offer a powerful way to describe points in 3D space using radius, , and . This system is especially useful for problems with spherical symmetry, like calculating volumes of spheres or analyzing radial fields.

Understanding the relationships between spherical and is crucial for solving complex 3D problems. The and are key tools for performing triple integrals, enabling us to tackle a wide range of real-world applications.

Spherical Coordinate System

Coordinate System Components

Top images from around the web for Coordinate System Components
Top images from around the web for Coordinate System Components
  • Spherical coordinates define a point in 3D space using radius, polar angle, and azimuthal angle
  • Radius (ρ) measures the distance from the origin to the point
    • Always non-negative (ρ0ρ ≥ 0)
  • Polar angle (θ) measures the angle between the positive z-axis and the line from origin to point
    • Range is 0θπ0 ≤ θ ≤ π
    • θ=0θ = 0 corresponds to positive z-axis, θ=π/2θ = π/2 corresponds to xy-plane, θ=πθ = π corresponds to negative z-axis
  • Azimuthal angle (φ) measures the angle in the xy-plane from positive x-axis to the projection of line from origin to point
    • Range is 0φ<2π0 ≤ φ < 2π
    • φ=0φ = 0 corresponds to positive x-axis, φ=π/2φ = π/2 to positive y-axis, φ=πφ = π to negative x-axis, φ=3π/2φ = 3π/2 to negative y-axis

Coordinate Relationships

  • Points with same radius ρρ lie on a sphere centered at origin
  • Points with same polar angle θθ lie on a circular cone with vertex at origin and axis along the z-axis
    • Angle between cone and z-axis is θθ
  • Points with same azimuthal angle φφ lie on a vertical half-plane emanating from z-axis
    • Half-plane makes angle φφ with the xz-plane

Coordinate Transformations

Cartesian to Spherical

  • Given Cartesian coordinates (x,y,z)(x, y, z), spherical coordinates (ρ,θ,φ)(ρ, θ, φ) are:
    • ρ=x2+y2+z2ρ = \sqrt{x^2 + y^2 + z^2}
    • θ=arccos(zx2+y2+z2)θ = \arccos(\frac{z}{\sqrt{x^2 + y^2 + z^2}})
      • If ρ=0ρ = 0, θθ is undefined
    • φ=arctan(yx)φ = \arctan(\frac{y}{x})
      • If x>0x > 0, φ=arctan(yx)φ = \arctan(\frac{y}{x})
      • If x<0x < 0 and y0y ≥ 0, φ=arctan(yx)+πφ = \arctan(\frac{y}{x}) + π
      • If x<0x < 0 and y<0y < 0, φ=arctan(yx)πφ = \arctan(\frac{y}{x}) - π
      • If x=0x = 0 and y>0y > 0, φ=π/2φ = π/2
      • If x=0x = 0 and y<0y < 0, φ=π/2φ = -π/2
      • If x=0x = 0 and y=0y = 0, φφ is undefined

Spherical to Cartesian

  • Given spherical coordinates (ρ,θ,φ)(ρ, θ, φ), Cartesian coordinates (x,y,z)(x, y, z) are:
    • x=ρsinθcosφx = ρ \sin θ \cos φ
    • y=ρsinθsinφy = ρ \sin θ \sin φ
    • z=ρcosθz = ρ \cos θ

Jacobian Determinant

  • The Jacobian determinant J|J| is used for change of variables in multiple integrals
  • For transformation from Cartesian (x,y,z)(x, y, z) to spherical (ρ,θ,φ)(ρ, θ, φ):
\frac{∂x}{∂ρ} & \frac{∂x}{∂θ} & \frac{∂x}{∂φ} \\ \frac{∂y}{∂ρ} & \frac{∂y}{∂θ} & \frac{∂y}{∂φ} \\ \frac{∂z}{∂ρ} & \frac{∂z}{∂θ} & \frac{∂z}{∂φ} \end{vmatrix} = ρ^2 \sin θ$$ ## Integration in Spherical Coordinates ### Volume Element - The volume element $dV$ in spherical coordinates is the Jacobian determinant $|J|$ multiplied by the differentials: $$dV = |J| dρ dθ dφ = ρ^2 \sin θ dρ dθ dφ$$ - Triple integrals in spherical coordinates have the form: $$\iiint_E f(ρ,θ,φ) ρ^2 \sin θ dρ dθ dφ$$ - $E$ is the region of integration - $f(ρ,θ,φ)$ is the integrand function in spherical coordinates - Order of integration is typically $dρ$ first, then $dθ$, then $dφ$ - Limits of integration depend on the specific region $E$

Key Terms to Review (13)

Azimuthal angle: The azimuthal angle is a spherical coordinate that represents the angle in the horizontal plane, measured from a reference direction, usually the positive x-axis. This angle helps describe the orientation of a point in three-dimensional space, playing a key role in various coordinate transformations and integrals.
Cartesian Coordinates: Cartesian coordinates are a system that uses ordered pairs or triples of numbers to specify the position of points in a plane or space. They provide a way to represent geometric figures and analyze relationships between points, lines, and shapes in two or three dimensions, making them essential for various mathematical applications.
Change of Variables Theorem: The change of variables theorem is a powerful tool in calculus that allows for the evaluation of integrals by transforming them from one coordinate system to another, which can simplify the process. This theorem is particularly useful when working with integrals in polar or spherical coordinates, enabling the conversion of complex regions into more manageable shapes.
Coordinate transformation: Coordinate transformation refers to the process of converting coordinates from one system to another, allowing for different perspectives on geometric shapes and mathematical problems. This concept is crucial as it facilitates the transition between various coordinate systems, such as Cartesian, polar, cylindrical, and spherical, which helps in simplifying equations and computations in different contexts.
Integration bounds: Integration bounds refer to the specific limits that define the range of integration in a definite integral. These bounds establish the interval over which a function is integrated, playing a crucial role in determining the area under the curve or the volume in multi-dimensional spaces, particularly when transforming coordinates, like from Cartesian to spherical systems.
Jacobian Determinant: The Jacobian determinant is a scalar value that represents the rate of change of a function with respect to its variables, particularly when transforming coordinates from one system to another. It is crucial for understanding how volume and area scale under these transformations, and it plays a significant role in evaluating integrals across different coordinate systems.
Polar angle: The polar angle is a coordinate that represents the angle formed between a reference direction, typically the positive z-axis, and the line connecting the origin to a point in three-dimensional space in spherical coordinates. This angle helps define the position of a point in relation to the vertical axis and is essential for converting between Cartesian and spherical coordinate systems.
Spherical coordinates: Spherical coordinates are a three-dimensional coordinate system that uses a radius, an angle from the vertical axis, and an angle in the horizontal plane to specify the position of a point in space. This system is particularly useful in evaluating triple integrals, calculating volumes and masses, and transforming coordinates for easier integration in complex geometries.
Triple Integral: A triple integral is a mathematical operation used to compute the volume under a surface defined by a function of three variables, typically denoted as $$f(x,y,z)$$, over a three-dimensional region. It extends the concept of double integrals to three dimensions, allowing for the evaluation of quantities like mass, volume, and charge density across three-dimensional shapes.
Volume element in spherical coordinates: The volume element in spherical coordinates, denoted as $dV$, is a differential element that represents an infinitesimal volume in three-dimensional space using spherical coordinates. It is expressed mathematically as $dV = r^2 \sin(\theta) \, dr \, d\theta \, d\phi$, where $r$ is the radial distance from the origin, $\theta$ is the polar angle measured from the positive z-axis, and $\phi$ is the azimuthal angle in the xy-plane. This expression shows how the volume element changes depending on the position in space and highlights the geometry of spherical coordinates compared to Cartesian coordinates.
X = ρ sin(φ) cos(θ): The equation x = ρ sin(φ) cos(θ) represents the Cartesian coordinate x in the spherical coordinate system, where ρ is the radial distance from the origin, φ is the polar angle measured from the positive z-axis, and θ is the azimuthal angle measured from the positive x-axis. This equation is crucial for transforming spherical coordinates into Cartesian coordinates, allowing for easier calculations and visualizations in three-dimensional space.
Y = ρ sin(φ) sin(θ): The equation $y = \rho \sin(\phi) \sin(\theta)$ describes the y-coordinate in a spherical coordinate system, which represents a point in three-dimensional space. This coordinate system is defined by three parameters: the radial distance $\rho$, the polar angle $\phi$, and the azimuthal angle $\theta$. The relationship allows for conversion between Cartesian and spherical coordinates, which is essential for solving various problems in calculus and physics.
Z = ρ cos(φ): The equation z = ρ cos(φ) defines the relationship between the Cartesian and spherical coordinate systems, specifically in how the vertical coordinate (z) relates to the spherical coordinates (ρ and φ). In this context, ρ represents the radial distance from the origin to a point in space, while φ is the angle from the positive z-axis down to that point. This transformation helps to convert points in three-dimensional space from spherical coordinates into Cartesian coordinates, which are often more intuitive to work with in many applications.
© 2024 Fiveable Inc. All rights reserved.
AP® and SAT® are trademarks registered by the College Board, which is not affiliated with, and does not endorse this website.