Chapter 6: Problem 18
Show that the shortest path between two given points in a plane is a straight line, using plane polar coordinates.
Short Answer
Expert verified
The shortest path is a straight line, as shown by minimizing the polar coordinate distance formula with \( \theta_2 - \theta_1 = \pi \) or \( -\pi \).
Step by step solution
01
Define the Points in Polar Coordinates
Consider two points in polar coordinates. Let the first point, \( P_1 \), have coordinates \( (r_1, \theta_1) \) and the second point, \( P_2 \), have coordinates \( (r_2, \theta_2) \). In polar coordinates, a point is described by its radial distance \( r \) from the origin and angle \( \theta \) from the positive x-axis.
02
Express Distance in Terms of Polar Coordinates
The distance \( d \) between two points \( (r_1, \theta_1) \) and \( (r_2, \theta_2) \) can be expressed using the polar form of the Euclidean distance formula. This formula is:\[ d = \sqrt{r_1^2 + r_2^2 - 2r_1r_2\cos(\theta_2 - \theta_1)} \]This step involves using the law of cosines where \( \theta_2 - \theta_1 \) is the angle between the line connecting the origin to \( P_1 \) and the line connecting the origin to \( P_2 \).
03
Simplify the Distance Expression
To simplify, we know that the distance formula represents a straight path when the expression inside the square root is minimized. For a fixed \( r_1 \) and \( r_2 \), the expression \[ -2r_1r_2\cos(\theta_2 - \theta_1) \]is minimized (most negative) when \( \cos(\theta_2 - \theta_1) = -1 \), indicating that \( \theta_2 - \theta_1 = \pi \) or \( -\pi \). These correspond to the points lying on a straight line through the origin.
04
Conclude the Shortest Path as a Straight Line
Once it is shown that the expression is minimized under these conditions, the path minimizing the distance \( d \) between \( P_1 \) and \( P_2 \) aligns with the simplest linear path on the polar plane. Thus, the shortest path between the points is indeed a straight line.
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Key Concepts
These are the key concepts you need to understand to accurately answer the question.
Polar Coordinates
In mathematics, polar coordinates offer a fascinating method to describe the position of a point in a plane using a pair of numbers. These numbers are represented as \, \((r, \theta)\), where \(r\) is the radial distance from the origin (the center of the coordinate system) and \(\theta\) is the angle at which the point is located with respect to the positive x-axis.
Key features of polar coordinates include:
These coordinates are especially beneficial in dealing with problems involving circular and rotational symmetry, as they simplify the equations when dealing with curves and circular paths. By applying polar coordinates, you can easily convert between Cartesian and polar systems when necessary.
Key features of polar coordinates include:
- The radial coordinate \, \(r\) tells you how far away the point is from the origin.
- The angular coordinate \, \(\theta\) specifies the direction of the point, measured in radians or degrees.
These coordinates are especially beneficial in dealing with problems involving circular and rotational symmetry, as they simplify the equations when dealing with curves and circular paths. By applying polar coordinates, you can easily convert between Cartesian and polar systems when necessary.
Euclidean Distance
Euclidean distance is a measure of the straight line distance between two points in a plane or space. In a two-dimensional Cartesian plane, this distance is calculated using the Pythagorean theorem:
However, for polar coordinates, the Euclidean distance \, \(d\) formula is adapted to involve trigonometric functions. The distance between two polar coordinates \, \((r_1, \theta_1)\) and \, \((r_2, \theta_2)\) can be expressed as:\[ d = \sqrt{r_1^2 + r_2^2 - 2r_1r_2\cos(\theta_2 - \theta_1)} \]This formula effectively uses the distance formula by integrating the direction (angles) and magnitudes (radii) of the coordinates. The transformation of coordinates and use of trigonometric identities make computation straightforward and useful in various applications, including physics and engineering.
- For two points, \(A(x_1,y_1)\) and \(B(x_2,y_2)\), the Euclidean distance \, \(d\) is calculated as: \(d = \sqrt{(x_2 - x_1)^2 + (y_2 - y_1)^2}\).
However, for polar coordinates, the Euclidean distance \, \(d\) formula is adapted to involve trigonometric functions. The distance between two polar coordinates \, \((r_1, \theta_1)\) and \, \((r_2, \theta_2)\) can be expressed as:\[ d = \sqrt{r_1^2 + r_2^2 - 2r_1r_2\cos(\theta_2 - \theta_1)} \]This formula effectively uses the distance formula by integrating the direction (angles) and magnitudes (radii) of the coordinates. The transformation of coordinates and use of trigonometric identities make computation straightforward and useful in various applications, including physics and engineering.
Law of Cosines
The Law of Cosines is akin to the Pythagorean theorem but extends to cases where a triangle is not necessarily right-angled. It relates the lengths of the sides of a triangle to the cosine of one of its angles. In the context of the shortest path problem, it's applied to connect polar coordinates.
Given a triangle with sides \, \(a\), \, \(b\), and \, \(c\) and the angle \, \(C\) opposite the side \, \(c\), the Law of Cosines states:\[ c^2 = a^2 + b^2 - 2ab\cos(C) \]
In polar coordinate geometry, the Law of Cosines provides a bridge to calculating the straight-line distance between two points by transforming angular differences into linear distances. This forms the base for calculating Euclidean distance in the polar coordinate system.
Given a triangle with sides \, \(a\), \, \(b\), and \, \(c\) and the angle \, \(C\) opposite the side \, \(c\), the Law of Cosines states:\[ c^2 = a^2 + b^2 - 2ab\cos(C) \]
- This relation helps solve for an unknown side when two sides and the included angle are known.
- It simplifies problems involving polar coordinates by reducing them to algebraic equations.
In polar coordinate geometry, the Law of Cosines provides a bridge to calculating the straight-line distance between two points by transforming angular differences into linear distances. This forms the base for calculating Euclidean distance in the polar coordinate system.
Angle Minimization
Angle minimization is crucial in determining the shortest path between two points using polar coordinates. When finding such paths, we aim to minimize expressions involving angles to ensure the calculated distance is the smallest possible.
One critical part of angle minimization is understanding how to use the cosine function's properties. For the cosine function, minimizing involves making \, \(\cos(\theta_2 - \theta_1)\) as negative as possible. Since the most negative cosine value happens at \, \(-1\), the angle difference \, \(\theta_2 - \theta_1\) must be \, \(\pi\) or \, \(-\pi\) for minimal distance. This implies:
Angle minimization therefore aids in proving that the shortest path between two points in a polar coordinate system, essentially, follows a direct, linear course.
One critical part of angle minimization is understanding how to use the cosine function's properties. For the cosine function, minimizing involves making \, \(\cos(\theta_2 - \theta_1)\) as negative as possible. Since the most negative cosine value happens at \, \(-1\), the angle difference \, \(\theta_2 - \theta_1\) must be \, \(\pi\) or \, \(-\pi\) for minimal distance. This implies:
- The straight line condition: When two points align so that their angles with respect to the origin differ by exactly \, \(\pi\), they lie on a straight line.
Angle minimization therefore aids in proving that the shortest path between two points in a polar coordinate system, essentially, follows a direct, linear course.