Although everything above has been stated in terms of general
rectangular matrices, for the rest of this tutorial, we'll consider
only two kinds of matrices (but of any dimension): square matrices,
where the number of rows is equal to the number of columns, and column
matrices, where there is only one column. These column matrices are
often called ``vectors'', and there are many applications where they
correspond exactly to what you commonly use as sets of coordinates for
points in space. In the two-dimensional
-
plane, the
coordinates
represent a point that is one unit to the right
of the origin (in the direction of the
-axis), and three units
above the origin (in the direction of the
-axis). That same point
can be written as the following column vector:
If you wish to work in three dimensions, you'll need three coordinates
to locate a point relative to the (three-dimensional) origin--an
-coordinate, a
-coordinate, and a
-coordinate. So the
point you'd normally write as
can be represented by
the column vector:
Quite often we will work with a combination of square matrices and
column matrices, and in that case, if the square matrix has
dimensions
, the column vectors will have dimension
(
rows and 1 column)1.