, a solid angle (symbol: ) is a measure of the amount of the field of view
from some particular point that a given object covers. That is, it is a measure of how large the object appears to an observer looking from that point.
The point from which the object is viewed is called the ''apex'' of the solid angle, and the object is said to ''subtend
'' its solid angle from that point.
In the International System of Units
(SI), a solid angle is expressed in a dimensionless unit
called a ''steradian
'' (symbol: sr). One steradian corresponds to one unit of area on the unit sphere
surrounding the apex, so an object that blocks all rays from the apex would cover a number of steradians equal to the total surface area
of the unit sphere,
. Solid angles can also be measured in squares of angular measures such as degrees
, minutes, and seconds.
A small object nearby may subtend the same solid angle as a larger object farther away. For example, although the Moon
is much smaller than the Sun
, it is also much closer to Earth
. Indeed, as viewed from any point on Earth, both objects have approximately the same solid angle as well as apparent size. This is evident during a solar eclipse
Definition and properties
An object's solid angle in steradian
s is equal to the area
of the segment of a unit sphere
, centered at the apex, that the object covers. A solid angle in steradians equals the area of a segment of a unit sphere in the same way a planar angle
s equals the length of an arc of a unit circle
; therefore, just like a planar angle in radians is the ratio of the length of a circular arc to its radius, a solid angle in steradians is the following ratio:
where A is the spherical surface area and r is the radius of the considered sphere.
Solid angles are often used in astronomy
, and in particular astrophysics
. The solid angle of an object that is very far away is roughly proportional to the ratio of area to squared distance. Here "area" means the area of the object when projected along the viewing direction.
The solid angle of a sphere measured from any point in its interior is 4Pi|
sr, and the solid angle subtended at the center of a cube by one of its faces is one-sixth of that, or sr. Solid angles can also be measured in square degree
s (1 sr = ()2
square degrees), in square minutes and square seconds, or in fractions of the sphere (1 sr = fractional area), also known as spat
(1 sp = 4 sr).
In spherical coordinates
there is a formula for the differential
where is the colatitude
(angle from the North pole) and is the longitude.
The solid angle for an arbitrary oriented surface
S subtended at a point P is equal to the solid angle of the projection of the surface S to the unit sphere with center P, which can be calculated as the surface integral
is the unit vector
, the position vector
of an infinitesimal area of surface with respect to point P, and where
represents the unit normal vector
to . Even if the projection on the unit sphere to the surface S is not isomorphic
, the multiple folds are correctly considered according to the surface orientation described by the sign of the scalar product
Thus one can approximate the solid angle subtended by a small facet
having flat surface area , orientation
, and distance from the viewer as:
where the surface area of a sphere
*Defining luminous intensity
, and the correspondent radiometric quantities radiant intensity
*Calculating spherical excess
of a spherical triangle
*The calculation of potentials by using the boundary element method
*Evaluating the size of ligand
s in metal complexes, see ligand cone angle
*Calculating the electric field
and magnetic field
strength around charge distributions
*Deriving Gauss's Law
*Calculating emissive power and irradiation in heat transfer
*Calculating cross sections in Rutherford scattering
*Calculating cross sections in Raman scattering
*The solid angle of the acceptance cone
of the optical fiber
Solid angles for common objects
Cone, spherical cap, hemisphere
250px|Section of cone (1) and spherical cap (2) inside a sphere. In this figure and .
The solid angle of a cone
with its apex at the apex of the solid angle, and with apex
angle 2, is the area of a spherical cap
on a unit sphere
For small such that , this reduces to the area of a circle .
The above is found by computing the following double integral
using the unit surface element in spherical coordinates
This formula can also be derived without the use of calculus
. Over 2200 years ago Archimedes
proved that the surface area of a spherical cap is always equal to the area of a circle whose radius equals the distance from the rim of the spherical cap to the point where the cap's axis of symmetry intersects the cap. In the diagram this radius is given as:
Hence for a unit sphere the solid angle of the spherical cap is given as:
When = , the spherical cap becomes a hemisphere
having a solid angle 2.
The solid angle of the complement of the cone is:
This is also the solid angle of the part of the celestial sphere
that an astronomical observer positioned at latitude can see as the earth rotates. At the equator all of the celestial sphere is visible; at either pole, only one half.
The solid angle subtended by a segment of a spherical cap cut by a plane at angle from the cone's axis and passing through the cone's apex can be calculated by the formula:
For example, if , then the formula reduces to the spherical cap formula above: the first term becomes , and the second .
Let OABC be the vertices of a tetrahedron
with an origin at O subtended by the triangular face ABC where
are the vector positions of the vertices A, B and C. Define the vertex angle to be the angle BOC and define , correspondingly. Let
be the dihedral angle
between the planes that contain the tetrahedral faces OAC and OBC and define
correspondingly. The solid angle subtended by the triangular surface ABC is given by
This follows from the theory of spherical excess
and it leads to the fact that there is an analogous theorem to the theorem that ''"The sum of internal angles of a planar triangle is equal to "'', for the sum of the four internal solid angles of a tetrahedron as follows:
ranges over all six of the dihedral angles between any two planes that contain the tetrahedral faces OAB, OAC, OBC and ABC.
A useful formula for calculating the solid angle of the tetrahedron at the origin O that is purely a function of the vertex angles , , is given by L'Huilier
's theorem as
Another interesting formula involves expressing the vertices as vectors in 3 dimensional space. Let
be the vector positions of the vertices A, B and C, and let , , and be the magnitude of each vector (the origin-point distance). The solid angle subtended by the triangular surface ABC is:
denotes the scalar triple product
of the three vectors and
denotes the scalar product
Care must be taken here to avoid negative or incorrect solid angles. One source of potential errors is that the scalar triple product can be negative if , , have the wrong winding
. Computing is a sufficient solution since no other portion of the equation depends on the winding. The other pitfall arises when the scalar triple product is positive but the divisor is negative. In this case returns a negative value that must be increased by .
The solid angle of a four-sided right rectangular pyramid
angles and (dihedral angle
s measured to the opposite side faces of the pyramid) is
If both the side lengths ( and ) of the base of the pyramid and the distance () from the center of the base rectangle to the apex of the pyramid (the center of the sphere) are known, then the above equation can be manipulated to give
The solid angle of a right -gonal pyramid, where the pyramid base is a regular -sided polygon of circumradius , with a
pyramid height is
The solid angle of an arbitrary pyramid with an -sided base defined by the sequence of unit vectors representing edges can be efficiently computed by:
where parentheses (* *) is a scalar product
and square brackets * *
is a scalar triple product
, and is an imaginary unit
. Indices are cycled: and .
The solid angle of a latitude-longitude rectangle on a globe
where and are north and south lines of latitude
(measured from the equator
s with angle increasing northward), and and are east and west lines of longitude
(where the angle in radians increases eastward). Mathematically, this represents an arc of angle swept around a sphere by radians. When longitude spans 2 radians and latitude spans radians, the solid angle is that of a sphere.
A latitude-longitude rectangle should not be confused with the solid angle of a rectangular pyramid. All four sides of a rectangular pyramid intersect the sphere's surface in great circle
arcs. With a latitude-longitude rectangle, only lines of longitude are great circle arcs; lines of latitude are not.
Sun and Moon
is seen from Earth at an average angular diameter
of 0.5334 degrees or 9.310 radians. The Moon
is seen from Earth at an average angular diameter of 9.22 radians. We can substitute these into the equation given above for the solid angle subtended by a cone with apex
The resulting value for the Sun
is 6.807 steradians. The resulting value for the Moon
is 6.67 steradians. In terms of the total celestial sphere, the Sun
and the Moon
subtend ''fractional areas'' of 0.000542% (5.42 ppm
) and 0.000531% (5.31 ppm), respectively. On average, the Sun
is larger in the sky than the Moon
even though it is much, much farther away.
Solid angles in arbitrary dimensions
The solid angle subtended by the complete ()-dimensional spherical surface of the unit sphere in -dimensional Euclidean space
can be defined in any number of dimensions . One often needs this solid angle factor in calculations with spherical symmetry. It is given by the formula
where is the gamma function
. When is an integer, the gamma function can be computed explicitly. It follows that
This gives the expected results of 4 steradians for the 3D sphere bounded by a surface of area and 2 radians for the 2D circle bounded by a circumference of length . It also gives the slightly less obvious 2 for the 1D case, in which the origin-centered 1D "sphere" is the interval and this is bounded by two limiting points.
The counterpart to the vector formula in arbitrary dimension was derived by Aomoto
and independently by Ribando.
It expresses them as an infinite multivariate Taylor series:
Given unit vectors
defining the angle, let denote the matrix formed by combining them so the th column is
. The variables
form a multivariable
. For a "congruent" integer multiexponent
means the variable
, similarly for the exponents
Hence, the term
means the sum over all terms in
in which l appears as either the first or second index.
Where this series converges, it converges to the solid angle defined by the vectors.
External links HCR's Theory of Polygon(solid angle subtended by any polygon)
*Arthur P. Norton, A Star Atlas, Gall and Inglis, Edinburgh, 1969.
*M. G. Kendall, A Course in the Geometry of N Dimensions, No. 8 of Griffin's Statistical Monographs & Courses, ed. M. G. Kendall, Charles Griffin & Co. Ltd, London, 1961
Category:Euclidean solid geometry