/*! This file is auto-generated */ .wp-block-button__link{color:#fff;background-color:#32373c;border-radius:9999px;box-shadow:none;text-decoration:none;padding:calc(.667em + 2px) calc(1.333em + 2px);font-size:1.125em}.wp-block-file__button{background:#32373c;color:#fff;text-decoration:none} Problem 53 Find an equation in \(x\) and \(... [FREE SOLUTION] | 91Ó°ÊÓ

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Find an equation in \(x\) and \(y\) that has the same graph as the polar equation. Use it to help sketch the graph in an \(r \theta\) -plane. $$r(\sin \theta-2 \cos \theta)=6$$

Short Answer

Expert verified
The equivalent rectangular equation is \(y = 2x + 6\), a straight line.

Step by step solution

01

Expand the given polar equation

The given polar equation is \(r(\sin \theta - 2 \cos \theta) = 6\). Expand this equation by multiplying \(r\) with each term inside the bracket: \[ r \sin \theta - 2r \cos \theta = 6 \]
02

Convert to rectangular coordinates

In polar coordinates, we can use the transformations \(x = r \cos \theta\) and \(y = r \sin \theta\). Substitute these into the equation:\[ y - 2x = 6 \] which is the equation in rectangular coordinates.
03

Solve for y

To find the expression for \(y\), add \(2x\) to both sides of the equation:\[ y = 2x + 6 \]
04

Sketch the graph in the \(r \theta\)-plane

The derived equation \(y = 2x + 6\) is a straight line with a slope of 2 and y-intercept 6. Use the equivalent polar transformations to sketch in an \(r \theta\) plane, noting this straight line becomes a linear relationship in polar form, altered by the trigonometric transformations.

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Key Concepts

These are the key concepts you need to understand to accurately answer the question.

Polar Coordinates
Polar coordinates offer a unique way to describe points in a plane. Instead of using horizontal and vertical distances, known as Cartesian coordinates, polar coordinates use a combination of a radius and an angle.
In polar coordinates, a point is represented as \( (r, \theta) \), where \( r \) is the distance from the origin (also called the pole), and \( \theta \) is the angle measured from the positive x-axis. This system is especially useful in scenarios involving circular or spiral shapes and in fields like robotics and navigation.
It is important to remember that in the polar coordinate system, different pairs \( (r, \theta) \) can represent the same point on the plane due to the periodic nature of the trigonometric functions used to define these coordinates.
Rectangular Coordinates
Rectangular coordinates, often known as Cartesian coordinates, are the most common way to describe locations in a 2D plane. Here, each point is defined by two values, \( (x, y) \). These values represent distances along two perpendicular axes: the x-axis (horizontal) and y-axis (vertical).
One key property of rectangular coordinates is their ability to easily describe linear relationships. For example, the equation \( y = 2x + 6 \) defines a straight line with a specific slope and y-intercept.
The conversion from polar coordinates to rectangular coordinates involves using the formulas:
  • \( x = r \cos \theta \)
  • \( y = r \sin \theta \)
This transformation translates the radial and angular information of polar coordinates into the horizontal and vertical positioning of rectangular coordinates.
Graphing
Graphing is a visual way to represent equations and illustrate mathematical concepts. It transforms abstract numbers into shapes and lines, offering a better understanding of the relationships they describe.
When graphing equations, such as \( y = 2x + 6 \), we plot points on a graph by calculating coordinates. The function describes a line with a slope of 2, indicating that for every unit increase in x, the value of y increases by 2. This helps visualize which way the line leans and how steep it is.
Graphing in a polar plane is different than in a rectangular coordinate system. The transformation can sometimes alter the shape of the graph, especially when representing a polar equation with trigonometric functions. However, through graphing, we can see how equations translate into spatial orientation.
Linear Equations
Linear equations express the relationship between two variables along a straight line, typically structured as \( y = mx + c \), where \( m \) stands for slope and \( c \) for the y-intercept. This form makes it straightforward to determine how one variable changes in relation to the other.
In the context of converting polar equations to rectangular, the linear equation derived reflects a constant rate of change, indicating a linear progression or relationship.
Using the equation \( y = 2x + 6 \) as an example, \( m = 2 \), indicating the line rises by 2 units for each 1 unit moved horizontally. \( c = 6 \) tells us where the line crosses the y-axis, giving a visual starting point on a graph. Understanding linear equations is crucial for analyzing and predicting relationships in various mathematical and real-world applications.

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Most popular questions from this chapter

Cooling tower A cooling tower, such as the one shown in the figure, is a hyperbolic structure. Suppose its base diameter is 100 meters and its smallest diameter of 48 meters occurs 84 meters from the base. If the tower is 120 meters high, approximate its diameter at the top. GRAPH CANT COPY

Polar equations of conics can be used to describe the motion of comets. These paths can be graphed using the polar equation $$r=\frac{r_{p e r}(1+e)}{1-e \cos \theta}$$ where \(e\) is the eccentricity of the conic and \(r_{\mathrm{per}}\) is the perihelion distance measured in AU. (a) For each comet, determine whether its trajectory is elliptical, parabolic, or hyperbolic. (b) The orbit of Saturn has \(r_{\text {per }}=9.006\) and \(e=0.056\) Graph both the motion of the comet and the orbit of Saturn in the specified viewing rectangle. Encke's Comet \(\quad r_{\text {per }}=0.3317, \quad e=0.8499\) $$[-18,18,3] \text { by }[-12,12,3]$$

Kepler's first law asserts that planets travel in elliptical orbits with the sun at one focus. To find an equation of an orbit, place the pole \(O\) at the center of the sun and the polar axis along the major axis of the ellipse (see the figure). (a) Show that an equation of the orbit is $$r=\frac{\left(1-e^{2}\right) a}{1-e \cos \theta}$$ where \(e\) is the eccentricity and \(2 a\) is the length of the major axis. (b) The perihelion distance \(r_{\text {per }}\) and aphelion distance \(r_{\text {aph }}\) are defined as the minimum and maximum distances, respectively, of a planet from the sun. Show that \(r_{\text {per }}=a(1-e) \quad\) and \(\quad r_{\text {aph }}=a(1+e)\) (IMAGE CAN NOT COPY)

Sketch the graph of the polar equation. $$r=2 \theta, \theta \geq 0$$

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