Polar Coordinates and Vectors
9.1 Polar Coordinates
Introduction to polar system as an alternative to the Cartesian coordinate system for plotting points in a plane.
The Cartesian coordinate system labels a point as , 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 .
If r > 0, then is the distance from the point to the pole; is the angle formed by the polar axis and a ray from the pole through the point.
are called the polar coordinates of the point.
Polar Coordinates with Negative r
If r < 0, the point is on the ray from the pole extending in the direction opposite the terminal side of at a distance of 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 , along with the same value for , will yield a different set of coordinates that describes the same point.
If r > 0, any angle coterminal with will work.
If r < 0, any angle coterminal with will work.
All polar coordinates that represent the same point as can be written as or , where .
Conversion from Polar to Cartesian Coordinates
To convert from polar to Cartesian coordinates, use the definitions of trigonometric functions: and .
Multiplying both equations by yields the conversion formulas: and .
Conversion from Cartesian to Polar Coordinates
To convert from Cartesian to polar coordinates:
Use to find .
Use to find , provided that .
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 .
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:
is a horizontal line: a units above the pole if a > 0, a units below the pole if a < 0.
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:
is a circle with radius a and center .
is a circle with radius a and center .
is a circle with radius a and center .
is a circle with radius a and center .
Checking for symmetry can reduce the number of points needed to sketch the graph.
In polar coordinates:
Points and are symmetric with respect to the polar axis (x-axis).
If can be replaced with and the resulting equation is equivalent, the graph is symmetric with respect to the x-axis.
Points and are symmetric with respect to the line (the y-axis).
If can be replaced with and the resulting equation is equivalent, the graph is symmetric with respect to the y-axis.
Points and are symmetric with respect to the pole (origin).
If can be replaced with 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 and finding the resulting value for .
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: or .
With x-axis symmetry: or .
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: or .
With x-axis symmetry: or .
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: or .
With x-axis symmetry: or .
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: or .
With x-axis symmetry: or .
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 and n is an integer with :
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 :
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 , where a and b are real numbers.
Complex numbers can be plotted in the Argand plane (complex plane), where is plotted in the same position as the point in the normal coordinate plane.
Therefore, a complex number can have a polar form: If , then is the polar form for z (a standard shorthand notation for the polar form is ).
In general, , which is the same formula for the magnitude of z ().
Operations with Complex Numbers in Polar Form
Let and be two complex numbers. Then the following properties hold:
Alternately,
DeMoivre's Theorem
If is a complex number and n is a positive integer, then .
Finding Roots of Complex Numbers
Let w and z be complex numbers, and suppose that 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 be a complex number, and let be an integer. If , then there are n distinct complex nth roots of w, given by the formula
, where .
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 (. The zero vector has the property that for any vector 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
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:
if and only if v = 0
Further, if , 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 and be vectors, and let a be a scalar. Then:
$||||||= \sqrt{\alpha1^2 + b1^2} 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 aAs 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