Conway triangle notation

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In geometry, the Conway triangle notation, named after English mathematician John Horton Conway,[1] allows trigonometric functions of a triangle to be managed algebraically. However, though the notation was promoted by Conway, a much earlier reference to the notation goes back to the Spanish nineteenth century mathematician gl:Juan Jacobo Durán Loriga.[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 S = 2 × area of reference triangle and

Sφ=Scot⁡φ.,[3][4]

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.
Sπ3=Scot⁡π3=S33,
S2φ=Sφ2−S22SφSφ2=Sφ+Sφ2+S2,    for values of   φ  where   0<φ<π,
Sϑ+φ=SϑSφ−S2Sϑ+SφSϑ−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=SSA,
a2=SB+SCb2=SA+SCc2=SA+SB.

Important identities

∑cyclicSA=SA+SB+SC=Sω,
S2=b2c2−SA2=a2c2−SB2=a2b2−SC2,
SBC=SBSC=S2−a2SASAC=SASC=S2−b2SBSAB=SASB=S2−c2SC,
SABC=SASBSC=S2(Sω−4R2)Sω=s2−r2−4rR,

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

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 pa : pb : pc and qa : qb : qc. Let Kp = apa + bpb + cpc and let Kq = aqa + bqb + cqc. Then D is given by the formula:

D2=∑cyclica2SA(paKp−qaKq)2,.[5]

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 = SBSC/a

Kp=∑cyclica2SA=2S2Kq=∑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,

OH=9R2−2Sω,.[6]

See also

References

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