Law of Sines

Trigonometry |
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Reference |

Laws and theorems |

Calculus |

In trigonometry, the **law of sines**, **sine law**, **sine formula**, or **sine rule** is an equation relating the lengths of the sides of any triangle to the sines of its angles. According to the law,

where

The law of sines can be used to compute the remaining sides of a triangle when two angles and a side are known—a technique known as triangulation. It can also be used when two sides and one of the non-enclosed angles are known. In some such cases, the triangle is not uniquely determined by this data (called the

The law of sines is one of two trigonometric equations commonly applied to find lengths and angles in scalene triangles, with the other being the law of cosines.

The law of sines can be generalized to higher dimensions on surfaces with constant curvature.^{[1]}

H.J.J. Wilson's book Eastern Science^{[2]} states that the 7th century Indian mathematician Brahmagupta describes what we now know as the law of sines in his astronomical treatise Brāhmasphuṭasiddhānta. In his partial translation of this work, Colebrooke^{[3]} translates Brahmagupta's statement of the sine rule as: The product of the two sides of a triangle, divided by twice the perpendicular, is the central line; and the double of this is the diameter of the central line.

According to Ubiratàn D'Ambrosio and Helaine Selin, the spherical law of sines was discovered in the 10th century. It is variously attributed to Abu-Mahmud Khojandi, Abu al-Wafa' Buzjani, Nasir al-Din al-Tusi and Abu Nasr Mansur.^{[4]}

Ibn Muʿādh al-Jayyānī's *The book of unknown arcs of a sphere* in the 11th century contains the spherical law of sines.^{[5]} The plane law of sines was later stated in the 13th century by Nasīr al-Dīn al-Tūsī. In his *On the Sector Figure*, he stated the law of sines for plane and spherical triangles, and provided proofs for this law.^{[6]}

According to Glen Van Brummelen, "The Law of Sines is really Regiomontanus's foundation for his solutions of right-angled triangles in Book IV, and these solutions are in turn the bases for his solutions of general triangles."^{[7]} Regiomontanus was a 15th-century German mathematician.

The area of any triangle can be written as one half of its base times its height. Selecting one side of the triangle as the base, the height of the triangle relative to that base is computed as the length of another side times the sine of the angle between the chosen side and the base. Thus depending on the selection of the base, the area *T* of the triangle can be written as any of:

Multiplying these by 2/

When using the law of sines to find a side of a triangle, an ambiguous case occurs when two separate triangles can be constructed from the data provided (i.e., there are two different possible solutions to the triangle). In the case shown below they are triangles *ABC* and *ABC′*.

Given a general triangle, the following conditions would need to be fulfilled for the case to be ambiguous:

- The only information known about the triangle is the angle
*α*and the sides*a*and*c*. - The angle
*α*is acute (i.e.,*α*< 90°). - The side
*a*is shorter than the side*c*(i.e.,*a*<*c*). - The side
*a*is longer than the altitude*h*from angle*β*, where*h*=*c*sin*α*(i.e.,*a*>*h*).

If all the above conditions are true, then each of angles *β* and *β′* produces a valid triangle, meaning that both of the following are true:

From there we can find the corresponding *β* and *b* or *β′* and *b′* if required, where *b* is the side bounded by vertices *A* and *C* and *b′* is bounded by *A* and *C′*.

The following are examples of how to solve a problem using the law of sines.

Given: side *a* = 20, side *c* = 24, and angle *γ* = 40°. Angle *α* is desired.

Using the law of sines, we conclude that

Note that the potential solution *α* = 147.61° is excluded because that would necessarily give *α* + *β* + *γ* > 180°.

If the lengths of two sides of the triangle *a* and *b* are equal to *x*, the third side has length *c*, and the angles opposite the sides of lengths *a*, *b*, and *c* are *α*, *β*, and *γ* respectively then

In the identity

the common value of the three fractions is actually the diameter of the triangle's circumcircle. This result dates back to Ptolemy.

As shown in the figure, let there be a circle with inscribed and another inscribed that passes through the circle's center **O**. The has a central angle of and thus , by Thales's theorem. Since is a right triangle,

where is the radius of the circumscribing circle of the triangle.

Rearranging yields

Repeating the process of creating with other points gives

The area of a triangle is given by , where is the angle enclosed by the sides of lengths *a* and *b*. Substituting the sine law into this equation gives

Taking as the circumscribing radius,^{[10]}

It can also be shown that this equality implies

where

The second equality above readily simplifies to Heron's formula for the area.

The sine rule can also be used in deriving the following formula for the triangle's area: denoting the semi-sum of the angles' sines as , we have^{[11]}

where is the radius of the circumcircle: .

The spherical law of sines deals with triangles on a sphere, whose sides are arcs of great circles.

Suppose the radius of the sphere is 1. Let *a*, *b*, and *c* be the lengths of the great-arcs that are the sides of the triangle. Because it is a unit sphere, *a*, *b*, and *c* are the angles at the center of the sphere subtended by those arcs, in radians. Let *A*, *B*, and *C* be the angles opposite those respective sides. These are dihedral angles between the planes of the three great circles.

Then the spherical law of sines says:

Consider a unit sphere with three unit vectors **OA**, **OB** and **OC** drawn from the origin to the vertices of the triangle. Thus the angles *α*, *β*, and *γ* are the angles *a*, *b*, and *c*, respectively. The arc BC subtends an angle of magnitude *a* at the centre. Introduce a Cartesian basis with **OA** along the *z*-axis and **OB** in the *xz*-plane making an angle *c* with the *z*-axis. The vector **OC** projects to ON in the *xy*-plane and the angle between ON and the *x*-axis is *A*. Therefore, the three vectors have components:

The scalar triple product, **OA** ⋅ (**OB** × **OC**) is the volume of the parallelepiped formed by the position vectors of the vertices of the spherical triangle **OA**, **OB** and **OC**. This volume is invariant to the specific coordinate system used to represent **OA**, **OB** and **OC**. The value of the scalar triple product **OA** ⋅ (**OB** × **OC**) is the 3 × 3 determinant with **OA**, **OB** and **OC** as its rows. With the *z*-axis along **OA** the square of this determinant is

Repeating this calculation with the

where V is the volume of the parallelepiped formed by the position vector of the vertices of the spherical triangle. Consequently, the result follows.

It is easy to see how for small spherical triangles, when the radius of the sphere is much greater than the sides of the triangle, this formula becomes the planar formula at the limit, since

and the same for sin

Consider a unit sphere with:

Construct point and point such that

Construct point such that

It can therefore be seen that and

Notice that is the projection of on plane . Therefore

By basic trigonometry, we have:

But

Combining them we have:

By applying similar reasoning, we obtain the spherical law of sine:

See also: Spherical trigonometry, Spherical law of cosines, and Half-side formula |

A purely algebraic proof can be constructed from the spherical law of cosines. From the identity and the explicit expression for from the spherical law of cosines

Since the right hand side is invariant under a cyclic permutation of the spherical sine rule follows immediately.

The figure used in the Geometric proof above is used by and also provided in Banerjee^{[12]} (see Figure 3 in this paper) to derive the sine law using elementary linear algebra and projection matrices.

In hyperbolic geometry when the curvature is −1, the law of sines becomes

In the special case when *B* is a right angle, one gets

which is the analog of the formula in Euclidean geometry expressing the sine of an angle as the opposite side divided by the hypotenuse.

See also: Hyperbolic triangle |

Define a generalized sine function, depending also on a real parameter *K*:

The law of sines in constant curvature *K* reads as^{[1]}

By substituting *K* = 0, *K* = 1, and *K* = −1, one obtains respectively the Euclidean, spherical, and hyperbolic cases of the law of sines described above.

Let *p*_{K}(*r*) indicate the circumference of a circle of radius *r* in a space of constant curvature *K*. Then *p*_{K}(*r*) = 2*π* sin_{K} *r*. Therefore, the law of sines can also be expressed as:

This formulation was discovered by János Bolyai.^{[13]}

A tetrahedron has four triangular facets. The absolute value of the polar sine (psin) of the normal vectors to the three facets that share a vertex of the tetrahedron, divided by the area of the fourth facet will not depend upon the choice of the vertex:^{[14]}

More generally, for an *n*-dimensional simplex (i.e., triangle (*n* = 2), tetrahedron (*n* = 3), pentatope (*n* = 4), etc.) in *n*-dimensional Euclidean space, the absolute value of the polar sine of the normal vectors of the facets that meet at a vertex, divided by the hyperarea of the facet opposite the vertex is independent of the choice of the vertex. Writing *V* for the hypervolume of the *n*-dimensional simplex and *P* for the product of the hyperareas of its (*n* − 1)-dimensional facets, the common ratio is