%%% This file is part of PlanetMath snapshot of 2009-01-12 %%% Primary Title: symmetry %%% Primary Category Code: 51A15 %%% Filename: Symmetry2.tex %%% Version: 15 %%% Owner: Wkbj79 %%% Author(s): Wkbj79, CWoo %%% PlanetMath is released under the GNU Free Documentation License. %%% You should have received a file called fdl.txt along with this file. %%% If not, please write to gnu@gnu.org. \documentclass[12pt]{article} \pagestyle{empty} \setlength{\paperwidth}{8.5in} \setlength{\paperheight}{11in} \setlength{\topmargin}{0.00in} \setlength{\headsep}{0.00in} \setlength{\headheight}{0.00in} \setlength{\evensidemargin}{0.00in} \setlength{\oddsidemargin}{0.00in} \setlength{\textwidth}{6.5in} \setlength{\textheight}{9.00in} \setlength{\voffset}{0.00in} \setlength{\hoffset}{0.00in} \setlength{\marginparwidth}{0.00in} \setlength{\marginparsep}{0.00in} \setlength{\parindent}{0.00in} \setlength{\parskip}{0.15in} \usepackage{html} \usepackage{pstricks} \usepackage{psfrag} \usepackage{amssymb} \usepackage{amsmath} \usepackage{amsfonts} \usepackage{graphicx} \usepackage{amsthm} \usepackage{xypic} \begin{document} Let $V$ be a \htmladdnormallink{Euclidean vector space}{http://planetmath.org/encyclopedia/EuclideanVectorSpace2.html}, $F \subseteq V$, and $E \colon V \to V$ be a \htmladdnormallink{Euclidean transformation}{http://planetmath.org/encyclopedia/Rotate.html} that is not the \htmladdnormallink{identity map}{http://planetmath.org/encyclopedia/IdentityOperator.html}. The following terms are used to indicate that $E(F)=F$ if $E$ is a \htmladdnormallink{rotation}{http://planetmath.org/encyclopedia/Rotate.html}: \begin{itemize} \item $F$ has \emph{rotational symmetry}; \item $F$ has \emph{point symmetry}; \item $F$ has \emph{symmetry about a point}; \item $F$ is \emph{symmetric about a point}. \end{itemize} If $V=\mathbb{R}^2$, then the last two terms may be used to indicate the specific case in which $E$ is conjugate to $\displaystyle \left( \begin{array}{rr} -1 & 0 \\ 0 & -1 \end{array} \right)$, \htmladdnormallink{i.e.}{http://planetmath.org/encyclopedia/Ie.html} the \htmladdnormallink{angle of rotation}{http://planetmath.org/encyclopedia/Rotate.html} is $180^{\circ}$. The following are classic examples of rotational symmetry in $\mathbb{R}^2$: \begin{itemize} \item \htmladdnormallink{Regular polygons}{http://planetmath.org/encyclopedia/Center9.html}: A regular $n$-gon is symmetric about its \htmladdnormallink{center}{http://planetmath.org/encyclopedia/Center9.html} with valid angles of rotation $\displaystyle \theta=\left( \frac{360k}{n} \right)^{\circ}$ for any \htmladdnormallink{positive}{http://planetmath.org/encyclopedia/Negative.html} \htmladdnormallink{integer}{http://planetmath.org/encyclopedia/RationalInteger.html} $k}(3,-0.5)(3,2.5) \end{pspicture} \end{center} In the picture above, the boundary of $T$ is drawn in black, and the line $x=3$ is drawn in cyan. \end{document}