Polar Coordinates and Vectors

9.1 Polar Coordinates

  • Introduction to polar coordinatecoordinate system as an alternative to the Cartesian coordinate system for plotting points in a plane.

  • The Cartesian coordinate system labels a point as (x,y)(x, y), representing the signed distance from the y-axis and x-axis, respectively.

  • In the polar coordinate system, the origin is called the pole, and points are described relative to the pole.

  • The polar axis is the positive x-axis.

  • A point in the polar coordinate system is represented by an ordered pair (r,θ)(r, \theta).

    • If r > 0, then rr is the distance from the point to the pole; theta\,theta is the angle formed by the polar axis and a ray from the pole through the point.

    • (r,θ)(r, \theta) are called the polar coordinates of the point.

Polar Coordinates with Negative r

  • If r < 0, the point (r,θ)(r, \theta) is on the ray from the pole extending in the direction opposite the terminal side of theta\,theta at a distance of r|r| units from the pole.

Non-Unique Coordinates in Polar System

  • One drawback of the polar coordinate system is that points do not have unique coordinates.

  • Any angle coterminal with theta\,theta, along with the same value for rr, will yield a different set of coordinates that describes the same point.

  • If r > 0, any angle coterminal with fracpi4\,frac{\,pi}{4} will work.

  • If r < 0, any angle coterminal with 5pi4\frac{5\,pi}{4} will work.

  • All polar coordinates that represent the same point as (2,pi4)(2, \frac{\,pi}{4}) can be written as (2,pi4+2pik)(2, \frac{\,pi}{4} + 2\,pi k) or (2,5pi4+2pik)(-2, \frac{5\,pi}{4} + 2\,pi k), where kZk \in \mathbb{Z}.

Conversion from Polar to Cartesian Coordinates

  • To convert from polar to Cartesian coordinates, use the definitions of trigonometric functions: cosθ=xr\,cos \theta = \frac{x}{r} and sinθ=yr\,sin \theta = \frac{y}{r}.

  • Multiplying both equations by rr yields the conversion formulas: x=rcosθx = r \,cos \theta and y=rsinθy = r \,sin \theta.

Conversion from Cartesian to Polar Coordinates

  • To convert from Cartesian to polar coordinates:

    • Use x2+y2=r2x^2 + y^2 = r^2 to find rr.

    • Use tantheta=yxtan \,theta = \frac{y}{x} to find theta\,theta, provided that x0x \neq 0.

Transforming Equations Between Coordinate Systems

  • The equations used to convert points between systems can also transform equations.

  • Two common techniques to transform from polar to rectangular form:

    • Multiply both sides of the equation by rr.

    • Square both sides of the equation.

9.2 Polar Equations & Graphs

  • To sketch polar graphs, use a polar grid consisting of concentric circles and lines.

  • One way to sketch polar graphs is to transform the polar equation into a rectangular one.

  • Let a ≠ 0. Then:

    • rsinθ=ar \,sin \theta = a is a horizontal line: a units above the pole if a > 0, a units below the pole if a < 0.

    • rcosθ=ar \,cos \theta = a is a vertical line: a units to the right of the pole if a > 0, a units to the left of the pole if a < 0.

  • Let a > 0. Then:

    • r=2asinθr = 2a \,sin \theta is a circle with radius a and center (0,a)(0, a).

    • r=2asinθr = -2a \,sin \theta is a circle with radius a and center (0,a)(0, -a).

    • r=2acosθr = 2a \,cos \theta is a circle with radius a and center (a,0)(a, 0).

    • r=2acosθr = -2a \,cos \theta is a circle with radius a and center (a,0)(-a, 0).

  • Checking for symmetry can reduce the number of points needed to sketch the graph.

  • In polar coordinates:

    • Points (r,θ)(r, \theta) and (r,θ)(r, -\theta) are symmetric with respect to the polar axis (x-axis).

    • If theta\,theta can be replaced with theta-{\,theta} and the resulting equation is equivalent, the graph is symmetric with respect to the x-axis.

    • Points (r,θ)(r, \theta) and (r,piθ)(r, \,pi - \theta) are symmetric with respect to the line θ=pi2\theta = \frac{\,pi}{2} (the y-axis).

    • If theta\,theta can be replaced with piθ\,pi - \theta and the resulting equation is equivalent, the graph is symmetric with respect to the y-axis.

    • Points (r,θ)(r, \theta) and (r,θ)(-r, \theta) are symmetric with respect to the pole (origin).

    • If rr can be replaced with r-r and the resulting equation is equivalent, the graph is symmetric with respect to the origin.

  • A second method for sketching polar graphs is to plot points by plugging in values for theta\,theta and finding the resulting value for rr.

Cardioid

  • A cardioid is a heart-shaped curve.

  • Cardioids can be written in one of the following forms, where a > 0:

    • With y-axis symmetry: r=a(1+sinθ)r = a(1 + \,sin \theta) or r=a(1sinθ)r = a(1 - \,sin \theta).

    • With x-axis symmetry: r=a(1+cosθ)r = a(1 + \,cos \theta) or r=a(1cosθ)r = a(1 - \,cos \theta).

  • All cardioids will pass through the pole.

Limaçon without a Loop

  • Limaçons without loops can be written in one of the following forms, where a > b > 0:

    • With y-axis symmetry: r=a+bsinθr = a + b \,sin \theta or r=absinθr = a - b \,sin \theta.

    • With x-axis symmetry: r=a+bcosθr = a + b \,cos \theta or r=abcosθr = a - b \,cos \theta.

  • All limaçons without loops will not pass through the pole.

Limaçon with an Inner Loop

  • Limaçons with inner loops can be written in one of the following forms, where b > a > 0:

    • With y-axis symmetry: r=a+bsinθr = a + b \,sin \theta or r=absinθr = a - b \,sin \theta.

    • With x-axis symmetry: r=a+bcosθr = a + b \,cos \theta or r=abcosθr = a - b \,cos \theta.

  • All limaçons with inner loops will pass through the pole twice.

  • All cardioids and limaçons (with or without loops) have one of the following equations, where a and b are positive real numbers:

    • With y-axis symmetry: r=a+bsinθr = a + b \,sin \theta or r=absinθr = a - b \,sin \theta.

    • With x-axis symmetry: r=a+bcosθr = a + b \,cos \theta or r=abcosθr = a - b \,cos \theta.

  • The distinction between types comes from the relationship between a and b:

    • If a = b, the graph is a cardioid.

    • If a > b, the graph is a limaçon without a loop.

    • If a < b, the graph is a limaçon with an inner loop.

Rose Curves

  • All roses can be written in one of the following forms, where a0a \neq 0 and n is an integer with n0,±1n \neq 0, \pm 1:

    • r=acos(ntheta)r = a \,cos(n \,theta)

    • r=asin(ntheta)r = a \,sin(n \,theta)

    • If n is even, the graph has 2n petals. If n is odd, the graph has n petals.

Lemniscates

  • All lemniscates can be written in one of the following forms, where a0a \neq 0:

    • r2=a2sin(2theta)r^2 = a^2 \,sin(2 \,theta)

    • r2=a2cos(2theta)r^2 = a^2 \,cos(2 \,theta)

  • All lemniscates have graphs shaped like propellers.

Spirals

  • Spirals can have a variety of equation types, so those are a little harder to classify.

9.3 Polar Form for Complex Numbers

  • A complex number is a number in the form a+bia + bi, where a and b are real numbers.

  • Complex numbers can be plotted in the Argand plane (complex plane), where a+bia + bi is plotted in the same position as the point (a,b)(a, b) in the normal coordinate plane.

  • Therefore, a complex number can have a polar form: If z=a+biz = a + bi, then z=(rcosθ)+(rsinθ)i=r(cosθ+isinθ)z = (r \,cos \theta) + (r \,sin \theta)i = r(\,cos \theta + i \,sin \theta) is the polar form for z (a standard shorthand notation for the polar form is z=rcisθz = r \,cis \theta).

  • In general, r=a2+b2r = \sqrt{a^2 + b^2}, which is the same formula for the magnitude of z (z=r|z| = r).

Operations with Complex Numbers in Polar Form

  • Let z<em>1=r</em>1(cosθ<em>1+isinθ</em>1)z<em>1 = r</em>1(\,cos \theta<em>1 + i \,sin \theta</em>1) and z<em>2=r</em>2(cosθ<em>2+isinθ</em>2)z<em>2 = r</em>2(\,cos \theta<em>2 + i \,sin \theta</em>2) be two complex numbers. Then the following properties hold:

    • z<em>1z</em>2=r<em>1r</em>2(cos(θ<em>1+θ</em>2)+isin(θ<em>1+θ</em>2))z<em>1 z</em>2 = r<em>1 r</em>2 (\,cos(\theta<em>1 + \theta</em>2) + i \,sin(\theta<em>1 + \theta</em>2))

    • z<em>1z</em>2=r<em>1r</em>2(cos(θ<em>1θ</em>2)+isin(θ<em>1θ</em>2))\frac{z<em>1}{z</em>2} = \frac{r<em>1}{r</em>2} (\,cos(\theta<em>1 - \theta</em>2) + i \,sin(\theta<em>1 - \theta</em>2))

  • Alternately,

    • (r<em>1cisθ</em>1)(r<em>2cisθ</em>2)=r<em>1r</em>2cis(θ<em>1+θ</em>2)(r<em>1 \,cis \theta</em>1)(r<em>2 \,cis \theta</em>2) = r<em>1 r</em>2 \,cis(\theta<em>1 + \theta</em>2)

    • r<em>1cisθ</em>1r<em>2cisθ</em>2=r<em>1r</em>2cis(θ<em>1θ</em>2)\frac{r<em>1 \,cis \theta</em>1}{r<em>2 \,cis \theta</em>2} = \frac{r<em>1}{r</em>2} \,cis(\theta<em>1 - \theta</em>2)

DeMoivre's Theorem

  • If z=r(cosθ+isinθ)z = r(\,cos \theta + i \,sin \theta) is a complex number and n is a positive integer, then zn=rn(cos(ntheta)+isin(ntheta))z^n = r^n (\,cos(n \,theta) + i \,sin(n \,theta)).

Finding Roots of Complex Numbers

  • Let w and z be complex numbers, and suppose that zn=wz^n = w for some positive integer n. In this case, we call z a complex nth root of w.

  • When w = 1, the values of z are called the nth roots of unity.

  • Let w=r(cosθ+isinθ)w = r(\,cos \theta + i \,sin \theta) be a complex number, and let n2n \geq 2 be an integer. If w0w \neq 0, then there are n distinct complex nth roots of w, given by the formula

    • zk=rncis(theta+2kpin)z_k = \sqrt[n]{r} \,\,\,\,\,\,\,\,\,\,\, cis(\frac{\,theta + 2k\,pi}{n} ), where k=0,1,2,,n1k = 0, 1, 2, …, n-1.

9.4 - Vectors

  • A vector is a quantity with both magnitude and direction.

  • It is customary to write a vector as an arrow-the length of the arrow indicates the vector's magnitude while the arrowhead indicates the vector's direction.

  • If P and Q are two distinct points in the coordinate plane, there is exactly one line through them. The points on the line joining P and Q is called the line segment PQ.

  • If we order the points so that they proceed from P to Q, we have a directed line segment, or geometric vector, denoted as PQ. In this directed line segment, we call P the initial point and Q the terminal point.

  • The magnitude of this vector is simply the distance between points P and Q.

  • If a vector v has the same magnitude and direction as PQ, then we write v = PQ (some books use boldface type rather than write the arrows over the quantity in order to distinguish a vector from a number). We call these vectors equal.

  • The zero vector, 0, is the vector whose magnitude is 0, and we generally don't assign it any direction.

  • The sum v+w of two vectors is defined as follows: position the two vectors so that the terminal point of ✓ coincides with the initial point of w. The vector v+w is defined to be the vector whose initial point is the initial point of v and whose terminal point is the terminal point of w.

  • Vector addition is commutative (u+v=V+u), and associative (uˉ+(vˉ+wˉ)=(uˉ+vˉ)+wˉ)\bar{u}+ (\bar{v}+\bar{w}) = (\bar{u}+\bar{v})+\bar{w}). The zero vector has the property that for any vector v,
    vˉ+0=0+vˉ=vˉ\bar{v}+ 0 = 0 + \bar{v} = \bar{v}''

  • If v is a vector, then -v is a vector with the same magnitude as v but opposite direction.

  • Clearly, based on this definition, v+(-v)=0.

  • The difference v-w of two vectors is defined as follows: v-w=v+(-w).

  • A scalar is a real quantity that only has magnitude. If a is a scalar and v is a vector, the scalar multiple av is defined as follows:

    • If a>0, av is the vector whose magnitude is a times the magnitude of v and whose direction is the same as v.

    • If a<0, av is the vector whose magnitude is a times the magnitude of v and whose direction is opposite that of v.

    • If α=0 or if v = 0, then av=0.

  • Scalar multiples have the following properties, where v is a vector:

    • 1v=v

    • -1v =-V

    • (α+β)v=αv+βv(\alpha + \beta)v= \alpha v + \beta v

    • α(v+w)=αv+αw\alpha (v+w)=\alpha v+\alpha w

    • α(βv)=(αβ)v\alpha (\beta v)=(\alpha \beta)v

  • We use the symbol || to represent the magnitude of vector V, which will represent the length of v. Because of this, the following properties hold for V, where v is a vector and α is a scalar:

    • v=0||v||=0 if and only if v = 0

    • αv=αv||\alpha v||=||\alpha| \,||v||

  • Further, if v=1||v||=1, we call ū a unit vector.

  • Algebraically, we represent a vector ✓ as ✓ = (a,b), where a and b are real numbers called the components of V. If the initial point of v = (a,b) is the origin, then we call v a position vector. If v = (a,b) is a position vector, then its terminal point is the ordered pair (a,b).

  • Because any vectors with the same magnitude and direction are equal, we can see that if a vector v has initial point P₁ (✗₁,Y₁) and terminal point P2(X2,Y₂), then v=P₁₁₂ is equal to the position vector (×2 − × ₁, Y₂ — Y₁):

  • Two position vectors are equal if and only if they have the same terminal point.

  • Therefore, two vectors v and w are equal if and only if their corresponding components are equal; i.e., if v = (a₁,b₁) and w = (a₂, b₂), then v=w if and only if α₁ =α₂ and b₁ = b₂.

  • An alternate algebraic notation for vectors, common in physical sciences, is as follows:

    • Let /= (1,0) be the unit vector whose direction is along the positive x-axis, and let j = (0,1) be the unit vector whose direction is along the positive y-axis. Any vector v = (a,b) may be written as v = (a,b) = a(1,0)+b(0,1)=ai+bj, and we call a and b the horizontal and vertical components of V, respectively. For example, for v = (5,4)=57+4j, 5 is the horizontal component while 4 is the vertical component.

  • Let v=α<em>1i+b</em>1j=(α<em>1,b</em>1)v=\alpha<em>1i+b</em>1j = (\alpha<em>1 ,b</em>1) and w=α<em>2i+b</em>2j=(α<em>2,b</em>2)w=\alpha<em>2i+b</em>2j = (\alpha<em>2 ,b</em>2) be vectors, and let a be a scalar. Then:
    +wˉ=(α<em>1+α</em>2)i+(b<em>1+b</em>2)j=(a<em>1+a</em>2),(b<em>1+b</em>2)\,\,\,+ \bar{w}=\,(\alpha<em>1 + \alpha</em>2) i +\, (b<em>1 +b</em>2) j = (a<em>1 +a</em>2), (b<em>1 + b</em>2)
    wˉ=(α<em>1α</em>2)i+(b<em>1b</em>2)j=(a<em>1a</em>2);(b<em>1b</em>2)\,\,\,-\bar{w}= (\,\alpha<em>1 - \alpha</em>2) i + (b<em>1 - b</em>2) j = (a<em>1 - a</em>2 );(b<em>1 -b</em>2)
    αv=(αa<em>1)i+( alphab</em>1)j=(αa<em>1),(αb</em>1)\,\,\,\alpha v= (\alpha a<em>1) i+ (\ alpha b</em>1)j= (\, \alpha a<em>1), (\alpha b</em>1)
    $||||||= \sqrt{\alpha1^2 + b1^2}</p></li><li><p>Foranynonzerovector,thevectoruˉ=</p></li><li><p>For any nonzero vector ✓, the vector ū= v/||v|| is a unit vector in the same direction as v.
    same direction since u = (1/||V||) v
    is a
    positive scalar multiple
    magnitude, since ||u|| ||1/||V||| ||V|| = 1
    is a

  • As a consequence of this, if u is a unit vector in the same direction as vector v, then
    v=||V||u.

  • If a vector represents the speed and direction of an object, it is called a velocity vector. If a vector represents the direction and amount of force acting on an object, it is called a force vector. In many applications, a vector is described in terms of its magnitude and direction (ex. projectile launched at 25 miles per hour at 30° angle of inclination) rather than in terms of its components. Therefore, suppose we are given the magnitude || of a nonzero vector ✓ and the direction angle a, 0° ≤a<360°

  • between v and i. Using standard position trigonometry and the definitions of sine and cosine in reference to the standard position angle on the unit circle, we can determine that ū=(cosa)+(sina)]. Along with the formula v = ||||u
    v=||((cosa)+(sina)])=(|||cosa)+(||sina)=(cosa,sina)

  • Since forces can be represented by vectors, two forces