Notation for trigonometric relationships
In geometry , the Conway triangle notation simplifies and clarifies the algebraic expression of various trigonometric relationships in a triangle . Using the symbol S for twice the triangle's area , the symbol Sφ is defined to mean S times the cotangent of any arbitrary angle φ .
The notation is named after English mathematician John Horton Conway ,[ 1] who promoted its use, but essentially the same notation (using p instead of S ) can be found in an 1894 paper by Spanish mathematician Juan Jacobo Durán Loriga [ gl ] .[ 2]
Given a reference triangle whose sides are a , b and c and whose corresponding internal angles are A , B , and C then the Conway triangle notation is simply represented as follows:
S
=
b
c
sin
A
=
a
c
sin
B
=
a
b
sin
C
,
{\displaystyle S=bc\sin A=ac\sin B=ab\sin C,}
where[ 3] [ 4]
S
=
2
×
reference triangle area
,
S
φ
=
S
cot
φ
.
{\displaystyle {\begin{aligned}S&=2\times {\text{reference triangle area}},\\[2pt]S_{\varphi }&=S\cot \varphi .\end{aligned}}}
In particular:
S
A
=
S
cot
A
=
b
c
cos
A
=
b
2
+
c
2
−
a
2
2
,
S
B
=
S
cot
B
=
a
c
cos
B
=
a
2
+
c
2
−
b
2
2
,
S
C
=
S
cot
C
=
a
b
cos
C
=
a
2
+
b
2
−
c
2
2
,
S
ω
=
S
cot
ω
=
a
2
+
b
2
+
c
2
2
,
{\displaystyle {\begin{aligned}S_{A}&=S\cot A=bc\cos A={\frac {b^{2}+c^{2}-a^{2}}{2}},\\[2pt]S_{B}&=S\cot B=ac\cos B={\frac {a^{2}+c^{2}-b^{2}}{2}},\\[2pt]S_{C}&=S\cot C=ab\cos C={\frac {a^{2}+b^{2}-c^{2}}{2}},\\[2pt]S_{\omega }&=S\cot \omega ={\frac {a^{2}+b^{2}+c^{2}}{2}},\end{aligned}}}
where ω is the Brocard angle . The law of cosines is used:
a
2
=
b
2
+
c
2
−
2
b
c
cos
A
.
{\displaystyle a^{2}=b^{2}+c^{2}-2bc\cos A.}
Third-, double-, and half-angle identities:
S
π
3
=
S
cot
π
3
=
S
3
3
S
2
φ
=
S
φ
2
−
S
2
2
S
φ
S
φ
2
=
S
φ
+
S
φ
2
+
S
2
{\displaystyle {\begin{aligned}S_{\frac {\pi }{3}}&=S\cot {\frac {\pi }{3}}=S{\frac {\sqrt {3}}{3}}\\[2pt]S_{2\varphi }&={\frac {S_{\varphi }^{2}-S^{2}}{2S_{\varphi }}}\\[2pt]S_{\frac {\varphi }{2}}&=S_{\varphi }+{\sqrt {S_{\varphi }^{2}+S^{2}}}\end{aligned}}}
for values of φ where 0 < φ < π ,
S
ϑ
+
φ
=
S
ϑ
S
φ
−
S
2
S
ϑ
+
S
φ
,
S
ϑ
−
φ
=
S
ϑ
S
φ
+
S
2
S
φ
−
S
ϑ
.
{\displaystyle {\begin{aligned}S_{\vartheta +\varphi }&={\frac {S_{\vartheta }S_{\varphi }-S^{2}}{S_{\vartheta }+S_{\varphi }}},\\[2pt]S_{\vartheta -\varphi }&={\frac {S_{\vartheta }S_{\varphi }+S^{2}}{S_{\varphi }-S_{\vartheta }}}.\end{aligned}}}
Furthermore the convention uses a shorthand notation for
S
ϑ
S
φ
=
S
ϑ
φ
,
{\displaystyle S_{\vartheta }S_{\varphi }=S_{\vartheta \varphi },}
and
S
ϑ
S
φ
S
ψ
=
S
ϑ
φ
ψ
.
{\displaystyle S_{\vartheta }S_{\varphi }S_{\psi }=S_{\vartheta \varphi \psi }.}
Trigonometric relationships [ edit ]
sin
A
=
S
b
c
=
S
S
A
2
+
S
2
cos
A
=
S
A
b
c
=
S
A
S
A
2
+
S
2
tan
A
=
S
S
A
a
2
=
S
B
+
S
C
b
2
=
S
A
+
S
C
c
2
=
S
A
+
S
B
{\displaystyle {\begin{aligned}\sin A&={\frac {S}{bc}}={\frac {S}{\sqrt {S_{A}^{2}+S^{2}}}}\\[2pt]\cos A&={\frac {S_{A}}{bc}}={\frac {S_{A}}{\sqrt {S_{A}^{2}+S^{2}}}}\\[2pt]\tan A&={\frac {S}{S_{A}}}\\[6pt]a^{2}&=S_{B}+S_{C}\\[2pt]b^{2}&=S_{A}+S_{C}\\[2pt]c^{2}&=S_{A}+S_{B}\end{aligned}}}
Trigonometric conversions [ edit ]
sin
A
sin
B
sin
C
=
S
4
R
2
cos
A
cos
B
cos
C
=
S
ω
−
4
R
2
4
R
2
{\displaystyle {\begin{aligned}\sin A\sin B\sin C&={\frac {S}{4R^{2}}}\\[2pt]\cos A\cos B\cos C&={\frac {S_{\omega }-4R^{2}}{4R^{2}}}\end{aligned}}}
∑
cyclic
sin
A
=
S
2
R
r
=
s
R
∑
cyclic
cos
A
=
r
+
R
R
∑
cyclic
tan
A
=
S
S
ω
−
4
R
2
=
tan
A
tan
B
tan
C
{\displaystyle {\begin{aligned}\sum _{\text{cyclic}}\sin A&={\frac {S}{2Rr}}={\frac {s}{R}}\\[2pt]\sum _{\text{cyclic}}\cos A&={\frac {r+R}{R}}\\[2pt]\sum _{\text{cyclic}}\tan A&={\frac {S}{S_{\omega }-4R^{2}}}=\tan A\tan B\tan C\end{aligned}}}
∑
cyclic
a
2
S
A
=
a
2
S
A
+
b
2
S
B
+
c
2
S
C
=
2
S
2
∑
cyclic
a
4
=
2
(
S
ω
2
−
S
2
)
∑
cyclic
S
A
2
=
S
ω
2
−
2
S
2
∑
cyclic
S
B
C
=
∑
cyclic
S
B
S
C
=
S
2
∑
cyclic
b
2
c
2
=
S
ω
2
+
S
2
{\displaystyle {\begin{array}{ll}\displaystyle \sum _{\text{cyclic}}a^{2}S_{A}\!\!&=&a^{2}S_{A}+b^{2}S_{B}+c^{2}S_{C}=2S^{2}\\[2pt]\displaystyle \sum _{\text{cyclic}}a^{4}&=&2(S_{\omega }^{2}-S^{2})\\[2pt]\displaystyle \sum _{\text{cyclic}}S_{A}^{2}&=&S_{\omega }^{2}-2S^{2}\\[2pt]\displaystyle \sum _{\text{cyclic}}S_{BC}&=&\displaystyle \sum _{\text{cyclic}}S_{B}S_{C}=S^{2}\\[2pt]\displaystyle \sum _{\text{cyclic}}b^{2}c^{2}&=&S_{\omega }^{2}+S^{2}\end{array}}}
Let D be the distance between two points P and Q whose trilinear coordinates are
P
=
p
a
:
p
b
:
p
c
,
Q
=
q
a
:
q
b
:
q
c
.
{\displaystyle {\begin{aligned}P=p_{a}:p_{b}:p_{c},\\Q=q_{a}:q_{b}:q_{c}.\end{aligned}}}
Let
K
p
=
a
p
a
+
b
p
b
+
c
p
c
,
K
q
=
a
q
a
+
b
q
b
+
c
q
c
.
{\displaystyle {\begin{aligned}K_{p}&=ap_{a}+bp_{b}+cp_{c},\\K_{q}&=aq_{a}+bq_{b}+cq_{c}.\end{aligned}}}
Then D is given by the formula:[ 5]
D
2
=
∑
cyclic
a
2
S
A
(
p
a
K
p
−
q
a
K
q
)
2
{\displaystyle D^{2}=\sum _{\text{cyclic}}a^{2}S_{A}\left({\frac {p_{a}}{K_{p}}}-{\frac {q_{a}}{K_{q}}}\right)^{2}}
Distance between circumcenter and orthocenter [ edit ]
Using this formula it is possible to determine |OH | , the distance between the circumcenter and the orthocenter as follows:
For the circumcenter
p
a
=
a
S
A
,
{\displaystyle p_{a}=aS_{A},}
and for the orthocenter
q
a
=
S
B
S
C
a
,
{\displaystyle q_{a}={\frac {S_{B}S_{C}}{a}},}
K
p
=
∑
cyclic
a
2
S
A
=
2
S
2
,
K
q
=
∑
cyclic
S
B
S
C
=
S
2
.
{\displaystyle {\begin{aligned}K_{p}&=\sum _{\text{cyclic}}a^{2}S_{A}=2S^{2},\\[2pt]K_{q}&=\sum _{\text{cyclic}}S_{B}S_{C}=S^{2}.\end{aligned}}}
Hence:
D
2
=
∑
cyclic
a
2
S
A
(
a
S
A
2
S
2
−
S
B
S
C
a
S
2
)
2
=
1
4
S
4
∑
cyclic
a
4
S
A
3
−
S
A
S
B
S
C
S
4
∑
cyclic
a
2
S
A
+
S
A
S
B
S
C
S
4
∑
cyclic
S
B
S
C
=
1
4
S
4
∑
cyclic
a
2
S
A
2
(
S
2
−
S
B
S
C
)
−
2
(
S
ω
−
4
R
2
)
+
(
S
ω
−
4
R
2
)
=
1
4
S
2
∑
cyclic
a
2
S
A
2
−
S
A
S
B
S
C
S
4
∑
cyclic
a
2
S
A
−
(
S
ω
−
4
R
2
)
=
1
4
S
2
∑
cyclic
a
2
(
b
2
c
2
−
S
2
)
−
1
2
(
S
ω
−
4
R
2
)
−
(
S
ω
−
4
R
2
)
=
3
a
2
b
2
c
2
4
S
2
−
1
4
∑
cyclic
a
2
−
3
2
(
S
ω
−
4
R
2
)
=
3
R
2
−
1
2
S
ω
−
3
2
S
ω
+
6
R
2
=
9
R
2
−
2
S
ω
.
{\displaystyle {\begin{aligned}D^{2}&=\sum _{\text{cyclic}}a^{2}S_{A}\left({\frac {aS_{A}}{2S^{2}}}-{\frac {S_{B}S_{C}}{aS^{2}}}\right)^{2}\\[2pt]&={\frac {1}{4S^{4}}}\sum _{\text{cyclic}}a^{4}S_{A}^{3}-{\frac {S_{A}S_{B}S_{C}}{S^{4}}}\sum _{\text{cyclic}}a^{2}S_{A}+{\frac {S_{A}S_{B}S_{C}}{S^{4}}}\sum _{\text{cyclic}}S_{B}S_{C}\\[2pt]&={\frac {1}{4S^{4}}}\sum _{\text{cyclic}}a^{2}S_{A}^{2}(S^{2}-S_{B}S_{C})-2(S_{\omega }-4R^{2})+(S_{\omega }-4R^{2})\\[2pt]&={\frac {1}{4S^{2}}}\sum _{\text{cyclic}}a^{2}S_{A}^{2}-{\frac {S_{A}S_{B}S_{C}}{S^{4}}}\sum _{\text{cyclic}}a^{2}S_{A}-(S_{\omega }-4R^{2})\\[2pt]&={\frac {1}{4S^{2}}}\sum _{\text{cyclic}}a^{2}(b^{2}c^{2}-S^{2})-{\frac {1}{2}}(S_{\omega }-4R^{2})-(S_{\omega }-4R^{2})\\[2pt]&={\frac {3a^{2}b^{2}c^{2}}{4S^{2}}}-{\frac {1}{4}}\sum _{\text{cyclic}}a^{2}-{\frac {3}{2}}(S_{\omega }-4R^{2})\\[2pt]&=3R^{2}-{\frac {1}{2}}S_{\omega }-{\frac {3}{2}}S_{\omega }+6R^{2}\\[10pt]&=9R^{2}-2S_{\omega }.\end{aligned}}}
Thus,[ 6]
|
O
H
|
=
9
R
2
−
2
S
ω
.
{\displaystyle |OH|={\sqrt {9R^{2}-2S_{\omega }}}.}
↑ Chen, Evan (2016). Euclidean Geometry in Mathematical Olympiads . Mathematical Association of America . p. 132. ISBN 978-0883858394 .
↑ Loriga, Juan Jacobo Durán, "Nota sobre el triángulo", en El Progreso Matemático, tomo IV (1894), pages 313-316. , Periodico de Matematicas Puras y Aplicadas .
↑ Yiu, Paul (2002), "Notation." §3.4.1 in Introduction to the Geometry of the Triangle. pp. 33-34, Version 2.0402, April 2002 (PDF) , Department of Mathematics Florida Atlantic University, pp. 33– 34 .
↑ Kimberling, Clark, Encyclopedia of Triangle Centers - ETC, Part 1 "Introduced on November 1, 2011: Combos" Note 6 , University of Evansville .
↑ Yiu, Paul (2002), "The distance formula" §7.1 in Introduction to the Geometry of the Triangle. p. 87, Version 2.0402, April 2002 (PDF) , Department of Mathematics Florida Atlantic University, p. 87 .
↑ Weisstein, Eric W. "Orthocenter §(14)" . MathWorld .