Computational geometry
Contents
- 1 Introduction and Scope
- 2 Points
- 3 Lines
- 3.1 What is a line?
- 3.2 The equation of a line
- 3.3 Standard Form of the equation of a line
- 3.4 Slope and intercepts of the line in standard form
- 3.5 Determining if a point is on a line
- 3.6 Construction of the line through two given points
- 3.7 Parallel and coincident lines
- 3.8 Finding the point of intersection of two lines
- 3.9 Direction numbers for a line
- 3.10 Dropping a perpendicular
- 3.11 The distance from a point to a line
- 3.12 On which side of a line does a point lie?
- 3.13 The distance between two lines
- 4 Line segments
- 4.1 Introduction to line segments
- 4.2 Coincidence (equivalence) of line segments
- 4.3 Length of a line segment
- 4.4 Partitioning by length
- 4.5 Containing line
- 4.6 Determining if a point lies on a line segment
- 4.7 Intersection of line segments
- 4.8 Do two line segments cross?
- 4.9 Direction numbers for the containing line
- 4.10 Perpendicular bisector of a line segment
- 4.11 Conclusion - lines and line segments
- 5 Angles
- 6 Vectors
- 7 Circles
Introduction and Scope
Definition
Computational geometry, as one can easily guess from the name, is the branch of computer science encompassing geometrical problems and how their solutions may be implemented (efficiently, one would hope) on a computer.
Scope
Essentially all of the computational geometry you will encounter in high-school level competitions, even competitions such as the IOI, is plane Euclidean geometry, the noble subject on which Euclid wrote his Elements and a favorite of mathematical competitions. You would be hard-pressed to find contests containing geometry problems in three dimensions or higher. You also do not need to worry about non-Euclidean geometries in which the angles of a triangle don't quite add to 180 degrees, and that sort of thing. In short, the type of geometry that shows up in computer science contests is the type of geometry to which you have been exposed, countless times, in mathematics class, perhaps without being told that other geometries exist. So in all that follows, the universe is two-dimensional, parallel lines never meet, the area of a circle with radius is , and so on. This article discusses basic two-dimensional computational geometry; more advanced topics, such as computation of convex hulls, are discussed in separate articles.
Points
Introduction to points
Many would claim that the point is the fundamental unit of geometry. Lines, circles, and polygons are all merely (infinite) collections of points and in fact we will initially consider them as such in order to derive several important results. A point is an exact location in space. Operations on points are very easy to perform computationally, simply because points themselves are such simple objects.
Representation: Cartesian coordinates
In our case, "space" is actually a plane, two-dimensional. That means that we need two real numbers to
describe any point in our space. Most of the time, we will be using the Cartesian (rectangular) coordinate
system. In fact, when points are given in the input of a programming problem, they are almost always
given in Cartesian coordinates. The Cartesian coordinate system is easy to understand and every pair of
real numbers corresponds to exactly one point in the plane (and vice versa), making it an ideal choice for
computational geometry.
Thus, a point will be represented in the computer's memory by an ordered pair of real numbers. Due to the
nature of geometry, it is usually inappropriate to use integers, as points generally do not fit neatly into the
integer lattice! Even if the input consists only of points with integer coordinates, calculations with these
coordinates will often yield points with non-integral coordinates, which can often cause counter-intuitive
behavior that will have you scratching your head! For example, in C++, when one integer is divided by
another, the result is always truncated to fit into an integer, and this is usually not desirable.
Determining whether two points coincide
Using the useful property of the Cartesian coordinate system discussed above, we can determine whether or not two given points coincide. Denote the two points by and , with coordinates and , respectively, and then:
Read: The statement that and are the same point is equivalent to the statement that their corresponding coordinates are equal. That is, and having both the same x-coordinates and also the same y-coordinates is both sufficient and necessary for the two to be the same point.
The distance between two points
To find the distance between two points, we use the Euclidean formula. Given two points and , the distance between them is given by:
(Note that when we write , we mean that is a point with x-coordinate and y-coordinate .)
The midpoint of the line segment joining two points
Given two points, how may we find the midpoint of the line segment joining two points? (Intuitively, it is the point that is "right in the middle" of two given points. One might think that we require some knowledge about line segments in order to answer this, but it is for precisely the reason that, in a certain sense, no such knowledge is required to understand the answer, that this operation is found in the Points section. So, given two points and , this midpoint is given by
Lines
What is a line?
In axiomatic geometry, some terms such as point and line are left undefined, because an infinite regression of definitions is clearly absurd. In the algebraic approach we are taking, the line is defined in terms of the points which lie on it; that will be discussed in the following section. It will just be pointed out here that the word line is being used in the modern mathematical sense. Lines are straight; the terms line and straight line shall have identical meaning. Lines extend indefinitely in both directions, unlike rays and line segments.
The equation of a line
In computational geometry, we have to treat all aspects of geometry algebraically. Computers are excellent at dealing with numbers but have no mechanism for dealing with geometrical constructions; rather we must reduce
them to algebra if we wish to accomplish anything.
In Ontario high schools, the equation of a line is taught in the ninth grade. For example, the line which passes through the points (0,1) and (1,0) has the equation . Precisely, this means that for a given point , the statement is equivalent to, or sufficient and necessary for, the point to be on the line.
The form of the equation of the line which is first introduced is generally the , in which is the slope of the line and is the y-intercept. For example, the line discussed above has the equation , that is, and . By substituting different values for and , we can obtain various (different) lines. But there's a problem here: if your line is vertical, then it is not
possible to choose values of and for the line. (Try it!) This is because the y-coordinate is no longer a function of the x-coordinate.
Thus, when dealing with lines computationally, it seems we would need to have
a special case: check if the line is vertical; if so, then do something,
otherwise do something else. This is a time-consuming and error-prone way of
coding.
Standard Form of the equation of a line
Even though the slope-intercept form cannot describe a vertical line, there is an equation that describes a vertical line. For example, the line passing through (3,1) and (3,8) is . In fact, almost any line can be described by an equation of the form . (Try it if you don't believe me. I have merely switched around and from the slope-intercept form.) Except... horizontal lines. So we have two forms of the equation of a line: one which fails on vertical lines and one which fails on horizontal lines. Can we combine them to give an equation of the line which is valid for any
line?
As it turns out, it is indeed possible.
That equation, the standard form of the equation of the line is:
By substituting appropriate values of , , and , one can
describe any line with this equation. And by storing values of , , and , one can represent a line in the computer's memory.
Here are some pairs of points and possible equations for each:
As you can see, it handles vertical and horizontal lines properly, as well
as lines which are neither.
Note that the standard form is not unique: for example, the equation of the
first line could have just as well been or perhaps
. Any given line has infinitely many representations
in the standard form. However, each standard form representation describes
at most one line.
If and are both zero, the standard form describes no line
at all.
Slope and intercepts of the line in standard form
By isolating from the standard form, we obtain the slope and y-intercept form for line () when (that is, when the line is not vertical):
The y-intercept is obtained by letting and then:
Similarly, the x-intercept is given by:
In order for the x-intercept to exist, the line must not be horizontal, that is, .
Determining if a point is on a line
Using the definition of the equation of a line, it becomes evident that to determine whether or not a point lies on a line, we simply substitute its coordinates into the equation of the line, and check if the LHS is, indeed, equal to zero. This allows us to determine, for example, that is on the last line given in the table above, whereas is not on that line.
Construction of the line through two given points
A good question is: how do we determine that fourth equation above, the equation of the line through (6,6) and (4,9)? It's not immediately obvious from the two points given, whereas the other three are pretty easy.
For the slope-y-intercept form , you first determined the slope
, and then solved for . A similar procedure can be used for
standard form.
We state here the following pseudocode for determining the
coefficients , , of the equation of the line through
points and in standard form:
(It is one thing to derive a formula or algorithm and quite another thing to prove it. The derivation of this formula is not shown, but proving it is as easy as substituting to determine that the line really does pass through the two given points.)
Parallel and coincident lines
In the slope and y-intercept form, two lines are either parallel or coincident if they have the same slope. So given two lines () and (), we obtain, for :
Cross-multiplying gives a result that is valid even if either or both lines are vertical, that is, it is valid for any pair of lines in standard form:
Now, in the slope-y-intercept form, two lines coincide if their slopes and y-intercepts both coincide. In a manner similar to that of the previous section, we obtain:
or, if x-intercepts are used instead:
Two lines coincide if and either of the two equations above holds. (As a matter of fact, if the two lines are coincident, they will both hold, but only one of them needs to be checked.) If but the lines are not coincident, they are parallel.
Finding the point of intersection of two lines
If two lines are coincident, every point on either line is an intersection
point. If they are parallel, then no intersection points exist. We consider the
general case in which neither is true.
In general, two lines intersect at a single point. That is, the intersection
point is the single point that lies on both lines. Since it lies on both lines,
it must satisfy the equations of both lines simultaneously. So to find the
intersection point of and , we seek the ordered pair which satisfies:
This is a system of two linear equations in two unknowns and is solved by Gaussian elimination. Multiply the first by and the second by , giving:
Subtracting the former from the latter gives, with cancellation of the term:
Instead of redoing this to obtain the value of , we take advantage of symmetry and simply swap all the 's with the 's. (If you don't believe that this works, do the derivation the long way.)
or:
Notice the quantity , and how it forms the denominator of the expressions for both and . When solving for the intersection point on the computer, you only need to calculate this quantity once. (This quantity, called a determinant, will resurface later on.) Here is pseudocode for finding the intersection point:
When , the lines are either parallel or coincident. We now see algebraically that the division by zero prevents us from finding a unique intersection point for such pairs of lines.
Direction numbers for a line
This in itself is not very useful, but it will become important in the
following sections as a simplifying concept.
Lines are straight; effectively they always point in the same direction. One
way to express that direction has been slope, which unfortunately is undefined
for vertical lines. The slope for a line told us that you could
start at any point on the line, move units to the right, then
move units up, and you would again be located on the line.
Thus we can say that is a pair of direction numbers for that line.
This means that if is on a line, and and
are in the ratio , for that line, then
is on the same line. This means that
is also a set of direction numbers for that line, or, indeed, any
multiple of other than . (
clearly tells you nothing about the line.)
We can define something similar for the line in standard form. Choose some
starting point on line . Now, move to a new point
. In order for this point to be on the line
, we must have
Expanding and rearranging gives
We know that since is on line . Therefore,
Convince yourself, by examining the equation above, that is a set
of direction numbers for line . Similarly, if we have a pair of
direction numbers , although this does not define a
unique line, we can obtain possible values of and as
and , respectively.
The relationship between direction numbers and points on the corresponding line
is an "if-and-only-if" relationship. If and are
in the ratio , then we can "shift" by ,
and vice versa.
Any line perpendicular to will have the direction numbers ,
and thus a possible equation starts .
(This is the same as saying, for non-vertical lines, that the product of slopes
of perpendicular lines is -1. Examine the equation for the slope of a line
given in standard form and you'll see why.) In fact, in an algebraic treatment of geometry
such as this, we do not prove this claim, but instead proclaim it the definition of
perpendicularity: given two lines with direction numbers and
, they are perpendicular if and only if
.
Given some line, all lines parallel to that one have the same direction numbers. That is, the direction
numbers, while providing information about a line's direction, provide no
information about its position. However, sometimes all that is needed is the direction, and here the
direction numbers are very useful.
Dropping a perpendicular
Given a line and a point which may or may not be on , can we find the line perpendicular to passing through ? By Euclid's Fifth Postulate, there exists exactly one such line. The algorithm to find it is given below:
where is the perpendicular line desired.
There is nothing difficult to memorize here: we already noted in the previous
section how to find the values of and , and finding the value
of is merely setting equal to zero (so that the
point will be on the resulting line).
The foot of the perpendicular is the point at which it intersects the
line . It is guaranteed to exist since two lines cannot, of course, be
both perpendicular and parallel. Combining the above algorithm with the line intersection algorithm
explained earlier gives a solution for the location of the point. A bit of algebra gives
this optimized algorithm:
where are the coordinates of the foot of the perpendicular from to .
The distance from a point to a line
By the distance from a point to a line
what is meant is the closest possible distance from
to any point on . What point on is closest to ?
It is intuitive perhaps that it is obtained by dropping a perpendicular
from to . That is, we choose a point such that
, and the distance from to is then the length
of line segment , denoted .
The reason why this is the shortest distance possible is this: Choose any other
point on . Now, is right-angled at .
The longest side of a right triangle is the hypotenuse, so that
. Thus is truly the shortest possible distance.
Now, as noted earlier, the line , being perpendicular to , has the direction numbers . Thus, for any , the point is on
. For some choice of , this point must coincide with .
Since that point lies on , we have
This instantly gives the formula for the foot of the perpendicular given in
the previous section.
Now, the distance is found with the Euclidean formula:
The last line is the formula to remember. To restate,
(It was noted earlier that if and are both zero, then we don't actually have a line. Therefore, the denominator above can never be zero, which is a good thing.)
On which side of a line does a point lie?
A line partitions the plane into two regions. For example, a vertical line
divides the plane into a region on the left and a region on the right. Now,
when a point does not satisfy the equation of a line
, can we determine on which side of the line it lies?
Yes we can, with a certain restriction. If , then the
point lies on one side of the line; if , then it lies
on the other side. However, it's a bit pointless to say which side it
lies on: does it lie on the left or the right? If the line is horizontal, then
this question becomes meaningless. Also, notice that if we flip the signs of
, , and , then the value of is
negated also, but that changes neither the point or the line. It is enough,
however, to tell if two points are on the same side of the line or on opposite
sides; simply determine whether has the same sign for both,
or different signs.
The distance between two lines
If two lines intersect, the closest distance between them is zero, namely at their intersection point. If they are coincident, then the distance is similarly zero. If two lines are parallel, however, there is a nonzero distance between them, and it is defined similarly to the distance between a point and a line. To find this distance, we notice that the lines and are coincident, where is the origin, is the foot of the perpendicular from to , and is the foot of the perpendicular from to . We know, by substituting for both () and () that:
Now here we come up against a complication. If is on the line segment , then we have to add and to get the desired . That is, if is on the same side of both lines. Otherwise, we have to take the difference. Here's some code that takes care of these details:
Line segments
Introduction to line segments
A line segment is the part of a line located "between" two points on that
line, called endpoints. Any pair of points defines a unique line
segment. Most definitions of "line segment" allow the endpoints to coincide,
giving a single point, but this case will often not arise in programming
problems and it is trivial to handle when it does arise, so we will not discuss
it here; we assume the endpoints must be distinct. Thus, every line segment
defines exactly one line.
We may represent a line segment in memory as a pair of points: that is, four
numbers in total.
Coincidence (equivalence) of line segments
Two line segments coincide if they have the same endpoints. However, they may have them in any order, hence we have:
(The parentheses are unnecessary and are added only for the sake of clarity.)
Length of a line segment
The length of a line segment is nothing more than the distance between its endpoints.
Partitioning by length
Suppose we wish to partition a line segment by introducing a point on such that . That is, we wish to partition it into two line segments with their lengths in the ratio . We may do so as follows:
In the special case that , we have the midpoint, as discussed in the Points section.
Containing line
All we have to do is find the line passing through both endpoints; the algorithm to do this is discussed in the section "Construction of the line through two given points".
Determining if a point lies on a line segment
Here is one interesting idea: if a point lies on segment , then the relation will hold. If it is on the line but not on the segment , then it is the difference between and that will equal , not the sum. If it is not on this line, then the points , , and form a triangle, and by the Triangle Inequality, . Thus:
Although this test is mathematically ingenious, it should not be used in
practice, since the extraction of a square root is a slow operation. (Think about how much work it takes by hand, for example, to compute a square root, relative to carrying out multiplication or division by hand.)
A faster method is to obtain the line containing the line segment (see
previous section); if multiple queries are to be made on the same line segment
then it is advisable to store the values of , , and
rather than computing them over and over again; and we first check if the point
to test is on the line; if it is, then we must check if it is on the
segment by checking if each coordinate of the point is between the
corresponding coordinates of the endpoints of the segment.
For a one-time query (when we do not expect to see the line again), the use of
the properties of similar triangles yields the following test: the point is on
the line segment if and only if
and is between and . When this test is used several
times with different segments, the number of multiplications required is only
half of the number required for the test via the containing line, but
if the line is reused, then the test via the containing line ends up
using fewer additions/subtractions in the long run.
Intersection of line segments
Given two line segments and , how do we
determine whether they intersect?
First, if the containing lines are coincident, then the line segments intersect
if and only if at least one of the endpoints of one of the segments is on the
other segment. In general, when the containing lines do not coincide,
the segments intersect if and only if and
are not on the same side of and and are
not on the same side of . That is, extend each segment to a line and
then determine on which sides of the line lie the endpoints of the other segment. (If one point is on the line and the other is not, then they are not considered to be on the same side, since two
line segments can intersect even if the endpoint of one lies on the other.)
If the segments intersect, their intersection point can be determined by finding the intersection
point of the containing lines.
Another method for determining whether two line segments intersect is finding
the intersection point (if it exists) of the containing lines and checking if
it lies on both line segments (as in the end of the previous section). After
finding the containing lines, this method requires six multiplications and two
divisions, whereas the one above requires eight multiplications. Since
multiplications are generally faster, we prefer the method above to this one.
Do two line segments cross?
The word cross is used here in a stronger sense than intersect. Two line segments cross if they intersect and no point of intersection is an endpoint of either line segment. Intuitively, the two line segments form a (possibly distorted) X shape. Here, we can ignore the degenerate cases for line segment intersection: we simply test that and are on different sides of (this time the test fails if either of them is actually on it), and that and are on different sides of . The second method described in the previous section can again be applied, although again it is expected to be slower.
Direction numbers for the containing line
By the definition of the direction numbers, a set of direction numbers for the line segment is . This gives an instant proof for the "magic formula" for the line through two given points: we convert these direction numbers to values for and and then solve for using one of the points.
Perpendicular bisector of a line segment
The perpendicular bisector of a line segment is the line perpendicular to the line segment which also passes through the line segment's midpoint. Notice that the direction numbers obtained in the previous section can be used to obtain the direction numbers for a perpendicular line, and that these can in turn be used to reconstruct the values of and for that line. Given that the line must also pass through the midpoint:
This technique requires a total of two multiplications and two divisions. If we substitute the values of and into the last line and expand, we can change this to four multiplications and one division, which is almost certainly slower as division by two is a very fast operation.
Conclusion - lines and line segments
The techniques of the two preceding chapters should provide inspiration on how to achieve tasks that are "somewhere in-between". For example, we have not discussed the intersection of a line and a line segment. However, it is fairly clear that all that is required is to test on which sides of the line lie the endpoints of the segment: half of the test for two line segments. We also have not discussed the distance from a point to a line segment. We have omitted any discussion of rays altogether. If you thoroughly understand how these techniques work, though, extending them to problems not explicitly mentioned should not be difficult. Feel free to add these sections to this article; the exclusion of any material from the current draft is not an indication that such material does not belong in this article.
Angles
Introduction to angles
In trigonometry, one proves the Law of Cosines. In a purely algebraic approach to geometry, however the concept of angle is defined using the Law of Cosines, and the Law itself requires no proof. Still, we will not use that definition directly, because deriving everything from it would be unnecessarily complicated. Instead, we will assume that we already know some properties of angles. Storing angles in memory is very easy: just store the angle's radian measure. Why not degree measure? Degree measure is convenient for mental calculation, but radian measure is more mathematically convenient and, as such, trigonometric functions of most standard language libraries, such as those of Pascal and C/C++, expect their arguments in radians. (Inverse trigonometric functions return results in radians.) We will use radian measure throughout this chapter, without stating "radians", because radian measure is assumed when no units are given.
Straightforward applications of basic trigonometry, such as finding the angles in a triangle whose vertices are known (Law of Cosines), are not discussed here.
Directed angle and the atan2 function
Suppose a ray with its endpoint at the origin initially points along the
positive x-axis and is rotated counterclockwise around the origin by an angle
of . From elementary trigonometry, the ray now consists of points
, where . This angle
is a directed angle. Notice there is another ray with its endpoint at
the origin that makes an angle of with the positive x-axis:
obtained by rotating clockwise rather than counterclockwise. But the directed
angle in this case would be . Thus, by specifying a directed angle
from the positive x-axis
we can uniquely specify one particular ray.
Can we reverse this process? Can we find the directed angle from the positive
x-axis to the ray , where ? Notice that
when , , so taking the inverse tangent
should give back . There are just two problems with this: one is
that might be zero (but the angle will still be defined, either or ), the other is that the point will give
the same tangent even though it lies on the other side (and hence its directed
angle should differ from that of by .
However, because this is such a useful application, the Intel FPU has a
built-in instruction to compute the directed angle from the positive x-axis to
ray , and the libraries of both C and Free Pascal
contain functions for this purpose. C's is called atan2
, and it takes
two arguments, and , in that order, returning an angle in
radians, the desired directed angle, a real number satisfying
. (Notice that as with undirected angles, adding
to a directed angle leaves it unchanged). Remember that
comes first and not ; the reason for this has to do with the design of
the Intel FPU and the calling convention of C. Free Pascal's math library aims
to largely emulate that of C, so it provides the arctan2
function
which takes the same arguments and produces the same return value.
The angle between a line and the x-axis
When two lines intersect, two pairs of angles are formed (the two angles in
each pair are equal). They are supplementary. To find one of these angles, let
us shift the line until it passes through the x-axis. Then, adding the
direction numbers to the origin gives another point. We now apply
the atan2
function: atan2
(). (Notice that we have
reversed the order of and , as required.) The result may be
negative; we can add to it to make it non-negative.
The angle between two lines
To find one of the two angles between two lines, we find the angle between each line and the x-axis, then subtract. (Draw a diagram to convince yourself that this works.) If the result is negative, add degrees, once or twice as necessary. The other angle is obtained by subtracting from .
The angle bisector of a pair of intersecting lines
Using the result of the previous section and a great deal of algebra and trigonometry, together with the line intersection algorithm, gives the following algorithm for finding one of the two angle bisectors of a pair of (intersecting) lines and (the bisector is represented as ):
The other angle bisector, of course, is perpendicular to this line and also passes through that intersection point.
Vectors
Introduction to vectors
Although the word vector has a formal definition, we will not find it useful. It is better, in the context of computational geometry, to think of a vector as an idealized object which represents a given translation. Visually, a vector may be represented as an arrow with a fixed length pointing in a fixed direction, but without a fixed location. For example, on the Cartesian plane, consider the translation "3 units down and 4 units right". If you start at the point (8,10) and apply this translation, (12,7) is obtained. This can also be represented as an arrow with length 5 units and direction approximately 37 degrees south of east. Placing the tail of this arrow at (8,10) results in the head resting upon the point (12,7). The vector from (0,0) to (4,-3) is the same vector, as it also represents a translation 3 units down and 4 units right, and has the same length and direction. However, the vector from (12,7) to (8,10) and the vector from (0,0) to (-3,4) are different from the one from (8,10) to (12,7); they have the same lengths, but their directions are different, and so they are different vectors. The vector from (0,0) to (8,-6) is also different; it has the same direction, but a different length. In both cases, these are simply different translations, and hence different vectors. The word vector is from the Latin, meaning carrier, appropriate as it carries from one location (a point) to another. In text, vectors are represented as letters with small rightward-pointing arrows over them, e.g., .
Representation
We could represent a vector by its magnitude and direction, but it is usually not convenient to do so. (If you must, refer to the sections #Length of a line segment and #Directed angle and the atan2 function for the necessary mathematics.) Instead, we will use the Cartesian representation. If we place the tail of a vector on the origin, the head rests upon a certain point; the Cartesian coordinates of this point are the Cartesian components of the vector. We thus represent a vector as we do a point, as an ordered pair of real numbers, but we shall enclose these in brackets instead of parentheses. The vector discussed above is then [4,-3], as when the tail is placed on (0,0), the head rests upon (4,-3).
Circles
Introduction to circles
A circle is the locus of points in the plane equidistant from a given point. That is, we choose some point , the centre, and some distance , the radius, and the circle consists exactly of those points whose Euclidean distance from is exactly . When storing a circle in memory, we store merely the centre and the radius.
Equation of a circle
Suppose the circle has centre and radius . Then, from the definition, we know that any point on the circle must satisfy . This means , or .
Inside, outside, or on the circle
The equation of a circle is a sufficient and necessary condition for a point to be on the circle. If it is not on the circle, it must be either inside the circle or outside the circle. It will be inside the circle when its distance from the centre is less than , or , and similarly it will be outside the circle when .
Intersection of a circle with a line
To determine points of intersection of a circle with another figure (it might also be a circle), solve the simultaneous equations obtained in and . For example, given a circle centered at (2,3) with radius 2, and the line , we would solve the simultaneous equations and . If there are multiple solutions, each is a different point of intersection; if there are no solutions then the two figures do not intersect. Here then are general results. Note that if you do not check the "no intersection" condition beforehand and plunge straight into the quadratic formula (after reducing the two simultaneous equations to one equation), you will try to extract the square root of a negative number, which will crash some languages (such as Pascal).
No points of intersection
When the closest distance from the centre of the circle to the line is greater than the radius of the circle, the circle and line do not intersect. (The formula for the distance from a point to a line can be found in the Lines section of this article.)
One point of intersection
When the closest distance from the centre of the circle to the line is exactly the circle's radius, the line is tangent to the circle. One way of finding this point of tangency, the single point of intersection, is to drop a perpendicular from the centre of the circle to the line. (The technique for doing so is found in the Lines section.) This will, of course, yield the same answer as solving the simultaneous equations.
Two points of intersection
When the closest distance from the centre of the circle to the line is less than the circle's radius, the line intersects the circle twice. The algebraic method must be used to find these points of intersection.
Intersection of a circle with a circle
Finding the points of intersection of two circles follows the same basic idea as the circle-line intersection. Here's how to determine the nature of the intersection beforehand, to avoid accidentally trying to take the square root of a negative number:
No points of intersection
When the distance between the centres of the circles is less than the difference between their radii, the circle with smaller radius will be contained completely within the circle of larger radius. When the distance between the centres of the circles is greater than the sum of their radii, neither circle will be inside the other, but still the two will not intersect.
One point of intersection
When the distance between the centres of the circles is exactly the difference between their radii, the two circles will be internally tangent. When the distance between the centres of the circles is exactly the sum of their radii, they will be externally tangent.
Two points of intersection
In all other cases, there will be two points of intersection.