Here I continue some thoughts initiated in BarycentricCoordinates.html . Given the triangle of reference ABC, the corresponding Barycentric coordinates represent a mapping between two copies of the projectified euclidean plane. Denote by P2 and Q2 the two projective planes and by F: P2 --> Q2 the corresponding map. F is completely determined by the conditions:
1) There is a distinguished equilateral triangle A*B*C* with centroid M*.
2) F maps the vertices of the equilateral to corresponding vertices of the triangle (A*->A, B*->B, C*->C) and the centroid M* to the corresponding centroid M of ABC.
This map could be geometrically realized through the projectification of an affine transformation of two planes in the euclidean three space. The first plane, representing the affine part of P2, would be the affine plane given by the equation x+y+z=1 . A*, B*, C* would be the endpoints of the three standard unit coordinate vectors e1, e2, e3. The other affine plane, representing the affine part of Q2, would be defined by z= 1 and A, B, C would be defined by the endpoints of three linearly independent vectors emanating from the origin. F would then be defined by the linear application represented by the matrix:
Here (px,py,pz) denote the coordinates of P* and (P1, P2, P3) denote the homogeneous coordinates of P.
[1] The mapping sends the line at infinity of the first plane, defined by px+py+pz=0, to the line at infinity of the second plane defined by P3=0.
[2] Denote by F' the affine restriction of F to the corresponding affine planes. F' being affine, preserves the parallelity of lines, the middles of segments and, more generally, the ratios of three points on a line. Thus, in the above picture: P*A*/P*D* = PA/PD and D*B*/D*C* = DB/DC.
[3] Besides, F preserves the nature of conics, mapping ellipses to ellipses, hyperbolas to hyperbolas and parabolas to parabolas correspondingly.
[4] From the linearity of F' follows also the formula for the area of a triangle DEF, as explained in BarycentricsFormulas.html .
[5] Barycentric coordinates use the standard projective coordinates of point P* as parameters for P. Thus, lines are represented by linear equations like k*px+m*py+n*pz = 0, and conics with quadratic equations:
[6] In particular, conics passing through the vertices of triangle ABC have their equations satisfied by the coordinate vectors (1,0,0), (0,1,0) and (0,0,1), implying a11=a22=a33=0. They are images under F of conics circumscribing A*B*C*.
[7] In particular, the circumcircle of A*B*C* is mapped by F onto the outer Steiner ellipse of triangle ABC. To see this, notice first that the circumconics of ABC are completely determined through their tangents at the three vertices (see PascalOnTriangles.html ). The Steiner ellipse is the one for which the tangents to the vertices are parallel to the corresponding opposite sides.
See Also
BarycentricCoordinates.html
BarycentricCoordinates2.html
BarycentricCoordinates3.html
BarycentricsFormulas.html
PascalOnTriangles.html
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