<?xml version="1.0" encoding="UTF-8"?>

<record version="2" id="96">
 <title>centre of mass</title>
 <name>CentreOfMass</name>
 <created>2005-08-31 17:51:22</created>
 <modified>2006-03-24 06:29:54</modified>
 <type>Definition</type>
 <creator id="0" name=""/>
 <modifier id="17" name="pbruin"/>
 <author id="17" name="pbruin"/>
 <classification>
	<category scheme="msc" code="45.40.-f"/>
	<category scheme="msc" code="45.50.Dd"/>
 </classification>
 <synonyms>
	<synonym concept="centre of mass" alias="center of mass"/>
 </synonyms>
 <preamble>% this is the default PlanetPhysics preamble.  as your knowledge
% of TeX increases, you will probably want to edit this, but
% it should be fine as is for beginners.

% almost certainly you want these
\usepackage{amssymb}
\usepackage{amsmath}
\usepackage{amsfonts}

% used for TeXing text within eps files
%\usepackage{psfrag}
% need this for including graphics (\includegraphics)
%\usepackage{graphicx}
% for neatly defining theorems and propositions
%\usepackage{amsthm}
% making logically defined graphics
%\usepackage{xypic}

% there are many more packages, add them here as you need them

% define commands here</preamble>
 <content>The \emph{centre of mass} of an object is a point in space where, for many purposes, the mass of the object may be assumed to be concentrated.  For example, an object hung from a string in a uniform gravitational field will have its centre of mass straight below the string.  The centre of mass can be used in many other ways to simplify a complicated system by treating it as a point particle.  The momentum of an object with total mass $M$ is
$$
\mathbf{p}=M\mathbf{v}_{\mathrm{cm}},
$$
and if a total force $\mathbf{F}$ acts on the object, Newton's second law may be formulated as
$$
\mathbf{F}=M\mathbf{a}_{\mathrm{cm}}.
$$
In these equations $\mathbf{v}_{\mathrm{cm}}$ and $\mathbf{a}_{\mathrm{cm}}$ are the velocity and the acceleration of its centre of mass, respectively; these are defined below.

The centre of mass of a solid object occupying a region $V$ in space is defined as the average position of all the points of $V$, each point $\mathbf{x}$ being weighted with the density of the object at that point, $\rho(\mathbf{x})$.  This average is a volume integral over the region $V$:
$$
\mathbf{x}_{\mathrm{cm}}\equiv\frac{1}{M}\int_V
\rho(\mathbf{x})\mathbf{x}\,\mathrm{d}V.
$$
Here $M$ is the total mass of the object:
$$
M\equiv\int_V \rho(\mathbf{x})\,\mathrm{d}V.
$$

If the object consists of a number of point particles, these integrals become sums over the particles.  The centre of mass of a collection of $N$ particles with masses $m_1,m_2,\ldots,m_N$ located at the positions $\mathbf{x}_1,\mathbf{x}_2,\ldots,\mathbf{x}_N$ is
$$
\mathbf{x}_{\mathrm{cm}}\equiv\frac{1}{M}\sum_{i=1}^N m_i\mathbf{x}_i,
$$
where $M$ is now the sum of the masses of the particles:
$$
M\equiv\sum_{i=1}^N m_i.
$$

The velocity and acceleration of the centre of mass are now simply defined as the first and second time derivatives of $\mathbf{x}_{\mathrm{cm}}$:
$$
\mathbf{v}_{\mathrm{cm}}\equiv\mathbf{\dot x}_{\mathrm{cm}},\qquad
\mathbf{a}_{\mathrm{cm}}\equiv\mathbf{\ddot x}_{\mathrm{cm}}.
$$</content>
</record>
