We want
, and we have
and
. If we could get the angle
, then we could use the cosine rule to determine
. This is possible, as
is a right-angled triangle. We know this from circle geometry, that any triangle circumscribed by a circle with one side going through the origin, is right-angled. As we have two angles of
, we know
and hence
. Using the cosine rule, we can get
.
Thus
Now the cosine rule gives
For the diagram on the right,
Find
in terms of
.
Find an expression for:
Using the above, show that
.
Now do the same for
and
.
is a diameter of circle
with radius
.
,
and
.
Show that
.
The figure below shows a cyclic quadrilateral with
.
Show that the area of the cyclic quadrilateral is
.
Find expressions for
and
in terms of the quadrilateral sides.
Show that
.
Suppose that
,
,
and
. Find
.
Find the angle
using your expression for
. Hence find the area of
.
Problems in 3 dimensions
is the top of a tower of height
. Its base is at
. The triangle
lies on the ground (a horizontal plane). If we have that
,
,
and
, show that
We have that the triangle
is right-angled. Thus we can relate the height
with the angle
and either the length
or
(using sines or cosines). But we have two angles and a length for
, and thus can work out all the remaining lengths and angles of this triangle. We can thus work out
.
We have that
Now we need
in terms of the given angles and length
. Considering the triangle
, we see that we can use the sine rule.
But
, and
So
The line
represents a tall tower, with
at its foot. Its angle of elevation from
is
. We are also given that
.
Find the height of the tower
in terms of
,
and
.
Find
if we are given that
,
and
.
Other geometries
Taxicab geometry
Taxicab geometry, considered by Hermann Minkowski in the 19th century, is a form of geometry in which the usual metric of Euclidean geometry is replaced by a new metric in which the distance between two points is the sum of the (absolute) differences of their coordinates.
Manhattan distance
The metric in taxi-cab geometry, is known as the
Manhattan distance , between two points in an Euclidean space with fixed Cartesian coordinate system as the sum of the lengths of the projections of the line segment between the points onto the coordinate axes.
For example, the Manhattan distance between the point
with coordinates
and the point
at
is