More calculus with parametric curves

01 Theory - Arclength

Theory 2

Arclength formula

The arclength of a parametric curve with coordinate functions x(t) and y(t) is:

L=∫ab(x′)2+(y′)2dt

This formula assumes the curve is traversed one time as t increases from a to b.

Counts total traversal

This formula applies when the curve image is traversed one time by the moving point.

Sometimes a parametric curve traverses its image with repetitions. The arclength formula would add length from each repetition!

Extra - Derivation of arclength formula

The arclength of a parametric curve is calculated by integrating the infinitesimal arc element:

ds=dx2+dy2L=∫abds

In order to integrate ds in the t variable, as we must for parametric curves, we convert ds to a function of t:

ds=dx2+dy2≫≫1dt2⋅(dx2+dy2)⋅dt2≫≫dx2dt2+dy2dt2⋅dt2≫≫(dxdt)2+(dydt)2dt≫≫ds=x′(t)2+y′(t)2dt

So we obtain ds=(x′)2+(y′)2dt and the arclength formula follows from this:

L=∫ab(x′)2+(y′)2dt
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02 Illustration

Example - Perimeter of a circles

Perimeter of a circle

(1) The perimeter of the circle (Rcos⁡t,Rsin⁡t) is easily found. We have (x′,y′)=(−Rsin⁡t,Rcos⁡t), and therefore:

(x′)2+(y′)2=(−Rsin⁡t)2+(Rcos⁡t)2≫≫R2sin2⁡t+R2cos2⁡t≫≫R2ds=(x′)2+(y′)2dt=Rdt

(2) Integrate around the circle:

Perimeter=∫02πds≫≫∫02πRdt≫≫Rt|02π=2πR Link to original

Example - Perimeter of an asteroid

Perimeter of an asteroid

Find the perimeter length of the ‘asteroid’ given parametrically by (x,y)=(acos3⁡θ,asin3⁡θ) for a=2.

Solution

(1) Notice: Throughout this problem we use the parameter θ instead of t. This does not mean we are using polar coordinates!

Compute the derivatives in θ:

(x′,y′)=(3acos2⁡θsin⁡θ,3asin2⁡θcos⁡θ)

(2) Compute the infinitesimal arc element.

(x′)2+(y′)2≫≫9a2cos4⁡θsin2⁡θ+9a2sin4⁡θcos2⁡θ≫≫9a2sin2⁡θcos2⁡θ(cos2⁡θ+sin2⁡θ)≫≫9a2sin2⁡θcos2⁡θ

Plug into the arc element, simplify:

ds=(x′)2+y′)2dθ≫≫9a2sin2⁡θcos2⁡θdθ≫≫ds=3a|sin⁡θcos⁡θ|dθ

(3) Bounds of integration?

Easiest to use θ∈[0,π/2]. This covers one edge of the asteroid. Then multiply by 4 for the final answer.

On the interval θ∈[0,π/2], the factor 3asin⁡θcos⁡θ is positive. So we can drop the absolute value and integrate directly.

Absolute values matter!

If we tried to integrate on the whole range θ∈[0,2π], then 3asin⁡θcos⁡θ really does change sign.

To perform integration properly with these absolute values, we’d need to convert to a piecewise function by adding appropriate minus signs.


(4) Integrate the arc element:

∫0π/2ds≫≫∫0π/23asin⁡θcos⁡θdθ≫≫3a∫u=01udu(u=sin⁡θ)≫≫3au22|01≫≫3a2

Finally, multiply by 4 to get the total perimeter: L=6a

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03 Theory - Distance, speed

Theory 3

Distance function

The distance function s(t) returns the total distance traveled by the particle from a chosen starting time t0 up to the (input) time t:

s(t)=∫t0tds=∫t0tx′(u)2+y′(u)2du

We need the dummy variable u so that the integration process does not conflict with t in the upper bound.


Speed function

The speed of a moving particle is the rate of change of distance:

v(t)=s′(t)=x′(t)2+y′(t)2

This formula can be explained in either of two ways:

  1. Apply the Fundamental Theorem of Calculus to the integral formula for s(t).
  2. Consider ds=x′(t)2+y′(t)2dt for a small change dt: so the rate of change of arclength is dsdt, in other words s′(t).
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04 Illustration

Example - Speed, distance, displacement

Speed, distance, displacement

The parametric curve (t,23t3/2) describes the position of a moving particle (t measuring seconds). (a) What is the speed function?

Suppose the particle travels for 8 seconds starting at t=0. (b) What is the total distance traveled? (c) What is the total displacement?

Solution

(a)

Compute derivatives:

(x′,y′)=(1,t1/2)

Now compute the speed:

(x′)2+(y′)2=1+(t1/2)2=1+t≫≫v(t)=(x′)2+(y′)2=1+t

(b)

Distance traveled by using speed.

Compute total distance traveled function:

s(t)=∫u=0t1+udu

Substitute w=1+u and dw=du. New bounds are 1 and 1+t. Calculate:

≫≫∫11+twdw≫≫23w3/2|11+t≫≫23((1+t)3/2−1)

The distance traveled up to t=8 is:

s(8)=23(93/2−1)≫≫23(27−1)≫≫523

(c)

Displacement formula: d=(x1−x0)2+(y1−y0)2

Now compute starting and ending points.

For starting point, insert t=0:

(x(t),y(t))|t=0≫≫(t,23t3/2)|t=0≫≫(0,0)

For ending point, insert t=8:

(x(t),y(t))|t=8≫≫(t,23t3/2)|t=8≫≫(8,2383/2)≫≫(8,3223)

Insert (0,0) and (8,322/3):

≫≫82+(3223)2≫≫64+20489≫≫26243 Link to original

05 Theory - Surface area of revolutions

Theory 4

Surface area of a surface of revolution: thin bands

Suppose a parametric curve (x(t),y(t)) is revolved around the x-axis or the y-axis.

The surface area is:

A=∫ab2πR(t)(x′)2+(y′)2dt

The radius R(t) should be the distance to the axis:

R(t)=y(t)revolution about x-axisR(t)=x(t)revolution about y-axis

This formulas adds the areas of thin bands, but the bands are demarcated using parametric functions instead of input values of a graphed function.

The formula assumes that the curve is traversed one time as t increases from a to b.

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06 Illustration

Example - Surface of revolution - parametric circle

Surface of revolution - parametric circle

By revolving the unit upper semicircle about the x-axis, we can compute the surface area of the unit sphere.

Parametrization of the unit upper semicircle:

(x,y)=(cos⁡t,sin⁡t)≫≫(x′,y′)=(−sin⁡t,cos⁡t)

Therefore, the arc element:

ds=(x′)2+(y′)2dt≫≫(−sin⁡t)2+(cos⁡t)2dt≫≫dt

Now for R(t) we choose R(t)=y(t)=sin⁡t because we are revolving about the x-axis.


Plugging all this into the integral formula and evaluating gives:

A=∫0π2πsin⁡tdt≫≫−2πcos⁡t|0π≫≫4π

Notice: This method is a little easier than the method using the graph y=1−x2.

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Example - Surface of revolution - parametric curve

Surface of revolution - parametric curve

Set up the integral which computes the surface area of the surface generated by revolving about the x-axis the curve (t3,t2−1) for 0≤t≤1.

Solution

For revolution about the x-axis, we set R=y(t)=t2−1.

Then compute ds:

ds=(x′)2+(y′)2≫≫(3t2)2+(2t)2≫≫9t4+4t2≫≫t2(9t2+4)≫≫t9t2+4

Therefore the desired integral is:

A=∫012πRds≫≫∫012π(t2−1)t9t2+4dtLink to original

Polar curves

Videos

Review Videos

Videos, Organic Chemistry Tutor

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07 Theory - Polar points, polar curves

Theory 1

Polar coordinates are pairs of numbers (r,θ) which identify points in the plane in terms of distance to origin and angle from +x-axis:

Converting Polar↔Cartesian

Polar→Cartesianx=rcos⁡θy=rsin⁡θCartesian→Polarr=x2+y2tan⁡θ=yx(x≠0)

Polar coordinates have many redundancies: unlike Cartesian which are unique!

  • For example: (r,θ)=(r,θ+2π)
    • And therefore also (r,θ)=(r,θ−2π) (negative θ can happen)
  • For example: (−r,θ)=(r,θ+π) for every r,θ
  • For example: (0,θ)=(0,0) for any θ

Polar coordinates cannot be added: they are not vector components!

  • For example (5,π/3)+(2,π/6)≠(7,π/2)
  • Whereas Cartesian coordinates can be added: (1,4)+(2,−2)=(3,2)

The transition formulas Cartesian→Polar require careful choice of θ.

  • The standard definition of tan−1⁡(yx) sometimes gives wrong θ
    • This is because it uses the restricted domain θ∈(−π/2,π/2); the polar interpretation is: only points in Quadrant I and Quadrant IV (SAFE QUADRANTS)
  • Therefore: check signs of x and y to see which quadrant, maybe need π-correction!
    • Quadrant I or IV: polar angle is tan−1⁡(yx)
    • Quadrant II or III: polar angle is tan−1⁡(yx)+π


Equations (as well as points) can also be converted to polar.

For Cartesian→Polar, look for cancellation from cos2⁡θ+sin2⁡θ=1.

For Polar→Cartesian, try to keep θ inside of trig functions.

  • For example:
r=sin2⁡θ≫≫x2+y2=(yx2+y2)2 Link to original

08 Illustration

Example - Converting to polar: π-correction

Converting to polar: pi-correction

Compute the polar coordinates of (−12,+32) and of (+22,−22).

Solution

For (−12,32) we observe first that it lies in Quadrant II.

Next compute:

tan−1⁡(3/2−1/2)≫≫tan−1⁡(−3)≫≫−π/3

This angle is in Quadrant IV. We add π to get the polar angle in Quadrant II:

θ=π−π/3≫≫2π/3

The radius is of course 1 since this point lies on the unit circle. Therefore polar coordinates are (r,θ)=(1,2π/3).

For (+22,−22) we observe first that it lies in Quadrant IV. (No extra π needed.)

Next compute:

tan−1⁡(−2/2+2/2)≫≫tan−1⁡(−1)≫≫−π/4

So the point in polar is (1,−π/4).

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Example - Shifted circle in polar

Shifted circle in polar

For example, let’s convert a shifted circle to polar. Say we have the Cartesian equation:

x2+(y−3)2=9

Then to find the polar we substitute x=rcos⁡θ and y=rsin⁡θ and simplify:

x2+(y−3)2=9≫≫r2cos2⁡θ+(rsin⁡θ−3)2=9≫≫r2cos2⁡θ+r2sin2⁡θ−6rsin⁡θ+9=9≫≫r2(sin2⁡θ+cos2⁡θ)−6rsin⁡θ=0≫≫r2−6rsin⁡θ=0≫≫r=6sin⁡θ

So this shifted circle is the polar graph of the polar function r(θ)=6sin⁡θ.

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