope of the tangent
line at P is − b2x1a2y1
. The slope of F1P isy1
x1 + cand of F2P is
y1x1 − c
. By the formula from Problems Plus, we have
tanα=
y1x1 + c
+b2x1a2y1
1− b2x1y1a2y1(x1 + c)
=a2y21 + b2x1(x1 + c)
a2y1(x1 + c)− b2x1y1=
a2b2 + b2cx1c2x1y1 + a2cy1
using b2x21 + a2y21 = a2b2,and a2 − b2 = c2
=b2 cx1 + a2
cy1(cx1 + a2)=
b2
cy1
and tanβ =
− b2x1a2y1
− y1x1 − c
1− b2x1y1a2y1(x1 − c)
=−a2y21 − b2x1(x1 − c)
a2y1 (x1 − c)− b2x1y1=−a2b2 + b2cx1c2x1y1 − a2cy1
=b2 cx1 − a2
cy1(cx1 − a2)=
b2
cy1
Thus, α = β.
32 ¤ CHAPTER 11 PARAMETRIC EQUATIONS AND POLAR COORDINATES ET CHAPTER 10
11.6 Conic Sections in Polar Coordinates ET 10.6
1. The directrix y = 6 is above the focus at the origin, so we use the form with “+ e sin θ” in the denominator. [See Theorem 6
and Figure 2(c).] r =ed
1 + e sin θ=
74· 6
1 + 74 sin θ
=42
4 + 7 sin θ
3. The directrix x = −5 is to the left of the focus at the origin, so we use the form with “− e cos θ” in the denominator.
r =ed
1− e cos θ=
34· 5
1− 34cos θ
=15
4− 3 cos θ
5. The vertex (4, 3π/2) is 4 units below the focus at the origin, so the directrix is 8 units below the focus (d = 8), and we use the
form with “−e sin θ ” in the denominator. e = 1 for a parabola, so an equation is r = ed
1− e sin θ=
1(8)
1− 1 sin θ =8
1− sin θ .
7. The directrix r = 4 sec θ (equivalent to r cos θ = 4 or x = 4) is to the right of the focus at the origin, so we will use the form
with “+e cos θ” in the denominator. The distance from the focus to the directrix is d = 4, so an equation is
r =ed
1 + e cos θ=
12 (4)
1 + 12cos θ
· 22=
4
2 + cos θ.
9. r = 1
1 + sin θ=
ed
1 + e sin θ, where d = e = 1.
(a) Eccentricity= e = 1
(b) Since e = 1, the conic is a parabola.
(c) Since “+e sin θ ” appears in the denominator, the directrix is above the
focus at the origin. d = |Fl| = 1, so an equation of the directrix is y = 1.
(d) The vertex is at 12, π2, midway between the focus and the directrix.
11. r = 12
4− sin θ ·1/4
1/4=
3
1− 14 sin θ
, where e = 14 and ed = 3 ⇒ d = 12.
(a) Eccentricity= e = 14
(b) Since e = 14< 1, the conic is an ellipse.
(c) Since “−e sin θ ” appears in the denominator, the directrix is below the focusat the origin. d = |Fl| = 12, so an equation of the directrix is y = −12.
(d) The vertices are 4, π2and 12
5, 3π2, so the center is midway between them,
that is, 45, π2.
SECTION 11.6 CONIC SECTIONS IN POLAR COORDINATES ET SECTION 10.6 ¤ 33
13. r = 9
6 + 2 cos θ· 1/61/6
=3/2
1 + 13 cos θ
, where e = 13and ed = 3
2⇒ d = 9
2.
(a) Eccentricity= e = 13
(b) Since e = 13 < 1, the conic is an ellipse.
(c) Since “+e cos θ ” appears in the denominator, the directrix is to the right of
the focus at the origin. d = |Fl| = 92, so an equation of the directrix is
x = 92.
(d) The vertices are 98, 0 and 9
4, π , so the center is midway between them,
that is, 916 , π .
15. r = 3
4− 8 cos θ ·1/4
1/4=
3/4
1− 2 cos θ , where e = 2 and ed =34 ⇒ d = 3
8 .
(a) Eccentricity= e = 2
(b) Since e = 2 > 1, the conic is a hyperbola.
(c) Since “−e cos θ ” appears in the denominator, the directrix is to the left ofthe focus at the origin. d = |Fl| = 3
8, so an equation of the directrix is
x = − 38 .
(d) The vertices are − 34, 0 and 1
4, π , so the center is midway between them,
that is, 12, π .
17. (a) r = 1
1− 2 sin θ , where e = 2 and ed = 1 ⇒ d = 12. The eccentricity
e = 2 > 1, so the conic is a hyperbola. Since “−e sin θ ” appears in thedenominator, the directrix is below the focus at the origin. d = |Fl| = 1
2 ,
so an equation of the directrix is y = − 12. The vertices are −1, π
2and
13 ,
3π2, so the center is midway between them, that is, 2
3 ,3π2.
(b) By the discussion that precedes Example 4, the equation
is r = 1
1− 2 sin θ − 3π4
.
34 ¤ CHAPTER 11 PARAMETRIC EQUATIONS AND POLAR COORDINATES ET CHAPTER 10
19. For e < 1 the curve is an ellipse. It is nearly circular when e is close to 0. As e
increases, the graph is stretched out to the right, and grows larger (that is, its
right-hand focus moves to the right while its left-hand focus remains at the
origin.) At e = 1, the curve becomes a parabola with focus at the origin.
21. |PF | = e |Pl| ⇒ r = e[d− r cos(π − θ)] = e(d+ r cos θ) ⇒
r(1− e cos θ) = ed ⇒ r =ed
1− e cos θ
23. |PF | = e |Pl| ⇒ r = e[d− r sin(θ − π)] = e(d+ r sin θ) ⇒
r(1− e sin θ) = ed ⇒ r =ed
1− e sin θ
25. We are given e = 0.093 and a = 2.28× 108. By (7), we have
r =a(1− e2)
1 + e cos θ=2.28× 108[1− (0.093)2]
1 + 0.093 cos θ≈ 2.26× 1081 + 0.093 cos θ
27. Here 2a = length of major axis = 36.18 AU ⇒ a = 18.09 AU and e = 0.97. By (7), the equation of the orbit is
r =18.09 1− (0.97)21− 0.97 cos θ ≈ 1.07
1− 0.97 cos θ . By (8), the maximum distance from the comet to the sun is
18.09(1 + 0.97) ≈ 35.64 AU or about 3.314 billion miles.
29. The minimum distance is at perihelion, where 4.6× 107 = r = a(1− e) = a(1− 0.206) = a(0.794) ⇒
a = 4.6 × 107/0.794. So the maximum distance, which is at aphelion, is
r = a(1 + e) = 4.6× 107/0.794 (1.206) ≈ 7.0× 107 km.
31. From Exercise 29, we have e = 0.206 and a(1− e) = 4.6× 107 km. Thus, a = 4.6× 107/0.794. From (7), we can write the
equation of Mercury’s orbit as r = a1− e2
1− e cos θ. So since
dr
dθ=−a(1− e2)e sin θ
(1− e cos θ)2⇒
r2 +dr
dθ
2
=a2(1− e2)2
(1− e cos θ)2+
a2(1− e2)2 e2 sin2 θ
(1− e cos θ)4=
a2(1− e2)2
(1− e cos θ)4(1− 2e cos θ + e2)
CHAPTER 11 REVIEW ET CHAPTER 10 ¤ 35
the length of the orbit is
L =2π
0
r2 + (dr/dθ)2 dθ = a(1− e2)2π
0
√1 + e2 − 2e cos θ(1− e cos θ)2
dθ ≈ 3.6× 108 km
This seems reasonable, since Mercury’s orbit is nearly circular, and the circumference of a circle of radius a
is 2πa ≈ 3.6× 108 km.
11 Review ET 10
1. (a) A parametric curve is a set of points of the form (x, y) = (f(t), g(t)), where f and g are continuous functions of a
variable t.
(b) Sketching a parametric curve, like sketching the graph of a function, is difficult to do in general. We can plot points on the
curve by finding f(t) and g(t) for various values of t, either by hand or with a calculator or computer. Sometimes, when
f and g are given by formulas, we can eliminate t from the equations x = f(t) and y = g(t) to get a Cartesian equation
relating x and y. It may be easier to graph that equation than to work with the original formulas for x and y in terms of t.
2. (a) You can find dy
dxas a function of t by calculating dy
dx=
dy/dt
dx/dt[if dx/dt 6= 0].
(b) Calculate the area as b
ay dx =
β
αg(t) f 0(t)dt [or α
βg(t) f 0(t)dt if the leftmost point is (f(β), g(β)) rather
than (f(α), g(α))].
3. (a) L = β
α(dx/dt)2 + (dy/dt)2 dt =
β
α[f 0(t)]2 + [g0(t)]2 dt
(b) S = β
α2πy (dx/dt)2 + (dy/dt)2 dt =
β
α2πg(t) [f 0(t)]2 + [g0(t)]2 dt
4. (a) See Figure 5 in Section 11.3 [ ET 10.3].
(b) x = r cos θ, y = r sin θ
(c) To find a polar representation (r, θ) with r ≥ 0 and 0 ≤ θ < 2π, first calculate r = x2 + y2. Then θ is specified by
cos θ = x/r and sin θ = y/r.
5. (a) Calculate dydx
=
dy
dθdx
dθ
=
d
dθ(y)
d
dθ(x)
=
d
dθ(r sin θ)
d
dθ(r cos θ)
=
dr
dθsin θ + r cos θ
dr
dθcos θ − r sin θ
, where r = f(θ).
(b) Calculate A = b
a12r2 dθ =
b
a12[f(θ)]2 dθ
(c) L = b
a(dx/dθ)2 + (dy/dθ)2 dθ =
b
ar2 + (dr/dθ)2 dθ =
b
a[f(θ)]2 + [f 0(θ)]2 dθ
6. (a) A parabola is a set of points in a plane whose distances from a fixed point F (the focus) and a fixed line l (the directrix)
are equal.
(b) x2 = 4py; y2 = 4px
36 ¤ CHAPTER 11 PARAMETRIC EQUATIONS AND POLAR COORDINATES ET CHAPTER 10
7. (a) An ellipse is a set of points in a plane the sum of whose distances from two fixed points (the foci) is a constant.
(b) x2
a2+
y2
a2 − c2= 1.
8. (a) A hyperbola is a set of points in a plane the difference of whose distances from two fixed points (the foci) is a constant.
This difference should be interpreted as the larger distance minus the smaller distance.
(b) x2
a2− y2
c2 − a2= 1
(c) y = ±√c2 − a2
ax
9. (a) If a conic section has focus F and corresponding directrix l, then the eccentricity e is the fixed ratio |PF | / |Pl| for pointsP of the conic section.
(b) e < 1 for an ellipse; e > 1 for a hyperbola; e = 1 for a parabola.
(c) x = d: r = ed
1 + e cos θ. x = −d: r = ed
1− e cos θ. y = d: r = ed
1 + e sin θ. y = −d: r = ed
1− e sin θ.
1. False. Consider the curve defined by x = f(t) = (t− 1)3 and y = g(t) = (t− 1)2. Then g0(t) = 2(t− 1), so g0(1) = 0,but its graph has a vertical tangent when t = 1. Note: The statement is true if f 0(1) 6= 0 when g0(1) = 0.
3. False. For example, if f(t) = cos t and g(t) = sin t for 0 ≤ t ≤ 4π, then the curve is a circle of radius 1, hence its lengthis 2π, but 4π
0[f 0(t)]2 + [g0(t)]2 dt = 4π
0(− sin t)2 + (cos t)2 dt = 4π
01 dt = 4π, since as t increases
from 0 to 4π, the circle is traversed twice.
5. True. The curve r = 1− sin 2θ is unchanged if we rotate it through 180◦ about O because1− sin 2(θ + π) = 1− sin(2θ + 2π) = 1− sin 2θ. So it’s unchanged if we replace r by −r. (See the discussionafter Example 8 in Section 11.3 [ ET 10.3].) In other words, it’s the same curve as r = −(1− sin 2θ) = sin 2θ − 1.
7. False. The first pair of equations gives the portion of the parabola y = x2 with x ≥ 0, whereas the second pair of equationstraces out the whole parabola y = x2.
9. True. By rotating and translating the parabola, we can assume it has an equation of the form y = cx2, where c > 0.
The tangent at the point a, ca2 is the line y − ca2 = 2ca(x− a); i.e., y = 2cax− ca2. This tangent meets
the parabola at the points x, cx2 where cx2 = 2cax− ca2. This equation is equivalent to x2 = 2ax− a2
[since c > 0]. But x2 = 2ax− a2 ⇔ x2 − 2ax+ a2 = 0 ⇔ (x− a)2 = 0 ⇔ x = a ⇔x, cx2 = a, ca2 . This shows that each tangent meets the parabola at exactly one point.
CHAPTER 11 REVIEW ET CHAPTER 10 ¤ 37
1. x = t2 + 4t, y = 2− t, −4 ≤ t ≤ 1. t = 2− y, so
x = (2− y)2 + 4(2− y) = 4− 4y + y2 + 8− 4y = y2 − 8y + 12 ⇔x+ 4 = y2 − 8y + 16 = (y − 4)2. This is part of a parabola with vertex(−4, 4), opening to the right.
3. y = sec θ = 1
cos θ=1
x. Since 0 ≤ θ ≤ π/2, 0 < x ≤ 1 and y ≥ 1.
This is part of the hyperbola y = 1/x.
5. Three different sets of parametric equations for the curve y =√x are
(i) x = t, y =√t
(ii) x = t4, y = t2
(iii) x = tan2 t, y = tan t, 0 ≤ t < π/2
There are many other sets of equations that also give this curve.
7. (a) The Cartesian coordinates are x = 4cos 2π3= 4 − 1
2= −2 and
y = 4 sin 2π3= 4
√32
= 2√3, that is, the point −2, 2√3 .
(b) Given x = −3 and y = 3, we have r = (−3)2 + 32 = √18 = 3√2. Also, tan θ = y
x⇒ tan θ =
3
−3 , and since(−3, 3) is in the second quadrant, θ = 3π
4. Thus, one set of polar coordinates for (−3, 3) is 3√2, 3π
4, and two others are
3√2, 11π
4and −3√2, 7π
4.
9. r = 1− cos θ. This cardioid issymmetric about the polar axis.
38 ¤ CHAPTER 11 PARAMETRIC EQUATIONS AND POLAR COORDINATES ET CHAPTER 10
11. r = cos 3θ. This is a
three-leaved rose. The curve is
traced twice.
13. r = 1 + cos 2θ. The curve is
symmetric about the pole and
both the horizontal and verticalaxes.
15. r = 3
1 + 2 sin θ⇒ e = 2 > 1, so the conic is a hyperbola. de = 3 ⇒
d = 32 and the form “+2 sin θ” imply that the directrix is above the focus at
the origin and has equation y = 32. The vertices are 1, π
2and −3, 3π
2.
17. x+ y = 2 ⇔ r cos θ + r sin θ = 2 ⇔ r(cos θ + sin θ) = 2 ⇔ r =2
cos θ + sin θ
19. r = (sin θ)/θ. As θ→ ±∞, r → 0.
As θ → 0, r→ 1. In the first figure,
there are an infinite number ofx-intercepts at x = πn, n a nonzero
integer. These correspond to pole
points in the second figure.
21. x = ln t, y = 1 + t2; t = 1. dydt= 2t and dx
dt=1
t, so dy
dx=
dy/dt
dx/dt=2t
1/t= 2t2.
When t = 1, (x, y) = (0, 2) and dy/dx = 2.
23. r = e−θ ⇒ y = r sin θ = e−θ sin θ and x = r cos θ = e−θ cos θ ⇒dy
dx=
dy/dθ
dx/dθ=
drdθsin θ + r cos θ
drdθcos θ − r sin θ
=−e−θ sin θ + e−θ cos θ−e−θ cos θ − e−θ sin θ
· −eθ
−eθ =sin θ − cos θcos θ + sin θ
.
When θ = π, dydx
=0− (−1)−1 + 0 =
1
−1 = −1.
CHAPTER 11 REVIEW ET CHAPTER 10 ¤ 39
25. x = t+ sin t, y = t− cos t ⇒ dy
dx=
dy/dt
dx/dt=1 + sin t
1 + cos t⇒
d2y
dx2=
d
dt
dy
dx
dx/dt=
(1 + cos t) cos t− (1 + sin t)(− sin t)(1 + cos t)2
1 + cos t=cos t+ cos2 t+ sin t+ sin2 t
(1 + cos t)3=1 + cos t+ sin t
(1 + cos t)3
27. We graph the curve x = t3 − 3t, y = t2 + t+ 1 for −2.2 ≤ t ≤ 1.2.By zooming in or using a cursor, we find that the lowest point is about
(1.4, 0.75). To find the exact values, we find the t-value at which
dy/dt = 2t+ 1 = 0 ⇔ t = − 12 ⇔ (x, y) = 11
8 ,34
.
29. x = 2a cos t− a cos 2t ⇒ dx
dt= −2a sin t+ 2a sin 2t = 2a sin t(2 cos t− 1) = 0 ⇔
sin t = 0 or cos t = 12⇒ t = 0, π
3, π, or 5π
3.
y = 2a sin t− a sin 2t ⇒ dy
dt= 2a cos t− 2a cos 2t = 2a 1 + cos t− 2 cos2 t = 2a(1− cos t)(1 + 2 cos t) = 0 ⇒
t = 0, 2π3 , or
4π3 .
Thus the graph has vertical tangents where
t = π3, π and 5π
3, and horizontal tangents where
t = 2π3and 4π
3. To determine what the slope is
where t = 0, we use l’Hospital’s Rule to evaluate
limt→0
dy/dt
dx/dt= 0, so there is a horizontal tangent
there.
t x y
0 a 0π3
32a
√32a
2π3
− 12a 3
√3
2a
π −3a 04π3
− 12a − 3
√3
2a
5π3
32a −
√32a
31. The curve r2 = 9 cos 5θ has 10 “petals.” For instance, for − π10≤ θ ≤ π
10, there are two petals, one with r > 0 and one
with r < 0.
A = 10π/10
−π/1012r2 dθ = 5
π/10
−π/10 9 cos 5θ dθ = 5 · 9 · 2π/10
0cos 5θ dθ = 18 sin 5θ
π/10
0= 18
33. The curves intersect when 4 cos θ = 2 ⇒ cos θ = 12 ⇒ θ = ±π
3
for −π ≤ θ ≤ π. The points of intersection are 2, π3and 2,−π
3.
40 ¤ CHAPTER 11 PARAMETRIC EQUATIONS AND POLAR COORDINATES ET CHAPTER 10
35. The curves intersect where 2 sin θ = sin θ + cos θ ⇒sin θ = cos θ ⇒ θ = π
4, and also at the origin (at which θ = 3π
4
on the second curve).
A=π/4
012(2 sin θ)2 dθ +
3π/4
π/412(sin θ + cos θ)2 dθ
=π/4
0(1− cos 2θ) dθ + 1
2
3π/4
π/4(1 + sin 2θ) dθ
= θ − 12sin 2θ
π/4
0+ 1
2θ − 1
4cos 2θ
3π/4
π/4= 1
2(π − 1)
37. x = 3t2, y = 2t3.
L=2
0(dx/dt)2 + (dy/dt)2 dt =
2
0(6t)2 + (6t2)2 dt =
2
0
√36t2 + 36t4 dt =
2
0
√36t2
√1 + t2 dt
=2
06 |t|√1 + t2 dt = 6
2
0t√1 + t2 dt = 6
5
1u1/2 1
2du u = 1 + t2, du = 2t dt
= 6 · 12· 23u3/2
5
1= 2(53/2 − 1) = 2 5√5− 1
39. L = 2π
πr2 + (dr/dθ)2 dθ =
2π
π(1/θ)2 + (−1/θ2)2 dθ =
2π
π
θ2 + 1
θ2dθ
24= − θ2 + 1
θ+ ln θ + θ2 + 1
2π
π
=
√π2 + 1
π−√4π2 + 1
2π+ ln
2π +√4π2 + 1
π +√π2 + 1
=2√π2 + 1−√4π2 + 1
2π+ ln
2π +√4π2 + 1
π +√π2 + 1
41. x = 4√t, y = t3
3+
1
2t2, 1 ≤ t ≤ 4 ⇒
S =4
12πy (dx/dt)2 + (dy/dt)2 dt =
4
12π 1
3t3 + 1
2t−2 2/
√t
2+ (t2 − t−3)2 dt
= 2π4
113t3 + 1
2t−2 (t2 + t−3)2 dt = 2π 4
113t5 + 5
6+ 1
2t−5 dt = 2π 1
18t6 + 5
6t− 1
8t−4
4
1= 471,295
1024π
43. For all c except −1, the curve is asymptotic to the line x = 1. Forc < −1, the curve bulges to the right near y = 0. As c increases, thebulge becomes smaller, until at c = −1 the curve is the straight line x = 1.As c continues to increase, the curve bulges to the left, until at c = 0 there
is a cusp at the origin. For c > 0, there is a loop to the left of the origin,
whose size and roundness increase as c increases. Note that the x-intercept
of the curve is always −c.
CHAPTER 11 REVIEW ET CHAPTER 10 ¤ 41
45. x2
9+
y2
8= 1 is an ellipse with center (0, 0).
a = 3, b = 2√2, c = 1 ⇒
foci (±1, 0), vertices (±3, 0).
47. 6y2 + x− 36y + 55 = 0 ⇔6(y2 − 6y + 9) = −(x+ 1) ⇔(y − 3)2 = − 1
6(x+ 1), a parabola with vertex (−1, 3),
opening to the left, p = − 124
⇒ focus − 2524, 3 and
directrix x = − 2324 .
49. The ellipse with foci (±4, 0) and vertices (±5, 0) has center (0, 0) and a horizontal major axis, with a = 5 and c = 4,
so b2 = a2 − c2 = 52 − 42 = 9. An equation is x2
25+
y2
9= 1.
51. The center of a hyperbola with foci (0,±4) is (0, 0), so c = 4 and an equation is y2
a2− x2
b2= 1.
The asymptote y = 3x has slope 3, so ab=3
1⇒ a = 3b and a2 + b2 = c2 ⇒ (3b)2 + b2 = 42 ⇒
10b2 = 16 ⇒ b2 = 85and so a2 = 16− 8
5= 72
5. Thus, an equation is y2
72/5− x2
8/5= 1, or 5y
2
72− 5x2
8= 1.
53. x2 = −(y − 100) has its vertex at (0, 100), so one of the vertices of the ellipse is (0, 100). Another form of the equation of a
parabola is x2 = 4p(y − 100) so 4p(y − 100) = −(y − 100) ⇒ 4p = −1 ⇒ p = −14. Therefore the shared focus is
found at 0, 3994
so 2c = 3994− 0 ⇒ c = 399
8and the center of the ellipse is 0, 399
8. So a = 100− 399
8= 401
8and
b2 = a2 − c2 =4012 − 3992
82= 25. So the equation of the ellipse is x
2
b2+
y − 3998
2
a2= 1 ⇒ x2
25+
y − 3998
2
4018
2 = 1,
or x2
25+(8y − 399)2160,801
= 1.
55. Directrix x = 4 ⇒ d = 4, so e = 13 ⇒ r =
ed
1 + e cos θ=
4
3 + cos θ.
57. In polar coordinates, an equation for the circle is r = 2a sin θ. Thus, the coordinates ofQ are x = r cos θ = 2a sin θ cos θ
and y = r sin θ = 2a sin2 θ. The coordinates of R are x = 2a cot θ and y = 2a. Since P is the midpoint of QR, we use the
midpoint formula to get x = a(sin θ cos θ + cot θ) and y = a(1 + sin2 θ).
PROBLEMS PLUS1. x =
t
1
cosu
udu, y =
t
1
sinu
udu, so by FTC1, we have dx
dt=cos t
tand dy
dt=sin t
t. Vertical tangent lines occur when
dx
dt= 0 ⇔ cos t = 0. The parameter value corresponding to (x, y) = (0, 0) is t = 1, so the nearest vertical tangent
occurs when t = π2. Therefore, the arc length between these points is
L =π/2
1
dx
dt
2
+dy
dt
2
dt =π/2
1
cos2 t
t2+sin2 t
t2dt =
π/2
1
dt
t= ln t
π/2
1= ln π
2
3. In terms of x and y, we have x = r cos θ = (1 + c sin θ) cos θ = cos θ + c sin θ cos θ = cos θ + 12c sin 2θ and
y = r sin θ = (1 + c sin θ) sin θ = sin θ + c sin2 θ. Now−1 ≤ sin θ ≤ 1 ⇒ −1 ≤ sin θ + c sin2 θ ≤ 1 + c ≤ 2, so
−1 ≤ y ≤ 2. Furthermore, y = 2 when c = 1 and θ = π2, while y = −1 for c = 0 and θ = 3π
2. Therefore, we need a viewing
rectangle with −1 ≤ y ≤ 2.To find the x-values, look at the equation x = cos θ + 1
2c sin 2θ and use the fact that sin 2θ ≥ 0 for 0 ≤ θ ≤ π
2and
sin 2θ ≤ 0 for −π2≤ θ ≤ 0. [Because r = 1 + c sin θ is symmetric about the y-axis, we only need to consider
−π2 ≤ θ ≤ π
2 .] So for −π2 ≤ θ ≤ 0, x has a maximum value when c = 0 and then x = cos θ has a maximum value
of 1 at θ = 0. Thus, the maximum value of x must occur on 0, π2with c = 1. Then x = cos θ + 1
2 sin 2θ ⇒dxdθ= − sin θ + cos 2θ = − sin θ + 1− 2 sin2 θ ⇒ dx
dθ= −(2 sin θ − 1)(sin θ + 1) = 0 when sin θ = −1 or 1
2
[but sin θ 6= −1 for 0 ≤ θ ≤ π2 ]. If sin θ =
12 , then θ =
π6 and
x = cos π6+ 1
2sin π
3= 3
4
√3. Thus, the maximum value of x is 3
4
√3, and,
by symmetry, the minimum value is − 34
√3. Therefore, the smallest
viewing rectangle that contains every member of the family of polar curves
r = 1 + c sin θ, where 0 ≤ c ≤ 1, is − 34
√3, 3
4
√3 × [−1, 2].
5. (a) If (a, b) lies on the curve, then there is some parameter value t1 such that3t11 + t31
= a and 3t211 + t31
= b. If t1 = 0,
the point is (0, 0), which lies on the line y = x. If t1 6= 0, then the point corresponding to t = 1
t1is given by
x =3(1/t1)
1 + (1/t1)3=
3t21t31 + 1
= b, y = 3(1/t1)2
1 + (1/t1)3=
3t1t31 + 1
= a. So (b, a) also lies on the curve. [Another way to see
this is to do part (e) first; the result is immediate.] The curve intersects the line y = x when 3t
1 + t3=
3t2
1 + t3⇒
t = t2 ⇒ t = 0 or 1, so the points are (0, 0) and 32 ,
32.
43
44 ¤ PROBLEMS PLUS
(b) dydt=(1 + t3)(6t)− 3t2(3t2)
(1 + t3)2=6t− 3t4(1 + t3)2
= 0 when 6t− 3t4 = 3t(2− t3) = 0 ⇒ t = 0 or t = 3√2, so there are
horizontal tangents at (0, 0) and 3√2, 3√4 . Using the symmetry from part (a), we see that there are vertical tangents at
(0, 0) and 3√4, 3√2 .
(c) Notice that as t→ −1+, we have x→ −∞ and y →∞. As t→ −1−, we have x→∞ and y → −∞. Also
y − (−x− 1) = y + x+ 1 =3t+ 3t2 + (1 + t3)
1 + t3=(t+ 1)3
1 + t3=
(t+ 1)2
t2 − t+ 1→ 0 as t→ −1. So y = −x− 1 is a
slant asymptote.
(d) dxdt=(1 + t3)(3)− 3t(3t2)
(1 + t3)2=
3− 6t3(1 + t3)2
and from part (b) we have dydt=6t− 3t4(1 + t3)2
. So dy
dx=
dy/dt
dx/dt=
t(2− t3)
1− 2t3 .
Also d2y
dx2=
d
dt
dy
dx
dx/dt=2(1 + t3)4
3(1− 2t3)3 > 0 ⇔ t <13√2.
So the curve is concave upward there and has a minimum point at (0, 0)
and a maximum point at 3√2, 3√4 . Using this together with the
information from parts (a), (b), and (c), we sketch the curve.
(e) x3 + y3 =3t
1 + t3
3
+3t2
1 + t3
3
=27t3 + 27t6
(1 + t3)3=27t3(1 + t3)
(1 + t3)3=
27t3
(1 + t3)2and
3xy = 33t
1 + t33t2
1 + t3=
27t3
(1 + t3)2, so x3 + y3 = 3xy.
(f ) We start with the equation from part (e) and substitute x = r cos θ, y = r sin θ. Then x3 + y3 = 3xy ⇒
r3 cos3 θ + r3 sin3 θ = 3r2 cos θ sin θ. For r 6= 0, this gives r = 3 cos θ sin θ
cos3 θ + sin3 θ. Dividing numerator and denominator
by cos3 θ, we obtain r =3
1
cos θ
sin θ
cos θ
1 +sin3 θ
cos3 θ
=3 sec θ tan θ
1 + tan3 θ.
(g) The loop corresponds to θ ∈ 0, π2, so its area is
A=π/2
0
r2
2dθ =
1
2π/2
0
3 sec θ tan θ
1 + tan3 θ
2
dθ =9
2π/2
0
sec2 θ tan2 θ
(1 + tan3 θ)2dθ =
9
2
∞
0
u2 du
(1 + u3)2[let u = tan θ]
= limb→∞
92− 13 (1 + u3)−1
b
0= 3
2
(h) By symmetry, the area between the folium and the line y = −x− 1 is equal to the enclosed area in the third quadrant,plus twice the enclosed area in the fourth quadrant. The area in the third quadrant is 1
2, and since y = −x− 1 ⇒
r sin θ = −r cos θ − 1 ⇒ r = − 1
sin θ + cos θ, the area in the fourth quadrant is
1
2
−π/4
−π/2− 1
sin θ + cos θ
2
− 3 sec θ tan θ
1 + tan3 θ
2
dθCAS=1
2. Therefore, the total area is 1
2+ 2 1
2= 3
2.