Iterative refinement

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Also visit my website ... Hostgator Discount Voucher Solution of triangles (Template:Lang-lat) is the historical term for solving the main trigonometric problem of finding the characteristics of a triangle (angles and lengths of sides), when some of these are known. The triangle can be located on a plane or on a sphere. Applications requiring triangle solutions include geodesy, astronomy, construction, and navigation.

Solving plane triangles

Standard notation in the triangle

A general form triangle has 6 main characteristics (see picture): 3 linear (side lengths a,b,c) and 3 angular (α,β,γ). The classical plane trigonometry problem is to specify 3 of the 6 characteristics and determine the other three. At least one of the side lengths must be specified. If only the angles are given, the side lengths cannot be determined, because any similar triangle is a solution.

A triangle can be solved when given any of the following:[1][2]

  • Three sides (SSS)
  • Two sides and the included angle (SAS)
  • Two sides and an angle not included between them (SSA)
  • A side and the two angles adjacent to it (ASA)
  • A side, the angle opposite to it and an angle adjacent to it (AAS).

Main theorems

Overview of particular steps and tools used when solving plane triangles

The standard method of solving the problem is to use fundamental relations.

Law of cosines
a2=b2+c22bccosα
b2=a2+c22accosβ
c2=a2+b22abcosγ
Law of sines
asinα=bsinβ=csinγ
Sum of angles
α+β+γ=180
Law of tangents
aba+b=tan[12(αβ)]tan[12(α+β)].

There are other (sometimes practically useful) universal relations: the law of cotangents and Mollweide's formula.

Notes

  1. To find an unknown angle, law of cosines is safer than law of sines. The reason is that the value of sine for the angle of the triangle does not uniquely determine this angle. For example, if sinβ=0.5, the angle β can be equal either 30 or 150. Using the law of cosines avoids this problem: within the interval from 0 to 180 the cosine value determines its angle unambiguously. On the other hand, if the angle is small (or close to 180°), then it is more robust numerically to determine it from its sine than its cosine because the arc-cosine function has a divergent derivative at 1 (or −1).
  2. We assume that the relative position of specified characteristics is known. If not, the mirror reflection of the triangle will be the solution also. For example, three side lengths uniquely define either a triangle or its reflection.
Three sides given

Three sides given (SSS)

Let three side lengths a,b,c be specified. To find the angles α,β, you can use the law of cosines:[3]

α=arccosb2+c2a22bc
β=arccosa2+c2b22ac.

Then angle γ=180αβ.

Some sources recommend to find angle β from law of sines but (as Note 1 above states) there is a risk to confuse acute angle value with obtuse one.

Another method of calculating the angles from known sides is to apply the law of cotangents.

Two sides and the included angle given

Two sides and the included angle given (SAS)

Here we know the lengths of sides a,b and the angle γ between these sides. The third side can be determined from the law of cosines:[4]

c=a2+b22abcosγ.

Now we use law of cosines to find the second angle:

α=arccosb2+c2a22bc.

Finally, β=180αγ.

Two sides and non-included angle given

Two sides and non-included angle given (SSA)

This case is the most difficult and ambiguous. Let two sides b,c and the angle β are known. Equation for the angle γ we can imply from the law of sines:[5]

sinγ=cbsinβ.

We denote further D=cbsinβ (equation's right side). There are 4 possible cases.

  1. If D>1, no such triangle exists (the side b «not reaches» to the line BC).
  2. If D=1, unique solution exists: γ=90, i. e. the triangle is right-angled.
Two solutions for triangle
  1. If D<1 two alternatives are possible.
    1. If b<c, the angle γ may be acute: γ=arcsinD or obtuse: γ=180γ. The picture on right shows the point C, the side b and the angle γ as the first solution, and the point C, side b and the angle γ as the second solution.
    2. If bc then βγ (the larger side corresponds to a larger angle). Since no triangle can have two obtuse angles, γ is acute angle and the solution γ=arcsinD is unique.

The third angle α=180βγ. The third side can be found from law of sines:

a=b sinαsinβ
A side and two adjacent angles given

A side and two adjacent angles given (ASA)

Known characteristics are the side c and the angles α,β. The third angle γ=180αβ.

Two unknown side can be calculated from the law of sines:[6]

a=c sinαsinγ;b=c sinβsinγ.

A side, one adjacent angle and the opposite angle given (AAS)

The procedure for solving an AAS triangle is same as that of an ASA triangle: First, find the third angle by using the angle sum property of a triangle, then find the other two sides using the law of sines.

File:Spherical triangle 3d opti.png
Spherical triangle

Solving spherical triangles

General form spherical triangle is fully determined by three of its six characteristics (3 sides and 3 angles). Note that the sides of a spherical triangle a,b,c are usually measured rather by angular units than by linear, according to corresponding central angles.

Solution of triangles for non-Euclidean spherical geometry has some differences from the plane case. For example, the sum of the three angles α+β+γ depends on the triangle. In addition, there are no unequal similar triangles, and so the problem of constructing a triangle with specified three angles has a unique solution. Basic relations used to solve a problem are like to the planar case: see Law of cosines (spherical) and Law of sines (spherical).

Among other relationships may be useful half-side formula and Napier's analogies:[7]

File:Solve spherical triangle with a b c.png
Three sides given

Three sides given

Known: the sides a,b,c (in angular units). Triangle angles are defined from spherical law of cosines:

α=arccos(cosacosb coscsinb sinc),
β=arccos(cosbcosc cosasinc sina),
γ=arccos(cosccosa cosbsina sinb),


File:Solve spherical triangle with a b gamma.png
Two sides and the included angle given

Two sides and the included angle given

Known: the sides a,b and the angle γ among it. The side c can be found from the law of cosines:

c=arccos(cosacosb+sinasinbcosγ)

The angles α,β can be calculated as above, or by using Napier's analogies:

α=arctan 2sinatan(γ2)sin(b+a)+cot(γ2)sin(ba)
β=arctan 2sinbtan(γ2)sin(a+b)+cot(γ2)sin(ab).

This problem arises in the navigation problem of finding the great circle between 2 points on the earth specified by their latitude and longitude; in this application, it's important to use formulas which are not susceptible to round-off errors. For this purpose, the following formulas (which may be derived using vector algebra) can be used

c=arctan(sinacosbcosasinbcosγ)2+(sinbsinγ)2cosacosb+sinasinbcosγ,α=arctansinasinγsinbcosacosbsinacosγ,β=arctansinbsinγsinacosbcosasinbcosγ,

where the signs of the numerators and denominators in these expressions should be used to determine the quadrant of the arctangent.


File:Solve spherical triangle with b c beta.png
Two sides and non-included angle given

Two sides and non-included angle given

Known: the sides b,c and the angle β not among it. Solution exists if the following condition takes place:

b>arcsin(sincsinβ)

The angle γ can be found from the Law of sines (spherical):

γ=arcsin(sincsinβsinb)

As for the plane case, if b<c then there are two solutions: γ and 180γ. Other characteristics we can find by using Napier's analogies:

a=2arctan{tan(12(bc))sin(12(β+γ))sin(12(βγ))},
α=2arccot{tan(12(βγ))sin(12(b+c))sin(12(bc))}.
File:Solve spherical triangle with c alpha beta.png
A side and two adjacent angles given

A side and two adjacent angles given

Known: the side c and the angles α,β. At first we determine the angle γ using the law of cosines:

γ=arccos(sinαsinβcosccosαcosβ),

Two unknown sides we can find from the law of cosines (using the calculated angle γ):

a=arccos(cosα+cosβcosγsinβsinγ)
b=arccos(cosβ+cosγcosαsinγsinα)

or by using Napier's analogies:

a=arctan{2sinαcot(c/2)sin(β+α)+tan(c/2)sin(βα)},
b=arctan{2sinβcot(c/2)sin(α+β)+tan(c/2)sin(αβ)},


File:Solve spherical triangle with a alpha beta.png
A side, one adjacent angle and the opposite angle given

A side, one adjacent angle and the opposite angle given

Known: the side a and the angles α,β. The side b can be found from the law of sines:

b=arcsin(sinasinβsinα),

If the angle for the side a is acute and α>β, another solution exists:

b=πarcsin(sinasinβsinα)

Other characteristics we can find by using Napier's analogies:

c=2arctan{tan(12(ab))sin(12(α+β))sin(12(αβ))},
γ=2arccot{tan(12(αβ))sin(12(a+b))sin(12(ab))},


File:Solve spherical triangle with alpha beta gamma.png
Three angles given

Three angles given

Known: the angles α,β,γ. From the law of cosines we infer:

a=arccos(cosα+cosβcosγsinβsinγ),
b=arccos(cosβ+cosγcosαsinγsinα),
c=arccos(cosγ+cosαcosβsinαsinβ).


Solving right-angled spherical triangles

The above algorithms become much simpler if one of the angles of a triangle (for example, the angle C) is the right angle. Such a spherical triangle is fully defined by its two elements, and the other three can be calculated using Napier's Pentagon or the following relations.

sina=sincsinA (from the Law of sines (spherical))
tana=sinbtanA
cosc=cosacosb (from the law of cosines (spherical))
tanb=tanccosA
cosA=cosasinB (also from the law of cosines)
cosc=cotAcotB

Some applications

Triangulation

File:Distance by triangulation.svg
Distance measurement by triangulation
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Suppose you want to measure the distance d from shore to remote ship. You must mark on the shore two points with known distance l between them (base line). Let α,β are the angles between base line and the direction to ship.

From the formulas above (ASA case) one can define the length of the triangle height:

d=sinαsinβsin(α+β)l=tanαtanβtanα+tanβl

This method is used in cabotage. The angles α,β are defined by observations familiar landmarks from the ship.

File:Mountain height by triangulation.png
How to measure a mountain height

Another example: you want to measure the height h of a mountain or a high building. The angles α,β from two ground points to the top are specified. Let l be the distance between tis points. From the same ASA case formulas we obtain:

h=sinαsinβsin(βα)l=tanαtanβtanβtanαl

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The distance between two points on the globe

File:Distance on earth.png

That's how to calculate the distance between two points on the globe.

Point A: latitude λA, longitude LA
Point B: latitude λB, longitude LB

We consider the spherical triangleABC, where C is the north Pole. Some characteristics we know:

a=90oλB
b=90oλA
γ=LALB

It's the case: Two sides and the included angle given. From its formulas we obtain:

AB=Rarccos{sinλAsinλB+cosλAcosλBcos(LALB)},

Here R is the Earth radius.

See also

References

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