College Physics II – Mechanics, Sound, Oscillations, and Waves
Definition
The polar coordinate system represents points in a plane using a distance from a reference point (the origin) and an angle from a reference direction (usually the positive x-axis). It is commonly used in physics to simplify the analysis of rotational systems and wave functions.
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In polar coordinates, any point in the plane is described by two values: radius $r$ and angle $\theta$.
The conversion between Cartesian coordinates $(x, y)$ and polar coordinates $(r, \theta)$ is given by $x = r \cos(\theta)$ and $y = r \sin(\theta)$.
The angle $\theta$ is measured counterclockwise from the positive x-axis and can be expressed in radians or degrees.
Vectors can be represented in polar form as magnitude and direction, which are often easier to work with for problems involving circular motion or oscillations.
Polar coordinates are particularly useful in solving problems with symmetry about a point, such as gravitational fields around a planet or electromagnetic waves emanating from an antenna.
Review Questions
How do you convert the Cartesian coordinates (3, 4) into polar coordinates?
What are the polar coordinates of a point located at (0, -5) in Cartesian coordinates?
Why might one prefer using polar coordinates over Cartesian coordinates when dealing with circular motion?
Related terms
Cartesian Coordinate System: A coordinate system that specifies each point uniquely by a pair of numerical coordinates $(x, y)$ representing distances along perpendicular axes.
Projections of a vector along the axes of the coordinate system; in Cartesian coordinates, these components are typically labeled as $V_x$ and $V_y$.
Radians: A unit of angular measure used in many areas of mathematics. One radian is defined as the angle subtended at the center of a circle by an arc whose length is equal to its radius.