Spherical Wedge — Definition, Formula & Examples
A spherical wedge is the 3D region of a sphere enclosed between two half-planes that meet along a diameter. Think of it as a thick slice of an orange, where the blade cuts from the center outward on two sides.
Given a sphere of radius and a dihedral angle (in radians) formed by two half-planes sharing a common diameter, the spherical wedge (also called an ungula) is the solid region bounded by the sphere's surface and the two half-planes.
Key Formula
Where:
- = Volume of the spherical wedge
- = Radius of the sphere
- = Dihedral angle between the two half-planes, in radians
How It Works
A spherical wedge is defined by two ingredients: the sphere's radius and the dihedral angle between the two cutting planes. Since the wedge is a constant-angle fraction of the full sphere, its volume scales linearly with . When , the wedge is the entire sphere, recovering . The surface of the wedge that lies on the sphere itself is called a spherical lune.
Worked Example
Problem: Find the volume of a spherical wedge cut from a sphere of radius 6 cm by a dihedral angle of 60°.
Convert the angle to radians: Since 60° equals π/3 radians:
Apply the volume formula: Substitute r = 6 and θ = π/3 into the formula:
Compute the numerical result: Evaluate to get the approximate volume:
Answer: The volume of the spherical wedge is cm³.
Why It Matters
Spherical wedges appear in multivariable calculus when setting up triple integrals in spherical coordinates, since integration over an angle range θ naturally defines a wedge. They also arise in geophysics and astronomy when modeling sectors of planets or celestial spheres.
Common Mistakes
Mistake: Using the angle in degrees directly in the formula instead of converting to radians.
Correction: The formula requires in radians. Always convert first: multiply degrees by .
