Solving spherical triangles

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Solving spherical triangles Edit The general spherical triangle is fully determined by three of its six characteristics (3 sides and 3 angles). Note that the sides a, b, c of a spherical triangle are measured by angular rather than linear units, based on the corresponding central angles. The solution of triangles for non-Euclidean spherical geometry has some differences from the planar 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. The basic relations used to solve a problem are similar to those of the planar case: see Law of cosines (spherical) and Law of sines (spherical). Among other relationships that may be useful are the half-side formula and Napier’s analogies:[7] {displaystyle tan {frac {c}{2}}cos {frac {alpha -beta }{2}}=tan {frac {a+b}{2}}cos {frac {alpha +beta }{2}}} {displaystyle tan {frac {c}{2}}sin {frac {alpha -beta }{2}}=tan {frac {a-b}{2}}sin {frac {alpha +beta }{2}}} {displaystyle cot {frac {gamma }{2}}cos {frac {a-b}{2}}=tan {frac {alpha +beta }{2}}cos {frac {a+b}{2}}} {displaystyle cot {frac {gamma }{2}}sin {frac {a-b}{2}}=tan {frac {alpha -beta }{2}}sin {frac {a+b}{2}}.}  Three sides given Three sides given (spherical SSS) Edit Known: the sides a, b, c (in angular units). The triangle’s angles are computed from the spherical law of cosines: {displaystyle alpha =arccos left({frac {cos a-cos b cos c}{sin b sin c}}right),} {displaystyle beta =arccos left({frac {cos b-cos c cos a}{sin c sin a}}right),} {displaystyle gamma =arccos left({frac {cos c-cos a cos b}{sin a sin b}}right).}  Two sides and the included angle given Two sides and the included angle given (spherical SAS) Edit Known: the sides a, b and the angle γ between them. The side c can be found from the law of cosines: {displaystyle c=arccos left(cos acos b+sin asin bcos gamma right).} The angles α’, β can be calculated as above, or by using Napier’s analogies: {displaystyle alpha =arctan {frac {2sin a}{tan({frac {gamma }{2}})sin(b+a)+cot({frac {gamma }{2}})sin(b-a)}},} {displaystyle beta =arctan {frac {2sin b}{tan({frac {gamma }{2}})sin(a+b)+cot({frac {gamma }{2}})sin(a-b)}}.} This problem arises in the navigation problem of finding the great circle between two points on the earth specified by their latitude and longitude; in this application, it is 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: {displaystyle {begin{aligned}c&=arctan {frac {sqrt {(sin acos b-cos asin bcos gamma )^{2}+(sin bsin gamma )^{2}}}{cos acos b+sin asin bcos gamma }},\alpha &=arctan {frac {sin asin gamma }{sin bcos a-cos bsin acos gamma }},\beta &=arctan {frac {sin bsin gamma }{sin acos b-cos asin bcos gamma }},end{aligned}}} where the signs of the numerators and denominators in these expressions should be used to determine the quadrant of the arctangent.  Two sides and a non-included angle given Two sides and non-included angle given (spherical SSA) Edit This problem is not solvable in all cases; a solution is guaranteed to be unique only if the side length adjacent to the angle is shorter than the other side length. Known: the sides b, c and the angle β not between them. A solution exists if the following condition holds: {displaystyle b>arcsin(sin c,sin beta ).} The angle γ can be found from the spherical law of sines: {displaystyle gamma =arcsin left({frac {sin c,sin beta }{sin b}}right).} As for the plane case, if b < c then there are two solutions: γ and 180° – γ. We can find other characteristics by using Napier’s analogies: {displaystyle a=2arctan left[tan left({tfrac {1}{2}}(b-c)right){frac {sin left({tfrac {1}{2}}(beta +gamma )right)}{sin left({tfrac {1}{2}}(beta -gamma )right)}}right],} {displaystyle alpha =2operatorname {arccot} left[tan left({tfrac {1}{2}}(beta -gamma )right){frac {sin left({tfrac {1}{2}}(b+c)right)}{sin left({tfrac {1}{2}}(b-c)right)}}right].}  One side and two adjacent angles given A side and two adjacent angles given (spherical ASA) Edit
Three angles given (spherical AAA)Edit
Known: the angles αβγ. From the law of cosines we infer:
{displaystyle a=arccos left({frac {cos alpha +cos beta cos gamma }{sin beta sin gamma }}right),}{displaystyle b=arccos left({frac {cos beta +cos gamma cos alpha }{sin gamma sin alpha }}right),}{displaystyle c=arccos left({frac {cos gamma +cos alpha cos beta }{sin alpha sin beta }}right).}
Solving right-angled spherical trianglesEdit
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 usingNapier’s Pentagon or the following relations.
{displaystyle sin a=sin ccdot sin A} (from the Law of sines (spherical)){displaystyle tan a=sin bcdot tan A}{displaystyle cos c=cos acdot cos b} (from the law of cosines (spherical)){displaystyle tan b=tan ccdot cos A}{displaystyle cos A=cos acdot sin B} (also from the law of cosines){displaystyle cos c=cot Acdot cot B}
Some applicationsEdit
TriangulationEdit
Distance measurement by triangulation
Main article: Triangulation
If one wants to measure the distance dfrom shore to a remote ship via triangulation, one marks on the shore two points with known distance lbetween them (the baseline). Let αβ be the angles between the baseline and the direction to the ship.
From the formulae above (ASA case) one can define the length of the triangle height:
{displaystyle d={frac {sin alpha ,sin beta }{sin(alpha +beta )}},l={frac {tan alpha ,tan beta }{tan alpha +tan beta }},l.}
This method is used in cabotage. The angles αβ are defined by observation of familiar landmarks from the ship.
How to measure a mountain’s height
As another example, if one wants to measure the height h of a mountain or a high building, the angles αβ from two ground points to the top are specified. Let l be the distance between these points. From the same ASA case formulas we obtain:
{displaystyle h={frac {sin alpha ,sin beta }{sin(beta -alpha )}},l={frac {tan alpha ,tan beta }{tan beta -tan alpha }},l.}
The distance between two points on the globeEdit
Main article: Great-circle distance
To calculate the distance between two points on the globe,
Point A: latitude λA, longitude LA, andPoint B: latitude λB, longitude LB
we consider the spherical triangle ABC, where C is the North Pole. Some characteristics are:
{displaystyle a=90^{mathrm {o} }-lambda _{mathrm {B} },,}{displaystyle b=90^{mathrm {o} }-lambda _{mathrm {A} },,}{displaystyle gamma =L_{mathrm {A} }-L_{mathrm {B} }.,}
If two sides and the included angle given, we obtain from the formulas
{displaystyle mathrm {AB} =Rarccos left[sin lambda _{mathrm {A} },sin lambda _{mathrm {B} }+cos lambda _{mathrm {A} },cos lambda _{mathrm {B} },cos left(L_{mathrm {A} }-L_{mathrm {B} }right)right].}
Here R is the Earth’s radius.
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