Conway triangle notation

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Short description: 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]

Definition

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=bcsin⁡A=acsin⁡B=absin⁡C, where[3][4] S=2×reference triangle area,Sφ=Scot⁡φ.

Basic formulas

In particular: SA=Scot⁡A=bccos⁡A=b2+c2−a22,SB=Scot⁡B=accos⁡B=a2+c2−b22,SC=Scot⁡C=abcos⁡C=a2+b2−c22,Sω=Scot⁡ω=a2+b2+c22,

where ω is the Brocard angle. The law of cosines is used: a2=b2+c2−2bccos⁡A.

Third-, double-, and half-angle identities: Sπ3=Scot⁡π3=S33S2φ=Sφ2−S22SφSφ2=Sφ+Sφ2+S2

for values of φ where 0 < φ < π,

Sϑ+φ=SϑSφ−S2Sϑ+Sφ,Sϑ−φ=SϑSφ+S2Sφ−Sϑ.

Furthermore the convention uses a shorthand notation for SϑSφ=Sϑφ, and SϑSφSψ=Sϑφψ.

Trigonometric relationships

sin⁡A=Sbc=SSA2+S2cos⁡A=SAbc=SASA2+S2tan⁡A=SSAa2=SB+SCb2=SA+SCc2=SA+SB

Important identities

∑cyclicSA=SA+SB+SC=SωS2=b2c2−SA2=a2c2−SB2=a2b2−SC2SBC=SBSC=S2−a2SASAC=SASC=S2−b2SBSAB=SASB=S2−c2SCSABC=SASBSC=S2(Sω−4R2)Sω=s2−r2−4rR

where

R is the circumradius
r is the incenter
abc=2SR
s=a+b+c2
Sr=a+b+c

Trigonometric conversions

sin⁡Asin⁡Bsin⁡C=S4R2cos⁡Acos⁡Bcos⁡C=Sω−4R24R2

∑cyclicsin⁡A=S2Rr=sR∑cycliccos⁡A=r+RR∑cyclictan⁡A=SSω−4R2=tan⁡Atan⁡Btan⁡C

Useful formulas

∑cyclica2SA=a2SA+b2SB+c2SC=2S2∑cyclica4=2(Sω2−S2)∑cyclicSA2=Sω2−2S2∑cyclicSBC=∑cyclicSBSC=S2∑cyclicb2c2=Sω2+S2

Applications

Let D be the distance between two points P and Q whose trilinear coordinates are P=pa:pb:pc,Q=qa:qb:qc. Let Kp=apa+bpb+cpc,Kq=aqa+bqb+cqc. Then D is given by the formula:[5] D2=∑cyclica2SA(paKp−qaKq)2

Distance between circumcenter and orthocenter

Using this formula it is possible to determine |OH|, the distance between the circumcenter and the orthocenter as follows:

For the circumcenter pa=aSA,

and for the orthocenter qa=SBSCa,

Kp=∑cyclica2SA=2S2,Kq=∑cyclicSBSC=S2.

Hence:

D2=∑cyclica2SA(aSA2S2−SBSCaS2)2=14S4∑cyclica4SA3−SASBSCS4∑cyclica2SA+SASBSCS4∑cyclicSBSC=14S4∑cyclica2SA2(S2−SBSC)−2(Sω−4R2)+(Sω−4R2)=14S2∑cyclica2SA2−SASBSCS4∑cyclica2SA−(Sω−4R2)=14S2∑cyclica2(b2c2−S2)−12(Sω−4R2)−(Sω−4R2)=3a2b2c24S2−14∑cyclica2−32(Sω−4R2)=3R2−12Sω−32Sω+6R2=9R2−2Sω.

Thus,[6]

|OH|=9R2−2Sω.

See also

References