Steradian

A steradian is used to measure "solid angles"

A steradian is related to the surface area of a sphere in the same way a radian is related to the circumference of a circle:

A Radian "cuts out" a length of a circle's circumference
equal to the radius
  Circle showing one radian arc length equal to the radius
A Steradian "cuts out" an area of a sphere
equal to (radius)2
  Sphere showing one steradian surface area equal to the radius squared
The SI Unit abbreviation is sr
The name steradian is made up from the Greek stereos for "solid" and radian.

Sphere vs Steradian

So a full sphere has a surface area of 4π steradians which is about 12.57 steradians. That means one steradian covers roughly 8% of the sphere.

And because we are measuring angles, it doesn't matter what size the sphere is it will always measure 4π steradians.

Sphere divided into 4 pi steradian sections

Example: The "unit sphere":

  • has a radius of 1
  • has a surface area of 4π,
  • a steradian "cuts out" an area of 1

Radiant Intensity

Radiant intensity (how brightly something shines) can be measured in watts per steradian (W/sr).

Example: You measure the light coming from a powerful globe.

You hold a 50 mm × 50 mm sensor 2 m away and it measures 0.1 Watts.

What is the radiant intensity in W/sr (Watts per steradian)?

  • At 2 meters, one steradian covers an area of (2 m)2 = 4 m2
  • The sensor is small, so the area of sphere it occupies is about equal to its flat surface area: (0.05 m)2 = 0.0025 m2
  • Scale up the measured power: 0.1 W × 4 m20.0025 m2 = 160 W/sr

Square Degrees

Because we can convert from radians to degrees we can also convert from steradians to square degrees (deg2):

Since a radian is (180/π) degrees, we can square this to find that a steradian is (180/π)23282.8 square degrees

The full Moon in the night sky

Example: The Moon

The Moon's angular diameter is about 0.5°, so it covers:

π4 x (0.5°)2
≈ 0.2 deg2

For small parts of the sky like the Moon, we can treat the curved surface like a flat circle to find its area

That is a tiny fraction of the visible sky, which covers:

(360°)2π
≈ 41,253 deg2

It would take about 41,253 deg20.2 deg2210,000 Full Moons to cover the entire sky!