When we study two-dimensional geometry, angles measure how much one line must rotate around a point to overlap another. The complete rotation of a plane is 360 degrees, or radians. In three dimensions, a similar concept exists for describing how wide an object appears from a given vantage. The measurement is known as a solid angle and its units are steradians. Just as an ordinary angle corresponds to a portion of a circle, a solid angle corresponds to a portion of the surface area of a sphere.
The total surface area of a sphere is . If we project an object onto that sphere from its center, the solid angle is the ratio of the object’s projected area to . Mathematically,
The symbol denotes the solid angle. One steradian is defined as the solid angle that encloses a portion of surface area equal to . Since the surface area of an entire sphere is , a full sphere subtends steradians, which is approximately 12.57 sr. The fraction of that value tells you how much of the sphere the object covers.
A common scenario involves a conical field of view, such as the light beam from a flashlight or the portion of sky visible through a telescope. If the cone has an apex angle , the solid angle can be found using
When the cone angle is small, this formula approximates to if is in radians. Our calculator lets you specify a cone angle for convenience. When provided, the script computes the solid angle from that angle and the radius is ignored. Otherwise, it uses the area and radius.
Suppose you mount a sensor at the center of a spherical dome with radius 2 m. The sensor measures light from a small patch of the dome with area 0.5 m². Dividing area by radius squared gives steradians. Because a full sphere is about 12.57 steradians, this patch covers roughly 1 percent of the sensor’s surroundings. In terms of a cone, if you plug into the inverse of the cone formula, the half-angle works out to about 11.5 degrees.
Solid angles may feel abstract, yet they appear in many scientific fields. Astronomers use them to specify how large a planet or star appears from Earth. Radiologists describe the beam of a radiation source in steradians so they can calculate exposure. Antenna designers express directional gain as power per steradian to quantify how concentrated a radio signal is. Even everyday camera lenses list their field of view in degrees, which translates directly to a solid angle covering part of the viewer’s sphere.
The intensity of a source often depends on how much solid angle it covers. For example, the luminance of a display measures emitted light per unit area per unit solid angle. The brightness you perceive from a screen depends not only on how much light it emits but also on how widely that light spreads. Recognizing this relationship helps engineers design efficient optics, sensors, and illumination systems.
Object | Approximate Ω (sr) | Description |
---|---|---|
Full sphere | 4π ≈ 12.57 | Entire surrounding space |
Hemisphere | 2π ≈ 6.28 | Half the sphere |
90° cone | 2π(1 - cos 45°) ≈ 1.84 | Common flashlight beam |
Sun seen from Earth | ≈ 6.8×10-5 | Very small apparent size |
While the simple formulas presented here handle many cases, real objects rarely project perfectly onto a sphere. A rectangular screen, for example, subtends a slightly different solid angle than a cone with the same diagonal field of view. Moreover, small measurement errors in area or angle can lead to noticeable differences in when the values are tiny. For extremely precise work, such as calibrating a satellite sensor, engineers perform detailed ray-tracing or integrate over the exact shape.
Fill in the surface area of the patch and the radius from the observation point, or specify a cone angle for a symmetrical beam. When you click the Calculate button, the JavaScript computes the solid angle in steradians and also expresses it as a fraction of a full sphere. Because everything runs in your browser, the tool responds instantly without sending data anywhere.
If the cone angle is present, it takes priority. This allows quick conversions from a camera’s field of view specification to steradians. On the other hand, if you measure a real object’s surface area at a known distance, leave the angle blank and rely on the area-based formula. Both methods highlight the geometric meaning of a solid angle: a patch of the sphere as seen from its center.
Astronomy offers countless examples. Telescopes collect photons from distant galaxies that occupy only microsteradians of the sky. When astronomers quote the brightness of a nebula, they normalize the measurement by its solid angle so observers can compare extended objects to point sources. In radar engineering, antennas often radiate most strongly in a narrow solid angle. Understanding that pattern helps prevent interference and ensures energy is not wasted broadcasting in unwanted directions.
In lighting design, specifying a lamp’s beam spread in degrees hints at how concentrated the illumination will be. Converting that value to steradians allows direct comparisons between fixtures of different sizes and distances from the target surface. The same principle applies to infrared heaters, which deliver more energy to an object when the heater’s radiation is confined to a smaller solid angle.
Solid angles extend the idea of planar angles into three dimensions. By relating an observed area to the radius of a sphere, they quantify how much of the surrounding space something occupies. Cones, camera lenses, radar dishes, and even celestial bodies can all be described by their solid angles. This calculator makes it easy to experiment with different geometries and build intuition about steradians. Whether you’re planning an optical system or simply curious how much of the sky the Moon covers, understanding solid angles opens a window to spatial relationships in our three-dimensional world.
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